alminer
's various functions with examples.1.1 Query by target name
1.2 Query by position
1.3 Query by ALMA keywords
2. Filter & explore results
2.1 Explore results
2.2 Summarize results
2.3 Filter results
2.4 Line coverage
2.5 Coverage of CO, 13CO, and C18O lines
3. Plot results
3.1 Plot an overview of the observations
3.2 Plot an overview of a given line in the observations
3.3 Plot observed frequencies in each band
3.4 Plot observations in each band
3.5 Plot sky distribution
4. Create reports
4.1 Export results as a table
4.2 Save overview plots
5. Download data
6. Advanced query features
6.1 Create and run your own TAP query
6.2 Convert results to ALminer format
7. Glossary of all functions
8. Workstation
import alminer
import pandas
from astropy.io import ascii
This Section introduces three methods to query the ALMA archive:
The alminer.target
function allows one to query objects by name. This function uses the Astropy SESAME resolver which searches multiple databases (Simbad, NED, VizieR) to obtain the coordinates of the object of interest, and then queries the ALMA archive for those coordinates and a search radius around them. The search radius is by default 1.0 arcminute, but can be modified using the search_radius keyword (in arcmin units).
target
functionkeysearch
function and query the archive using the 'target_name' keyword (e.g. keysearch({'target_name': sources})
).myquery = alminer.target(['Orion KL', "AB Aur"])
================================ alminer.target results ================================ Target = Orion KL -------------------------------- Number of projects = 27 Number of observations = 63 Number of unique subbands = 226 Total number of subbands = 272 23 target(s) with ALMA data = ['Orion H2O maser outburst', 'OrionKL', 'Orion_Source_I', 'Orion KL', 'Orion-KL', 'Orion_KL', 'BN-KL', 'OrionKL-SV', 'f15', 'f14', 'OMC1_NW', 'Orion1', 'OMC1_SE', 'BN', 'f23', 'Orion', 'Orion_BNKL_source_I', 'OMC-1_Region2', 'orion_kl', 'orion-IRc2', 'Orion_KL_Field_1_Orion_Hot_Core', 'Orion_KL_Field_3_North-west_Clump', 'Orion_KL_Field_2_SMA1'] -------------------------------- Target = AB Aur -------------------------------- Number of projects = 3 Number of observations = 3 Number of unique subbands = 17 Total number of subbands = 17 3 target(s) with ALMA data = ['ab_aurigae', 'AB_Aur', 'AB_Auriga'] --------------------------------
Now let's increase the search radius:
myquery = alminer.target(['Orion KL', "AB Aur"], search_radius=2.0)
================================ alminer.target results ================================ Target = Orion KL -------------------------------- Number of projects = 35 Number of observations = 100 Number of unique subbands = 283 Total number of subbands = 451 46 target(s) with ALMA data = ['HC602_HC606_HC608', 'Orion H2O maser outburst', 'OrionField1-2', 'OrionKL', 'Orion_Source_I', 'HC672', 'OrionField1-1', 'OrionField2', 'Orion KL', 'OMC-1S', 'Orion-KL', '104', 'Orion_KL', '71', 'BN-KL', 'OrionKL-SV', 'f11', 'f12', 'f15', 'f13', 'f14', 'OMC1_SE', 'OMC1_NW', 'f10', 'Orion1', 'f8', 'f4', 'f5', 'f1', 'f7', 'f3', 'BN', 'f23', 'Orion', 'Orion_BNKL_source_I', 'f16', 'OMC-1_Region4', 'OMC-1_Region2', 'orion_kl', 'ONC_Mosaic', 'orion-IRc2', 'Orion_KL_Field_1_Orion_Hot_Core', 'ONC', 'Orion_KL_Field_3_North-west_Clump', 'Orion_KL_Field_2_SMA1', 'ORS-8'] -------------------------------- Target = AB Aur -------------------------------- Number of projects = 3 Number of observations = 3 Number of unique subbands = 17 Total number of subbands = 17 3 target(s) with ALMA data = ['ab_aurigae', 'AB_Aur', 'AB_Auriga'] --------------------------------
First create a catalog or a list of object names. In this example, the catalog Sample_cat.dat
has the following content:
Name RA DEC
------ -------- --------
AB_Aur 73.9412 30.5511
AK_Sco 253.6867 -36.8886
AS_310 278.3383 -4.9683
AS_470 324.0592 57.3586
AS_477 328.1421 47.2289
Note that the column that is used is the Name column and the coordinates are ignored in this example.
mylist = ascii.read("Sample_cat.dat", header_start=0, data_start=1)
myquery = alminer.target(mylist['Name'])
================================ alminer.target results ================================ Target = AB_Aur -------------------------------- Number of projects = 3 Number of observations = 3 Number of unique subbands = 17 Total number of subbands = 17 3 target(s) with ALMA data = ['ab_aurigae', 'AB_Aur', 'AB_Auriga'] -------------------------------- Target = AK_Sco -------------------------------- Number of projects = 3 Number of observations = 3 Number of unique subbands = 12 Total number of subbands = 12 2 target(s) with ALMA data = ['AK_Sco', 'HIP_82747'] -------------------------------- Target = AS_310 -------------------------------- No observations found. -------------------------------- Target = AS_470 -------------------------------- No observations found. -------------------------------- Target = AS_477 -------------------------------- No observations found. --------------------------------
myquery = alminer.target(mylist['Name'], public=None)
================================ alminer.target results ================================ Target = AB_Aur -------------------------------- Number of projects = 4 Number of observations = 5 Number of unique subbands = 25 Total number of subbands = 25 3 target(s) with ALMA data = ['ab_aurigae', 'AB_Aur', 'AB_Auriga'] -------------------------------- Target = AK_Sco -------------------------------- Number of projects = 4 Number of observations = 4 Number of unique subbands = 16 Total number of subbands = 16 2 target(s) with ALMA data = ['AK_Sco', 'HIP_82747'] -------------------------------- Target = AS_310 -------------------------------- No observations found. -------------------------------- Target = AS_470 -------------------------------- No observations found. -------------------------------- Target = AS_477 -------------------------------- No observations found. --------------------------------
The alminer.target
function will by default search whether the phase center of any ALMA observations lie within the search radius around the target of interest's position. To search whether any part of the observed region overlaps with the cone extending the search radius, one can set point=False. Note that this option is slower, hence it's not the dafault mode.
myquery = alminer.target(['Orion KL'], point=False)
================================ alminer.target results ================================ Target = Orion KL -------------------------------- Number of projects = 35 Number of observations = 90 Number of unique subbands = 283 Total number of subbands = 399 40 target(s) with ALMA data = ['HC602_HC606_HC608', 'Orion H2O maser outburst', 'OrionField1-2', 'OrionKL', 'Orion_Source_I', 'OrionField1-1', 'Orion KL', 'Orion-KL', '104', 'Orion_KL', 'BN-KL', 'OrionKL-SV', 'f11', 'f12', 'f15', 'f13', 'f14', 'OMC1_SE', 'OMC1_NW', 'f10', 'Orion1', 'f1', 'f3', 'BN', 'f23', 'Orion', 'OMC-1_Region5', 'Orion_BNKL_source_I', 'f16', 'OMC-1_Region4', 'OMC-1_Region2', 'orion_kl', 'OMC-1', 'ONC_Mosaic', 'orion-IRc2', 'Orion_KL_Field_1_Orion_Hot_Core', 'ONC', 'Orion_KL_Field_3_North-west_Clump', 'Orion_KL_Field_2_SMA1', 'ORS-8'] --------------------------------
The alminer.conesearch
and alminer.catalog
functions can be used to directly query the ALMA archive by positions in the sky and a search radius around them. The right ascension and declinations must be given in units of degrees (ICRS). You can use the Astropy coordinates package to convert your desired coordinates to degrees.
conesearch
functioncatalog
functionmyquery = alminer.conesearch(ra=201.365063, dec=-43.019112, search_radius=10.0)
-------------------------------- Number of projects = 23 Number of observations = 74 Number of unique subbands = 190 Total number of subbands = 301 9 target(s) with ALMA data = ['CenA', 'J1325-430', 'Centaurus_a', 'J1325-4301', 'Centaurus A', 'Centaurus_A', '3FGL_J1325.4-4301', 'NGC_5128', 'Cen_A'] --------------------------------
Let's first import a catalog, for example the catalog of Spitzer YSOs in Orion from Megeath et al. (2009), and create a PANDAS DataFrame using rows 866 to 869 of this catalog. Then use the alminer.catalog
function to query the ALMA archive for each target in the DataFrame.
Spitzer = ascii.read("Spitzer_sample.dat", header_start=0, data_start=866, data_end=869)
mycat = {"Name": Spitzer['Seq'],
"RAJ2000" : Spitzer["RA2000"],
"DEJ2000" : Spitzer["DEC2000"]}
mycat = pandas.DataFrame(mycat)
myquery = alminer.catalog(mycat, search_radius=1.)
================================ alminer.catalog results ================================ Target = 866 -------------------------------- Number of projects = 1 Number of observations = 1 Number of unique subbands = 4 Total number of subbands = 4 1 target(s) with ALMA data = ['M12_866'] -------------------------------- Target = 867 -------------------------------- Number of projects = 1 Number of observations = 1 Number of unique subbands = 4 Total number of subbands = 4 1 target(s) with ALMA data = ['M12_867'] -------------------------------- Target = 868 -------------------------------- Number of projects = 2 Number of observations = 2 Number of unique subbands = 8 Total number of subbands = 8 1 target(s) with ALMA data = ['HOPS-172'] --------------------------------
Query the ALMA archive for any (string-type) keywords defined in ALMA TAP system (see table below).
The power of this function is in combining keywords. When multiple keywords are provided, they are queried using 'AND' logic, while when multiple values are provided for a given keyword, they are queried using 'OR' logic. For example,
alminer.keysearch({"proposal_abstract": ["high-mass star formation outflow disk"]})
will query the archive for projects with the words "high-mass" AND "star" AND "formation" AND "outflow" AND "disk" in their proposal abstracts.
alminer.keysearch({"proposal_abstract": ["high-mass", "star", "formation", "outflow", "disk"]})
will query the archive for projects with the words "high-mass" OR "star" OR "formation" OR "outflow" OR "disk" in their proposal abstracts.
alminer.keysearch({"proposal_abstract": ["star formation"], "scientific_category":['Galaxy evolution']})
will query the archive for projects with the words "star" AND "formation" in their proposal abstracts AND projects that are within the scientific_category of 'Galaxy evolution'.
keysearch
functionALMA query keyword | Type | Description |
---|---|---|
access_format | char(9) | Content format of the data |
access_url | char(72*) | URL to download the data |
antenna_arrays | char(660*) | Blank-separated list of Pad:Antenna pairs, i.e., A109:DV09 J504:DV02 J505:DV05 for antennas DV09, DV02 and DV05 sitting on pads A109, J504, and J505, respectively. |
asdm_uid | char(32*) | UID of the ASDM containing this Field. |
authors | char(4000*) | Full list of first author and all co-authors |
band_list | char(30*) | Space delimited list of bands |
bib_reference | char(30*) | Bibliography code |
data_rights | char(11) | Access to data. |
dataproduct_type | char(5*) | type of product |
facility_name | char(3) | telescope name |
first_author | char(256*) | The first author as provided by telbib.eso.org. |
frequency_support | char(4000*) | All frequency ranges used by the field |
group_ous_uid | char(64*) | Group OUS ID |
instrument_name | char(4) | instrument name |
is_mosaic | char(1) | Flag to indicate if this ASDM represents a mosaic or not. |
lastModified | char(*) | Time stamp of last modification of the metadata |
member_ous_uid | char(64*) | Member OUS ID |
o_ucd | char(35) | UCD describing the observable axis (pixel values) |
obs_collection | char(4) | short name for the data collection |
obs_creator_name | char(256*) | case-insensitive partial match over the full PI name. Wildcards can be used |
obs_id | char(64*) | internal dataset identifier |
obs_publisher_did | char(33*) | publisher dataset identifier |
obs_release_date | char(*) | timestamp of date the data becomes publicly available |
obs_title | char(256*) | Case-insensitive search over the project title |
pol_states | char(64*) | polarization states present in the data |
proposal_abstract | char(4000*) | Text search on the proposal abstract. Only abstracts will be returned which contain the given text. The search is case-insensitive. |
proposal_authors | char(2000*) | Full name of CoIs. |
proposal_id | char(64*) | Identifier of proposal to which NO observation belongs. |
pub_abstract | char(4000*) | Case insensitive text search through the abstract of the publication. |
pub_title | char(256*) | Case insensitive search through the title of the publication. |
qa2_passed | char(1) | Quality Assessment 2 status: does the Member / Group OUS fulfil the PI's requirements? |
s_region | char(*) | region bounded by observation |
scan_intent | char(256*) | Scan intent list for the observed field. |
schedblock_name | char(128*) | Name of the Scheduling Block used as a template for executing the ASDM containing this Field. |
science_keyword | char(200*) | Chosen by the PI in the observing tool at the time of proposal submission. For an overview, see Appendix D of the ALMA Proposer's Guide. For a precise list, see Table of science keywords below. |
science_observation | char(1) | Flag to indicate whether this is a science observation. |
scientific_category | char(200*) | Chosen by the PI in the observing tool at the time of proposal submission. For an overview, see Appendix D of the ALMA Proposer's Guide. For a precise list, see Table of science categories below. |
target_name | char(256*) | name of intended target |
type | char(16*) | Type flags. |
ALMA science keyword |
---|
Active Galactic Nuclei (AGN)/Quasars (QSO) |
Astrochemistry |
Asymptotic Giant Branch (AGB) stars |
Black holes |
Brown dwarfs |
Cataclysmic stars |
Cosmic Microwave Background (CMB)/Sunyaev-Zel'dovich Effect (SZE)" |
Damped Lyman Alpha (DLA) systems |
Debris disks |
Disks around high-mass stars |
Disks around low-mass stars |
Dwarf/metal-poor galaxies |
Early-type galaxies |
Evolved stars - Chemistry |
Evolved stars - Shaping/physical structure |
Evolved stars: Shaping/physical structure |
Exo-planets |
Galactic centres/nuclei |
Galaxy Clusters |
Galaxy chemistry |
Galaxy groups and clusters |
Galaxy structure & evolution |
Gamma Ray Bursts (GRB) |
Giant Molecular Clouds (GMC) properties |
Gravitational lenses |
HII regions |
High-mass star formation |
High-z Active Galactic Nuclei (AGN) |
Hypergiants |
Infra-Red Dark Clouds (IRDC) |
Inter-Stellar Medium (ISM)/Molecular clouds |
Intermediate-mass star formation |
Low-mass star formation |
Luminous Blue Variables (LBV) |
Luminous and Ultra-Luminous Infra-Red Galaxies (LIRG & ULIRG) |
Lyman Alpha Emitters/Blobs (LAE/LAB) |
Lyman Break Galaxies (LBG) |
Magellanic Clouds |
Main sequence stars |
Merging and interacting galaxies |
Outflows, jets, feedback |
Outflows, jets and ionized winds |
Photon-Dominated Regions (PDR)/X-Ray Dominated Regions (XDR) |
Post-AGB stars |
Pre-stellar cores |
Pulsars and neutron stars |
Solar system - Asteroids |
Solar system - Comets |
Solar system - Planetary atmospheres |
Solar system - Planetary surfaces |
Solar system - Trans-Neptunian Objects (TNOs) |
Spiral galaxies |
Starburst galaxies |
Starbursts, star formation |
Sub-mm Galaxies (SMG) |
Supernovae (SN) ejecta |
Surveys of galaxies |
The Sun |
Transients |
White dwarfs |
myquery = alminer.keysearch({'target_name': ['GRB021004','SPT0319-47', 'G345']})
================================ alminer.keysearch results ================================ -------------------------------- Number of projects = 16 Number of observations = 28 Number of unique subbands = 121 Total number of subbands = 179 10 target(s) with ALMA data = ['GRB021004', 'G345.5', 'SPT0319-47', 'G345.5043+00.3480', 'G345.49+1.47', 'G345.50+0.35', 'G345.6487+0.0089', 'G345.01', 'G345.11', 'G345.0029-0.2241'] --------------------------------
myquery = alminer.keysearch({'proposal_id': ['2015.1.00664.S', '2016.1.00204.S']})
================================ alminer.keysearch results ================================ -------------------------------- Number of projects = 2 Number of observations = 16 Number of unique subbands = 16 Total number of subbands = 64 16 target(s) with ALMA data = ['KMOS3DGS4-27882', 'KMOS3DCOS4-24763', 'KMOS3DU4-34138', 'KMOS3DCOS4-19680', 'KMOS3DCOS4-13701', 'KMOS3DCOS4-10347', 'KMOS3DCOS4-13174', 'KMOS3DCOS4-15820', 'KMOS3DCOS4-15813', 'KMOS3DU4-22227', 'KMOS3DU4-20547', 'KMOS3DU4-32147', 'KMOS3DGS4-24110', 'KMOS3DGS4-11016', 'KMOS3DGS4-25151', 'AK_Sco'] --------------------------------
Query the ALMA archive for proposals that have the words 'high-mass' AND 'star' AND 'formation' AND 'outflow', and do not print the long list of target names in the summary.
myquery = alminer.keysearch({'proposal_abstract': ['high-mass star formation outflow']}, print_targets=False)
================================ alminer.keysearch results ================================ -------------------------------- Number of projects = 34 Number of observations = 419 Number of unique subbands = 416 Total number of subbands = 2799 Total number of targets with ALMA data = 239 --------------------------------
Query the ALMA archive for proposals that have the words ('high-mass' AND 'star' AND 'formation' AND 'outflow') OR ('massive' AND 'star' AND 'formation') corresponding to the scientific category of 'Galaxy evolution'.
myquery = alminer.keysearch({'proposal_abstract': ['high-mass star formation', 'massive star formation'],
'scientific_category':['Galaxy evolution']}, print_targets=False)
================================ alminer.keysearch results ================================ -------------------------------- Number of projects = 119 Number of observations = 2056 Number of unique subbands = 2481 Total number of subbands = 8247 Total number of targets with ALMA data = 1376 --------------------------------
myquery = alminer.keysearch({'science_keyword':['disks around low-mass stars'],
'pol_states':['XY', 'YX']}, print_targets=False)
================================ alminer.keysearch results ================================ -------------------------------- Number of projects = 27 Number of observations = 48 Number of unique subbands = 94 Total number of subbands = 192 Total number of targets with ALMA data = 34 --------------------------------
The querying functions presented in the previous section return a PANDAS DataFrame that can be used to further narrow down your search. This section presents some examples of how you can further filter and explore the results of your queries:
To explore these options, we will first query the archive using one of the methods presented in the previous section and use the results in the remainder of this tutorial.
observations = alminer.keysearch({'science_keyword':['Galaxy chemistry']}, print_targets=False)
================================ alminer.keysearch results ================================ -------------------------------- Number of projects = 47 Number of observations = 339 Number of unique subbands = 1162 Total number of subbands = 1361 Total number of targets with ALMA data = 63 --------------------------------
You can simply display the DataFrame table returned by the query functions using the name you gave it (in this case observations), but often there are limits to how many rows and columns are presented. With the alminer.explore
function, you can control whether or not you want to display all rows (allrows=True/False) and/or all columns (allcols=True/False). By default, only the 18 most useful columns are shown and the number of rows is truncated.
