# Observing Run Preparation Module¶

Lecturer: Robert Quimby
Jupyter Notebook Author: Shubham Srivastav & Cameron Hummels

This is a Jupyter notebook lesson taken from the GROWTH Winter School 2018. For other lessons and their accompanying lectures, please see: http://growth.caltech.edu/growth-astro-school-2018-resources.html

## Objective¶

Demonstrate how to plan observations prior to an observing run.

## Key steps¶

• Select targets
• Get visibility and airmass plots
• Get moon separation angles
• Calculate exposure times for targets

## Required dependencies¶

See GROWTH school webpage for detailed instructions on how to install these modules and packages. Nominally, you should be able to install the python modules with pip install <module>. The external astromatic packages are easiest installed using package managers (e.g., rpm, apt-get).

• python 3
• astropy
• numpy
• matplotlib
• astroplan
• pytz

### External packages¶

None

In [1]:
import numpy as np
from astropy import units as u
from astropy.time import Time
from astropy.coordinates import SkyCoord
from astropy.coordinates import EarthLocation
import pytz
%matplotlib inline
from astroplan import Observer, FixedTarget
from astropy.utils.iers import conf
conf.auto_max_age = None
from astropy.coordinates import get_sun, get_moon, get_body
from astroplan import moon_illumination


### Date and Time¶

• Dates and times are in UTC
• Default time is 00:00:00 UTC (verify this)
In [2]:
date = Time("2018-12-03", format='iso')
print(date)

2018-12-03 00:00:00.000


### What is the current UTC?¶

In [3]:
now = Time.now()
print(now)
print(now.jd)
print(now.mjd)
print(now.decimalyear)

2019-04-02 05:53:06.289935
2458575.7452116893
58575.24521168906
2019.24998688134


### Exercise¶

What time will it be (in UTC) after 1 hour 45 minutes from now? Complete the line below to print it out.

In [4]:
print("In 1 hour and 45 minutes, the time will be {0} UTC".format(now + 1*u.h + 45*u.min))

In 1 hour and 45 minutes, the time will be 2019-04-02 07:38:06.289935 UTC


### Using UT1¶

• To keep accurate time, the changes in earth's rotation period have to be taken into account.
• AstroPy does this using a convention called UT1, that is tied to the rotation of earth with respect to the position of distant quasars. IERS - International Earth Rotation and Reference Systems Service keeps continuous tabs on the orientation of the earth and updates the data in the IERS bulletin. Update the bulletin:
In [5]:
download_IERS_A()


### Check to see what observatories are available in the database.¶

In [6]:
print("Available observatories: \n{0}"
.format(', '.join(EarthLocation.get_site_names())))

Available observatories:
, , , ALMA, Anglo-Australian Observatory, Apache Point, Apache Point Observatory, Atacama Large Millimeter Array, BAO, Beijing XingLong Observatory, Black Moshannon Observatory, CHARA, Canada-France-Hawaii Telescope, Catalina Observatory, Cerro Pachon, Cerro Paranal, Cerro Tololo, Cerro Tololo Interamerican Observatory, DCT, Discovery Channel Telescope, Dominion Astrophysical Observatory, GBT, Gemini South, Green Bank Telescope, Hale Telescope, Haleakala Observatories, Happy Jack, IAO, JCMT, James Clerk Maxwell Telescope, Jansky Very Large Array, Keck Observatory, Kitt Peak, Kitt Peak National Observatory, La Silla Observatory, Large Binocular Telescope, Las Campanas Observatory, Lick Observatory, Lowell Observatory, MWA, Manastash Ridge Observatory, McDonald Observatory, Medicina, Medicina Dish, Michigan-Dartmouth-MIT Observatory, Mount Graham International Observatory, Mt Graham, Mt. Ekar 182 cm. Telescope, Mt. Stromlo Observatory, Multiple Mirror Telescope, Murchison Widefield Array, NOV, National Observatory of Venezuela, Noto, Observatorio Astronomico Nacional, San Pedro Martir, Observatorio Astronomico Nacional, Tonantzintla, Palomar, Paranal Observatory, Roque de los Muchachos, SAAO, SALT, SRT, Siding Spring Observatory, Southern African Large Telescope, Subaru, Subaru Telescope, Sutherland, TUG, UKIRT, United Kingdom Infrared Telescope, Vainu Bappu Observatory, Very Large Array, W. M. Keck Observatory, Whipple, Whipple Observatory, aao, alma, apo, bmo, cfht, ctio, dao, dct, ekar, example_site, flwo, gbt, gemini_north, gemini_south, gemn, gems, greenwich, haleakala, iao, irtf, jcmt, keck, kpno, lapalma, lasilla, lbt, lco, lick, lowell, mcdonald, mdm, medicina, mmt, mro, mso, mtbigelow, mwa, mwo, noto, ohp, paranal, salt, sirene, spm, srt, sso, tona, tug, ukirt, vbo, vla


