def date2dict_times(date):
day = Time(date, format='iso')
longitude = '78d57m53s'
latitude = '32d46m44s'
elevation = 4500 * u.m
location = EarthLocation.from_geodetic(longitude, latitude, elevation)
iaohanle = Observer(location=location,
name="IAO",
timezone='Asia/Kolkata',
description="GROWTH-India 70cm telescope")
sunset_iao = iaohanle.sun_set_time(day, which='next')
sunrise_iao = iaohanle.sun_rise_time(day, which='next')
twelve_twil_eve_iao = iaohanle.twilight_evening_nautical(day, which='next')
eighteen_twil_eve_iao = iaohanle.twilight_evening_astronomical(
day, which='next')
twelve_twil_morn_iao = iaohanle.twilight_morning_nautical(day,
which='next')
eighteen_twil_morn_iao = iaohanle.twilight_morning_astronomical(
day, which='next')
dict_times = OrderedDict()
dict_times['Sunset '] = time2utc_ist(sunset_iao)
dict_times['Sunrise '] = time2utc_ist(sunrise_iao)
dict_times['Twelve degree Evening Twilight '] = time2utc_ist(
twelve_twil_eve_iao)
dict_times['Eighteen degree Evening Twilight '] = time2utc_ist(
eighteen_twil_eve_iao)
dict_times['Twelve degree Morning Twilight '] = time2utc_ist(
twelve_twil_morn_iao)
dict_times['Eighteen degree Morning Twilight '] = time2utc_ist(
eighteen_twil_morn_iao)
return dict_times
def get_sunset_sunrise(self, time):
"""
Returns the sunset and sunrise times of the night containing the time provided
time is a astropy Time object
The sunset and sunrise times are returns as an astropy Time object with the same
settings as the provided Time object.
"""
observer = Observer(location=self.get_EarthLocation())
sunset = observer.sun_set_time(time, which='nearest')
sunrise = observer.sun_rise_time(time, which='nearest')
return sunset, sunrise
def timeline(request):
# get location
location = EarthLocation(
lon=settings.OBSERVER_LOCATION['longitude'] * u.deg,
lat=settings.OBSERVER_LOCATION['latitude'] * u.deg,
height=settings.OBSERVER_LOCATION['elevation'] * u.m)
# get observer and now
now = Time.now()
observer = Observer(location=location)
# night or day?
is_day = observer.sun_altaz(now).alt.degree > 0.
# get sunset to start with
sunset = observer.sun_set_time(now, which='next' if is_day else 'previous')
# list of events
events = []
events.append(sunset.isot)
# twilight at sunset
sunset_twilight = observer.sun_set_time(sunset,
which='next',
horizon=-12. * u.deg)
events.append(sunset_twilight.isot)
# twilight at sunrise
sunrise_twilight = observer.sun_rise_time(sunset_twilight,
which='next',
horizon=-12. * u.deg)
events.append(sunrise_twilight.isot)
# sunrise
sunrise = observer.sun_rise_time(sunset_twilight, which='next')
events.append(sunrise.isot)
# return all
return JsonResponse({'time': now.isot, 'events': events})
def get_twilights(start, end):
""" Determine sunrise and sunset times """
location = EarthLocation(
lat=+19.53602,
lon=-155.57608,
height=3400,
)
obs = Observer(location=location, name='VYSOS', timezone='US/Hawaii')
sunset = obs.sun_set_time(Time(start), which='next').datetime
sunrise = obs.sun_rise_time(Time(start), which='next').datetime
# Calculate and order twilights and set plotting alpha for each
twilights = [
(start, 'start', 0.0),
(sunset, 'sunset', 0.0),
(obs.twilight_evening_civil(Time(start),
which='next').datetime, 'ec', 0.1),
(obs.twilight_evening_nautical(Time(start),
which='next').datetime, 'en', 0.2),
(obs.twilight_evening_astronomical(Time(start),
which='next').datetime, 'ea', 0.3),
(obs.twilight_morning_astronomical(Time(start),
which='next').datetime, 'ma', 0.5),
(obs.twilight_morning_nautical(Time(start),
which='next').datetime, 'mn', 0.3),
(obs.twilight_morning_civil(Time(start),
which='next').datetime, 'mc', 0.2),
(sunrise, 'sunrise', 0.1),
]
twilights.sort(key=lambda x: x[0])
final = {
'sunset': 0.1,
'ec': 0.2,
'en': 0.3,
'ea': 0.5,
'ma': 0.3,
'mn': 0.2,
'mc': 0.1,
'sunrise': 0.0
}
twilights.append((end, 'end', final[twilights[-1][1]]))
return twilights
def get_twilights(self, config=None):
""" Determine sunrise and sunset times """
print(' Determining sunrise, sunset, and twilight times')
if config is None:
from pocs.utils.config import load_config as pocs_config
config = pocs_config()['location']
location = EarthLocation(
lat=config['latitude'],
lon=config['longitude'],
height=config['elevation'],
)
obs = Observer(location=location, name='PANOPTES',
timezone=config['timezone'])
sunset = obs.sun_set_time(Time(self.start), which='next').datetime
sunrise = obs.sun_rise_time(Time(self.start), which='next').datetime
# Calculate and order twilights and set plotting alpha for each
twilights = [(self.start, 'start', 0.0),