explore
functionalminer.explore(observations)
Obs | project_code | ALMA_source_name | RAJ2000 | DEJ2000 | ang_res_arcsec | min_freq_GHz | max_freq_GHz | central_freq_GHz | bandwidth_GHz | freq_res_kHz | vel_res_kms | LAS_arcsec | FoV_arcsec | cont_sens_bandwidth | line_sens_10kms | line_sens_native | MOUS_id | |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
0 | 1 | 2011.0.00268.S | LESS J0332-2756 | 53.122042 | -27.938694 | 1.167 | 239.50 | 241.37 | 240.43 | 1.875 | 976.56 | 1.213 | 8.943 | 23.564 | 79.299 | 1708.54 | 111.94 | uid://A002/X303d22/X7b |
1 | 2 | 2011.0.00268.S | LESS J0332-2756 | 53.122042 | -27.938694 | 1.167 | 252.85 | 254.73 | 253.79 | 1.875 | 976.56 | 1.149 | 8.943 | 23.564 | 79.299 | 1675.07 | 112.74 | uid://A002/X303d22/X7b |
2 | 3 | 2011.0.00405.S | PKS1830-211 | 278.416330 | -21.061080 | 1.331 | 105.07 | 106.95 | 106.01 | 1.878 | 976.56 | 2.737 | 12.937 | 58.774 | 29.824 | 1370.09 | 59.71 | uid://A002/X36d874/X80 |
3 | 4 | 2011.0.00405.S | PKS1830-211 | 278.416330 | -21.061080 | 0.455 | 283.51 | 285.39 | 284.45 | 1.874 | 976.56 | 1.026 | 3.448 | 20.113 | 60.429 | 1673.64 | 119.28 | uid://A002/X36d874/X7a |
4 | 5 | 2011.0.00405.S | PKS1830-211 | 278.416330 | -21.061080 | 0.455 | 281.64 | 283.51 | 282.57 | 1.874 | 976.56 | 1.033 | 3.448 | 20.113 | 60.429 | 1677.23 | 119.14 | uid://A002/X36d874/X7a |
5 | 6 | 2011.0.00405.S | PKS1830-211 | 278.416330 | -21.061080 | 1.331 | 103.20 | 105.08 | 104.14 | 1.878 | 976.56 | 2.786 | 12.937 | 58.774 | 29.824 | 1381.77 | 59.69 | uid://A002/X36d874/X80 |
6 | 7 | 2011.0.00405.S | PKS1830-211 | 278.416330 | -21.061080 | 0.563 | 259.58 | 261.47 | 260.52 | 1.894 | 976.56 | 1.120 | 5.088 | 23.118 | 74.597 | 2278.21 | 154.60 | uid://A002/X36d874/X7c |
7 | 8 | 2011.0.00405.S | PKS1830-211 | 278.416330 | -21.061080 | 0.442 | 292.55 | 294.43 | 293.49 | 1.880 | 976.56 | 0.994 | 4.104 | 19.504 | 68.197 | 1867.41 | 134.98 | uid://A002/X36d874/X7e |
8 | 9 | 2011.0.00405.S | PKS1830-211 | 278.416330 | -21.061080 | 1.331 | 91.20 | 93.08 | 92.14 | 1.878 | 976.56 | 3.145 | 12.937 | 58.774 | 29.824 | 1500.60 | 61.02 | uid://A002/X36d874/X80 |
9 | 10 | 2011.0.00405.S | PKS1830-211 | 278.416330 | -21.061080 | 0.563 | 256.63 | 258.53 | 257.58 | 1.894 | 976.56 | 1.132 | 5.088 | 23.118 | 74.597 | 2189.73 | 147.77 | uid://A002/X36d874/X7c |
10 | 11 | 2011.0.00405.S | PKS1830-211 | 278.416330 | -21.061080 | 0.563 | 244.13 | 246.02 | 245.08 | 1.893 | 976.56 | 1.190 | 5.088 | 23.118 | 74.597 | 2229.45 | 146.80 | uid://A002/X36d874/X7c |
11 | 12 | 2011.0.00405.S | PKS1830-211 | 278.416330 | -21.061080 | 0.455 | 295.51 | 297.38 | 296.45 | 1.874 | 976.56 | 0.984 | 3.448 | 20.113 | 60.429 | 1735.78 | 126.28 | uid://A002/X36d874/X7a |
12 | 13 | 2011.0.00405.S | PKS1830-211 | 278.416330 | -21.061080 | 0.455 | 293.63 | 295.51 | 294.57 | 1.874 | 976.56 | 0.991 | 3.448 | 20.113 | 60.429 | 1655.25 | 120.04 | uid://A002/X36d874/X7a |
13 | 14 | 2011.0.00405.S | PKS1830-211 | 278.416330 | -21.061080 | 0.563 | 242.31 | 244.20 | 243.25 | 1.894 | 976.56 | 1.199 | 5.088 | 23.118 | 74.597 | 2229.83 | 146.24 | uid://A002/X36d874/X7c |
14 | 15 | 2011.0.00405.S | PKS1830-211 | 278.416330 | -21.061080 | 0.442 | 304.55 | 306.43 | 305.49 | 1.880 | 976.56 | 0.955 | 4.104 | 19.504 | 68.197 | 1868.50 | 137.78 | uid://A002/X36d874/X7e |
15 | 16 | 2011.0.00405.S | PKS1830-211 | 278.416330 | -21.061080 | 1.331 | 93.07 | 94.95 | 94.01 | 1.878 | 976.56 | 3.083 | 12.937 | 58.774 | 29.824 | 1440.54 | 59.16 | uid://A002/X36d874/X80 |
16 | 17 | 2011.0.00405.S | PKS1830-211 | 278.416330 | -21.061080 | 0.442 | 290.68 | 292.56 | 291.62 | 1.880 | 976.56 | 1.001 | 4.104 | 19.504 | 68.197 | 1903.65 | 137.16 | uid://A002/X36d874/X7e |
17 | 18 | 2011.0.00405.S | PKS1830-211 | 278.416330 | -21.061080 | 0.442 | 302.68 | 304.56 | 303.62 | 1.880 | 976.56 | 0.961 | 4.104 | 19.504 | 68.197 | 1848.24 | 135.87 | uid://A002/X36d874/X7e |
18 | 19 | 2011.0.00820.S | ngc4418 | 186.727617 | -0.877642 | 0.665 | 261.72 | 263.60 | 262.66 | 1.874 | 976.56 | 1.111 | 8.262 | 22.748 | 191.363 | 5507.00 | 377.20 | uid://A002/X314ea1/X1fa |
19 | 20 | 2011.0.00820.S | ngc4418 | 186.727617 | -0.877642 | 1.355 | 97.88 | 99.75 | 98.82 | 1.875 | 976.56 | 2.935 | 9.305 | 63.355 | 60.616 | 2862.27 | 120.59 | uid://A002/X327408/X100 |
20 | 21 | 2011.0.00820.S | ngc4418 | 186.727617 | -0.877642 | 0.657 | 251.60 | 253.47 | 252.54 | 1.874 | 976.56 | 1.155 | 8.158 | 22.463 | 184.788 | 5492.90 | 368.94 | uid://A002/X314ea1/X1ee |
21 | 22 | 2011.0.00820.S | ngc4418 | 186.727617 | -0.877642 | 0.657 | 266.60 | 268.47 | 267.53 | 1.874 | 976.56 | 1.090 | 8.158 | 22.463 | 184.788 | 5382.61 | 372.08 | uid://A002/X314ea1/X1ee |
22 | 23 | 2011.0.00820.S | ngc4418 | 186.727617 | -0.877642 | 0.657 | 249.97 | 251.85 | 250.91 | 1.874 | 976.56 | 1.162 | 8.158 | 22.463 | 184.788 | 5505.70 | 368.62 | uid://A002/X314ea1/X1ee |
23 | 24 | 2011.0.00820.S | ngc4418 | 186.727617 | -0.877642 | 0.657 | 264.97 | 266.85 | 265.91 | 1.874 | 976.56 | 1.097 | 8.158 | 22.463 | 184.788 | 5393.90 | 371.73 | uid://A002/X314ea1/X1ee |
24 | 25 | 2011.0.00820.S | ngc4418 | 186.727617 | -0.877642 | 0.665 | 246.72 | 248.60 | 247.66 | 1.874 | 976.56 | 1.178 | 8.262 | 22.748 | 191.363 | 5623.83 | 374.09 | uid://A002/X314ea1/X1fa |
25 | 26 | 2011.0.00820.S | ngc4418 | 186.727617 | -0.877642 | 0.665 | 248.35 | 250.22 | 249.29 | 1.874 | 976.56 | 1.170 | 8.262 | 22.748 | 191.363 | 5610.45 | 374.41 | uid://A002/X314ea1/X1fa |
... | ... | ... | ... | ... | ... | ... | ... | ... | ... | ... | ... | ... | ... | ... | ... | ... | ... | ... |
1335 | 1336 | 2018.1.01395.S | NGC_253 | 11.888058 | -25.288800 | 0.019 | 217.98 | 219.85 | 218.91 | 1.874 | 1128.91 | 1.539 | 0.500 | 25.549 | 12.404 | 398.35 | 24.92 | uid://A001/X133d/X3025 |
1336 | 1337 | 2018.1.01395.S | NGC_253 | 11.888058 | -25.288800 | 0.019 | 235.98 | 237.85 | 236.91 | 1.874 | 1128.91 | 1.434 | 0.500 | 25.549 | 12.404 | 382.31 | 24.78 | uid://A001/X133d/X3025 |
1337 | 1338 | 2019.1.00130.S | NGC4418 | 186.727617 | -0.877642 | 1.357 | 108.29 | 110.16 | 109.23 | 1.873 | 1938.48 | 5.366 | 24.940 | 55.903 | 10.485 | 468.79 | 20.59 | uid://A001/X1465/X389c |
1338 | 1339 | 2019.1.00130.S | NGC4945 | 196.363663 | -49.467900 | 2.523 | 91.70 | 93.57 | 92.63 | 1.873 | 1938.48 | 6.210 | 27.132 | 59.612 | 10.282 | 508.68 | 20.77 | uid://A001/X1465/X3888 |
1339 | 1340 | 2019.1.00130.S | NGC4418 | 186.727617 | -0.877642 | 1.357 | 97.97 | 99.84 | 98.90 | 1.873 | 1938.48 | 5.820 | 24.940 | 55.903 | 10.485 | 507.47 | 21.40 | uid://A001/X1465/X389c |
1340 | 1341 | 2019.1.00130.S | NGC4418 | 186.727617 | -0.877642 | 1.357 | 96.28 | 98.15 | 97.21 | 1.873 | 1938.48 | 5.920 | 24.940 | 55.903 | 10.485 | 511.67 | 21.39 | uid://A001/X1465/X389c |
1341 | 1342 | 2019.1.00130.S | NGC4945 | 196.363663 | -49.467900 | 2.309 | 108.87 | 110.74 | 109.80 | 1.873 | 1938.48 | 5.338 | 22.321 | 55.608 | 18.936 | 799.25 | 35.19 | uid://A001/X1465/X388c |
1342 | 1343 | 2019.1.00130.S | NGC4945 | 196.363663 | -49.467900 | 2.309 | 110.76 | 112.63 | 111.69 | 1.873 | 1938.48 | 5.247 | 22.321 | 55.608 | 18.936 | 792.83 | 35.21 | uid://A001/X1465/X388c |
1343 | 1344 | 2019.1.00130.S | NGC4945 | 196.363663 | -49.467900 | 2.309 | 98.49 | 100.36 | 99.42 | 1.873 | 1938.48 | 5.791 | 22.321 | 55.608 | 18.936 | 976.30 | 41.27 | uid://A001/X1465/X388c |
1344 | 1345 | 2019.1.00130.S | NGC4945 | 196.363663 | -49.467900 | 2.309 | 96.80 | 98.67 | 97.73 | 1.873 | 1938.48 | 5.890 | 22.321 | 55.608 | 18.936 | 984.33 | 41.26 | uid://A001/X1465/X388c |
1345 | 1346 | 2019.1.00130.S | NGC1068 | 40.669879 | -0.013289 | 1.609 | 103.38 | 105.26 | 104.32 | 1.873 | 1938.48 | 5.621 | 20.838 | 59.730 | 9.858 | 461.89 | 19.82 | uid://A001/X1465/X3890 |
1346 | 1347 | 2019.1.00130.S | NGC1068 | 40.669879 | -0.013289 | 1.609 | 101.58 | 103.45 | 102.51 | 1.873 | 1938.48 | 5.721 | 20.838 | 59.730 | 9.858 | 459.66 | 19.55 | uid://A001/X1465/X3890 |
1347 | 1348 | 2019.1.00130.S | NGC1068 | 40.669879 | -0.013289 | 1.609 | 91.51 | 93.39 | 92.45 | 1.873 | 1938.48 | 6.223 | 20.838 | 59.730 | 9.858 | 480.47 | 19.59 | uid://A001/X1465/X3890 |
1348 | 1349 | 2019.1.00130.S | NGC1068 | 40.669879 | -0.013289 | 1.609 | 89.72 | 91.59 | 90.65 | 1.873 | 1938.48 | 6.345 | 20.838 | 59.730 | 9.858 | 494.60 | 19.97 | uid://A001/X1465/X3890 |
1349 | 1350 | 2019.1.00130.S | NGC4418 | 186.727617 | -0.877642 | 2.537 | 89.43 | 91.30 | 90.36 | 1.873 | 1938.48 | 6.364 | 27.048 | 59.922 | 9.343 | 466.81 | 18.82 | uid://A001/X1465/X3898 |
1350 | 1351 | 2019.1.00130.S | NGC4945 | 196.363663 | -49.467900 | 2.523 | 101.78 | 103.65 | 102.72 | 1.873 | 1938.48 | 5.710 | 27.132 | 59.612 | 10.282 | 475.79 | 20.26 | uid://A001/X1465/X3888 |
1351 | 1352 | 2019.1.00130.S | NGC1068 | 40.669879 | -0.013289 | 2.247 | 108.65 | 110.52 | 109.59 | 1.873 | 1938.48 | 5.349 | 21.118 | 55.719 | 21.996 | 960.67 | 42.25 | uid://A001/X1465/X3894 |
1352 | 1353 | 2019.1.00130.S | NGC1068 | 40.669879 | -0.013289 | 2.247 | 110.54 | 112.42 | 111.48 | 1.873 | 1938.48 | 5.257 | 21.118 | 55.719 | 21.996 | 1131.63 | 50.21 | uid://A001/X1465/X3894 |
1353 | 1354 | 2019.1.00130.S | NGC1068 | 40.669879 | -0.013289 | 2.247 | 98.29 | 100.16 | 99.23 | 1.873 | 1938.48 | 5.802 | 21.118 | 55.719 | 21.996 | 1007.18 | 42.54 | uid://A001/X1465/X3894 |
1354 | 1355 | 2019.1.00130.S | NGC4418 | 186.727617 | -0.877642 | 2.537 | 103.05 | 104.92 | 103.99 | 1.873 | 1938.48 | 5.639 | 27.048 | 59.922 | 9.343 | 436.95 | 18.72 | uid://A001/X1465/X3898 |
1355 | 1356 | 2019.1.00130.S | NGC4418 | 186.727617 | -0.877642 | 2.537 | 91.20 | 93.07 | 92.13 | 1.873 | 1938.48 | 6.243 | 27.048 | 59.922 | 9.343 | 459.55 | 18.71 | uid://A001/X1465/X3898 |
1356 | 1357 | 2019.1.00130.S | NGC4418 | 186.727617 | -0.877642 | 2.537 | 101.24 | 103.11 | 102.18 | 1.873 | 1938.48 | 5.740 | 27.048 | 59.922 | 9.343 | 437.00 | 18.56 | uid://A001/X1465/X3898 |
1357 | 1358 | 2019.1.00130.S | NGC1068 | 40.669879 | -0.013289 | 2.247 | 96.60 | 98.47 | 97.53 | 1.873 | 1938.48 | 5.902 | 21.118 | 55.719 | 21.996 | 1015.52 | 42.52 | uid://A001/X1465/X3894 |
1358 | 1359 | 2019.1.00130.S | NGC4945 | 196.363663 | -49.467900 | 2.523 | 103.59 | 105.46 | 104.52 | 1.873 | 1938.48 | 5.610 | 27.132 | 59.612 | 10.282 | 478.30 | 20.54 | uid://A001/X1465/X3888 |
1359 | 1360 | 2019.1.00130.S | NGC4945 | 196.363663 | -49.467900 | 2.523 | 89.90 | 91.77 | 90.84 | 1.873 | 1938.48 | 6.332 | 27.132 | 59.612 | 10.282 | 513.50 | 20.76 | uid://A001/X1465/X3888 |
1360 | 1361 | 2019.1.00130.S | NGC4418 | 186.727617 | -0.877642 | 1.357 | 110.17 | 112.05 | 111.11 | 1.873 | 1938.48 | 5.274 | 24.940 | 55.903 | 10.485 | 465.01 | 20.60 | uid://A001/X1465/X389c |
1361 rows × 18 columns
alminer.explore(observations, allcols=True, allrows=False)
# you can also set allrows=True to see all rows in the table but this may be slow for very large queries
Obs | project_code | ALMA_source_name | RAJ2000 | DEJ2000 | ang_res_arcsec | min_freq_GHz | max_freq_GHz | central_freq_GHz | bandwidth_GHz | freq_res_kHz | vel_res_kms | LAS_arcsec | FoV_arcsec | cont_sens_bandwidth | line_sens_10kms | line_sens_native | MOUS_id | access_url | access_format | proposal_id | data_rights | gal_longitude | gal_latitude | obs_publisher_did | obs_collection | facility_name | instrument_name | obs_id | dataproduct_type | calib_level | target_name | s_ra | s_dec | s_fov | s_region | s_resolution | t_min | t_max | t_exptime | t_resolution | em_min | em_max | em_res_power | pol_states | o_ucd | band_list | em_resolution | authors | pub_abstract | publication_year | proposal_abstract | schedblock_name | proposal_authors | sensitivity_10kms | cont_sensitivity_bandwidth | pwv | group_ous_uid | member_ous_uid | asdm_uid | obs_title | type | scan_intent | science_observation | spatial_scale_max | bandwidth | antenna_arrays | is_mosaic | obs_release_date | spatial_resolution | frequency_support | frequency | velocity_resolution | obs_creator_name | pub_title | first_author | qa2_passed | bib_reference | science_keyword | scientific_category | lastModified | |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
0 | 1 | 2011.0.00268.S | LESS J0332-2756 | 53.122042 | -27.938694 | 1.167 | 239.50 | 241.37 | 240.43 | 1.875 | 976.56 | 1.213 | 8.943 | 23.564 | 79.299 | 1708.54 | 111.94 | uid://A002/X303d22/X7b | http://almascience.org/aq?member_ous_id=uid://... | text/html | 2011.0.00268.S | Public | 223.796062 | -54.451922 | ADS/JAO.ALMA#2011.0.00268.S | ALMA | JAO | ALMA | uid://A002/X303d22/X7b | cube | 2 | LESS J0332-2756 | 53.122042 | -27.938694 | 0.006546 | Circle ICRS 53.122042 -27.938694 0.003273 | 1.167248 | 55936.913188 | 55939.193372 | 4536.000 | 4536.000 | 0.001242 | 0.001252 | 247134.408560 | /XX/YY/ | phot.flux.density;phys.polarization | 6 | 2.928016e+14 | Leon, S.; Cortes, P.C.; Guerard, M.; Villard, ... | Aims: We aim at analyzing the (sub-)millimeter... | 2012 | Metallicity of galaxies and its redshift evolu... | LESS J0332-2756 | De Breuck, Carlos; Hatsukade, Bunyo; Maiolino,... | 1.708538 | 0.079299 | 1.422843 | uid://A002/X303d22/X7b | uid://A002/X36a70f/X318 | Metallicity of a Submillimeter Galaxy at z=5 | S | TARGET WVR | T | 8.943092 | 1.875000e+09 | A002:PM02 A004:DV04 A009:DA43 A011:DV12 A013:D... | F | 2013-02-09T01:45:00.000 | 1.167248 | [239.50..241.37GHz,976.56kHz,1.7mJy/beam@10km/... | 247.112856 | 1149.468553 | Nagao, Tohru | ALMA reveals a chemically evolved submillimete... | Leon, S. Nagao, T. Ono, Yoshiaki | T | 2012A&A...542L..34N 2014ApJ...795....5O 2016A&... | Galaxy structure & evolution, Galaxy chemistry | Galaxy evolution | 2021-06-16T16:46:50.431 | |
1 | 2 | 2011.0.00268.S | LESS J0332-2756 | 53.122042 | -27.938694 | 1.167 | 252.85 | 254.73 | 253.79 | 1.875 | 976.56 | 1.149 | 8.943 | 23.564 | 79.299 | 1675.07 | 112.74 | uid://A002/X303d22/X7b | http://almascience.org/aq?member_ous_id=uid://... | text/html | 2011.0.00268.S | Public | 223.796062 | -54.451922 | ADS/JAO.ALMA#2011.0.00268.S | ALMA | JAO | ALMA | uid://A002/X303d22/X7b | cube | 2 | LESS J0332-2756 | 53.122042 | -27.938694 | 0.006546 | Circle ICRS 53.122042 -27.938694 0.003273 | 1.167248 | 55936.913188 | 55939.193372 | 4536.000 | 4536.000 | 0.001177 | 0.001186 | 260809.621360 | /XX/YY/ | phot.flux.density;phys.polarization | 6 | 2.928016e+14 | Leon, S.; Cortes, P.C.; Guerard, M.; Villard, ... | Aims: We aim at analyzing the (sub-)millimeter... | 2012 | Metallicity of galaxies and its redshift evolu... | LESS J0332-2756 | De Breuck, Carlos; Hatsukade, Bunyo; Maiolino,... | 1.675071 | 0.079299 | 1.422843 | uid://A002/X303d22/X7b | uid://A002/X36a70f/X318 | Metallicity of a Submillimeter Galaxy at z=5 | S | TARGET WVR | T | 8.943092 | 1.875000e+09 | A002:PM02 A004:DV04 A009:DA43 A011:DV12 A013:D... | F | 2013-02-09T01:45:00.000 | 1.167248 | [239.50..241.37GHz,976.56kHz,1.7mJy/beam@10km/... | 247.112856 | 1149.468553 | Nagao, Tohru | ALMA reveals a chemically evolved submillimete... | Leon, S. Nagao, T. Ono, Yoshiaki | T | 2012A&A...542L..34N 2014ApJ...795....5O 2016A&... | Galaxy structure & evolution, Galaxy chemistry | Galaxy evolution | 2021-06-16T16:46:50.431 | |