### Setting up observatory location¶

In [7]:
#Indian Astronomical Observatory is not listed in the database, so let's define the location
longitude = '78d57m53s'
latitude = '32d46m44s'
elevation = 4500 * u.m
location = EarthLocation.from_geodetic(longitude, latitude, elevation)
iaohanle = Observer(location = location, timezone = 'Asia/Kolkata',
name = "IAO", description = "GROWTH-India 70cm telescope")
iaohanle

Out[7]:
<Observer: name='IAO',
location (lon, lat, el)=(78.96472222222222 deg, 32.77888888888889 deg, 4499.999999999798 m),
timezone=<DstTzInfo 'Asia/Kolkata' LMT+5:53:00 STD>>

### Sunset, Sunrise, Midnight¶

In [8]:
#Calculating the sunset, midnight and sunrise times for our observatory
#What is astronomical twilight?
sunset_iao = iaohanle.sun_set_time(now, which='nearest')
eve_twil_iao = iaohanle.twilight_evening_astronomical(now, which='nearest')
midnight_iao = iaohanle.midnight(now, which='next')
morn_twil_iao = iaohanle.twilight_morning_astronomical(now, which='next')
sunrise_iao = iaohanle.sun_rise_time(now, which='next')

print("Sunset at IAO will be at {0.iso} UTC".format(sunset_iao))
print("Astronomical evening twilight at IAO will be at {0.iso} UTC".format(eve_twil_iao))
print("Midnight at IAO will be at {0.iso} UTC".format(midnight_iao))
print("Astronomical morning twilight at IAO will be at {0.iso} UTC".format(morn_twil_iao))
print("Sunrise at IAO will be at {0.iso} UTC".format(sunrise_iao))

Sunset at IAO will be at 2019-04-02 13:00:32.540 UTC
Astronomical evening twilight at IAO will be at 2019-04-02 14:28:19.957 UTC
Midnight at IAO will be at 2019-04-02 18:47:32.580 UTC
Astronomical morning twilight at IAO will be at 2019-04-02 23:06:42.282 UTC
Sunrise at IAO will be at 2019-04-03 00:34:25.511 UTC


### Exercise¶

Find the effective length of time (in hours) available for astronomical observations at IAO tonight

In [9]:
observing_time = (morn_twil_iao - eve_twil_iao).to(u.h)
print("You can observe for {0:.1f} at IAO tonight".format(observing_time))

You can observe for 8.6 h at IAO tonight


### Local Sidereal Time (LST)¶

In [10]:
#What is the LST now at IAO Hanle?
#What would the LST be at IAO at local midnight?
lst_now = iaohanle.local_sidereal_time(now)
lst_mid = iaohanle.local_sidereal_time(midnight_iao)
print("LST at IAO now is {0:.2f}".format(lst_now))
print("LST at IAO at local midnight will be {0:.2f}".format(lst_mid))

LST at IAO now is 23.84 hourangle
LST at IAO at local midnight will be 12.78 hourangle


### Choosing targets for observations¶

Targets can be defined by name or coordinates.