(sunset, 'sunset', 0.0),
(obs.twilight_evening_civil(Time(self.start),
which='next').datetime, 'ec', 0.1),
(obs.twilight_evening_nautical(Time(self.start),
which='next').datetime, 'en', 0.2),
(obs.twilight_evening_astronomical(Time(self.start),
which='next').datetime, 'ea', 0.3),
(obs.twilight_morning_astronomical(Time(self.start),
which='next').datetime, 'ma', 0.5),
(obs.twilight_morning_nautical(Time(self.start),
which='next').datetime, 'mn', 0.3),
(obs.twilight_morning_civil(Time(self.start),
which='next').datetime, 'mc', 0.2),
(sunrise, 'sunrise', 0.1),
]
twilights.sort(key=lambda x: x[0])
final = {'sunset': 0.1, 'ec': 0.2, 'en': 0.3, 'ea': 0.5,
'ma': 0.3, 'mn': 0.2, 'mc': 0.1, 'sunrise': 0.0}
twilights.append((self.end, 'end', final[twilights[-1][1]]))
return twilights
def get_twilights(start, end, webcfg, nsample=256):
""" Determine sunrise and sunset times """
location = c.EarthLocation(
lat=webcfg['site'].getfloat('site_lat'),
lon=webcfg['site'].getfloat('site_lon'),
height=webcfg['site'].getfloat('site_elevation'),
)
obs = Observer(location=location, name=webcfg['site'].get('name', ''))
sunset = obs.sun_set_time(Time(start), which='next').datetime
sunrise = obs.sun_rise_time(Time(start), which='next').datetime
# Calculate and order twilights and set plotting alpha for each
twilights = [
(start, 'start', 0.0),
(sunset, 'sunset', 0.0),
(obs.twilight_evening_civil(Time(start),
which='next').datetime, 'ec', 0.1),
(obs.twilight_evening_nautical(Time(start),
which='next').datetime, 'en', 0.2),
(obs.twilight_evening_astronomical(Time(start),
which='next').datetime, 'ea', 0.3),
(obs.twilight_morning_astronomical(Time(start),
which='next').datetime, 'ma', 0.5),
(obs.twilight_morning_nautical(Time(start),
which='next').datetime, 'mn', 0.3),
(obs.twilight_morning_civil(Time(start),
which='next').datetime, 'mc', 0.2),
(sunrise, 'sunrise', 0.1),
]
twilights.sort(key=lambda x: x[0])
final = {
'sunset': 0.1,
'ec': 0.2,
'en': 0.3,
'ea': 0.5,
'ma': 0.3,
'mn': 0.2,
'mc': 0.1,
'sunrise': 0.0
}
twilights.append((end, 'end', final[twilights[-1][1]]))
return twilights
def calculate_twilights(date):
""" Determine sunrise and sunset times """
from astropy import units as u
from astropy.time import Time
from astropy.coordinates import EarthLocation
from astroplan import Observer
h = 4.2 * u.km
R = (1.0 * u.earthRad).to(u.km)
d = np.sqrt(h * (2 * R + h))
phi = (np.arccos((d / R).value) * u.radian).to(u.deg)
MK = phi - 90 * u.deg
location = EarthLocation(
lat=19 + 49 / 60 + 33.40757 / 60**2,
lon=-(155 + 28 / 60 + 28.98665 / 60**2),
height=4159.58,
)
obs = Observer(location=location, name='Keck', timezone='US/Hawaii')
date = Time(dt.strptime(f'{date} 18:00:00', '%Y-%m-%d %H:%M:%S'))
t = {}
sunset = obs.sun_set_time(date, which='nearest', horizon=MK).datetime
t['seto'] = sunset
t['ento'] = obs.twilight_evening_nautical(Time(sunset),
which='next').datetime
t['eato'] = obs.twilight_evening_astronomical(Time(sunset),
which='next').datetime
t['mato'] = obs.twilight_morning_astronomical(Time(sunset),
which='next').datetime
t['mnto'] = obs.twilight_morning_nautical(Time(sunset),
which='next').datetime
t['riseo'] = obs.sun_rise_time(Time(sunset), which='next').datetime
t['set'] = t['seto'].strftime('%H:%M UT')
t['ent'] = t['ento'].strftime('%H:%M UT')
t['eat'] = t['eato'].strftime('%H:%M UT')
t['mat'] = t['mato'].strftime('%H:%M UT')
t['mnt'] = t['mnto'].strftime('%H:%M UT')
t['rise'] = t['riseo'].strftime('%H:%M UT')
return t
def calculate_twilights(date):
""" Determine sunrise and sunset times """
from astropy import units as u
from astropy.time import Time
from astropy.coordinates import EarthLocation
from astroplan import Observer
h = 4.2*u.km
R = (1.0*u.earthRad).to(u.km)
d = np.sqrt(h*(2*R+h))
phi = (np.arccos((d/R).value)*u.radian).to(u.deg)
MK = phi - 90*u.deg
location = EarthLocation(
lat=19+49/60+33.40757/60**2,
lon=-(155+28/60+28.98665/60**2),
height=4159.58,
)
obs = Observer(location=location, name='Keck', timezone='US/Hawaii')
date = Time(dt.strptime(f'{date} 18:00:00', '%Y-%m-%d %H:%M:%S'))
t = {}
sunset = obs.sun_set_time(date, which='nearest', horizon=MK).datetime
t['seto'] = sunset
t['ento'] = obs.twilight_evening_nautical(Time(sunset), which='next').datetime
t['eato'] = obs.twilight_evening_astronomical(Time(sunset), which='next').datetime
t['mato'] = obs.twilight_morning_astronomical(Time(sunset), which='next').datetime
t['mnto'] = obs.twilight_morning_nautical(Time(sunset), which='next').datetime