2 | 3 | 2011.0.00405.S | PKS1830-211 | 278.416330 | -21.061080 | 1.331 | 105.07 | 106.95 | 106.01 | 1.878 | 976.56 | 2.737 | 12.937 | 58.774 | 29.824 | 1370.09 | 59.71 | uid://A002/X36d874/X80 | http://almascience.org/aq?member_ous_id=uid://... | text/html | 2011.0.00405.S | Public | 12.165817 | -5.711677 | ADS/JAO.ALMA#2011.0.00405.S | ALMA | JAO | ALMA | uid://A002/X36d874/X80 | cube | 2 | PKS1830-211 | 278.416330 | -21.061080 | 0.016326 | Circle ICRS 278.416330 -21.061080 0.008163 | 1.331051 | 56069.374548 | 56093.397660 | 3719.520 | 3719.520 | 0.002803 | 0.002853 | 109524.742000 | /XX/YY/ | phot.flux.density;phys.polarization | 3 | 2.927369e+14 | Bagdonaite, J.; Daprà, M.; Jansen, P.; Bethlem... | A limit on a possible cosmological variation o... | 2013 | The z=0.89 (sub)mm molecular absorber toward t... | PKS1830_HCOplus_b3_run_x3 | Bethlem, Hendrick; Gerin, Maryvonne; Bottinell... | 1.370093 | 0.029824 | 0.923567 | uid://A002/X36d874/X80 | uid://A002/X411025/X441 | A survey of strong absorption lines at z=0.89 ... | S | TARGET | T | 12.936728 | 1.875000e+09 | A003:DA41 A004:DV04 A008:DV19 A011:DV12 A021:D... | F | 2013-10-10T14:47:51.000 | 1.331051 | [91.20..93.08GHz,976.56kHz,1.5mJy/beam@10km/s,... | 99.075504 | 2737.212182 | Muller, Sebastien | A strong magnetic field in the jet base of a s... | Bagdonaite, J. Martí-Vidal, I. Martí-Vidal, Iv... | T | 2013A&A...558A.123M 2013PhRvL.111w1101B 2014A&... | Galaxy structure & evolution, Galaxy chemistry | Galaxy evolution | 2021-06-16T16:46:50.431 | |
3 | 4 | 2011.0.00405.S | PKS1830-211 | 278.416330 | -21.061080 | 0.455 | 283.51 | 285.39 | 284.45 | 1.874 | 976.56 | 1.026 | 3.448 | 20.113 | 60.429 | 1673.64 | 119.28 | uid://A002/X36d874/X7a | http://almascience.org/aq?member_ous_id=uid://... | text/html | 2011.0.00405.S | Public | 12.165817 | -5.711677 | ADS/JAO.ALMA#2011.0.00405.S | ALMA | JAO | ALMA | uid://A002/X36d874/X7a | cube | 2 | PKS1830-211 | 278.416330 | -21.061080 | 0.005587 | Circle ICRS 278.416330 -21.061080 0.002793 | 0.454758 | 56028.238332 | 56028.363572 | 3144.960 | 3144.960 | 0.001050 | 0.001057 | 292274.950000 | /XX/YY/ | phot.flux.density;phys.polarization | 7 | 2.927253e+14 | Bagdonaite, J.; Daprà, M.; Jansen, P.; Bethlem... | A limit on a possible cosmological variation o... | 2013 | The z=0.89 (sub)mm molecular absorber toward t... | PKS1830_CH_and_H2O_b7_run_x2 | Bethlem, Hendrick; Gerin, Maryvonne; Bottinell... | 1.673643 | 0.060429 | 0.703871 | uid://A002/X36d874/X7a | uid://A002/X3cb0a0/X9e8 | A survey of strong absorption lines at z=0.89 ... | S | TARGET | T | 3.448268 | 1.875000e+09 | A003:DA41 A011:DV12 A025:DV14 A037:PM01 A045:D... | F | 2013-05-22T07:31:59.000 | 0.454758 | [281.64..283.51GHz,976.56kHz,1.7mJy/beam@10km/... | 289.509775 | 984.336598 | Muller, Sebastien | A strong magnetic field in the jet base of a s... | Bagdonaite, J. Martí-Vidal, I. Martí-Vidal, Iv... | T | 2013A&A...558A.123M 2013PhRvL.111w1101B 2014A&... | Galaxy structure & evolution, Galaxy chemistry | Galaxy evolution | 2021-06-16T16:46:50.431 | |
4 | 5 | 2011.0.00405.S | PKS1830-211 | 278.416330 | -21.061080 | 0.455 | 281.64 | 283.51 | 282.57 | 1.874 | 976.56 | 1.033 | 3.448 | 20.113 | 60.429 | 1677.23 | 119.14 | uid://A002/X36d874/X7a | http://almascience.org/aq?member_ous_id=uid://... | text/html | 2011.0.00405.S | Public | 12.165817 | -5.711677 | ADS/JAO.ALMA#2011.0.00405.S | ALMA | JAO | ALMA | uid://A002/X36d874/X7a | cube | 2 | PKS1830-211 | 278.416330 | -21.061080 | 0.005587 | Circle ICRS 278.416330 -21.061080 0.002793 | 0.454758 | 56028.238332 | 56028.363572 | 3144.960 | 3144.960 | 0.001057 | 0.001064 | 290354.950000 | /XX/YY/ | phot.flux.density;phys.polarization | 7 | 2.927253e+14 | Bagdonaite, J.; Daprà, M.; Jansen, P.; Bethlem... | A limit on a possible cosmological variation o... | 2013 | The z=0.89 (sub)mm molecular absorber toward t... | PKS1830_CH_and_H2O_b7_run_x2 | Bethlem, Hendrick; Gerin, Maryvonne; Bottinell... | 1.677226 | 0.060429 | 0.703871 | uid://A002/X36d874/X7a | uid://A002/X3cb0a0/X9e8 | A survey of strong absorption lines at z=0.89 ... | S | TARGET | T | 3.448268 | 1.875000e+09 | A003:DA41 A011:DV12 A025:DV14 A037:PM01 A045:D... | F | 2013-05-22T07:31:59.000 | 0.454758 | [281.64..283.51GHz,976.56kHz,1.7mJy/beam@10km/... | 289.509775 | 984.336598 | Muller, Sebastien | A strong magnetic field in the jet base of a s... | Bagdonaite, J. Martí-Vidal, I. Martí-Vidal, Iv... | T | 2013A&A...558A.123M 2013PhRvL.111w1101B 2014A&... | Galaxy structure & evolution, Galaxy chemistry | Galaxy evolution | 2021-06-16T16:46:50.431 | |
5 | 6 | 2011.0.00405.S | PKS1830-211 | 278.416330 | -21.061080 | 1.331 | 103.20 | 105.08 | 104.14 | 1.878 | 976.56 | 2.786 | 12.937 | 58.774 | 29.824 | 1381.77 | 59.69 | uid://A002/X36d874/X80 | http://almascience.org/aq?member_ous_id=uid://... | text/html | 2011.0.00405.S | Public | 12.165817 | -5.711677 | ADS/JAO.ALMA#2011.0.00405.S | ALMA | JAO | ALMA | uid://A002/X36d874/X80 | cube | 2 | PKS1830-211 | 278.416330 | -21.061080 | 0.016326 | Circle ICRS 278.416330 -21.061080 0.008163 | 1.331051 | 56069.374548 | 56093.397660 | 3719.520 | 3719.520 | 0.002853 | 0.002905 | 107605.766000 | /XX/YY/ | phot.flux.density;phys.polarization | 3 | 2.927369e+14 | Bagdonaite, J.; Daprà, M.; Jansen, P.; Bethlem... | A limit on a possible cosmological variation o... | 2013 | The z=0.89 (sub)mm molecular absorber toward t... | PKS1830_HCOplus_b3_run_x3 | Bethlem, Hendrick; Gerin, Maryvonne; Bottinell... | 1.381767 | 0.029824 | 0.923567 | uid://A002/X36d874/X80 | uid://A002/X411025/X441 | A survey of strong absorption lines at z=0.89 ... | S | TARGET | T | 12.936728 | 1.875000e+09 | A003:DA41 A004:DV04 A008:DV19 A011:DV12 A021:D... | F | 2013-10-10T14:47:51.000 | 1.331051 | [91.20..93.08GHz,976.56kHz,1.5mJy/beam@10km/s,... | 99.075504 | 2737.212182 | Muller, Sebastien | A strong magnetic field in the jet base of a s... | Bagdonaite, J. Martí-Vidal, I. Martí-Vidal, Iv... | T | 2013A&A...558A.123M 2013PhRvL.111w1101B 2014A&... | Galaxy structure & evolution, Galaxy chemistry | Galaxy evolution | 2021-06-16T16:46:50.431 | |
6 | 7 | 2011.0.00405.S | PKS1830-211 | 278.416330 | -21.061080 | 0.563 | 259.58 | 261.47 | 260.52 | 1.894 | 976.56 | 1.120 | 5.088 | 23.118 | 74.597 | 2278.21 | 154.60 | uid://A002/X36d874/X7c | http://almascience.org/aq?member_ous_id=uid://... | text/html | 2011.0.00405.S | Public | 12.165817 | -5.711677 | ADS/JAO.ALMA#2011.0.00405.S | ALMA | JAO | ALMA | uid://A002/X36d874/X7c | cube | 2 | PKS1830-211 | 278.416330 | -21.061080 | 0.006422 | Circle ICRS 278.416330 -21.061080 0.003211 | 0.562899 | 56026.250749 | 56093.330969 | 4838.400 | 4838.400 | 0.001147 | 0.001155 | 267762.499440 | /XX/YY/ | phot.flux.density;phys.polarization | 6 | 2.927251e+14 | Bagdonaite, J.; Daprà, M.; Jansen, P.; Bethlem... | A limit on a possible cosmological variation o... | 2013 | The z=0.89 (sub)mm molecular absorber toward t... | PKS1830-211_CO4-3_b6_run_x2 | Bethlem, Hendrick; Gerin, Maryvonne; Bottinell... | 2.278214 | 0.074597 | 2.122151 | uid://A002/X36d874/X7c | uid://A002/X3ca066/Xa6f | A survey of strong absorption lines at z=0.89 ... | S | TARGET | T | 5.088294 | 1.875000e+09 | A003:DA41 A004:DV04 A008:DV19 A011:DV12 A021:D... | F | 2013-10-19T12:40:13.000 | 0.562899 | [242.31..244.20GHz,976.56kHz,2.2mJy/beam@10km/... | 251.884124 | 1119.620778 | Muller, Sebastien | A strong magnetic field in the jet base of a s... | Bagdonaite, J. Martí-Vidal, I. Martí-Vidal, Iv... | T | 2013A&A...558A.123M 2013PhRvL.111w1101B 2014A&... | Galaxy structure & evolution, Galaxy chemistry | Galaxy evolution | 2021-06-16T16:46:50.431 | |
7 | 8 | 2011.0.00405.S | PKS1830-211 | 278.416330 | -21.061080 | 0.442 | 292.55 | 294.43 | 293.49 | 1.880 | 976.56 | 0.994 | 4.104 | 19.504 | 68.197 | 1867.41 | 134.98 | uid://A002/X36d874/X7e | http://almascience.org/aq?member_ous_id=uid://... | text/html | 2011.0.00405.S | Public | 12.165817 | -5.711677 | ADS/JAO.ALMA#2011.0.00405.S | ALMA | JAO | ALMA | uid://A002/X36d874/X7e | cube | 2 | PKS1830-211 | 278.416330 | -21.061080 | 0.005418 | Circle ICRS 278.416330 -21.061080 0.002709 | 0.441708 | 56070.225109 | 56082.381661 | 6048.000 | 6048.000 | 0.001018 | 0.001025 | 301521.659760 | /XX/YY/ | phot.flux.density;phys.polarization | 7 | 2.927369e+14 | Bagdonaite, J.; Daprà, M.; Jansen, P.; Bethlem... | A limit on a possible cosmological variation o... | 2013 | The z=0.89 (sub)mm molecular absorber toward t... | PKS1830_CO5-4_b7_run_x3 | Bethlem, Hendrick; Gerin, Maryvonne; Bottinell... | 1.867413 | 0.068197 | 1.027013 | uid://A002/X36d874/X7e | uid://A002/X4122f3/X133 | A survey of strong absorption lines at z=0.89 ... | S | TARGET | T | 4.104185 | 1.875000e+09 | A003:DA41 A004:DV04 A011:DV12 A021:DV08 A025:D... | F | 2013-07-05T11:49:39.000 | 0.441708 | [290.68..292.56GHz,976.56kHz,1.9mJy/beam@10km/... | 298.550728 | 955.332153 | Muller, Sebastien | A strong magnetic field in the jet base of a s... | Bagdonaite, J. Martí-Vidal, I. Martí-Vidal, Iv... | T | 2013A&A...558A.123M 2013PhRvL.111w1101B 2014A&... | Galaxy structure & evolution, Galaxy chemistry | Galaxy evolution | 2021-06-16T16:46:50.431 | |
8 | 9 | 2011.0.00405.S | PKS1830-211 | 278.416330 | -21.061080 | 1.331 | 91.20 | 93.08 | 92.14 | 1.878 | 976.56 | 3.145 | 12.937 | 58.774 | 29.824 | 1500.60 | 61.02 | uid://A002/X36d874/X80 | http://almascience.org/aq?member_ous_id=uid://... | text/html | 2011.0.00405.S | Public | 12.165817 | -5.711677 | ADS/JAO.ALMA#2011.0.00405.S | ALMA | JAO | ALMA | uid://A002/X36d874/X80 | cube | 2 | PKS1830-211 | 278.416330 | -21.061080 | 0.016326 | Circle ICRS 278.416330 -21.061080 0.008163 | 1.331051 | 56069.374548 | 56093.397660 | 3719.520 | 3719.520 | 0.003221 | 0.003287 | 95317.766000 | /XX/YY/ | phot.flux.density;phys.polarization | 3 | 2.927369e+14 | Bagdonaite, J.; Daprà, M.; Jansen, P.; Bethlem... | A limit on a possible cosmological variation o... | 2013 | The z=0.89 (sub)mm molecular absorber toward t... | PKS1830_HCOplus_b3_run_x3 | Bethlem, Hendrick; Gerin, Maryvonne; Bottinell... | 1.500603 | 0.029824 | 0.923567 | uid://A002/X36d874/X80 | uid://A002/X411025/X441 | A survey of strong absorption lines at z=0.89 ... | S | TARGET | T | 12.936728 | 1.875000e+09 | A003:DA41 A004:DV04 A008:DV19 A011:DV12 A021:D... | F | 2013-10-10T14:47:51.000 | 1.331051 | [91.20..93.08GHz,976.56kHz,1.5mJy/beam@10km/s,... | 99.075504 | 2737.212182 | Muller, Sebastien | A strong magnetic field in the jet base of a s... | Bagdonaite, J. Martí-Vidal, I. Martí-Vidal, Iv... | T | 2013A&A...558A.123M 2013PhRvL.111w1101B 2014A&... | Galaxy structure & evolution, Galaxy chemistry | Galaxy evolution | 2021-06-16T16:46:50.431 | |
9 | 10 | 2011.0.00405.S | PKS1830-211 | 278.416330 | -21.061080 | 0.563 | 256.63 | 258.53 | 257.58 | 1.894 | 976.56 | 1.132 | 5.088 | 23.118 | 74.597 | 2189.73 | 147.77 | uid://A002/X36d874/X7c | http://almascience.org/aq?member_ous_id=uid://... | text/html | 2011.0.00405.S | Public | 12.165817 | -5.711677 | ADS/JAO.ALMA#2011.0.00405.S | ALMA | JAO | ALMA | uid://A002/X36d874/X7c | cube | 2 | PKS1830-211 | 278.416330 | -21.061080 | 0.006422 | Circle ICRS 278.416330 -21.061080 0.003211 | 0.562899 | 56026.250749 | 56093.330969 | 4838.400 | 4838.400 | 0.001160 | 0.001168 | 264749.082480 | /XX/YY/ | phot.flux.density;phys.polarization | 6 | 2.927251e+14 | Bagdonaite, J.; Daprà, M.; Jansen, P.; Bethlem... | A limit on a possible cosmological variation o... | 2013 | The z=0.89 (sub)mm molecular absorber toward t... | PKS1830-211_CO4-3_b6_run_x2 | Bethlem, Hendrick; Gerin, Maryvonne; Bottinell... | 2.189729 | 0.074597 | 2.122151 | uid://A002/X36d874/X7c | uid://A002/X3ca066/Xa6f | A survey of strong absorption lines at z=0.89 ... | S | TARGET | T | 5.088294 | 1.875000e+09 | A003:DA41 A004:DV04 A008:DV19 A011:DV12 A021:D... | F | 2013-10-19T12:40:13.000 | 0.562899 | [242.31..244.20GHz,976.56kHz,2.2mJy/beam@10km/... | 251.884124 | 1119.620778 | Muller, Sebastien | A strong magnetic field in the jet base of a s... | Bagdonaite, J. Martí-Vidal, I. Martí-Vidal, Iv... | T | 2013A&A...558A.123M 2013PhRvL.111w1101B 2014A&... | Galaxy structure & evolution, Galaxy chemistry | Galaxy evolution | 2021-06-16T16:46:50.431 | |
10 | 11 | 2011.0.00405.S | PKS1830-211 | 278.416330 | -21.061080 | 0.563 | 244.13 | 246.02 | 245.08 | 1.893 | 976.56 | 1.190 | 5.088 | 23.118 | 74.597 | 2229.45 | 146.80 | uid://A002/X36d874/X7c | http://almascience.org/aq?member_ous_id=uid://... | text/html | 2011.0.00405.S | Public | 12.165817 | -5.711677 | ADS/JAO.ALMA#2011.0.00405.S | ALMA | JAO | ALMA | uid://A002/X36d874/X7c | cube | 2 | PKS1830-211 | 278.416330 | -21.061080 | 0.006422 | Circle ICRS 278.416330 -21.061080 0.003211 | 0.562899 | 56026.250749 | 56093.330969 | 4838.400 | 4838.400 | 0.001219 | 0.001228 | 251943.624560 | /XX/YY/ | phot.flux.density;phys.polarization | 6 | 2.927251e+14 | Bagdonaite, J.; Daprà, M.; Jansen, P.; Bethlem... | A limit on a possible cosmological variation o... | 2013 | The z=0.89 (sub)mm molecular absorber toward t... | PKS1830-211_CO4-3_b6_run_x2 | Bethlem, Hendrick; Gerin, Maryvonne; Bottinell... | 2.229454 | 0.074597 | 2.122151 | uid://A002/X36d874/X7c | uid://A002/X3ca066/Xa6f | A survey of strong absorption lines at z=0.89 ... | S | TARGET | T | 5.088294 | 1.875000e+09 | A003:DA41 A004:DV04 A008:DV19 A011:DV12 A021:D... | F | 2013-10-19T12:40:13.000 | 0.562899 | [242.31..244.20GHz,976.56kHz,2.2mJy/beam@10km/... | 251.884124 | 1119.620778 | Muller, Sebastien | A strong magnetic field in the jet base of a s... | Bagdonaite, J. Martí-Vidal, I. Martí-Vidal, Iv... | T | 2013A&A...558A.123M 2013PhRvL.111w1101B 2014A&... | Galaxy structure & evolution, Galaxy chemistry | Galaxy evolution | 2021-06-16T16:46:50.431 | |
11 | 12 | 2011.0.00405.S | PKS1830-211 | 278.416330 | -21.061080 | 0.455 | 295.51 | 297.38 | 296.45 | 1.874 | 976.56 | 0.984 | 3.448 | 20.113 | 60.429 | 1735.78 | 126.28 | uid://A002/X36d874/X7a | http://almascience.org/aq?member_ous_id=uid://... | text/html | 2011.0.00405.S | Public | 12.165817 | -5.711677 | ADS/JAO.ALMA#2011.0.00405.S | ALMA | JAO | ALMA | uid://A002/X36d874/X7a | cube | 2 | PKS1830-211 | 278.416330 | -21.061080 | 0.005587 | Circle ICRS 278.416330 -21.061080 0.002793 | 0.454758 | 56028.238332 | 56028.363572 | 3144.960 | 3144.960 | 0.001008 | 0.001014 | 304562.950000 | /XX/YY/ | phot.flux.density;phys.polarization | 7 | 2.927253e+14 | Bagdonaite, J.; Daprà, M.; Jansen, P.; Bethlem... | A limit on a possible cosmological variation o... | 2013 | The z=0.89 (sub)mm molecular absorber toward t... | PKS1830_CH_and_H2O_b7_run_x2 | Bethlem, Hendrick; Gerin, Maryvonne; Bottinell... | 1.735785 | 0.060429 | 0.703871 | uid://A002/X36d874/X7a | uid://A002/X3cb0a0/X9e8 | A survey of strong absorption lines at z=0.89 ... | S | TARGET | T | 3.448268 | 1.875000e+09 | A003:DA41 A011:DV12 A025:DV14 A037:PM01 A045:D... | F | 2013-05-22T07:31:59.000 | 0.454758 | [281.64..283.51GHz,976.56kHz,1.7mJy/beam@10km/... | 289.509775 | 984.336598 | Muller, Sebastien | A strong magnetic field in the jet base of a s... | Bagdonaite, J. Martí-Vidal, I. Martí-Vidal, Iv... | T | 2013A&A...558A.123M 2013PhRvL.111w1101B 2014A&... | Galaxy structure & evolution, Galaxy chemistry | Galaxy evolution | 2021-06-16T16:46:50.431 | |