In [11]:
coords = SkyCoord('00h42m41.8s', '+40d51m55.0s', frame='icrs') # coordinates of Andromeda Galaxy (M32)
m32 = FixedTarget(name = 'M32', coord=coords)
m32.ra.hms

Out[11]:
hms_tuple(h=0.0, m=42.0, s=41.799999999999926)
In [12]:
#Check to see if target is up at evening twilight.
#Also check if target is available at midnight and morning twilight.

print(iaohanle.target_is_up(eve_twil_iao, m32))
print(iaohanle.target_is_up(midnight_iao, m32))
print(iaohanle.target_is_up(morn_twil_iao, m32))

True
False
True

In [13]:
#Altitude and Azimuth of target
aa = iaohanle.altaz(eve_twil_iao, m32)
aa.alt.degree, aa.az.degree

Out[13]:
(4.53096054709229, 316.98764800592306)

Checking rise times of targets

In [14]:
m32rise = iaohanle.target_rise_time(now, m32, which = 'next', horizon = 0 * u.deg)
print(m32rise.iso)  #default format is JD

2019-04-02 22:27:58.640


### Defining targets by name¶

In [15]:
target = FixedTarget.from_name('m51') #Messier 51
target.coord

Out[15]:
<SkyCoord (ICRS): (ra, dec) in deg
(202.469575, 47.1952583)>

### Dealing with moving targets¶

In [16]:
get_body('jupiter', now)

Out[16]:
<SkyCoord (GCRS: obstime=2019-04-02 05:53:06.289935, obsgeoloc=(0., 0., 0.) m, obsgeovel=(0., 0., 0.) m / s): (ra, dec, distance) in (deg, deg, AU)
(263.46769437, -22.66809942, 4.92780141)>
In [17]:
#get moon position at midnight
get_moon(midnight_iao)

Out[17]:
<SkyCoord (GCRS: obstime=2458576.2830159706, obsgeoloc=(0., 0., 0.) m, obsgeovel=(0., 0., 0.) m / s): (ra, dec, distance) in (deg, deg, km)
(346.38883828, -10.02541931, 404098.19517621)>
In [18]:
#How bright is the moon at midnight?
moon_illumination(midnight_iao)

Out[18]:
0.0635173895581661
In [19]:
#We can turn solar system objects into 'pseudo-fixed' targets to plan observations
saturn_midnight = FixedTarget(name = 'Saturn', coord = get_body('saturn', midnight_iao))
saturn_midnight.coord

Out[19]:
<SkyCoord (GCRS: obstime=2458576.2830159706, obsgeoloc=(0., 0., 0.) m, obsgeovel=(0., 0., 0.) m / s): (ra, dec, distance) in (deg, deg, AU)
(291.20444303, -21.59108981, 10.13197767)>

### Airmass¶

• Ideally, targets should be observed when they have the least airmass. Airmass ranges from 1 (zenith) to ~38 at the horizon.
• Airmass is 2.0 at alt=30, 2.9 at alt=20 and 3.9 at alt=15 degrees
• As a general rule of thumb, try observing targets when airmass > 2
• Let us find the airmass of M33 at midnight at IAO
In [20]:
#Is the target up at IAO at midnight?
iaohanle.target_is_up(midnight_iao, target)

Out[20]:
True
In [21]:
#lets check the alt and az of the target at midnight
target_altaz = iaohanle.altaz(midnight_iao, target)
target_altaz.altaz

Out[21]:
<SkyCoord (AltAz: obstime=2458576.2830159706, location=(1028191.03516148, 5272251.01802928, 3435803.52567405) m, pressure=0.0 hPa, temperature=0.0 deg_C, relative_humidity=0.0, obswl=1.0 micron): (az, alt) in deg
(27.08622303, 73.41928233)>

That's a good enough elevation to observe the target.

In [22]:
#Find the airmass
target_altaz.secz

Out[22]:
$1.0433854 \; \mathrm{}$

Now we can visualize what we have done so far using some plots

In [23]:
import matplotlib.pyplot as plt
from astroplan.plots import plot_sky, plot_airmass

In [24]:
#position of target at midnight
plot_sky(target, iaohanle, midnight_iao)

/home/chummels/miniconda3/lib/python3.7/site-packages/matplotlib/cbook/deprecation.py:107: MatplotlibDeprecationWarning: The frac parameter was deprecated in version 2.1. Use tick padding via Axes.tick_params instead.
warnings.warn(message, mplDeprecation, stacklevel=1)