t['riseo'] = obs.sun_rise_time(Time(sunset), which='next').datetime
t['set'] = t['seto'].strftime('%H:%M UT')
t['ent'] = t['ento'].strftime('%H:%M UT')
t['eat'] = t['eato'].strftime('%H:%M UT')
t['mat'] = t['mato'].strftime('%H:%M UT')
t['mnt'] = t['mnto'].strftime('%H:%M UT')
t['rise'] = t['riseo'].strftime('%H:%M UT')
return t
def observe(request, method="POST"):
if request.POST['observing_date'] == "":
messages.error(request, 'Please choose a date!')
if request.POST['name'] == "":
messages.error(request, 'Object name cannot be empty!')
if request.POST['ra'] == "":
messages.error(request, 'Object RA cannot be empty!')
if request.POST['dec'] == "":
messages.error(request, 'Object Dec cannot be empty!')
if request.POST['observing_date'] == "" or request.POST[
'name'] == "" or request.POST['ra'] == "" or request.POST[
'dec'] == "":
return redirect('/')
observatory = None
offset = None
for idx, val in enumerate(T['name']):
if val == request.POST['observatory']:
observatory = Observer(longitude=T['longitude'][idx] * u.deg,
latitude=T['latitude'][idx] * u.deg,
elevation=T['altitude'][idx] * u.m,
name=T['name'][idx])
today = datetime.now()
if tf.certain_timezone_at(lat=T['latitude'][idx],
lng=T['longitude'][idx]) == None:
return redirect('/error')
tz_target = timezone(
tf.certain_timezone_at(lat=T['latitude'][idx],
lng=T['longitude'][idx]))
# ATTENTION: tf.certain_timezone_at(...) could be None! handle error case
today_target = tz_target.localize(today)
today_utc = utc.localize(today)
offset = (today_utc - today_target).total_seconds() * u.s
# # offset = offsetfunction(observatory)
observe_date = Time(request.POST['observing_date'] + ' 00:00:00',
format='iso')
sunset_here = observatory.sun_set_time(observe_date,
which="nearest") + offset
sunrise_here = observatory.sun_rise_time(observe_date,
which="next") + offset
midnight_here = observatory.midnight(observe_date,
which="nearest") + offset
astro_set = observatory.twilight_evening_astronomical(observe_date,
which='nearest')
astro_rise = observatory.twilight_morning_astronomical(observe_date,
which='next')
coords = SkyCoord(request.POST['ra'], request.POST['dec'], frame='icrs')
target = FixedTarget(name=request.POST['name'], coord=coords)
start_time = astro_set
end_time = astro_rise
delta_t = end_time - start_time
observe_time = start_time + delta_t * np.linspace(0.0, 2.0, 100)
plt.ioff()
sky = plot_sky(target, observatory, observe_time)
sky.figure.savefig('apps/project_app/static/project_app/plot_sky.png')
plt.close()
plt.ioff()
airmass = plot_airmass(target, observatory, observe_time)
airmass.figure.savefig(
'apps/project_app/static/project_app/plot_airmass.png')
plt.close()
plt.ioff()
finder_image = plot_finder_image(target)
finder_image[0].figure.savefig(
'apps/project_app/static/project_app/plot_finder_image.png')
plt.close()
request.session['context'] = {
"sunset": Time(sunset_here, format="iso").value,
"sunrise": Time(sunrise_here, format="iso").value,
"date": Time(observe_date, format="iso").value,
"midnight": Time(midnight_here, format="iso").value,
"site": request.POST['observatory'],
"ra": request.POST['ra'],
"dec": request.POST['dec'],
"name": request.POST['name']
}
return redirect('/display')
# Dates are assumed to be UTC by default """ We can ask about typical times of interest at this observing position Returned dates are assumed to be in the observer's time zone for convenience. The date parameter, if given, can be an astropy Time or a datetime instance. If no parameter is given, the current date/time is assumed. """ # Define a time from astropy.time import Time time_obs = Time(2457189.500000, format='jd') # sun_set_time obs.sun_set_time(time_obs, which='nearest') # Default obs.sun_set_time(time_obs, which='next') obs.sun_set_time(time_obs, which='previous') obs.sun_set_time() # Will be use time=Time.now(), which='nearest' # sun_rise_time obs.sun_rise_time(time_obs, which='nearest') # Default obs.sun_rise_time(time_obs, which='next') obs.sun_rise_time(time_obs, which='previous') # moon rise obs.moon_rise(time_obs, which='nearest') # moon set obs.moon_set(time_obs, which='nearest')
def getalt(dt, locname, lat, lng):
#get time zone
tf = timezonefinder.TimezoneFinder()
timezone_str = tf.certain_timezone_at(lat=lat, lng=lng)
#set location for observer object
loc = EarthLocation.from_geodetic(lng, lat)
#setup observer object
observer = Observer(name=locname,
location=loc,
timezone=timezone(timezone_str))
#get the sunset time for the given day, given a date string.