12 | 13 | 2011.0.00405.S | PKS1830-211 | 278.416330 | -21.061080 | 0.455 | 293.63 | 295.51 | 294.57 | 1.874 | 976.56 | 0.991 | 3.448 | 20.113 | 60.429 | 1655.25 | 120.04 | uid://A002/X36d874/X7a | http://almascience.org/aq?member_ous_id=uid://... | text/html | 2011.0.00405.S | Public | 12.165817 | -5.711677 | ADS/JAO.ALMA#2011.0.00405.S | ALMA | JAO | ALMA | uid://A002/X36d874/X7a | cube | 2 | PKS1830-211 | 278.416330 | -21.061080 | 0.005587 | Circle ICRS 278.416330 -21.061080 0.002793 | 0.454758 | 56028.238332 | 56028.363572 | 3144.960 | 3144.960 | 0.001014 | 0.001021 | 302642.950000 | /XX/YY/ | phot.flux.density;phys.polarization | 7 | 2.927253e+14 | Bagdonaite, J.; Daprà, M.; Jansen, P.; Bethlem... | A limit on a possible cosmological variation o... | 2013 | The z=0.89 (sub)mm molecular absorber toward t... | PKS1830_CH_and_H2O_b7_run_x2 | Bethlem, Hendrick; Gerin, Maryvonne; Bottinell... | 1.655253 | 0.060429 | 0.703871 | uid://A002/X36d874/X7a | uid://A002/X3cb0a0/X9e8 | A survey of strong absorption lines at z=0.89 ... | S | TARGET | T | 3.448268 | 1.875000e+09 | A003:DA41 A011:DV12 A025:DV14 A037:PM01 A045:D... | F | 2013-05-22T07:31:59.000 | 0.454758 | [281.64..283.51GHz,976.56kHz,1.7mJy/beam@10km/... | 289.509775 | 984.336598 | Muller, Sebastien | A strong magnetic field in the jet base of a s... | Bagdonaite, J. Martí-Vidal, I. Martí-Vidal, Iv... | T | 2013A&A...558A.123M 2013PhRvL.111w1101B 2014A&... | Galaxy structure & evolution, Galaxy chemistry | Galaxy evolution | 2021-06-16T16:46:50.431 | |
13 | 14 | 2011.0.00405.S | PKS1830-211 | 278.416330 | -21.061080 | 0.563 | 242.31 | 244.20 | 243.25 | 1.894 | 976.56 | 1.199 | 5.088 | 23.118 | 74.597 | 2229.83 | 146.24 | uid://A002/X36d874/X7c | http://almascience.org/aq?member_ous_id=uid://... | text/html | 2011.0.00405.S | Public | 12.165817 | -5.711677 | ADS/JAO.ALMA#2011.0.00405.S | ALMA | JAO | ALMA | uid://A002/X36d874/X7c | cube | 2 | PKS1830-211 | 278.416330 | -21.061080 | 0.006422 | Circle ICRS 278.416330 -21.061080 0.003211 | 0.562899 | 56026.250749 | 56093.330969 | 4838.400 | 4838.400 | 0.001228 | 0.001237 | 250078.682480 | /XX/YY/ | phot.flux.density;phys.polarization | 6 | 2.927251e+14 | Bagdonaite, J.; Daprà, M.; Jansen, P.; Bethlem... | A limit on a possible cosmological variation o... | 2013 | The z=0.89 (sub)mm molecular absorber toward t... | PKS1830-211_CO4-3_b6_run_x2 | Bethlem, Hendrick; Gerin, Maryvonne; Bottinell... | 2.229828 | 0.074597 | 2.122151 | uid://A002/X36d874/X7c | uid://A002/X3ca066/Xa6f | A survey of strong absorption lines at z=0.89 ... | S | TARGET | T | 5.088294 | 1.875000e+09 | A003:DA41 A004:DV04 A008:DV19 A011:DV12 A021:D... | F | 2013-10-19T12:40:13.000 | 0.562899 | [242.31..244.20GHz,976.56kHz,2.2mJy/beam@10km/... | 251.884124 | 1119.620778 | Muller, Sebastien | A strong magnetic field in the jet base of a s... | Bagdonaite, J. Martí-Vidal, I. Martí-Vidal, Iv... | T | 2013A&A...558A.123M 2013PhRvL.111w1101B 2014A&... | Galaxy structure & evolution, Galaxy chemistry | Galaxy evolution | 2021-06-16T16:46:50.431 | |
14 | 15 | 2011.0.00405.S | PKS1830-211 | 278.416330 | -21.061080 | 0.442 | 304.55 | 306.43 | 305.49 | 1.880 | 976.56 | 0.955 | 4.104 | 19.504 | 68.197 | 1868.50 | 137.78 | uid://A002/X36d874/X7e | http://almascience.org/aq?member_ous_id=uid://... | text/html | 2011.0.00405.S | Public | 12.165817 | -5.711677 | ADS/JAO.ALMA#2011.0.00405.S | ALMA | JAO | ALMA | uid://A002/X36d874/X7e | cube | 2 | PKS1830-211 | 278.416330 | -21.061080 | 0.005418 | Circle ICRS 278.416330 -21.061080 0.002709 | 0.441708 | 56070.225109 | 56082.381661 | 6048.000 | 6048.000 | 0.000978 | 0.000984 | 313809.659760 | /XX/YY/ | phot.flux.density;phys.polarization | 7 | 2.927369e+14 | Bagdonaite, J.; Daprà, M.; Jansen, P.; Bethlem... | A limit on a possible cosmological variation o... | 2013 | The z=0.89 (sub)mm molecular absorber toward t... | PKS1830_CO5-4_b7_run_x3 | Bethlem, Hendrick; Gerin, Maryvonne; Bottinell... | 1.868498 | 0.068197 | 1.027013 | uid://A002/X36d874/X7e | uid://A002/X4122f3/X133 | A survey of strong absorption lines at z=0.89 ... | S | TARGET | T | 4.104185 | 1.875000e+09 | A003:DA41 A004:DV04 A011:DV12 A021:DV08 A025:D... | F | 2013-07-05T11:49:39.000 | 0.441708 | [290.68..292.56GHz,976.56kHz,1.9mJy/beam@10km/... | 298.550728 | 955.332153 | Muller, Sebastien | A strong magnetic field in the jet base of a s... | Bagdonaite, J. Martí-Vidal, I. Martí-Vidal, Iv... | T | 2013A&A...558A.123M 2013PhRvL.111w1101B 2014A&... | Galaxy structure & evolution, Galaxy chemistry | Galaxy evolution | 2021-06-16T16:46:50.431 | |
15 | 16 | 2011.0.00405.S | PKS1830-211 | 278.416330 | -21.061080 | 1.331 | 93.07 | 94.95 | 94.01 | 1.878 | 976.56 | 3.083 | 12.937 | 58.774 | 29.824 | 1440.54 | 59.16 | uid://A002/X36d874/X80 | http://almascience.org/aq?member_ous_id=uid://... | text/html | 2011.0.00405.S | Public | 12.165817 | -5.711677 | ADS/JAO.ALMA#2011.0.00405.S | ALMA | JAO | ALMA | uid://A002/X36d874/X80 | cube | 2 | PKS1830-211 | 278.416330 | -21.061080 | 0.016326 | Circle ICRS 278.416330 -21.061080 0.008163 | 1.331051 | 56069.374548 | 56093.397660 | 3719.520 | 3719.520 | 0.003157 | 0.003221 | 97236.742000 | /XX/YY/ | phot.flux.density;phys.polarization | 3 | 2.927369e+14 | Bagdonaite, J.; Daprà, M.; Jansen, P.; Bethlem... | A limit on a possible cosmological variation o... | 2013 | The z=0.89 (sub)mm molecular absorber toward t... | PKS1830_HCOplus_b3_run_x3 | Bethlem, Hendrick; Gerin, Maryvonne; Bottinell... | 1.440543 | 0.029824 | 0.923567 | uid://A002/X36d874/X80 | uid://A002/X411025/X441 | A survey of strong absorption lines at z=0.89 ... | S | TARGET | T | 12.936728 | 1.875000e+09 | A003:DA41 A004:DV04 A008:DV19 A011:DV12 A021:D... | F | 2013-10-10T14:47:51.000 | 1.331051 | [91.20..93.08GHz,976.56kHz,1.5mJy/beam@10km/s,... | 99.075504 | 2737.212182 | Muller, Sebastien | A strong magnetic field in the jet base of a s... | Bagdonaite, J. Martí-Vidal, I. Martí-Vidal, Iv... | T | 2013A&A...558A.123M 2013PhRvL.111w1101B 2014A&... | Galaxy structure & evolution, Galaxy chemistry | Galaxy evolution | 2021-06-16T16:46:50.431 | |
16 | 17 | 2011.0.00405.S | PKS1830-211 | 278.416330 | -21.061080 | 0.442 | 290.68 | 292.56 | 291.62 | 1.880 | 976.56 | 1.001 | 4.104 | 19.504 | 68.197 | 1903.65 | 137.16 | uid://A002/X36d874/X7e | http://almascience.org/aq?member_ous_id=uid://... | text/html | 2011.0.00405.S | Public | 12.165817 | -5.711677 | ADS/JAO.ALMA#2011.0.00405.S | ALMA | JAO | ALMA | uid://A002/X36d874/X7e | cube | 2 | PKS1830-211 | 278.416330 | -21.061080 | 0.005418 | Circle ICRS 278.416330 -21.061080 0.002709 | 0.441708 | 56070.225109 | 56082.381661 | 6048.000 | 6048.000 | 0.001025 | 0.001031 | 299601.659760 | /XX/YY/ | phot.flux.density;phys.polarization | 7 | 2.927369e+14 | Bagdonaite, J.; Daprà, M.; Jansen, P.; Bethlem... | A limit on a possible cosmological variation o... | 2013 | The z=0.89 (sub)mm molecular absorber toward t... | PKS1830_CO5-4_b7_run_x3 | Bethlem, Hendrick; Gerin, Maryvonne; Bottinell... | 1.903645 | 0.068197 | 1.027013 | uid://A002/X36d874/X7e | uid://A002/X4122f3/X133 | A survey of strong absorption lines at z=0.89 ... | S | TARGET | T | 4.104185 | 1.875000e+09 | A003:DA41 A004:DV04 A011:DV12 A021:DV08 A025:D... | F | 2013-07-05T11:49:39.000 | 0.441708 | [290.68..292.56GHz,976.56kHz,1.9mJy/beam@10km/... | 298.550728 | 955.332153 | Muller, Sebastien | A strong magnetic field in the jet base of a s... | Bagdonaite, J. Martí-Vidal, I. Martí-Vidal, Iv... | T | 2013A&A...558A.123M 2013PhRvL.111w1101B 2014A&... | Galaxy structure & evolution, Galaxy chemistry | Galaxy evolution | 2021-06-16T16:46:50.431 | |
17 | 18 | 2011.0.00405.S | PKS1830-211 | 278.416330 | -21.061080 | 0.442 | 302.68 | 304.56 | 303.62 | 1.880 | 976.56 | 0.961 | 4.104 | 19.504 | 68.197 | 1848.24 | 135.87 | uid://A002/X36d874/X7e | http://almascience.org/aq?member_ous_id=uid://... | text/html | 2011.0.00405.S | Public | 12.165817 | -5.711677 | ADS/JAO.ALMA#2011.0.00405.S | ALMA | JAO | ALMA | uid://A002/X36d874/X7e | cube | 2 | PKS1830-211 | 278.416330 | -21.061080 | 0.005418 | Circle ICRS 278.416330 -21.061080 0.002709 | 0.441708 | 56070.225109 | 56082.381661 | 6048.000 | 6048.000 | 0.000984 | 0.000990 | 311889.659760 | /XX/YY/ | phot.flux.density;phys.polarization | 7 | 2.927369e+14 | Bagdonaite, J.; Daprà, M.; Jansen, P.; Bethlem... | A limit on a possible cosmological variation o... | 2013 | The z=0.89 (sub)mm molecular absorber toward t... | PKS1830_CO5-4_b7_run_x3 | Bethlem, Hendrick; Gerin, Maryvonne; Bottinell... | 1.848243 | 0.068197 | 1.027013 | uid://A002/X36d874/X7e | uid://A002/X4122f3/X133 | A survey of strong absorption lines at z=0.89 ... | S | TARGET | T | 4.104185 | 1.875000e+09 | A003:DA41 A004:DV04 A011:DV12 A021:DV08 A025:D... | F | 2013-07-05T11:49:39.000 | 0.441708 | [290.68..292.56GHz,976.56kHz,1.9mJy/beam@10km/... | 298.550728 | 955.332153 | Muller, Sebastien | A strong magnetic field in the jet base of a s... | Bagdonaite, J. Martí-Vidal, I. Martí-Vidal, Iv... | T | 2013A&A...558A.123M 2013PhRvL.111w1101B 2014A&... | Galaxy structure & evolution, Galaxy chemistry | Galaxy evolution | 2021-06-16T16:46:50.431 | |
18 | 19 | 2011.0.00820.S | ngc4418 | 186.727617 | -0.877642 | 0.665 | 261.72 | 263.60 | 262.66 | 1.874 | 976.56 | 1.111 | 8.262 | 22.748 | 191.363 | 5507.00 | 377.20 | uid://A002/X314ea1/X1fa | http://almascience.org/aq?member_ous_id=uid://... | text/html | 2011.0.00820.S | Public | 290.048542 | 61.379017 | ADS/JAO.ALMA#2011.0.00820.S | ALMA | JAO | ALMA | uid://A002/X314ea1/X1fa | cube | 2 | ngc4418 | 186.727617 | -0.877642 | 0.006319 | Circle ICRS 186.727617 -0.877642 0.003159 | 0.664926 | 56293.314401 | 56293.327148 | 151.200 | 151.200 | 0.001137 | 0.001145 | 269951.750000 | /XX/YY/ | phot.flux.density;phys.polarization | 6 | 2.927348e+14 | Costagliola, F.; Sakamoto, K.; Muller, S.; Mar... | Context. Extragalactic observations allow the ... | 2015 | A wide-band, high-quality, unbiased census of ... | ngc4418 B6 Setup 12 | Garcia-Burillo, Santiago; Muehle, Stefanie; Aa... | 5.507000 | 0.191363 | 2.751811 | uid://A002/X314ea1/X1fa | uid://A002/X590461/X17e6 | A 170 GHz-wide Complete Spectral Scan of an IR... | S | TARGET | T | 8.261900 | 1.875000e+09 | A001:DV01 A003:DA41 A004:DV04 A006:DV07 A007:D... | F | 2014-01-18T12:52:22.000 | 0.664926 | [246.72..248.60GHz,976.56kHz,5.6mJy/beam@10km/... | 255.972659 | 1103.737386 | Costagliola, Francesco | Abundance measurements of Titan's stratospheri... | Costagliola, F. Thelen, Alexander E. | T | 2015A&A...582A..91C 2019Icar..319..417T | Luminous and Ultra-Luminous Infra-Red Galaxies... | Galaxy evolution | 2021-06-16T16:46:50.431 | |
19 | 20 | 2011.0.00820.S | ngc4418 | 186.727617 | -0.877642 | 1.355 | 97.88 | 99.75 | 98.82 | 1.875 | 976.56 | 2.935 | 9.305 | 63.355 | 60.616 | 2862.27 | 120.59 | uid://A002/X327408/X100 | http://almascience.org/aq?member_ous_id=uid://... | text/html | 2011.0.00820.S | Public | 290.048542 | 61.379017 | ADS/JAO.ALMA#2011.0.00820.S | ALMA | JAO | ALMA | uid://A002/X327408/X100 | cube | 2 | ngc4418 | 186.727617 | -0.877642 | 0.017599 | Circle ICRS 186.727617 -0.877642 0.008799 | 1.354752 | 56042.089628 | 56042.109167 | 332.640 | 332.640 | 0.003005 | 0.003063 | 102143.801200 | /XX/YY/ | phot.flux.density;phys.polarization | 3 | 2.927779e+14 | Costagliola, F.; Sakamoto, K.; Muller, S.; Mar... | Context. Extragalactic observations allow the ... | 2015 | A wide-band, high-quality, unbiased census of ... | ngc4418 B3 Setup 1: Run x 1 | Garcia-Burillo, Santiago; Muehle, Stefanie; Aa... | 2.862267 | 0.060616 | 2.623814 | uid://A002/X327408/X100 | uid://A002/X3e3a61/Xce | A 170 GHz-wide Complete Spectral Scan of an IR... | S | TARGET | T | 9.304600 | 1.875000e+09 | A003:DA41 A021:DV08 A025:DV14 A045:DV11 A046:D... | F | 2013-06-15T09:26:34.000 | 1.354752 | [84.07..85.94GHz,976.56kHz,3.2mJy/beam@10km/s,... | 91.910024 | 2935.003931 | Costagliola, Francesco | Abundance measurements of Titan's stratospheri... | Costagliola, F. Thelen, Alexander E. | T | 2015A&A...582A..91C 2019Icar..319..417T | Luminous and Ultra-Luminous Infra-Red Galaxies... | Galaxy evolution | 2021-06-16T16:46:50.431 | |
20 | 21 | 2011.0.00820.S | ngc4418 | 186.727617 | -0.877642 | 0.657 | 251.60 | 253.47 | 252.54 | 1.874 | 976.56 | 1.155 | 8.158 | 22.463 | 184.788 | 5492.90 | 368.94 | uid://A002/X314ea1/X1ee | http://almascience.org/aq?member_ous_id=uid://... | text/html | 2011.0.00820.S | Public | 290.048542 | 61.379017 | ADS/JAO.ALMA#2011.0.00820.S | ALMA | JAO | ALMA | uid://A002/X314ea1/X1ee | cube | 2 | ngc4418 | 186.727617 | -0.877642 | 0.006240 | Circle ICRS 186.727617 -0.877642 0.003120 | 0.656589 | 56293.474235 | 56293.487242 | 151.200 | 151.200 | 0.001183 | 0.001192 | 259583.750000 | /XX/YY/ | phot.flux.density;phys.polarization | 6 | 2.927352e+14 | Costagliola, F.; Sakamoto, K.; Muller, S.; Mar... | Context. Extragalactic observations allow the ... | 2015 | A wide-band, high-quality, unbiased census of ... | ngc4418 B6 Setup 13 | Garcia-Burillo, Santiago; Muehle, Stefanie; Aa... | 5.492896 | 0.184788 | 3.761806 | uid://A002/X314ea1/X1ee | uid://A002/X590461/X1b27 | A 170 GHz-wide Complete Spectral Scan of an IR... | S | TARGET | T | 8.158316 | 1.875000e+09 | A001:DV01 A003:DA41 A004:DV04 A006:DV07 A007:D... | F | 2014-06-25T06:41:57.000 | 0.656589 | [249.97..251.85GHz,976.56kHz,5.5mJy/beam@10km/... | 259.222672 | 1090.377424 | Costagliola, Francesco | Abundance measurements of Titan's stratospheri... | Costagliola, F. Thelen, Alexander E. | T | 2015A&A...582A..91C 2019Icar..319..417T | Luminous and Ultra-Luminous Infra-Red Galaxies... | Galaxy evolution | 2021-06-16T16:46:50.431 | |
21 | 22 | 2011.0.00820.S | ngc4418 | 186.727617 | -0.877642 | 0.657 | 266.60 | 268.47 | 267.53 | 1.874 | 976.56 | 1.090 | 8.158 | 22.463 | 184.788 | 5382.61 | 372.08 | uid://A002/X314ea1/X1ee | http://almascience.org/aq?member_ous_id=uid://... | text/html | 2011.0.00820.S | Public | 290.048542 | 61.379017 | ADS/JAO.ALMA#2011.0.00820.S | ALMA | JAO | ALMA | uid://A002/X314ea1/X1ee | cube | 2 | ngc4418 | 186.727617 | -0.877642 | 0.006240 | Circle ICRS 186.727617 -0.877642 0.003120 | 0.656589 | 56293.474235 | 56293.487242 | 151.200 | 151.200 | 0.001117 | 0.001125 | 274943.750000 | /XX/YY/ | phot.flux.density;phys.polarization | 6 | 2.927352e+14 | Costagliola, F.; Sakamoto, K.; Muller, S.; Mar... | Context. Extragalactic observations allow the ... | 2015 | A wide-band, high-quality, unbiased census of ... | ngc4418 B6 Setup 13 | Garcia-Burillo, Santiago; Muehle, Stefanie; Aa... | 5.382614 | 0.184788 | 3.761806 | uid://A002/X314ea1/X1ee | uid://A002/X590461/X1b27 | A 170 GHz-wide Complete Spectral Scan of an IR... | S | TARGET | T | 8.158316 | 1.875000e+09 | A001:DV01 A003:DA41 A004:DV04 A006:DV07 A007:D... | F | 2014-06-25T06:41:57.000 | 0.656589 | [249.97..251.85GHz,976.56kHz,5.5mJy/beam@10km/... | 259.222672 | 1090.377424 | Costagliola, Francesco | Abundance measurements of Titan's stratospheri... | Costagliola, F. Thelen, Alexander E. | T | 2015A&A...582A..91C 2019Icar..319..417T | Luminous and Ultra-Luminous Infra-Red Galaxies... | Galaxy evolution | 2021-06-16T16:46:50.431 | |