Out[24]:
<matplotlib.axes._subplots.PolarAxesSubplot at 0x7f85856100f0>

Now let us see how the target moves over the course of the night

In [25]:
t_start = eve_twil_iao
t_end = morn_twil_iao
t_observe = t_start + (t_end - t_start) * np.linspace(0.0, 1.0, 20)
plot_sky(target, iaohanle, t_observe)

Out[25]:
<matplotlib.axes._subplots.PolarAxesSubplot at 0x7f85869f8828>

Now let's plot the airmass as a function of time

In [26]:
plot_airmass(target, iaohanle, t_observe)
plt.ylim(4,0.5)

Out[26]:
(4, 0.5)

The airmass is above 2 for the better part of the night, making M51 a good target to observe from IAO tonight. Note that the default airmass limit is 3 in astroplan, corresponding to ~19 degrees elevation.

### Finder Charts¶

In [27]:
from astroplan.plots import plot_finder_image
from astroquery.skyview import SkyView

In [28]:
plot_finder_image(target, fov_radius = 20 * u.arcmin)  #field of view corresponding to the GROWTH-India telesocpe

Out[28]:
(<matplotlib.axes._subplots.WCSAxesSubplot at 0x7f85878706d8>,
<astropy.io.fits.hdu.image.PrimaryHDU at 0x7f8588c6e400>)

Now let's define an array of targets to work with

In [29]:
target_names = ['vega', 'polaris', 'm1', 'm42', 'm55']
targets = [FixedTarget.from_name(target) for target in target_names]
targets

Out[29]:
[<FixedTarget "vega" at SkyCoord (ICRS): (ra, dec) in deg (279.23473479, 38.78368896)>,
<FixedTarget "polaris" at SkyCoord (ICRS): (ra, dec) in deg (37.95456067, 89.26410897)>,
<FixedTarget "m1" at SkyCoord (ICRS): (ra, dec) in deg (83.633083, 22.0145)>,
<FixedTarget "m42" at SkyCoord (ICRS): (ra, dec) in deg (83.82208, -5.39111)>,
<FixedTarget "m55" at SkyCoord (ICRS): (ra, dec) in deg (294.998792, -30.96475)>]

Which of these targets is up now?

In [30]:
iaohanle.target_is_up(now, targets)

Out[30]:
array([ True,  True,  True,  True,  True])
In [31]:
iaohanle.target_is_up(midnight_iao, targets)

Out[31]:
array([ True,  True, False, False, False])

### Exercise¶

Find out the times at which the targets rise to an elevation of 10 degrees. Use target_rise_time.

In [32]:
for target in targets:
print(iaohanle.target_rise_time(now, target, which = 'next', horizon = 10*u.deg).iso)

2019-04-02 17:40:03.863
-4715-02-28 12:00:00.000
2019-04-03 05:26:07.416
2019-04-02 06:41:16.114
2019-04-02 22:16:38.379

WARNING: TargetAlwaysUpWarning: Target with index 0 does not cross horizon=10.0 deg within 24 hours [astroplan.observer]
WARNING: ErfaWarning: ERFA function "d2dtf" yielded 1 of "dubious year (Note 5)" [astropy._erfa.core]


What is the elevation of Vega now?

In [33]:
iaohanle.altaz(now, targets[0])

Out[33]:
<SkyCoord (AltAz: obstime=2019-04-02 05:53:06.289935, location=(1028191.03516148, 5272251.01802928, 3435803.52567405) m, pressure=0.0 hPa, temperature=0.0 deg_C, relative_humidity=0.0, obswl=1.0 micron): (az, alt) in deg
(299.98263436, 28.28822783)>

Now let's plot the elevation of Vega to see how it varies over the night

In [34]:
times = (t_start - 0.5 * u.h) + (t_end - t_start + 1 * u.h) * np.linspace(0.0, 1.0, 40)
elevations = iaohanle.altaz(times, targets[0]).alt
ax = plt.gca()
ax.plot_date(times.plot_date, elevations.deg)
ax.set(xlabel = 'Time UTC [MM-DD HH]' ,ylabel = 'Altitude [deg]')
plt.setp(ax.get_xticklabels(), rotation=45, ha='right')
plt.show()