# for our given location
sunsettime = observer.sun_set_time(dt, which='next')
#alternative, can also use nautical twilight as a criteria
#get nautical twilight time for the given day, given a date string.
#nautical twilight is when the sun is 12 degrees below the horizon
# for our given location
#nautitime=observer.twilight_evening_nautical(dt, which='next')
#convert time to datetime so that we can manipulate the timezone
sunset_dt = sunsettime.to_datetime()
#add utc timezone
sunset_utc = sunset_dt.replace(tzinfo=timezone('utc'))
#apply our local time zone
localtime = sunset_utc.astimezone(timezone(timezone_str))
#set time
t = sunsettime
#setup a dictionary for the visible planets, sun and moon
bodies = {
"sun": '',
"moon": '',
"mercury": '',
"venus": '',
"mars": '',
"jupiter": '',
"saturn": ''
}
#set up a dictionary for the symbols for the bodies
bodies_names = {
"sun": '\u2609',
#"sun" : '\u1f31e',
"moon": '\u263d',
#"moon" : '\u1f31b',
"mercury": '\u263f',
"venus": '\u2640',
"mars": '\u2642',
"jupiter": '\u2643',
"saturn": '\u2644'
}
#get the alt az position of the bodies for our given time and location
#we will use the alt number
with solar_system_ephemeris.set('builtin'):
for key in bodies:
bodies[key] = get_body(key, t, loc).transform_to(
AltAz(obstime=t, location=loc))
fig = plt.figure(figsize=(10, 10))
ax = fig.add_subplot(111, polar=True)
ax.set_theta_direction(-1)
ax.set_thetamin(180)
ax.set_thetamax(360)
ax.set_xticks(np.pi / 180. * np.linspace(180, 360, 5))
ax.set_xticklabels(['S', 'SW', 'W', 'NW', 'N'])
ax.set_rorigin(-90)
ax.set_title("Naked Eye planets, Sun and Moon at sunset on " +
str(localtime) + " in " + locname)
for key, values in bodies.items():
az_rad = values.az.wrap_at(180 * u.deg).radian
if key == 'sun':
plotplanet = ax.scatter(az_rad,
values.alt,
marker='o'.format(bodies_names[key]),
alpha=0.3,
s=700,
color='orange')
plotplanet.set_label(key)
else:
plotplanet = ax.scatter(az_rad,
values.alt,
marker=r"$ {} $".format(bodies_names[key]),
s=250)
altstr = (values.alt).to_string(precision=0)
plotplanet.set_label(key + " " + altstr)
r = np.zeros(360)
theta = np.arange(0, 2 * np.pi, 2 * np.pi / 360)
ax.plot(theta, r, color='orange')
ax.legend(loc='right',
labelspacing=1.2,
borderpad=1,
bbox_to_anchor=(1.4, .55))
plt.show()
# Start log file to record runs
f = open('MessierLog.txt', 'w')
# Set up the plots
fig = plt.figure(figsize=(8, 7))
gs = gridspec.GridSpec(2, 1, height_ratios=[1, 1])
# Set up the current skyview plot
ax1 = fig.add_subplot(gs[0], projection="polar")
# Set up the full skyview plot
ax2 = fig.add_subplot(gs[1], projection="mollweide")
# Initialize time
t = Time(Site.sun_set_time(t0, which="next"), format='iso')
f.write("Start at: {}\n".format(t))
# Initialize Observed list with starting object
Observed = [Start(t)]
# Run the Program
Final = Run_Through(t, Observed)
# Add to the counter
c += 1
# Get list of all non observed objects
NO = []
for g in grid:
if g not in Final:
def component_compare_daily_all(dataFrame, outliers=None):
componentName = 'H'
if dataFrame.empty:
print('No data is available to plot')
return
import pytz
import datetime
import matplotlib.dates as mdates
import helper_astro as astro
from astroplan import Observer
from datetime import datetime
from astropy.time import Time
import astropy.units as u
import matplotlib.pyplot as plt
print('Daily comparison graph is being generated.')