22 | 23 | 2011.0.00820.S | ngc4418 | 186.727617 | -0.877642 | 0.657 | 249.97 | 251.85 | 250.91 | 1.874 | 976.56 | 1.162 | 8.158 | 22.463 | 184.788 | 5505.70 | 368.62 | uid://A002/X314ea1/X1ee | http://almascience.org/aq?member_ous_id=uid://... | text/html | 2011.0.00820.S | Public | 290.048542 | 61.379017 | ADS/JAO.ALMA#2011.0.00820.S | ALMA | JAO | ALMA | uid://A002/X314ea1/X1ee | cube | 2 | ngc4418 | 186.727617 | -0.877642 | 0.006240 | Circle ICRS 186.727617 -0.877642 0.003120 | 0.656589 | 56293.474235 | 56293.487242 | 151.200 | 151.200 | 0.001190 | 0.001199 | 257919.750000 | /XX/YY/ | phot.flux.density;phys.polarization | 6 | 2.927352e+14 | Costagliola, F.; Sakamoto, K.; Muller, S.; Mar... | Context. Extragalactic observations allow the ... | 2015 | A wide-band, high-quality, unbiased census of ... | ngc4418 B6 Setup 13 | Garcia-Burillo, Santiago; Muehle, Stefanie; Aa... | 5.505704 | 0.184788 | 3.761806 | uid://A002/X314ea1/X1ee | uid://A002/X590461/X1b27 | A 170 GHz-wide Complete Spectral Scan of an IR... | S | TARGET | T | 8.158316 | 1.875000e+09 | A001:DV01 A003:DA41 A004:DV04 A006:DV07 A007:D... | F | 2014-06-25T06:41:57.000 | 0.656589 | [249.97..251.85GHz,976.56kHz,5.5mJy/beam@10km/... | 259.222672 | 1090.377424 | Costagliola, Francesco | Abundance measurements of Titan's stratospheri... | Costagliola, F. Thelen, Alexander E. | T | 2015A&A...582A..91C 2019Icar..319..417T | Luminous and Ultra-Luminous Infra-Red Galaxies... | Galaxy evolution | 2021-06-16T16:46:50.431 | |
23 | 24 | 2011.0.00820.S | ngc4418 | 186.727617 | -0.877642 | 0.657 | 264.97 | 266.85 | 265.91 | 1.874 | 976.56 | 1.097 | 8.158 | 22.463 | 184.788 | 5393.90 | 371.73 | uid://A002/X314ea1/X1ee | http://almascience.org/aq?member_ous_id=uid://... | text/html | 2011.0.00820.S | Public | 290.048542 | 61.379017 | ADS/JAO.ALMA#2011.0.00820.S | ALMA | JAO | ALMA | uid://A002/X314ea1/X1ee | cube | 2 | ngc4418 | 186.727617 | -0.877642 | 0.006240 | Circle ICRS 186.727617 -0.877642 0.003120 | 0.656589 | 56293.474235 | 56293.487242 | 151.200 | 151.200 | 0.001123 | 0.001131 | 273279.750000 | /XX/YY/ | phot.flux.density;phys.polarization | 6 | 2.927352e+14 | Costagliola, F.; Sakamoto, K.; Muller, S.; Mar... | Context. Extragalactic observations allow the ... | 2015 | A wide-band, high-quality, unbiased census of ... | ngc4418 B6 Setup 13 | Garcia-Burillo, Santiago; Muehle, Stefanie; Aa... | 5.393897 | 0.184788 | 3.761806 | uid://A002/X314ea1/X1ee | uid://A002/X590461/X1b27 | A 170 GHz-wide Complete Spectral Scan of an IR... | S | TARGET | T | 8.158316 | 1.875000e+09 | A001:DV01 A003:DA41 A004:DV04 A006:DV07 A007:D... | F | 2014-06-25T06:41:57.000 | 0.656589 | [249.97..251.85GHz,976.56kHz,5.5mJy/beam@10km/... | 259.222672 | 1090.377424 | Costagliola, Francesco | Abundance measurements of Titan's stratospheri... | Costagliola, F. Thelen, Alexander E. | T | 2015A&A...582A..91C 2019Icar..319..417T | Luminous and Ultra-Luminous Infra-Red Galaxies... | Galaxy evolution | 2021-06-16T16:46:50.431 | |
24 | 25 | 2011.0.00820.S | ngc4418 | 186.727617 | -0.877642 | 0.665 | 246.72 | 248.60 | 247.66 | 1.874 | 976.56 | 1.178 | 8.262 | 22.748 | 191.363 | 5623.83 | 374.09 | uid://A002/X314ea1/X1fa | http://almascience.org/aq?member_ous_id=uid://... | text/html | 2011.0.00820.S | Public | 290.048542 | 61.379017 | ADS/JAO.ALMA#2011.0.00820.S | ALMA | JAO | ALMA | uid://A002/X314ea1/X1fa | cube | 2 | ngc4418 | 186.727617 | -0.877642 | 0.006319 | Circle ICRS 186.727617 -0.877642 0.003159 | 0.664926 | 56293.314401 | 56293.327148 | 151.200 | 151.200 | 0.001206 | 0.001215 | 254591.750000 | /XX/YY/ | phot.flux.density;phys.polarization | 6 | 2.927348e+14 | Costagliola, F.; Sakamoto, K.; Muller, S.; Mar... | Context. Extragalactic observations allow the ... | 2015 | A wide-band, high-quality, unbiased census of ... | ngc4418 B6 Setup 12 | Garcia-Burillo, Santiago; Muehle, Stefanie; Aa... | 5.623833 | 0.191363 | 2.751811 | uid://A002/X314ea1/X1fa | uid://A002/X590461/X17e6 | A 170 GHz-wide Complete Spectral Scan of an IR... | S | TARGET | T | 8.261900 | 1.875000e+09 | A001:DV01 A003:DA41 A004:DV04 A006:DV07 A007:D... | F | 2014-01-18T12:52:22.000 | 0.664926 | [246.72..248.60GHz,976.56kHz,5.6mJy/beam@10km/... | 255.972659 | 1103.737386 | Costagliola, Francesco | Abundance measurements of Titan's stratospheri... | Costagliola, F. Thelen, Alexander E. | T | 2015A&A...582A..91C 2019Icar..319..417T | Luminous and Ultra-Luminous Infra-Red Galaxies... | Galaxy evolution | 2021-06-16T16:46:50.431 | |
25 | 26 | 2011.0.00820.S | ngc4418 | 186.727617 | -0.877642 | 0.665 | 248.35 | 250.22 | 249.29 | 1.874 | 976.56 | 1.170 | 8.262 | 22.748 | 191.363 | 5610.45 | 374.41 | uid://A002/X314ea1/X1fa | http://almascience.org/aq?member_ous_id=uid://... | text/html | 2011.0.00820.S | Public | 290.048542 | 61.379017 | ADS/JAO.ALMA#2011.0.00820.S | ALMA | JAO | ALMA | uid://A002/X314ea1/X1fa | cube | 2 | ngc4418 | 186.727617 | -0.877642 | 0.006319 | Circle ICRS 186.727617 -0.877642 0.003159 | 0.664926 | 56293.314401 | 56293.327148 | 151.200 | 151.200 | 0.001198 | 0.001207 | 256255.750000 | /XX/YY/ | phot.flux.density;phys.polarization | 6 | 2.927348e+14 | Costagliola, F.; Sakamoto, K.; Muller, S.; Mar... | Context. Extragalactic observations allow the ... | 2015 | A wide-band, high-quality, unbiased census of ... | ngc4418 B6 Setup 12 | Garcia-Burillo, Santiago; Muehle, Stefanie; Aa... | 5.610448 | 0.191363 | 2.751811 | uid://A002/X314ea1/X1fa | uid://A002/X590461/X17e6 | A 170 GHz-wide Complete Spectral Scan of an IR... | S | TARGET | T | 8.261900 | 1.875000e+09 | A001:DV01 A003:DA41 A004:DV04 A006:DV07 A007:D... | F | 2014-01-18T12:52:22.000 | 0.664926 | [246.72..248.60GHz,976.56kHz,5.6mJy/beam@10km/... | 255.972659 | 1103.737386 | Costagliola, Francesco | Abundance measurements of Titan's stratospheri... | Costagliola, F. Thelen, Alexander E. | T | 2015A&A...582A..91C 2019Icar..319..417T | Luminous and Ultra-Luminous Infra-Red Galaxies... | Galaxy evolution | 2021-06-16T16:46:50.431 | |
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1335 | 1336 | 2018.1.01395.S | NGC_253 | 11.888058 | -25.288800 | 0.019 | 217.98 | 219.85 | 218.91 | 1.874 | 1128.91 | 1.539 | 0.500 | 25.549 | 12.404 | 398.35 | 24.92 | uid://A001/X133d/X3025 | http://almascience.org/aq?member_ous_id=uid://... | text/html | 2018.1.01395.S | Public | 97.364395 | -87.964503 | ADS/JAO.ALMA#2018.1.01395.S | ALMA | JAO | ALMA | uid://A001/X133d/X3025 | cube | 2 | NGC_253 | 11.888058 | -25.288800 | 0.007097 | Polygon ICRS 11.888794 -25.292286 11.887323 -2... | 0.018645 | 58640.446034 | 58674.467208 | 16003.008 | 16003.008 | 0.001364 | 0.001375 | 194758.820482 | /XX/YY/ | phot.flux.density;phys.polarization | 6 | 3.384169e+14 | <NA> | We have used 0.2" ALMA images of the HC3N vibr... | NGC_253_a_06_TM1 | Martin-Pintado, Jesus; Martin, Sergio; Gonzale... | 0.398353 | 0.012404 | 0.911870 | uid://A001/X133d/X3024 | uid://A001/X133d/X3025 | uid://A002/Xdd4cf3/X33a6 | Witnessing the early stages of the formation o... | S | TARGET | T | 0.499517 | 1.875000e+09 | A015:DA64 A058:DA41 A069:DV16 A074:DV09 A082:D... | F | 2021-02-12T18:33:55.000 | 0.018645 | [217.98..219.85GHz,1128.91kHz,398.4uJy/beam@10... | 227.913497 | 1434.115718 | Rico Villas, Fernando | T | Starbursts, star formation, Galaxy chemistry | Active galaxies | 2021-06-16T16:46:50.431 | |||||
1336 | 1337 | 2018.1.01395.S | NGC_253 | 11.888058 | -25.288800 | 0.019 | 235.98 | 237.85 | 236.91 | 1.874 | 1128.91 | 1.434 | 0.500 | 25.549 | 12.404 | 382.31 | 24.78 | uid://A001/X133d/X3025 | http://almascience.org/aq?member_ous_id=uid://... | text/html | 2018.1.01395.S | Public | 97.364395 | -87.964503 | ADS/JAO.ALMA#2018.1.01395.S | ALMA | JAO | ALMA | uid://A001/X133d/X3025 | cube | 2 | NGC_253 | 11.888058 | -25.288800 | 0.007097 | Polygon ICRS 11.888794 -25.292286 11.887323 -2... | 0.018645 | 58640.446034 | 58674.467208 | 16003.008 | 16003.008 | 0.001260 | 0.001270 | 209043.422558 | /XX/YY/ | phot.flux.density;phys.polarization | 6 | 3.384169e+14 | <NA> | We have used 0.2" ALMA images of the HC3N vibr... | NGC_253_a_06_TM1 | Martin-Pintado, Jesus; Martin, Sergio; Gonzale... | 0.382310 | 0.012404 | 0.911870 | uid://A001/X133d/X3024 | uid://A001/X133d/X3025 | uid://A002/Xdd4cf3/X33a6 | Witnessing the early stages of the formation o... | S | TARGET | T | 0.499517 | 1.875000e+09 | A015:DA64 A058:DA41 A069:DV16 A074:DV09 A082:D... | F | 2021-02-12T18:33:55.000 | 0.018645 | [217.98..219.85GHz,1128.91kHz,398.4uJy/beam@10... | 227.913497 | 1434.115718 | Rico Villas, Fernando | T | Starbursts, star formation, Galaxy chemistry | Active galaxies | 2021-06-16T16:46:50.431 | |||||
1337 | 1338 | 2019.1.00130.S | NGC4418 | 186.727617 | -0.877642 | 1.357 | 108.29 | 110.16 | 109.23 | 1.873 | 1938.48 | 5.366 | 24.940 | 55.903 | 10.485 | 468.79 | 20.59 | uid://A001/X1465/X389c | http://almascience.org/aq?member_ous_id=uid://... | text/html | 2019.1.00130.S | Public | 290.048542 | 61.379017 | ADS/JAO.ALMA#2019.1.00130.S | ALMA | JAO | ALMA | uid://A001/X1465/X389c | cube | 2 | NGC4418 | 186.727617 | -0.877642 | 0.015529 | Polygon ICRS 186.727617 -0.869878 186.729072 -... | 1.356746 | 58787.582055 | 58825.599964 | 4898.880 | 4898.880 | 0.002721 | 0.002768 | 55868.832936 | /XX/YY/ | phot.flux.density;phys.polarization | 3 | 5.810830e+14 | <NA> | The 12C/13C isotopic ratio is a good tracer of... | NGC4418_b_03_TM1 | Krips, Melanie; Garcia-Burillo, Santiago; Mueh... | 0.468785 | 0.010485 | 2.368327 | uid://A001/X1465/X389b | uid://A001/X1465/X389c | uid://A002/Xe2ada9/X15596 | A decisive answer on the carbon isotopic ratio... | S | TARGET | T | 24.939648 | 1.875000e+09 | A001:DA48 A002:DA44 A003:DV23 A004:DA56 A005:D... | F | 2021-03-17T19:10:59.000 | 1.356746 | [96.28..98.15GHz,1938.48kHz,511.7uJy/beam@10km... | 104.161888 | 5274.300699 | Martin, Sergio | T | Starbursts, star formation, Galaxy chemistry | Active galaxies | 2021-06-16T16:46:50.431 | |||||
1338 | 1339 | 2019.1.00130.S | NGC4945 | 196.363663 | -49.467900 | 2.523 | 91.70 | 93.57 | 92.63 | 1.873 | 1938.48 | 6.210 | 27.132 | 59.612 | 10.282 | 508.68 | 20.77 | uid://A001/X1465/X3888 | http://almascience.org/aq?member_ous_id=uid://... | text/html | 2019.1.00130.S | Public | 305.271559 | 13.340115 | ADS/JAO.ALMA#2019.1.00130.S | ALMA | JAO | ALMA | uid://A001/X1465/X3888 | cube | 2 | NGC4945 | 196.363663 | -49.467900 | 0.016559 | Polygon ICRS 196.371150 -49.461202 196.372949 ... | 2.522933 | 58830.525869 | 58831.619778 | 10765.440 | 10765.440 | 0.003204 | 0.003269 | 48272.592043 | /XX/YY/ | phot.flux.density;phys.polarization | 3 | 5.811169e+14 | <NA> | The 12C/13C isotopic ratio is a good tracer of... | NGC4945_a_03_TM1 | Krips, Melanie; Garcia-Burillo, Santiago; Mueh... | 0.508682 | 0.010282 | 3.740537 | uid://A001/X1465/X3887 | uid://A001/X1465/X3888 | uid://A002/Xe50c9e/X11047 | A decisive answer on the carbon isotopic ratio... | S | TARGET | T | 27.131876 | 1.875000e+09 | A001:DA48 A002:DA44 A003:DV23 A004:DA56 A005:D... | F | 2021-04-06T23:21:24.000 | 2.522933 | [89.90..91.77GHz,1938.48kHz,513.5uJy/beam@10km... | 97.681492 | 5609.869359 | Martin, Sergio | T | Starbursts, star formation, Galaxy chemistry | Active galaxies | 2021-06-16T16:46:50.431 | |||||
1339 | 1340 | 2019.1.00130.S | NGC4418 | 186.727617 | -0.877642 | 1.357 | 97.97 | 99.84 | 98.90 | 1.873 | 1938.48 | 5.820 | 24.940 | 55.903 | 10.485 | 507.47 | 21.40 | uid://A001/X1465/X389c | http://almascience.org/aq?member_ous_id=uid://... | text/html | 2019.1.00130.S | Public | 290.048542 | 61.379017 | ADS/JAO.ALMA#2019.1.00130.S | ALMA | JAO | ALMA | uid://A001/X1465/X389c | cube | 2 | NGC4418 | 186.727617 | -0.877642 | 0.015529 | Polygon ICRS 186.727617 -0.869878 186.729072 -... | 1.356746 | 58787.582055 | 58825.599964 | 4898.880 | 4898.880 | 0.003003 | 0.003060 | 51508.746588 | /XX/YY/ | phot.flux.density;phys.polarization | 3 | 5.810830e+14 | <NA> | The 12C/13C isotopic ratio is a good tracer of... | NGC4418_b_03_TM1 | Krips, Melanie; Garcia-Burillo, Santiago; Mueh... | 0.507473 | 0.010485 | 2.368327 | uid://A001/X1465/X389b | uid://A001/X1465/X389c | uid://A002/Xe2ada9/X15596 | A decisive answer on the carbon isotopic ratio... | S | TARGET | T | 24.939648 | 1.875000e+09 | A001:DA48 A002:DA44 A003:DV23 A004:DA56 A005:D... | F | 2021-03-17T19:10:59.000 | 1.356746 | [96.28..98.15GHz,1938.48kHz,511.7uJy/beam@10km... | 104.161888 | 5274.300699 | Martin, Sergio | T | Starbursts, star formation, Galaxy chemistry | Active galaxies | 2021-06-16T16:46:50.431 | |||||
1340 | 1341 | 2019.1.00130.S | NGC4418 | 186.727617 | -0.877642 | 1.357 | 96.28 | 98.15 | 97.21 | 1.873 | 1938.48 | 5.920 | 24.940 | 55.903 | 10.485 | 511.67 | 21.39 | uid://A001/X1465/X389c | http://almascience.org/aq?member_ous_id=uid://... | text/html | 2019.1.00130.S | Public | 290.048542 | 61.379017 | ADS/JAO.ALMA#2019.1.00130.S | ALMA | JAO | ALMA | uid://A001/X1465/X389c | cube | 2 | NGC4418 | 186.727617 | -0.877642 | 0.015529 | Polygon ICRS 186.727617 -0.869878 186.729072 -... | 1.356746 | 58787.582055 | 58825.599964 | 4898.880 | 4898.880 | 0.003054 | 0.003114 | 50638.217620 | /XX/YY/ | phot.flux.density;phys.polarization | 3 | 5.810830e+14 | <NA> | The 12C/13C isotopic ratio is a good tracer of... | NGC4418_b_03_TM1 | Krips, Melanie; Garcia-Burillo, Santiago; Mueh... | 0.511673 | 0.010485 | 2.368327 | uid://A001/X1465/X389b | uid://A001/X1465/X389c | uid://A002/Xe2ada9/X15596 | A decisive answer on the carbon isotopic ratio... | S | TARGET | T | 24.939648 | 1.875000e+09 | A001:DA48 A002:DA44 A003:DV23 A004:DA56 A005:D... | F | 2021-03-17T19:10:59.000 | 1.356746 | [96.28..98.15GHz,1938.48kHz,511.7uJy/beam@10km... | 104.161888 | 5274.300699 | Martin, Sergio | T | Starbursts, star formation, Galaxy chemistry | Active galaxies | 2021-06-16T16:46:50.431 | |||||
1341 | 1342 | 2019.1.00130.S | NGC4945 | 196.363663 | -49.467900 | 2.309 | 108.87 | 110.74 | 109.80 | 1.873 | 1938.48 | 5.338 | 22.321 | 55.608 | 18.936 | 799.25 | 35.19 | uid://A001/X1465/X388c | http://almascience.org/aq?member_ous_id=uid://... | text/html | 2019.1.00130.S | Public | 305.271559 | 13.340115 | ADS/JAO.ALMA#2019.1.00130.S | ALMA | JAO | ALMA | uid://A001/X1465/X388c | cube | 2 | NGC4945 | 196.363663 | -49.467900 | 0.015447 | Circle ICRS 196.363663 -49.467900 0.007723 | 2.309410 | 58803.513052 | 58803.528983 | 876.960 | 876.960 | 0.002707 | 0.002754 | 56162.029463 | /XX/YY/ | phot.flux.density;phys.polarization | 3 | 5.811359e+14 | <NA> | The 12C/13C isotopic ratio is a good tracer of... | NGC4945_b_03_TM1 | Krips, Melanie; Garcia-Burillo, Santiago; Mueh... | 0.799253 | 0.018936 | 3.860288 | uid://A001/X1465/X388b | uid://A001/X1465/X388c | uid://A002/Xe37224/X14cf9 | A decisive answer on the carbon isotopic ratio... | S | TARGET | T | 22.320877 | 1.875000e+09 | A001:DA48 A002:DA44 A004:DA56 A005:DV22 A006:D... | F | 2021-03-05T20:54:34.000 | 2.309410 | [96.80..98.67GHz,1938.48kHz,984.3uJy/beam@10km... | 104.713465 | 5246.997281 | Martin, Sergio | T | Starbursts, star formation, Galaxy chemistry | Active galaxies | 2021-06-16T16:46:50.431 | |||||