### Exercise¶

Plot the altitude as a function of time for tonight for each of the targets in a single plot

In [35]:
times = t_start + (t_end - t_start) * np.linspace(0.0, 1.0, 20)
elevations = []
for target in targets:
elevations.append(iaohanle.altaz(times, target).alt)

ax = plt.gca()
for elevation in elevations:
ax.plot_date(times.plot_date, elevation)

ax.set(xlabel = 'Time UTC [MM-DD HH]' ,ylabel = 'Altitude [deg]')
plt.setp(ax.get_xticklabels(), rotation=45, ha='right')
plt.legend()

No handles with labels found to put in legend.

Out[35]:
<matplotlib.legend.Legend at 0x7f85874de160>

### Exercise¶

Plot sky positions for each target using plot_sky for tonight at IAO in a single plot.

In [36]:
times = (t_start - 0.5 * u.h) + (t_end - t_start + 1 * u.h) * np.linspace(0.0, 1.0, 20)
for target in targets:
plot_sky(target, iaohanle, times)
plt.legend(loc=[1.1,0])

/home/chummels/miniconda3/lib/python3.7/site-packages/matplotlib/cbook/deprecation.py:107: MatplotlibDeprecationWarning: The frac parameter was deprecated in version 2.1. Use tick padding via Axes.tick_params instead.
warnings.warn(message, mplDeprecation, stacklevel=1)

Out[36]:
<matplotlib.legend.Legend at 0x7f8587488b70>

### Exercise¶

Plot airmass vs time for each target in targets for tonight at IAO.

In [37]:
for target in targets:
plot_airmass(target, iaohanle, t_observe)
plt.ylim(4,0.5)
plt.legend()

Out[37]:
<matplotlib.legend.Legend at 0x7f85873c7438>

### Observational Constraints¶

• between civil twilights
• airmass
• altitude limits
In [38]:
from astroplan import (AltitudeConstraint, AirmassConstraint,
AtNightConstraint, MoonSeparationConstraint)
constraints = [AltitudeConstraint(15*u.deg, 84*u.deg),
AirmassConstraint(3), AtNightConstraint.twilight_civil(), MoonSeparationConstraint(min = 10 * u.deg)]
t_range = Time([t_start - 0.5 * u.hour, t_end + 0.5 * u.hour])

In [39]:
from astroplan import is_observable, is_always_observable, months_observable
# Are targets ever observable in the time range?
ever_observable = is_observable(constraints, iaohanle, targets, time_range=t_range)
print(ever_observable)
# Are targets always observable in the time range?
always_observable = is_always_observable(constraints, iaohanle, targets, time_range=t_range)
print(always_observable)
# During what months are the targets ever observable?
obs_months = months_observable(constraints, iaohanle, targets)

[ True  True  True  True False]
[False  True False False False]


The functions is_observable and ever_observable return boolean arrays. Let's print their output in tabular form.

In [40]:
from astropy.table import Table
observability_table = Table()
observability_table['targets'] = [target.name for target in targets]
observability_table['ever_observable'] = ever_observable
observability_table['always_observable'] = always_observable
print(observability_table)

targets ever_observable always_observable
------- --------------- -----------------
vega            True             False
polaris            True              True
m1            True             False
m42            True             False
m55           False             False


Or we could do this directly using the observability_table function

In [41]:
from astroplan import observability_table
table = observability_table(constraints, iaohanle, targets, time_range = t_range)
print(table)

target name ever observable always observable fraction of time observable
----------- --------------- ----------------- ---------------------------
vega            True             False                         0.5
polaris            True              True                         1.0
m1            True             False                         0.3
m42            True             False                         0.2
m55           False             False                         0.0


### Exercise¶

• Create a list of your favourite targets and store it in a text file with 3 columns - name, RA and Dec. Or you could use 'targetlists.txt' which already contains a list of targets.
• Read the text file, and store the targets as FixedTarget objects.
• Get observability tables for all the targets for different moon separation angles (10, 20, 30... degrees)
• Plot airmass and sky position as a function of time for tonight for all your targets.
In [42]:
from astropy.io import ascii