dayDateTimeObj = dataFrame['Date_Time'][
0] # just get one of elements from 'Date_Time' list. Will be used to for certian calculations
localTZ = dayDateTimeObj.tzinfo
subaru = Observer(longitude=80.07 * u.deg,
latitude=6.97 * u.deg,
elevation=0 * u.m,
name="Subaru",
timezone=localTZ)
noonTimeUTC = subaru.noon(Time(dayDateTimeObj),
which='next').to_datetime(pytz.timezone('UTC'))
print('Local noon time (utc) : ' +
noonTimeUTC.strftime('%Y-%m-%d %H:%M:%S %z'))
noonTimeLocal = subaru.noon(Time(dayDateTimeObj),
which='next').to_datetime(localTZ)
print('Local noon time (local time zone) : ' +
noonTimeLocal.strftime('%Y-%m-%d %H:%M:%S %z'))
sunRiseTimeLocal = subaru.sun_rise_time(Time(dayDateTimeObj),
which="next").to_datetime(localTZ)
sunRiseTimeLocalTwilight = subaru.sun_rise_time(Time(dayDateTimeObj),
which="next",
horizon=-6 *
u.deg).to_datetime(localTZ)
sunSetTimeLocal = subaru.sun_set_time(Time(dayDateTimeObj),
which='next').to_datetime(localTZ)
print('Sun rise time (local time zone) : ' +
sunRiseTimeLocal.strftime('%Y-%m-%d %H:%M:%S %z'))
print('Sun set time (local time zone) : ' +
sunSetTimeLocal.strftime('%Y-%m-%d %H:%M:%S %z'))
fig, ax = plt.subplots()
ax.plot(dataFrame['Date_Time'],
dataFrame[componentName],
label=componentName + ' Comp')
hours = mdates.HourLocator(interval=1)
h_fmt = mdates.DateFormatter('%d %H:%M:%S', localTZ)
ax.xaxis.set_major_locator(hours)
ax.xaxis.set_major_formatter(h_fmt)
if outliers is not None:
y_min, y_max = ax.get_ylim()
outliers[componentName] = y_min
kw = dict(marker='o', linestyle='none', color='r', alpha=0.3)
ax.plot(outliers[componentName],
label=componentName + '-outlier',
**kw)
moon_phase = astro.moon_get_moon_phase(dataFrame['Date_Time'][0])
t = ax.text(0.03,
0.9,
'Lunar phase {:3.0f}%'.format(moon_phase * 100),
horizontalalignment='left',
verticalalignment='center',
transform=ax.transAxes)
t.set_bbox(dict(facecolor='red', alpha=0.5, edgecolor='red'))
minValueIndex = dataFrame[componentName].idxmin()
maxValueIndex = dataFrame[componentName].idxmax()
print('Max value : ' + str(dataFrame.loc[maxValueIndex][componentName]) +
', at : ' + dataFrame.loc[maxValueIndex]['Date_Time'].strftime(
'%Y-%m-%d %H:%M:%S %z'))
print('Min value : ' + str(dataFrame.loc[minValueIndex][componentName]) +
', at : ' + dataFrame.loc[minValueIndex]['Date_Time'].strftime(
'%Y-%m-%d %H:%M:%S %z'))
yAxisMiddle = dataFrame.loc[minValueIndex][componentName] + (
(dataFrame.loc[maxValueIndex][componentName] -
dataFrame.loc[minValueIndex][componentName]) / 2)
noonTimeRow = dataFrame[(dataFrame['Date_Time'] == noonTimeLocal.replace(
second=0, microsecond=0))]
print('Noon time value of ' + componentName +
'-Component {:6.3f}'.format(noonTimeRow[componentName][0]))
ax.axvline(x=noonTimeRow['Date_Time'][0], ls='--', c='orange')
ax.text(noonTimeRow['Date_Time'][0],
yAxisMiddle,
'Local noon',
rotation=90,
ha='left',
va='center')
ax.axvline(x=sunRiseTimeLocal, ls='--', c='gray')
ax.axvline(x=sunRiseTimeLocalTwilight, ls='--', c='gray')
ax.text(sunRiseTimeLocal,
dataFrame.loc[minValueIndex][componentName],
'Sun rise',
rotation=90,
ha='left',
va='bottom')
ax.axvline(x=sunSetTimeLocal, ls='--', c='gray')
ax.text(sunSetTimeLocal,
dataFrame.loc[minValueIndex][componentName],
'Sun set',
rotation=90,
ha='left',
va='bottom')
ax.axvline(x=dataFrame.loc[maxValueIndex]['Date_Time'], ls='--', c='green')
ax.text(dataFrame.loc[maxValueIndex]['Date_Time'],
yAxisMiddle,
'Max value',
rotation=90,
ha='left',
va='center')
plt.xlabel('Time (hours)')
plt.xticks(rotation=90)
plt.ylabel(componentName + ' Component (nT)')
plt.legend()
plt.show()
def main(args=None):
p = parser()
opts = p.parse_args(args)
# Late imports
import operator
import sys
from astroplan import Observer
from astroplan.plots import plot_airmass
from astropy.coordinates import EarthLocation, SkyCoord
from astropy.table import Table
from astropy.time import Time
from astropy import units as u
from matplotlib import dates
from matplotlib.cm import ScalarMappable
from matplotlib.colors import Normalize
from matplotlib.patches import Patch
from matplotlib import pyplot as plt
from tqdm import tqdm
import pytz
from ..io import fits
from .. import moc
from .. import plot # noqa
from ..extern.quantile import percentile
if opts.site is None:
if opts.site_longitude is None or opts.site_latitude is None:
p.error('must specify either --site or both '
'--site-longitude and --site-latitude')
location = EarthLocation(lon=opts.site_longitude * u.deg,
lat=opts.site_latitude * u.deg,
height=(opts.site_height or 0) * u.m)
if opts.site_timezone is not None:
location.info.meta = {'timezone': opts.site_timezone}
observer = Observer(location)
else:
if not ((opts.site_longitude is None) and
(opts.site_latitude is None) and (opts.site_height is None) and
(opts.site_timezone is None)):
p.error('argument --site not allowed with arguments '
'--site-longitude, --site-latitude, '
'--site-height, or --site-timezone')
observer = Observer.at_site(opts.site)
m = fits.read_sky_map(opts.input.name, moc=True)