1342 | 1343 | 2019.1.00130.S | NGC4945 | 196.363663 | -49.467900 | 2.309 | 110.76 | 112.63 | 111.69 | 1.873 | 1938.48 | 5.247 | 22.321 | 55.608 | 18.936 | 792.83 | 35.21 | uid://A001/X1465/X388c | http://almascience.org/aq?member_ous_id=uid://... | text/html | 2019.1.00130.S | Public | 305.271559 | 13.340115 | ADS/JAO.ALMA#2019.1.00130.S | ALMA | JAO | ALMA | uid://A001/X1465/X388c | cube | 2 | NGC4945 | 196.363663 | -49.467900 | 0.015447 | Circle ICRS 196.363663 -49.467900 0.007723 | 2.309410 | 58803.513052 | 58803.528983 | 876.960 | 876.960 | 0.002662 | 0.002707 | 57136.004067 | /XX/YY/ | phot.flux.density;phys.polarization | 3 | 5.811359e+14 | <NA> | The 12C/13C isotopic ratio is a good tracer of... | NGC4945_b_03_TM1 | Krips, Melanie; Garcia-Burillo, Santiago; Mueh... | 0.792833 | 0.018936 | 3.860288 | uid://A001/X1465/X388b | uid://A001/X1465/X388c | uid://A002/Xe37224/X14cf9 | A decisive answer on the carbon isotopic ratio... | S | TARGET | T | 22.320877 | 1.875000e+09 | A001:DA48 A002:DA44 A004:DA56 A005:DV22 A006:D... | F | 2021-03-05T20:54:34.000 | 2.309410 | [96.80..98.67GHz,1938.48kHz,984.3uJy/beam@10km... | 104.713465 | 5246.997281 | Martin, Sergio | T | Starbursts, star formation, Galaxy chemistry | Active galaxies | 2021-06-16T16:46:50.431 | |||||
1343 | 1344 | 2019.1.00130.S | NGC4945 | 196.363663 | -49.467900 | 2.309 | 98.49 | 100.36 | 99.42 | 1.873 | 1938.48 | 5.791 | 22.321 | 55.608 | 18.936 | 976.30 | 41.27 | uid://A001/X1465/X388c | http://almascience.org/aq?member_ous_id=uid://... | text/html | 2019.1.00130.S | Public | 305.271559 | 13.340115 | ADS/JAO.ALMA#2019.1.00130.S | ALMA | JAO | ALMA | uid://A001/X1465/X388c | cube | 2 | NGC4945 | 196.363663 | -49.467900 | 0.015447 | Circle ICRS 196.363663 -49.467900 0.007723 | 2.309410 | 58803.513052 | 58803.528983 | 876.960 | 876.960 | 0.002987 | 0.003044 | 51772.734587 | /XX/YY/ | phot.flux.density;phys.polarization | 3 | 5.811359e+14 | <NA> | The 12C/13C isotopic ratio is a good tracer of... | NGC4945_b_03_TM1 | Krips, Melanie; Garcia-Burillo, Santiago; Mueh... | 0.976296 | 0.018936 | 3.860288 | uid://A001/X1465/X388b | uid://A001/X1465/X388c | uid://A002/Xe37224/X14cf9 | A decisive answer on the carbon isotopic ratio... | S | TARGET | T | 22.320877 | 1.875000e+09 | A001:DA48 A002:DA44 A004:DA56 A005:DV22 A006:D... | F | 2021-03-05T20:54:34.000 | 2.309410 | [96.80..98.67GHz,1938.48kHz,984.3uJy/beam@10km... | 104.713465 | 5246.997281 | Martin, Sergio | T | Starbursts, star formation, Galaxy chemistry | Active galaxies | 2021-06-16T16:46:50.431 | |||||
1344 | 1345 | 2019.1.00130.S | NGC4945 | 196.363663 | -49.467900 | 2.309 | 96.80 | 98.67 | 97.73 | 1.873 | 1938.48 | 5.890 | 22.321 | 55.608 | 18.936 | 984.33 | 41.26 | uid://A001/X1465/X388c | http://almascience.org/aq?member_ous_id=uid://... | text/html | 2019.1.00130.S | Public | 305.271559 | 13.340115 | ADS/JAO.ALMA#2019.1.00130.S | ALMA | JAO | ALMA | uid://A001/X1465/X388c | cube | 2 | NGC4945 | 196.363663 | -49.467900 | 0.015447 | Circle ICRS 196.363663 -49.467900 0.007723 | 2.309410 | 58803.513052 | 58803.528983 | 876.960 | 876.960 | 0.003038 | 0.003097 | 50901.751170 | /XX/YY/ | phot.flux.density;phys.polarization | 3 | 5.811359e+14 | <NA> | The 12C/13C isotopic ratio is a good tracer of... | NGC4945_b_03_TM1 | Krips, Melanie; Garcia-Burillo, Santiago; Mueh... | 0.984333 | 0.018936 | 3.860288 | uid://A001/X1465/X388b | uid://A001/X1465/X388c | uid://A002/Xe37224/X14cf9 | A decisive answer on the carbon isotopic ratio... | S | TARGET | T | 22.320877 | 1.875000e+09 | A001:DA48 A002:DA44 A004:DA56 A005:DV22 A006:D... | F | 2021-03-05T20:54:34.000 | 2.309410 | [96.80..98.67GHz,1938.48kHz,984.3uJy/beam@10km... | 104.713465 | 5246.997281 | Martin, Sergio | T | Starbursts, star formation, Galaxy chemistry | Active galaxies | 2021-06-16T16:46:50.431 | |||||
1345 | 1346 | 2019.1.00130.S | NGC1068 | 40.669879 | -0.013289 | 1.609 | 103.38 | 105.26 | 104.32 | 1.873 | 1938.48 | 5.621 | 20.838 | 59.730 | 9.858 | 461.89 | 19.82 | uid://A001/X1465/X3890 | http://almascience.org/aq?member_ous_id=uid://... | text/html | 2019.1.00130.S | Public | 172.103977 | -51.933584 | ADS/JAO.ALMA#2019.1.00130.S | ALMA | JAO | ALMA | uid://A001/X1465/X3890 | cube | 2 | NGC1068 | 40.669879 | -0.013289 | 0.016592 | Polygon ICRS 40.669879 -0.021585 40.668325 -0.... | 1.608789 | 58790.229826 | 58802.118198 | 9918.720 | 9918.720 | 0.002848 | 0.002900 | 53330.846587 | /XX/YY/ | phot.flux.density;phys.polarization | 3 | 5.811652e+14 | <NA> | The 12C/13C isotopic ratio is a good tracer of... | NGC1068_a_03_TM1 | Krips, Melanie; Garcia-Burillo, Santiago; Mueh... | 0.461887 | 0.009858 | 2.751755 | uid://A001/X1465/X388f | uid://A001/X1465/X3890 | uid://A002/Xe2eefc/X31df | A decisive answer on the carbon isotopic ratio... | S | TARGET | T | 20.837939 | 1.875000e+09 | A001:DA48 A002:DA44 A003:DV23 A004:DA56 A005:D... | F | 2021-03-10T20:24:07.000 | 1.608789 | [89.72..91.59GHz,1938.48kHz,494.6uJy/beam@10km... | 97.487731 | 5621.370692 | Martin, Sergio | T | Starbursts, star formation, Galaxy chemistry | Active galaxies | 2021-06-16T16:46:50.431 | |||||
1346 | 1347 | 2019.1.00130.S | NGC1068 | 40.669879 | -0.013289 | 1.609 | 101.58 | 103.45 | 102.51 | 1.873 | 1938.48 | 5.721 | 20.838 | 59.730 | 9.858 | 459.66 | 19.55 | uid://A001/X1465/X3890 | http://almascience.org/aq?member_ous_id=uid://... | text/html | 2019.1.00130.S | Public | 172.103977 | -51.933584 | ADS/JAO.ALMA#2019.1.00130.S | ALMA | JAO | ALMA | uid://A001/X1465/X3890 | cube | 2 | NGC1068 | 40.669879 | -0.013289 | 0.016592 | Polygon ICRS 40.669879 -0.021585 40.668325 -0.... | 1.608789 | 58790.229826 | 58802.118198 | 9918.720 | 9918.720 | 0.002898 | 0.002951 | 52398.067385 | /XX/YY/ | phot.flux.density;phys.polarization | 3 | 5.811652e+14 | <NA> | The 12C/13C isotopic ratio is a good tracer of... | NGC1068_a_03_TM1 | Krips, Melanie; Garcia-Burillo, Santiago; Mueh... | 0.459663 | 0.009858 | 2.751755 | uid://A001/X1465/X388f | uid://A001/X1465/X3890 | uid://A002/Xe2eefc/X31df | A decisive answer on the carbon isotopic ratio... | S | TARGET | T | 20.837939 | 1.875000e+09 | A001:DA48 A002:DA44 A003:DV23 A004:DA56 A005:D... | F | 2021-03-10T20:24:07.000 | 1.608789 | [89.72..91.59GHz,1938.48kHz,494.6uJy/beam@10km... | 97.487731 | 5621.370692 | Martin, Sergio | T | Starbursts, star formation, Galaxy chemistry | Active galaxies | 2021-06-16T16:46:50.431 | |||||
1347 | 1348 | 2019.1.00130.S | NGC1068 | 40.669879 | -0.013289 | 1.609 | 91.51 | 93.39 | 92.45 | 1.873 | 1938.48 | 6.223 | 20.838 | 59.730 | 9.858 | 480.47 | 19.59 | uid://A001/X1465/X3890 | http://almascience.org/aq?member_ous_id=uid://... | text/html | 2019.1.00130.S | Public | 172.103977 | -51.933584 | ADS/JAO.ALMA#2019.1.00130.S | ALMA | JAO | ALMA | uid://A001/X1465/X3890 | cube | 2 | NGC1068 | 40.669879 | -0.013289 | 0.016592 | Polygon ICRS 40.669879 -0.021585 40.668325 -0.... | 1.608789 | 58790.229826 | 58802.118198 | 9918.720 | 9918.720 | 0.003210 | 0.003276 | 48173.837781 | /XX/YY/ | phot.flux.density;phys.polarization | 3 | 5.811652e+14 | <NA> | The 12C/13C isotopic ratio is a good tracer of... | NGC1068_a_03_TM1 | Krips, Melanie; Garcia-Burillo, Santiago; Mueh... | 0.480466 | 0.009858 | 2.751755 | uid://A001/X1465/X388f | uid://A001/X1465/X3890 | uid://A002/Xe2eefc/X31df | A decisive answer on the carbon isotopic ratio... | S | TARGET | T | 20.837939 | 1.875000e+09 | A001:DA48 A002:DA44 A003:DV23 A004:DA56 A005:D... | F | 2021-03-10T20:24:07.000 | 1.608789 | [89.72..91.59GHz,1938.48kHz,494.6uJy/beam@10km... | 97.487731 | 5621.370692 | Martin, Sergio | T | Starbursts, star formation, Galaxy chemistry | Active galaxies | 2021-06-16T16:46:50.431 | |||||
1348 | 1349 | 2019.1.00130.S | NGC1068 | 40.669879 | -0.013289 | 1.609 | 89.72 | 91.59 | 90.65 | 1.873 | 1938.48 | 6.345 | 20.838 | 59.730 | 9.858 | 494.60 | 19.97 | uid://A001/X1465/X3890 | http://almascience.org/aq?member_ous_id=uid://... | text/html | 2019.1.00130.S | Public | 172.103977 | -51.933584 | ADS/JAO.ALMA#2019.1.00130.S | ALMA | JAO | ALMA | uid://A001/X1465/X3890 | cube | 2 | NGC1068 | 40.669879 | -0.013289 | 0.016592 | Polygon ICRS 40.669879 -0.021585 40.668325 -0.... | 1.608789 | 58790.229826 | 58802.118198 | 9918.720 | 9918.720 | 0.003273 | 0.003342 | 47246.711574 | /XX/YY/ | phot.flux.density;phys.polarization | 3 | 5.811652e+14 | <NA> | The 12C/13C isotopic ratio is a good tracer of... | NGC1068_a_03_TM1 | Krips, Melanie; Garcia-Burillo, Santiago; Mueh... | 0.494603 | 0.009858 | 2.751755 | uid://A001/X1465/X388f | uid://A001/X1465/X3890 | uid://A002/Xe2eefc/X31df | A decisive answer on the carbon isotopic ratio... | S | TARGET | T | 20.837939 | 1.875000e+09 | A001:DA48 A002:DA44 A003:DV23 A004:DA56 A005:D... | F | 2021-03-10T20:24:07.000 | 1.608789 | [89.72..91.59GHz,1938.48kHz,494.6uJy/beam@10km... | 97.487731 | 5621.370692 | Martin, Sergio | T | Starbursts, star formation, Galaxy chemistry | Active galaxies | 2021-06-16T16:46:50.431 | |||||
1349 | 1350 | 2019.1.00130.S | NGC4418 | 186.727617 | -0.877642 | 2.537 | 89.43 | 91.30 | 90.36 | 1.873 | 1938.48 | 6.364 | 27.048 | 59.922 | 9.343 | 466.81 | 18.82 | uid://A001/X1465/X3898 | http://almascience.org/aq?member_ous_id=uid://... | text/html | 2019.1.00130.S | Public | 290.048542 | 61.379017 | ADS/JAO.ALMA#2019.1.00130.S | ALMA | JAO | ALMA | uid://A001/X1465/X3898 | cube | 2 | NGC4418 | 186.727617 | -0.877642 | 0.016645 | Polygon ICRS 186.727617 -0.869320 186.729177 -... | 2.537301 | 58810.445022 | 58842.573071 | 16632.000 | 16632.000 | 0.003284 | 0.003352 | 47103.985999 | /XX/YY/ | phot.flux.density;phys.polarization | 3 | 5.810791e+14 | <NA> | The 12C/13C isotopic ratio is a good tracer of... | NGC4418_a_03_TM1 | Krips, Melanie; Garcia-Burillo, Santiago; Mueh... | 0.466810 | 0.009343 | 2.977325 | uid://A001/X1465/X3897 | uid://A001/X1465/X3898 | uid://A002/Xe3f5bb/X3259 | A decisive answer on the carbon isotopic ratio... | S | TARGET | T | 27.047713 | 1.875000e+09 | A001:DA48 A002:DA44 A003:DV23 A004:DA56 A005:D... | F | 2021-04-07T00:23:33.000 | 2.537301 | [89.43..91.30GHz,1938.48kHz,466.8uJy/beam@10km... | 97.175661 | 5638.752118 | Martin, Sergio | T | Starbursts, star formation, Galaxy chemistry | Active galaxies | 2021-06-16T16:46:50.431 | |||||
1350 | 1351 | 2019.1.00130.S | NGC4945 | 196.363663 | -49.467900 | 2.523 | 101.78 | 103.65 | 102.72 | 1.873 | 1938.48 | 5.710 | 27.132 | 59.612 | 10.282 | 475.79 | 20.26 | uid://A001/X1465/X3888 | http://almascience.org/aq?member_ous_id=uid://... | text/html | 2019.1.00130.S | Public | 305.271559 | 13.340115 | ADS/JAO.ALMA#2019.1.00130.S | ALMA | JAO | ALMA | uid://A001/X1465/X3888 | cube | 2 | NGC4945 | 196.363663 | -49.467900 | 0.016559 | Polygon ICRS 196.371150 -49.461202 196.372949 ... | 2.522933 | 58830.525869 | 58831.619778 | 10765.440 | 10765.440 | 0.002892 | 0.002945 | 52507.569686 | /XX/YY/ | phot.flux.density;phys.polarization | 3 | 5.811169e+14 | <NA> | The 12C/13C isotopic ratio is a good tracer of... | NGC4945_a_03_TM1 | Krips, Melanie; Garcia-Burillo, Santiago; Mueh... | 0.475794 | 0.010282 | 3.740537 | uid://A001/X1465/X3887 | uid://A001/X1465/X3888 | uid://A002/Xe50c9e/X11047 | A decisive answer on the carbon isotopic ratio... | S | TARGET | T | 27.131876 | 1.875000e+09 | A001:DA48 A002:DA44 A003:DV23 A004:DA56 A005:D... | F | 2021-04-06T23:21:24.000 | 2.522933 | [89.90..91.77GHz,1938.48kHz,513.5uJy/beam@10km... | 97.681492 | 5609.869359 | Martin, Sergio | T | Starbursts, star formation, Galaxy chemistry | Active galaxies | 2021-06-16T16:46:50.431 | |||||
1351 | 1352 | 2019.1.00130.S | NGC1068 | 40.669879 | -0.013289 | 2.247 | 108.65 | 110.52 | 109.59 | 1.873 | 1938.48 | 5.349 | 21.118 | 55.719 | 21.996 | 960.67 | 42.25 | uid://A001/X1465/X3894 | http://almascience.org/aq?member_ous_id=uid://... | text/html | 2019.1.00130.S | Public | 172.103977 | -51.933584 | ADS/JAO.ALMA#2019.1.00130.S | ALMA | JAO | ALMA | uid://A001/X1465/X3894 | cube | 2 | NGC1068 | 40.669879 | -0.013289 | 0.015477 | Circle ICRS 40.669879 -0.013289 0.007739 | 2.246874 | 58803.153086 | 58803.168742 | 846.720 | 846.720 | 0.002712 | 0.002759 | 56045.630140 | /XX/YY/ | phot.flux.density;phys.polarization | 3 | 5.811774e+14 | <NA> | The 12C/13C isotopic ratio is a good tracer of... | NGC1068_b_03_TM1 | Krips, Melanie; Garcia-Burillo, Santiago; Mueh... | 0.960667 | 0.021996 | 5.121032 | uid://A001/X1465/X3893 | uid://A001/X1465/X3894 | uid://A002/Xe37224/X12917 | A decisive answer on the carbon isotopic ratio... | S | TARGET | T | 21.118095 | 1.875000e+09 | A001:DA48 A002:DA44 A003:DV23 A004:DA56 A005:D... | F | 2021-03-05T21:54:54.000 | 2.246874 | [96.60..98.47GHz,1938.48kHz,1mJy/beam@10km/s,4... | 104.505756 | 5257.484293 | Martin, Sergio | T | Starbursts, star formation, Galaxy chemistry | Active galaxies | 2021-06-16T16:46:50.431 | |||||
1352 | 1353 | 2019.1.00130.S | NGC1068 | 40.669879 | -0.013289 | 2.247 | 110.54 | 112.42 | 111.48 | 1.873 | 1938.48 | 5.257 | 21.118 | 55.719 | 21.996 | 1131.63 | 50.21 | uid://A001/X1465/X3894 | http://almascience.org/aq?member_ous_id=uid://... | text/html | 2019.1.00130.S | Public | 172.103977 | -51.933584 | ADS/JAO.ALMA#2019.1.00130.S | ALMA | JAO | ALMA | uid://A001/X1465/X3894 | cube | 2 | NGC1068 | 40.669879 | -0.013289 | 0.015477 | Circle ICRS 40.669879 -0.013289 0.007739 | 2.246874 | 58803.153086 | 58803.168742 | 846.720 | 846.720 | 0.002667 | 0.002712 | 57022.035883 | /XX/YY/ | phot.flux.density;phys.polarization | 3 | 5.811774e+14 | <NA> | The 12C/13C isotopic ratio is a good tracer of... | NGC1068_b_03_TM1 | Krips, Melanie; Garcia-Burillo, Santiago; Mueh... | 1.131625 | 0.021996 | 5.121032 | uid://A001/X1465/X3893 | uid://A001/X1465/X3894 | uid://A002/Xe37224/X12917 | A decisive answer on the carbon isotopic ratio... | S | TARGET | T | 21.118095 | 1.875000e+09 | A001:DA48 A002:DA44 A003:DV23 A004:DA56 A005:D... | F | 2021-03-05T21:54:54.000 | 2.246874 | [96.60..98.47GHz,1938.48kHz,1mJy/beam@10km/s,4... | 104.505756 | 5257.484293 | Martin, Sergio | T | Starbursts, star formation, Galaxy chemistry | Active galaxies | 2021-06-16T16:46:50.431 | |||||
1353 | 1354 | 2019.1.00130.S | NGC1068 | 40.669879 | -0.013289 | 2.247 | 98.29 | 100.16 | 99.23 | 1.873 | 1938.48 | 5.802 | 21.118 | 55.719 | 21.996 | 1007.18 | 42.54 | uid://A001/X1465/X3894 | http://almascience.org/aq?member_ous_id=uid://... | text/html | 2019.1.00130.S | Public | 172.103977 | -51.933584 | ADS/JAO.ALMA#2019.1.00130.S | ALMA | JAO | ALMA | uid://A001/X1465/X3894 | cube | 2 | NGC1068 | 40.669879 | -0.013289 | 0.015477 | Circle ICRS 40.669879 -0.013289 0.007739 | 2.246874 | 58803.153086 | 58803.168742 | 846.720 | 846.720 | 0.002993 | 0.003050 | 51667.340290 | /XX/YY/ | phot.flux.density;phys.polarization | 3 | 5.811774e+14 | <NA> | The 12C/13C isotopic ratio is a good tracer of... | NGC1068_b_03_TM1 | Krips, Melanie; Garcia-Burillo, Santiago; Mueh... | 1.007181 | 0.021996 | 5.121032 | uid://A001/X1465/X3893 | uid://A001/X1465/X3894 | uid://A002/Xe37224/X12917 | A decisive answer on the carbon isotopic ratio... | S | TARGET | T | 21.118095 | 1.875000e+09 | A001:DA48 A002:DA44 A003:DV23 A004:DA56 A005:D... | F | 2021-03-05T21:54:54.000 | 2.246874 | [96.60..98.47GHz,1938.48kHz,1mJy/beam@10km/s,4... | 104.505756 | 5257.484293 | Martin, Sergio | T | Starbursts, star formation, Galaxy chemistry | Active galaxies | 2021-06-16T16:46:50.431 | |||||
1354 | 1355 | 2019.1.00130.S | NGC4418 | 186.727617 | -0.877642 | 2.537 | 103.05 | 104.92 | 103.99 | 1.873 | 1938.48 | 5.639 | 27.048 | 59.922 | 9.343 | 436.95 | 18.72 | uid://A001/X1465/X3898 | http://almascience.org/aq?member_ous_id=uid://... | text/html | 2019.1.00130.S | Public | 290.048542 | 61.379017 | ADS/JAO.ALMA#2019.1.00130.S | ALMA | JAO | ALMA | uid://A001/X1465/X3898 | cube | 2 | NGC4418 | 186.727617 | -0.877642 | 0.016645 | Polygon ICRS 186.727617 -0.869320 186.729177 -... | 2.537301 | 58810.445022 | 58842.573071 | 16632.000 | 16632.000 | 0.002857 | 0.002909 | 53166.454513 | /XX/YY/ | phot.flux.density;phys.polarization | 3 | 5.810791e+14 | <NA> | The 12C/13C isotopic ratio is a good tracer of... | NGC4418_a_03_TM1 | Krips, Melanie; Garcia-Burillo, Santiago; Mueh... | 0.436953 | 0.009343 | 2.977325 | uid://A001/X1465/X3897 | uid://A001/X1465/X3898 | uid://A002/Xe3f5bb/X3259 | A decisive answer on the carbon isotopic ratio... | S | TARGET | T | 27.047713 | 1.875000e+09 | A001:DA48 A002:DA44 A003:DV23 A004:DA56 A005:D... | F | 2021-04-07T00:23:33.000 | 2.537301 | [89.43..91.30GHz,1938.48kHz,466.8uJy/beam@10km... | 97.175661 | 5638.752118 | Martin, Sergio | T | Starbursts, star formation, Galaxy chemistry | Active galaxies | 2021-06-16T16:46:50.431 | |||||
1355 | 1356 | 2019.1.00130.S | NGC4418 | 186.727617 | -0.877642 | 2.537 | 91.20 | 93.07 | 92.13 | 1.873 | 1938.48 | 6.243 | 27.048 | 59.922 | 9.343 | 459.55 | 18.71 | uid://A001/X1465/X3898 | http://almascience.org/aq?member_ous_id=uid://... | text/html | 2019.1.00130.S | Public | 290.048542 | 61.379017 | ADS/JAO.ALMA#2019.1.00130.S | ALMA | JAO | ALMA | uid://A001/X1465/X3898 | cube | 2 | NGC4418 | 186.727617 | -0.877642 | 0.016645 | Polygon ICRS 186.727617 -0.869320 186.729177 -... | 2.537301 | 58810.445022 | 58842.573071 | 16632.000 | 16632.000 | 0.003221 | 0.003287 | 48017.332095 | /XX/YY/ | phot.flux.density;phys.polarization | 3 | 5.810791e+14 | <NA> | The 12C/13C isotopic ratio is a good tracer of... | NGC4418_a_03_TM1 | Krips, Melanie; Garcia-Burillo, Santiago; Mueh... | 0.459546 | 0.009343 | 2.977325 | uid://A001/X1465/X3897 | uid://A001/X1465/X3898 | uid://A002/Xe3f5bb/X3259 | A decisive answer on the carbon isotopic ratio... | S | TARGET | T | 27.047713 | 1.875000e+09 | A001:DA48 A002:DA44 A003:DV23 A004:DA56 A005:D... | F | 2021-04-07T00:23:33.000 | 2.537301 | [89.43..91.30GHz,1938.48kHz,466.8uJy/beam@10km... | 97.175661 | 5638.752118 | Martin, Sergio | T | Starbursts, star formation, Galaxy chemistry | Active galaxies | 2021-06-16T16:46:50.431 | |||||
1356 | 1357 | 2019.1.00130.S | NGC4418 | 186.727617 | -0.877642 | 2.537 | 101.24 | 103.11 | 102.18 | 1.873 | 1938.48 | 5.740 | 27.048 | 59.922 | 9.343 | 437.00 | 18.56 | uid://A001/X1465/X3898 | http://almascience.org/aq?member_ous_id=uid://... | text/html | 2019.1.00130.S | Public | 290.048542 | 61.379017 | ADS/JAO.ALMA#2019.1.00130.S | ALMA | JAO | ALMA | uid://A001/X1465/X3898 | cube | 2 | NGC4418 | 186.727617 | -0.877642 | 0.016645 | Polygon ICRS 186.727617 -0.869320 186.729177 -... | 2.537301 | 58810.445022 | 58842.573071 | 16632.000 | 16632.000 | 0.002907 | 0.002961 | 52231.920422 | /XX/YY/ | phot.flux.density;phys.polarization | 3 | 5.810791e+14 | <NA> | The 12C/13C isotopic ratio is a good tracer of... | NGC4418_a_03_TM1 | Krips, Melanie; Garcia-Burillo, Santiago; Mueh... | 0.436998 | 0.009343 | 2.977325 | uid://A001/X1465/X3897 | uid://A001/X1465/X3898 | uid://A002/Xe3f5bb/X3259 | A decisive answer on the carbon isotopic ratio... | S | TARGET | T | 27.047713 | 1.875000e+09 | A001:DA48 A002:DA44 A003:DV23 A004:DA56 A005:D... | F | 2021-04-07T00:23:33.000 | 2.537301 | [89.43..91.30GHz,1938.48kHz,466.8uJy/beam@10km... | 97.175661 | 5638.752118 | Martin, Sergio | T | Starbursts, star formation, Galaxy chemistry | Active galaxies | 2021-06-16T16:46:50.431 | |||||
1357 | 1358 | 2019.1.00130.S | NGC1068 | 40.669879 | -0.013289 | 2.247 | 96.60 | 98.47 | 97.53 | 1.873 | 1938.48 | 5.902 | 21.118 | 55.719 | 21.996 | 1015.52 | 42.52 | uid://A001/X1465/X3894 | http://almascience.org/aq?member_ous_id=uid://... | text/html | 2019.1.00130.S | Public | 172.103977 | -51.933584 | ADS/JAO.ALMA#2019.1.00130.S | ALMA | JAO | ALMA | uid://A001/X1465/X3894 | cube | 2 | NGC1068 | 40.669879 | -0.013289 | 0.015477 | Circle ICRS 40.669879 -0.013289 0.007739 | 2.246874 | 58803.153086 | 58803.168742 | 846.720 | 846.720 | 0.003045 | 0.003104 | 50793.714099 | /XX/YY/ | phot.flux.density;phys.polarization | 3 | 5.811774e+14 | <NA> | The 12C/13C isotopic ratio is a good tracer of... | NGC1068_b_03_TM1 | Krips, Melanie; Garcia-Burillo, Santiago; Mueh... | 1.015517 | 0.021996 | 5.121032 | uid://A001/X1465/X3893 | uid://A001/X1465/X3894 | uid://A002/Xe37224/X12917 | A decisive answer on the carbon isotopic ratio... | S | TARGET | T | 21.118095 | 1.875000e+09 | A001:DA48 A002:DA44 A003:DV23 A004:DA56 A005:D... | F | 2021-03-05T21:54:54.000 | 2.246874 | [96.60..98.47GHz,1938.48kHz,1mJy/beam@10km/s,4... | 104.505756 | 5257.484293 | Martin, Sergio | T | Starbursts, star formation, Galaxy chemistry | Active galaxies | 2021-06-16T16:46:50.431 | |||||
1358 | 1359 | 2019.1.00130.S | NGC4945 | 196.363663 | -49.467900 | 2.523 | 103.59 | 105.46 | 104.52 | 1.873 | 1938.48 | 5.610 | 27.132 | 59.612 | 10.282 | 478.30 | 20.54 | uid://A001/X1465/X3888 | http://almascience.org/aq?member_ous_id=uid://... | text/html | 2019.1.00130.S | Public | 305.271559 | 13.340115 | ADS/JAO.ALMA#2019.1.00130.S | ALMA | JAO | ALMA | uid://A001/X1465/X3888 | cube | 2 | NGC4945 | 196.363663 | -49.467900 | 0.016559 | Polygon ICRS 196.371150 -49.461202 196.372949 ... | 2.522933 | 58830.525869 | 58831.619778 | 10765.440 | 10765.440 | 0.002843 | 0.002894 | 53440.185286 | /XX/YY/ | phot.flux.density;phys.polarization | 3 | 5.811169e+14 | <NA> | The 12C/13C isotopic ratio is a good tracer of... | NGC4945_a_03_TM1 | Krips, Melanie; Garcia-Burillo, Santiago; Mueh... | 0.478302 | 0.010282 | 3.740537 | uid://A001/X1465/X3887 | uid://A001/X1465/X3888 | uid://A002/Xe50c9e/X11047 | A decisive answer on the carbon isotopic ratio... | S | TARGET | T | 27.131876 | 1.875000e+09 | A001:DA48 A002:DA44 A003:DV23 A004:DA56 A005:D... | F | 2021-04-06T23:21:24.000 | 2.522933 | [89.90..91.77GHz,1938.48kHz,513.5uJy/beam@10km... | 97.681492 | 5609.869359 | Martin, Sergio | T | Starbursts, star formation, Galaxy chemistry | Active galaxies | 2021-06-16T16:46:50.431 | |||||
1359 | 1360 | 2019.1.00130.S | NGC4945 | 196.363663 | -49.467900 | 2.523 | 89.90 | 91.77 | 90.84 | 1.873 | 1938.48 | 6.332 | 27.132 | 59.612 | 10.282 | 513.50 | 20.76 | uid://A001/X1465/X3888 | http://almascience.org/aq?member_ous_id=uid://... | text/html | 2019.1.00130.S | Public | 305.271559 | 13.340115 | ADS/JAO.ALMA#2019.1.00130.S | ALMA | JAO | ALMA | uid://A001/X1465/X3888 | cube | 2 | NGC4945 | 196.363663 | -49.467900 | 0.016559 | Polygon ICRS 196.371150 -49.461202 196.372949 ... | 2.522933 | 58830.525869 | 58831.619778 | 10765.440 | 10765.440 | 0.003267 | 0.003335 | 47345.641143 | /XX/YY/ | phot.flux.density;phys.polarization | 3 | 5.811169e+14 | <NA> | The 12C/13C isotopic ratio is a good tracer of... | NGC4945_a_03_TM1 | Krips, Melanie; Garcia-Burillo, Santiago; Mueh... | 0.513502 | 0.010282 | 3.740537 | uid://A001/X1465/X3887 | uid://A001/X1465/X3888 | uid://A002/Xe50c9e/X11047 | A decisive answer on the carbon isotopic ratio... | S | TARGET | T | 27.131876 | 1.875000e+09 | A001:DA48 A002:DA44 A003:DV23 A004:DA56 A005:D... | F | 2021-04-06T23:21:24.000 | 2.522933 | [89.90..91.77GHz,1938.48kHz,513.5uJy/beam@10km... | 97.681492 | 5609.869359 | Martin, Sergio | T | Starbursts, star formation, Galaxy chemistry | Active galaxies | 2021-06-16T16:46:50.431 | |||||
1360 | 1361 | 2019.1.00130.S | NGC4418 | 186.727617 | -0.877642 | 1.357 | 110.17 | 112.05 | 111.11 | 1.873 | 1938.48 | 5.274 | 24.940 | 55.903 | 10.485 | 465.01 | 20.60 | uid://A001/X1465/X389c | http://almascience.org/aq?member_ous_id=uid://... | text/html | 2019.1.00130.S | Public | 290.048542 | 61.379017 | ADS/JAO.ALMA#2019.1.00130.S | ALMA | JAO | ALMA | uid://A001/X1465/X389c | cube | 2 | NGC4418 | 186.727617 | -0.877642 | 0.015529 | Polygon ICRS 186.727617 -0.869878 186.729072 -... | 1.356746 | 58787.582055 | 58825.599964 | 4898.880 | 4898.880 | 0.002676 | 0.002721 | 56840.228703 | /XX/YY/ | phot.flux.density;phys.polarization | 3 | 5.810830e+14 | <NA> | The 12C/13C isotopic ratio is a good tracer of... | NGC4418_b_03_TM1 | Krips, Melanie; Garcia-Burillo, Santiago; Mueh... | 0.465008 | 0.010485 | 2.368327 | uid://A001/X1465/X389b | uid://A001/X1465/X389c | uid://A002/Xe2ada9/X15596 | A decisive answer on the carbon isotopic ratio... | S | TARGET | T | 24.939648 | 1.875000e+09 | A001:DA48 A002:DA44 A003:DV23 A004:DA56 A005:D... | F | 2021-03-17T19:10:59.000 | 1.356746 | [96.28..98.15GHz,1938.48kHz,511.7uJy/beam@10km... | 104.161888 | 5274.300699 | Martin, Sergio | T | Starbursts, star formation, Galaxy chemistry | Active galaxies | 2021-06-16T16:46:50.431 |
1361 rows × 81 columns
The alminer.summary
function will print a summary of the observations. This is done by default when the query is run, but it's a useful function if the results are filtered further, as shown in the next section.
summary
functionalminer.summary(observations)
-------------------------------- Number of projects = 47 Number of observations = 339 Number of unique subbands = 1162 Total number of subbands = 1361 63 target(s) with ALMA data = ['LESS J0332-2756', 'PKS1830-211', 'ngc4418', 'NGC7469', 'NGC_1097', 'Arp220', 'NGC_5253', 'M83', 'NGC253', 'NGC1266', 'vv114', 'Mystery_Object', 'Sgr_A_star', 'SDSS_J080430.99+360718.1', 'ngc_3256', 'NGC_3256', 'NGC_55', 'ngc3256', 'NGC4418', 'NGC_3627_BE', 'circinus', 'IRAS_F16399-0937', 'ngc6240', 'ngc613', 'n613', 'ngc253', 'N159-E', 'N159-W', 'N159-W_south', 'm83', 'IRAS_13120-5453', 'ngc4945', 'HE1353-1917', 'HE0108-4743', 'HE1108-2813', 'HE1029-1831', 'HE0433-1028', 'Y052343.48-680033.9', 'Y045406.43-664601.4', 'Y045358.57-691106.7', 'Y051912.27-690907.2', 'Y045100.16-691934.4', 'Y052210.08-673459.6', 'Y052423.39-693904.7', 'ST6', 'Y051916.87-693757.5', 'Y054826.21-700850.2', 'Y050953.89-685336.7', 'Y052333.40-693712.1', 'Y053952.11-710930.7', 'Y045622.61-663656.9', 'Y054248.90-694446.3', 'Y054629.32-693514.2', 'Y051344.99-693510.6', 'Y050355.87-672045.1', 'Y044854.41-690948.3', 'ST10', 'ngc4526', 'Cloverleaf', 'ngc7465', 'NGC_253', 'NGC4945', 'NGC1068'] --------------------------------
For big tables, it is useful to avoid printing the list of target names in the summary. This can be done by setting print_targets=False.
alminer.summary(observations, print_targets=False)
-------------------------------- Number of projects = 47 Number of observations = 339 Number of unique subbands = 1162 Total number of subbands = 1361 Total number of targets with ALMA data = 63 --------------------------------
The search results can be further narrowed down by using PANDAS DataFrame functions. See also this introduction to data structures. For example, you can use your_query.columns
to get a list of all columns in the DataFrame.
To get the description and units of any column use the function alminer.get_info('column_name')
where column_name is the name of the column.
get_info
functionLet's first check what the description and units of ang_res_arcsec column are:
alminer.get_info('ang_res_arcsec')
-------------------------------- Column: ang_res_arcsec -------------------------------- Description: typical spatial resolution Units: arcsec --------------------------------
Now we can do the some further filtering, say to only keep observations with angular resolutions < 0.5":
selected = observations[observations['ang_res_arcsec'] < 0.5]
and print the summary:
alminer.summary(selected, print_targets=False)
-------------------------------- Number of projects = 23 Number of observations = 121 Number of unique subbands = 367 Total number of subbands = 484 Total number of targets with ALMA data = 41 --------------------------------
selected = observations[(observations['ang_res_arcsec'] < 0.5) &
(observations['vel_res_kms'] < 1.0)]
alminer.summary(selected, print_targets=False)
-------------------------------- Number of projects = 9 Number of observations = 48 Number of unique subbands = 65 Total number of subbands = 109 Total number of targets with ALMA data = 26 --------------------------------
freq = 220.5
selected = observations[(observations["min_freq_GHz"] < freq) &
(observations["max_freq_GHz"] > freq)]
alminer.summary(selected, print_targets=False)
-------------------------------- Number of projects = 6 Number of observations = 7 Number of unique subbands = 7 Total number of subbands = 7 Total number of targets with ALMA data = 5 --------------------------------
An alternative to the last example in the previous section is the alminer.line_coverage
function which determines how many targets were observed at a given frequency with the option to include a redshift for the line of interest to be taken into account. Some notes:
line_coverage
functionmyline_obs = alminer.line_coverage(observations,
line_freq=220.5,
z=0,
line_name="My favourite line",
print_targets=True)
-------------------------------- Summary of 'My favourite line' observations at 220.5 GHz -------------------------------- Number of projects = 6 Number of observations = 7 Number of unique subbands = 7 Total number of subbands = 7 5 target(s) with ALMA data = ['Arp220', 'ngc_3256', 'IRAS_13120-5453', 'ngc253', 'NGC_253'] --------------------------------
myline_obs = alminer.line_coverage(observations,
line_freq=400.0,
z=0.5,
line_name="My favourite line",
print_targets=True)
-------------------------------- Summary of 'My favourite line' observations at 400.0 GHz (266.667 GHz at z=0.5) -------------------------------- Number of projects = 8 Number of observations = 10 Number of unique subbands = 11 Total number of subbands = 11 6 target(s) with ALMA data = ['ngc4418', 'Arp220', 'ngc_3256', 'circinus', 'ngc4945', 'ngc253'] --------------------------------
The alminer.CO_lines
function determines how many CO, 13CO, and C18O lines were observed in the provided DataFrame and returns a DataFrame containing all observations of these transitions.