# Make an empty airmass chart.
t0 = Time(opts.time) if opts.time is not None else Time.now()
t0 = observer.midnight(t0)
ax = plot_airmass([], observer, t0, altitude_yaxis=True)
# Remove the fake source and determine times that were used for the plot.
del ax.lines[:]
times = Time(np.linspace(*ax.get_xlim()), format='plot_date')
theta, phi = moc.uniq2ang(m['UNIQ'])
coords = SkyCoord(phi, 0.5 * np.pi - theta, unit='rad')
prob = moc.uniq2pixarea(m['UNIQ']) * m['PROBDENSITY']
levels = np.arange(90, 0, -10)
nlevels = len(levels)
percentiles = np.concatenate((50 - 0.5 * levels, 50 + 0.5 * levels))
airmass = np.column_stack([
percentile(condition_secz(coords.transform_to(observer.altaz(t)).secz),
percentiles,
weights=prob) for t in tqdm(times)
])
cmap = ScalarMappable(Normalize(0, 100), plt.get_cmap())
for level, lo, hi in zip(levels, airmass[:nlevels], airmass[nlevels:]):
ax.fill_between(
times.plot_date,
clip_verylarge(lo), # Clip infinities to large but finite values
clip_verylarge(hi), # because fill_between cannot handle inf
color=cmap.to_rgba(level),
zorder=2)
ax.legend([Patch(facecolor=cmap.to_rgba(level)) for level in levels],
['{}%'.format(level) for level in levels])
# ax.set_title('{} from {}'.format(m.meta['objid'], observer.name))
# Adapted from astroplan
start = times[0]
twilights = [
(times[0].datetime, 0.0),
(observer.sun_set_time(Time(start), which='next').datetime, 0.0),
(observer.twilight_evening_civil(Time(start),
which='next').datetime, 0.1),
(observer.twilight_evening_nautical(Time(start),
which='next').datetime, 0.2),
(observer.twilight_evening_astronomical(Time(start),
which='next').datetime, 0.3),
(observer.twilight_morning_astronomical(Time(start),
which='next').datetime, 0.4),
(observer.twilight_morning_nautical(Time(start),
which='next').datetime, 0.3),
(observer.twilight_morning_civil(Time(start),
which='next').datetime, 0.2),
(observer.sun_rise_time(Time(start), which='next').datetime, 0.1),
(times[-1].datetime, 0.0),
]
twilights.sort(key=operator.itemgetter(0))
for i, twi in enumerate(twilights[1:], 1):
if twi[1] != 0:
ax.axvspan(twilights[i - 1][0],
twilights[i][0],
ymin=0,
ymax=1,
color='grey',
alpha=twi[1],
linewidth=0)
if twi[1] != 0.4:
ax.axvspan(twilights[i - 1][0],
twilights[i][0],
ymin=0,
ymax=1,
color='white',
alpha=0.8 - 2 * twi[1],
zorder=3,
linewidth=0)
# Add local time axis
timezone = (observer.location.info.meta or {}).get('timezone')
if timezone:
tzinfo = pytz.timezone(timezone)
ax2 = ax.twiny()
ax2.set_xlim(ax.get_xlim())
ax2.set_xticks(ax.get_xticks())
ax2.xaxis.set_major_formatter(dates.DateFormatter('%H:%M', tz=tzinfo))
plt.setp(ax2.get_xticklabels(), rotation=-30, ha='right')
ax2.set_xlabel("Time from {} [{}]".format(
min(times).to_datetime(tzinfo).date(), timezone))
if opts.verbose:
# Write airmass table to stdout.
times.format = 'isot'
table = Table(masked=True)
table['time'] = times
table['sun_alt'] = np.ma.masked_greater_equal(
observer.sun_altaz(times).alt, 0)
table['sun_alt'].format = lambda x: '{}'.format(int(np.round(x)))
for p, data in sorted(zip(percentiles, airmass)):
table[str(p)] = np.ma.masked_invalid(data)
table[str(p)].format = lambda x: '{:.01f}'.format(np.around(x, 1))
table.write(sys.stdout, format='ascii.fixed_width')
# Show or save output.
opts.output()
def Isky_parker(airmass, ecl_lat, gal_lat, gal_lon, tai, sun_alt, sun_sep, moon_phase, moon_ill, moon_alt, moon_sep):
''' Parker's sky model, which is a function of:
:param airmass:
airmass
:param ecl_lat:
ecliptic latitude (used for zodiacal light contribution)
:param gal_lat:
galactic latitude (used for ISL contribution)
:param gal_lon:
galactic longitude (used for ISL contribution)
:param tai:
time in seconds
:param sunalt:
sun altitude: 0 - 90 deg
:param sunsep:
sun separation: 0 - 90 deg
:param moonill:
moon illumination fraction: 0 - 1
:param moonalt:
moon altitude: 0 - 90 deg
:param moonsep:
moon separation angle: 0 - 180 deg
'''
from astroplan import Observer
from astropy.coordinates import EarthLocation
X = airmass # air mass
beta = ecl_lat # ecliptic latitude ( used for zodiacal light contribution )
l = gal_lat # galactic latitude ( used for ISL contribution )
b = gal_lon # galactic longitude ( used for ISL contribution )
_kpno = EarthLocation.of_site('kitt peak')
obs_time = Time(tai/86400., scale='tai', format='mjd', location=_kpno)
mjd = obs_time.mjd
# fractional months ( used for seasonal contribution)
month_frac = obs_time.datetime.month + obs_time.datetime.day/30.
# fractional hour ( used for hourly contribution)
kpno = Observer(_kpno)
sun_rise = kpno.sun_rise_time(obs_time, which='next')
sun_set = kpno.sun_set_time(obs_time, which='previous')
hour = ((obs_time - sun_set).sec)/3600.
hour_frac = hour/((Time(sun_rise, format='mjd') - Time(sun_set,format = 'mjd')).sec/3600.)
alpha = sun_alt # sun altitude
delta = sun_sep # sun separation (separation between the target and the sun's location)
# used for scattered moonlight
g = moon_phase # moon phase
altm = moon_alt
illm = moon_ill
delm = moon_sep
# get coefficients
coeffs = _read_parkerCoeffs()
# sky continuum
_w, _Icont = _parker_Icontinuum(coeffs, X, beta, l, b, mjd, month_frac, hour_frac, alpha, delta, altm, illm, delm, g)
S_continuum = _Icont / np.pi # BOSS has 2 arcsec diameter
# sky emission from the UVES continuum subtraction
w_uves, S_uves = np.loadtxt(''.join([UT.code_dir(), 'dat/sky/UVES_sky_emission.dat']),
unpack=True, usecols=[0,1])
f_uves = interp1d(w_uves, S_uves, bounds_error=False, fill_value='extrapolate')
S_emission = f_uves(_w)
return _w, S_continuum + S_emission
site = Site('LSST')
observer = Observer(longitude=site.longitude * u.deg,
latitude=site.latitude * u.deg,
elevation=site.height * u.m,
name="LSST")
# This blows up if I try to do it all at once? 250 GB of memory?
results = []
mjds_list = np.array_split(mjds, 500)
for i, mjds in enumerate(mjds_list):
print('chunk %i of %i' % (i, len(mjds_list)))
times = Time(mjds, format='mjd')
print('getting sunsets')
sunsets = observer.sun_set_time(times)
sunsets = np.unique(np.round(sunsets.mjd, decimals=4))
names = [
'night', 'sunset', 'sun_n12_setting', 'sun_n18_setting',
'sun_n18_rising', 'sun_n12_rising', 'sunrise', 'moonrise', 'moonset'
]
types = [int]
types.extend([float] * (len(names) - 1))
almanac = np.zeros(sunsets.size, dtype=list(zip(names, types)))
almanac['sunset'] = sunsets
times = Time(sunsets, format='mjd')
print('evening twilight 1')
almanac['sun_n12_setting'] = observer.twilight_evening_nautical(times).mjd
def post_save_night(sender, **kwargs):
if not kwargs.get('raw', False):
night = kwargs['instance']
location = night.location
astropy_time = Time(datetime.combine(night.date, time(12)))
astropy_time_delta = TimeDelta(600.0, format='sec')
# guess if the moon is waxing or waning
if ephem.next_full_moon(night.date) - ephem.Date(night.date) < ephem.Date(night.date) - ephem.previous_full_moon(night.date):