CO_lines
functionCO_obs = alminer.CO_lines(observations, print_targets=False)
-------------------------------- Summary of 'CO (1-0)' observations at 115.271 GHz -------------------------------- Number of projects = 4 Number of observations = 5 Number of unique subbands = 4 Total number of subbands = 5 Total number of targets with ALMA data = 3 -------------------------------- -------------------------------- Summary of 'CO (2-1)' observations at 230.538 GHz -------------------------------- Number of projects = 10 Number of observations = 13 Number of unique subbands = 13 Total number of subbands = 13 Total number of targets with ALMA data = 8 -------------------------------- -------------------------------- Summary of 'CO (3-2)' observations at 345.796 GHz -------------------------------- Number of projects = 3 Number of observations = 5 Number of unique subbands = 5 Total number of subbands = 5 Total number of targets with ALMA data = 4 -------------------------------- -------------------------------- Summary of 'CO (4-3)' observations at 461.041 GHz -------------------------------- No observations found. -------------------------------- -------------------------------- Summary of 'CO (5-4)' observations at 576.268 GHz -------------------------------- No observations found. -------------------------------- -------------------------------- Summary of 'CO (6-5)' observations at 691.473 GHz -------------------------------- No observations found. -------------------------------- -------------------------------- Summary of 'CO (7-6)' observations at 806.652 GHz -------------------------------- No observations found. -------------------------------- -------------------------------- Summary of 'CO (8-7)' observations at 921.8 GHz -------------------------------- No observations found. -------------------------------- -------------------------------- Summary of '13CO (1-0)' observations at 110.201 GHz -------------------------------- Number of projects = 18 Number of observations = 23 Number of unique subbands = 23 Total number of subbands = 25 Total number of targets with ALMA data = 17 -------------------------------- -------------------------------- Summary of '13CO (2-1)' observations at 220.399 GHz -------------------------------- Number of projects = 6 Number of observations = 7 Number of unique subbands = 7 Total number of subbands = 7 Total number of targets with ALMA data = 5 -------------------------------- -------------------------------- Summary of '13CO (3-2)' observations at 330.588 GHz -------------------------------- Number of projects = 2 Number of observations = 5 Number of unique subbands = 5 Total number of subbands = 5 Total number of targets with ALMA data = 4 -------------------------------- -------------------------------- Summary of '13CO (4-3)' observations at 440.765 GHz -------------------------------- Number of projects = 1 Number of observations = 1 Number of unique subbands = 1 Total number of subbands = 1 Total number of targets with ALMA data = 1 -------------------------------- -------------------------------- Summary of '13CO (5-4)' observations at 550.926 GHz -------------------------------- No observations found. -------------------------------- -------------------------------- Summary of '13CO (6-5)' observations at 661.067 GHz -------------------------------- No observations found. -------------------------------- -------------------------------- Summary of '13CO (7-6)' observations at 771.184 GHz -------------------------------- No observations found. -------------------------------- -------------------------------- Summary of '13CO (8-7)' observations at 881.273 GHz -------------------------------- No observations found. -------------------------------- -------------------------------- Summary of 'C18O (1-0)' observations at 109.782 GHz -------------------------------- Number of projects = 19 Number of observations = 24 Number of unique subbands = 25 Total number of subbands = 27 Total number of targets with ALMA data = 18 -------------------------------- -------------------------------- Summary of 'C18O (2-1)' observations at 219.56 GHz -------------------------------- Number of projects = 7 Number of observations = 9 Number of unique subbands = 12 Total number of subbands = 12 Total number of targets with ALMA data = 6 -------------------------------- -------------------------------- Summary of 'C18O (3-2)' observations at 329.331 GHz -------------------------------- Number of projects = 2 Number of observations = 3 Number of unique subbands = 3 Total number of subbands = 3 Total number of targets with ALMA data = 2 -------------------------------- -------------------------------- Summary of 'C18O (4-3)' observations at 439.089 GHz -------------------------------- No observations found. -------------------------------- -------------------------------- Summary of 'C18O (5-4)' observations at 548.831 GHz -------------------------------- No observations found. -------------------------------- -------------------------------- Summary of 'C18O (6-5)' observations at 658.553 GHz -------------------------------- No observations found. -------------------------------- -------------------------------- Summary of 'C18O (7-6)' observations at 768.252 GHz -------------------------------- No observations found. -------------------------------- -------------------------------- Summary of 'C18O (8-7)' observations at 877.922 GHz -------------------------------- No observations found. --------------------------------
CO_obs = alminer.CO_lines(observations, z=1, print_targets=False)
-------------------------------- Summary of 'CO (1-0)' observations at 115.2712018 GHz (57.636 GHz at z=1) -------------------------------- No observations found. -------------------------------- -------------------------------- Summary of 'CO (2-1)' observations at 230.538 GHz (115.269 GHz at z=1) -------------------------------- Number of projects = 4 Number of observations = 5 Number of unique subbands = 4 Total number of subbands = 5 Total number of targets with ALMA data = 3 -------------------------------- -------------------------------- Summary of 'CO (3-2)' observations at 345.7959899 GHz (172.898 GHz at z=1) -------------------------------- Number of projects = 2 Number of observations = 3 Number of unique subbands = 3 Total number of subbands = 3 Total number of targets with ALMA data = 2 -------------------------------- -------------------------------- Summary of 'CO (4-3)' observations at 461.0407682 GHz (230.52 GHz at z=1) -------------------------------- Number of projects = 10 Number of observations = 13 Number of unique subbands = 13 Total number of subbands = 13 Total number of targets with ALMA data = 8 -------------------------------- -------------------------------- Summary of 'CO (5-4)' observations at 576.2679305 GHz (288.134 GHz at z=1) -------------------------------- Number of projects = 3 Number of observations = 6 Number of unique subbands = 6 Total number of subbands = 6 Total number of targets with ALMA data = 3 -------------------------------- -------------------------------- Summary of 'CO (6-5)' observations at 691.4730763 GHz (345.737 GHz at z=1) -------------------------------- Number of projects = 3 Number of observations = 5 Number of unique subbands = 5 Total number of subbands = 5 Total number of targets with ALMA data = 4 -------------------------------- -------------------------------- Summary of 'CO (7-6)' observations at 806.651806 GHz (403.326 GHz at z=1) -------------------------------- No observations found. -------------------------------- -------------------------------- Summary of 'CO (8-7)' observations at 921.7997 GHz (460.9 GHz at z=1) -------------------------------- No observations found. -------------------------------- -------------------------------- Summary of '13CO (1-0)' observations at 110.2013218 GHz (55.101 GHz at z=1) -------------------------------- No observations found. -------------------------------- -------------------------------- Summary of '13CO (2-1)' observations at 220.3986195 GHz (110.199 GHz at z=1) -------------------------------- Number of projects = 18 Number of observations = 23 Number of unique subbands = 23 Total number of subbands = 25 Total number of targets with ALMA data = 17 -------------------------------- -------------------------------- Summary of '13CO (3-2)' observations at 330.5878671 GHz (165.294 GHz at z=1) -------------------------------- Number of projects = 1 Number of observations = 2 Number of unique subbands = 2 Total number of subbands = 2 Total number of targets with ALMA data = 1 -------------------------------- -------------------------------- Summary of '13CO (4-3)' observations at 440.7651735 GHz (220.383 GHz at z=1) -------------------------------- Number of projects = 6 Number of observations = 7 Number of unique subbands = 7 Total number of subbands = 7 Total number of targets with ALMA data = 5 -------------------------------- -------------------------------- Summary of '13CO (5-4)' observations at 550.9262851 GHz (275.463 GHz at z=1) -------------------------------- Number of projects = 3 Number of observations = 4 Number of unique subbands = 4 Total number of subbands = 4 Total number of targets with ALMA data = 3 -------------------------------- -------------------------------- Summary of '13CO (6-5)' observations at 661.0672766 GHz (330.534 GHz at z=1) -------------------------------- Number of projects = 2 Number of observations = 5 Number of unique subbands = 5 Total number of subbands = 5 Total number of targets with ALMA data = 4 -------------------------------- -------------------------------- Summary of '13CO (7-6)' observations at 771.184125 GHz (385.592 GHz at z=1) -------------------------------- No observations found. -------------------------------- -------------------------------- Summary of '13CO (8-7)' observations at 881.272808 GHz (440.636 GHz at z=1) -------------------------------- Number of projects = 1 Number of observations = 1 Number of unique subbands = 1 Total number of subbands = 1 Total number of targets with ALMA data = 1 -------------------------------- -------------------------------- Summary of 'C18O (1-0)' observations at 109.7821734 GHz (54.891 GHz at z=1) -------------------------------- No observations found. -------------------------------- -------------------------------- Summary of 'C18O (2-1)' observations at 219.5603541 GHz (109.78 GHz at z=1) -------------------------------- Number of projects = 19 Number of observations = 24 Number of unique subbands = 25 Total number of subbands = 27 Total number of targets with ALMA data = 18 -------------------------------- -------------------------------- Summary of 'C18O (3-2)' observations at 329.3305525 GHz (164.665 GHz at z=1) -------------------------------- Number of projects = 1 Number of observations = 2 Number of unique subbands = 2 Total number of subbands = 2 Total number of targets with ALMA data = 1 -------------------------------- -------------------------------- Summary of 'C18O (4-3)' observations at 439.0887658 GHz (219.544 GHz at z=1) -------------------------------- Number of projects = 7 Number of observations = 9 Number of unique subbands = 12 Total number of subbands = 12 Total number of targets with ALMA data = 6 -------------------------------- -------------------------------- Summary of 'C18O (5-4)' observations at 548.8310055 GHz (274.416 GHz at z=1) -------------------------------- Number of projects = 2 Number of observations = 3 Number of unique subbands = 3 Total number of subbands = 3 Total number of targets with ALMA data = 2 -------------------------------- -------------------------------- Summary of 'C18O (6-5)' observations at 658.5532782 GHz (329.277 GHz at z=1) -------------------------------- Number of projects = 2 Number of observations = 3 Number of unique subbands = 3 Total number of subbands = 3 Total number of targets with ALMA data = 2 -------------------------------- -------------------------------- Summary of 'C18O (7-6)' observations at 768.2515933 GHz (384.126 GHz at z=1) -------------------------------- No observations found. -------------------------------- -------------------------------- Summary of 'C18O (8-7)' observations at 877.9219553 GHz (438.961 GHz at z=1) -------------------------------- No observations found. --------------------------------
This section introduces all the plotting functions that help visualise the queried observations:
The alminer.plot_overview
function plots a summary of the observed frequencies, angular resolution, largest angular scales (LAS), and frequency and velocity resolutions.
Note: The histogram of observed frequencies displays the distribution of central frequencies and also depends on the choice of binning. To get an overview plot for a specific frequency, use alminer.plot_observations
and alminer.plot_line_overview
(see examples below).
plot_overview
functionalminer.plot_overview(observations, savefig='alma_galaxy_chemistry')
The alminer.plot_line_overview
function creates overview plots of observed frequencies, angular resolution, LAS, frequency and velocity resolutions for the input DataFrame, and highlights the observations of a give frequency (redshift if the z parameter is set) specified by the user.
plot_line_overview
functionalminer.plot_line_overview(observations, line_freq=100.0)
alminer.plot_line_overview(observations, line_freq=400.0, z=2)
The alminer.plot_bands
function creates detailed plots of observed frequencies in each band.
plot_bands
functionalminer.plot_bands(observations, mark_CO=True, z=0.5)
alminer.plot_bands(observations, mark_freq=[106.5, 245.0, 366.3])
The alminer.plot_observations
function creates a detailed plot of observations in each band showing the exact observed frequency ranges. Observation numbers are the input DataFrame's index values.
plot_observations
functionalminer.plot_observations(observations, mark_CO=True)
alminer.plot_observations(observations, mark_freq=[106.5, 245.0, 366.3])
The alminer.plot_sky
function creates a plot of the distribution of targets on the sky.
plot_sky
functionalminer.plot_sky(observations)
The alminer.save_table
function writes the provided DataFrame to a table in CSV format in the 'tables' folder within the current working directory. If the 'tables' folder does not exist, it will be created.
save_table
functionalminer.save_table(observations, filename="galaxy_chemistry")
The alminer.save_source_reports
function creates overview plots of observed frequencies, angular resolution, LAS, frequency and velocity resolutions for each source in the provided DataFrame and saves them in PDF format in the 'reports' folder in the current working directory. If the 'reports' folder does not exist, it will be created. The reports are named after the target names.
Note: Currently, the grouping is done based on ALMA target names, so the same source with a slighly different naming schemes will be treated as separate targets.
save_source_reports
functionLet's first narrow down our large query to a smaller subset to only a range of frequencies (Band 3) and angular resolutions < 0.5":
selected = observations[(observations["min_freq_GHz"] > 80.0) &
(observations["max_freq_GHz"] < 115.0) &
(observations["ang_res_arcsec"] < 0.5)]
alminer.summary(selected)
-------------------------------- Number of projects = 8 Number of observations = 21 Number of unique subbands = 81 Total number of subbands = 81 8 target(s) with ALMA data = ['NGC7469', 'NGC1266', 'Arp220', 'ngc6240', 'IRAS_F16399-0937', 'n613', 'NGC4418', 'Cloverleaf'] --------------------------------
Now we can create and save plots for each source, with CO and its isotopologues marked:
alminer.save_source_reports(selected, mark_CO=True)
The alminer.download_data
function allows the user to download the data from the archive directly to a location on the local disk.
download_data
function# This step is not necessary, but currently pyvo.dal.query contains
# an Astropy deprecation warning that we prefer to ignore
import warnings
warnings.filterwarnings("ignore")
alminer.download_data(selected, fitsonly=False, dryrun=True, location='./data', print_urls=False)
================================ This is a dryrun. To begin download, set dryrun=False. ================================ Download location = ./data Total number of Member OUSs to download = 21 Selected Member OUSs: ['uid://A002/X6444ba/X17d', 'uid://A001/X121/X3d8', 'uid://A001/X121/X3d5', 'uid://A001/X121/X3d2', 'uid://A001/X121/X3cf', 'uid://A001/X2fe/Xcce', 'uid://A001/X2fe/Xcda', 'uid://A001/X2fe/Xcd6', 'uid://A001/X2fe/Xcde', 'uid://A001/X2fe/Xcd2', 'uid://A001/X2fe/X728', 'uid://A001/X2fe/X724', 'uid://A001/X2fe/X738', 'uid://A001/X2fe/X734', 'uid://A001/X5a4/X155', 'uid://A001/X87d/X1f5', 'uid://A001/X87d/X1fb', 'uid://A001/X87d/X207', 'uid://A001/X1290/X17', 'uid://A001/X1288/X6c2', 'uid://A001/X1288/X6be'] Number of files to download = 114 Needed disk space = 3991.3 GB --------------------------------
alminer.download_data(selected, fitsonly=True, dryrun=True, location='./data',
filename_must_include=['_sci', '.pbcor', 'cont'], print_urls=True)
================================ This is a dryrun. To begin download, set dryrun=False. ================================ Download location = ./data Total number of Member OUSs to download = 21 Selected Member OUSs: ['uid://A002/X6444ba/X17d', 'uid://A001/X121/X3d8', 'uid://A001/X121/X3d5', 'uid://A001/X121/X3d2', 'uid://A001/X121/X3cf', 'uid://A001/X2fe/Xcce', 'uid://A001/X2fe/Xcda', 'uid://A001/X2fe/Xcd6', 'uid://A001/X2fe/Xcde', 'uid://A001/X2fe/Xcd2', 'uid://A001/X2fe/X728', 'uid://A001/X2fe/X724', 'uid://A001/X2fe/X738', 'uid://A001/X2fe/X734', 'uid://A001/X5a4/X155', 'uid://A001/X87d/X1f5', 'uid://A001/X87d/X1fb', 'uid://A001/X87d/X207', 'uid://A001/X1290/X17', 'uid://A001/X1288/X6c2', 'uid://A001/X1288/X6be'] Number of files to download = 19 Needed disk space = 0.3 GB File URLs to download = https://almascience.eso.org/dataPortal/member.uid___A001_X2fe_Xcda.Arp220_sci.spw25_27_29_31.cont.I.tt0.pbcor.fits https://almascience.eso.org/dataPortal/member.uid___A001_X2fe_Xcda.Arp220_sci.spw25_27_29_31.cont.I.tt1.pbcor.fits https://almascience.eso.org/dataPortal/member.uid___A001_X2fe_X728.ngc6240_sci.spw19_25_27_29.cont.I.tt0.pbcor.fits https://almascience.eso.org/dataPortal/member.uid___A001_X2fe_X728.ngc6240_sci.spw19_25_27_29.cont.I.tt1.pbcor.fits https://almascience.eso.org/dataPortal/member.uid___A001_X2fe_X724.ngc6240_sci.spw25_27_29_31.cont.I.tt0.pbcor.fits https://almascience.eso.org/dataPortal/member.uid___A001_X2fe_X724.ngc6240_sci.spw25_27_29_31.cont.I.tt1.pbcor.fits https://almascience.eso.org/dataPortal/member.uid___A001_X2fe_X738.IRAS_F16399-0937_sci.spw25_27_29_31.cont.I.tt0.pbcor.fits https://almascience.eso.org/dataPortal/member.uid___A001_X2fe_X738.IRAS_F16399-0937_sci.spw25_27_29_31.cont.I.tt1.pbcor.fits https://almascience.eso.org/dataPortal/member.uid___A001_X5a4_X155.n613_sci.spw25_27_29_31_33.cont.I.tt0.pbcor.fits https://almascience.eso.org/dataPortal/member.uid___A001_X5a4_X155.n613_sci.spw25_27_29_31_33.cont.I.tt1.pbcor.fits https://almascience.eso.org/dataPortal/member.uid___A001_X87d_X1f5.NGC4418_sci.spw25_27_29_31.cont.I.tt0.pbcor.fits https://almascience.eso.org/dataPortal/member.uid___A001_X87d_X1f5.NGC4418_sci.spw25_27_29_31.cont.I.tt1.pbcor.fits https://almascience.eso.org/dataPortal/member.uid___A001_X87d_X1fb.NGC4418_sci.spw25_27_29_31.cont.I.tt0.pbcor.fits https://almascience.eso.org/dataPortal/member.uid___A001_X87d_X1fb.NGC4418_sci.spw25_27_29_31.cont.I.tt1.pbcor.fits https://almascience.eso.org/dataPortal/member.uid___A001_X87d_X207.NGC4418_sci.spw25_27_29_31.cont.I.tt0.pbcor.fits https://almascience.eso.org/dataPortal/member.uid___A001_X87d_X207.NGC4418_sci.spw25_27_29_31.cont.I.tt1.pbcor.fits https://almascience.eso.org/dataPortal/member.uid___A001_X1290_X17.NGC7469_sci.spw19_21.cont.I.pbcor.fits https://almascience.eso.org/dataPortal/member.uid___A001_X1288_X6c2.Cloverleaf_sci.spw22_24_26.cont.I.pbcor.fits https://almascience.eso.org/dataPortal/member.uid___A001_X1288_X6be.Cloverleaf_sci.spw22_24_26.cont.I.pbcor.fits --------------------------------
You can use Astronomical Data Query Language (ADQL) to create more complex queries relevant for your work.
The ALminer querying functions provide an option to print the query string that was used to search the ALMA archive for the user by setting print_query parameter to True.
Once you have created the query string of interest, you can run it using the alminer.run_query
function.
run_query
functionobs = alminer.keysearch({'proposal_abstract': ['planet forming disk']},
print_targets=False, print_query=True)
================================ alminer.keysearch results ================================ Your query is: SELECT * FROM ivoa.obscore WHERE ((LOWER(proposal_abstract) LIKE '%planet%' AND LOWER(proposal_abstract) LIKE '%forming%' AND LOWER(proposal_abstract) LIKE '%disk%')) AND (LOWER(data_rights) LIKE '%public%') AND (LOWER(scan_intent) LIKE '%target%') ORDER BY proposal_id -------------------------------- Number of projects = 116 Number of observations = 1776 Number of unique subbands = 974 Total number of subbands = 8686 Total number of targets with ALMA data = 1234 --------------------------------
In the previous example, we searched the ALMA archive for projects with the words 'planet' AND 'forming' AND 'disk' in their abstracts. But let's say you want to search for the phrase 'planet forming disk' rather than the words individually.
You can modify the query string accordingly:
query_str = "SELECT * FROM ivoa.obscore WHERE ((LOWER(proposal_abstract) LIKE '%planet forming disk%')) AND (LOWER(data_rights) LIKE '%public%') AND (LOWER(scan_intent) LIKE '%target%') ORDER BY proposal_id"
And run the query
myquery = alminer.run_query(query_str)
To make use of other alminer
functions, the resulting DataFrame returned from running your query has to be converted to alminer
format where a few useful columns are added to the DataFrame. This can be done through the alminer.filter_results
function.
filter_results
functionmyquery_obs = alminer.filter_results(myquery)
-------------------------------- Number of projects = 3 Number of observations = 6 Number of unique subbands = 13 Total number of subbands = 28 6 target(s) with ALMA data = ['Sz_91', 'AA_Tau', 'L1448-mm', 'HH211', 'B1-c', 'B5-IRS1'] --------------------------------
Now you can use all the analysis and plotting routines presented before on these observations.
catalog
functionconesearch
functionkeysearch
functiontarget
functionkeysearch
function and query the archive using the 'target_name' keyword (e.g. keysearch({'target_name': sources})
).CO_lines
functionexplore
functionget_info
functionline_coverage
functionsummary
functionplot_bands
functionplot_line_overview
functionplot_observations
functionplot_overview
functionplot_sky
functionsave_source_reports
functionsave_table
functiondownload_data
functionfilter_results
functionrun_query
function