waxing_moon = True
else:
waxing_moon = False
observer = Observer(
longitude=location.longitude,
latitude=location.latitude,
timezone='UTC'
)
moon_phase = observer.moon_phase(astropy_time).value
if waxing_moon:
moon_phase = (math.pi - moon_phase) / (2 * math.pi)
else:
moon_phase = (math.pi + moon_phase) / (2 * math.pi)
times = {
'sunset': observer.sun_set_time(astropy_time, which='next'),
'civil_dusk': observer.twilight_evening_civil(astropy_time, which='next'),
'nautical_dusk': observer.twilight_evening_nautical(astropy_time, which='next'),
'astronomical_dusk': observer.twilight_evening_astronomical(astropy_time, which='next'),
'midnight': observer.midnight(astropy_time, which='next'),
'astronomical_dawn': observer.twilight_morning_astronomical(astropy_time, which='next'),
'nautical_dawn': observer.twilight_morning_nautical(astropy_time, which='next'),
'civil_dawn': observer.twilight_morning_civil(astropy_time, which='next'),
'sunrise': observer.sun_rise_time(astropy_time, which='next'),
}
night.mjd = int(astropy_time.mjd) + 1
night.moon_phase = moon_phase
for key in times:
if times[key].jd > 0:
setattr(night, key, times[key].to_datetime(timezone=utc))
post_save.disconnect(post_save_night, sender=sender)
night.save()
post_save.connect(post_save_night, sender=sender)
moon_positions = []
for i in range(144):
moon_altitude = observer.moon_altaz(astropy_time).alt.degree
moon_position = MoonPosition(
timestamp=astropy_time.to_datetime(timezone=utc),
altitude=moon_altitude,
location=location
)
moon_positions.append(moon_position)
astropy_time += astropy_time_delta
MoonPosition.objects.bulk_create(moon_positions)
class SkySpectrum(object):
def __init__(self, airmass, ecl_lat, SOLARFLUX, tai, gal_lat, gal_lon,
sun_alt, sun_sep, moon_phase, moon_ill, moon_sep, moon_alt,
no_zodi):
self.airmass = airmass
self.ecl_lat = ecl_lat
self.tai = tai
self.gal_lat = gal_lat
self.gal_lon = gal_lon
self.sun_alt = sun_alt
self.sun_sep = sun_sep
self.moon_phase = moon_phase
self.moon_ill = moon_ill
self.moon_sep = moon_sep
self.moon_alt = moon_alt
self.SOLARFLUX = SOLARFLUX
self.no_zodi = no_zodi
Results = pd.DataFrame.from_csv(
'/Users/parkerf/Research/SkyModel/BOSS_Sky/SkyModel/ContModel/python/MoonResults.csv'
)
Results.columns = [
'wl', 'model', 'data_var', 'unexplained_var', 'X2', 'rX2', 'c0',
'c_am', 'tau', 'tau2', 'c_zodi', 'c_isl', 'sol', 'I', 't0', 't1',
't2', 't3', 't4', 'm0', 'm1', 'm2', 'm3', 'm4', 'm5', 'm6', 'feb',
'mar', 'apr', 'may', 'jun', 'jul', 'aug', 'sep', 'oct', 'nov',
'dec', 'c2', 'c3', 'c4', 'c5', 'c6'
]
self.Results = Results[Results['model'] == 'moon']
THIS_DIR = '/Users/parkerf/Research/SkyModel/BOSS_Sky/SkyModel/ContModel/' #os.path.split(os.path.abspath(os.getcwd()))[0]
#print(THIS_DIR)
#calculate albedo
albedo_file = THIS_DIR + '/files/albedo_constants.csv'
albedo_table = pd.read_csv(albedo_file, delim_whitespace=True)
self.AlbedoConstants = {}
for constant in list(albedo_table):
line = interp1d(albedo_table['WAVELENGTH'],
albedo_table[constant],
bounds_error=False,
fill_value=0)
self.AlbedoConstants[constant] = line
#get solar flux data
solar_data = np.load(THIS_DIR + '/files/solar_flux.npy')
self.solar_flux = interp1d(solar_data['MJD'],
solar_data['fluxobsflux'],
bounds_error=False,
fill_value=0)
#get zenith extinction curve
self.zen_ext = np.loadtxt(
'/Users/parkerf/Research/SkyModel/BOSS_Sky/SkyModel/files/ZenithExtinction-KPNO.dat'
)
zen_wave = self.zen_ext[:, 0] / 10.
ext = self.zen_ext[:, 1]
zext = interp1d(zen_wave,
ext,
bounds_error=False,
fill_value='extrapolate')
k = zext(self.Results['wl'])
self.tput = 1 - (10**(-0.4 * k) - 10**(-0.4 * k * self.airmass))
self.apache = Observer(APACHE)
zodi_data = pickle.load(open(THIS_DIR + '/files/s10_zodi.pkl', 'rb'))
self.zodi = zodi_data(np.abs(self.ecl_lat))
isl_data = pickle.load(open(THIS_DIR + '/files/isl_map.pkl', 'rb'))
self.isl = isl_data(self.gal_lon, self.gal_lat)[0]
def albedo(self, moon_phase):
p1 = 4.06054
p2 = 12.8802
p3 = -30.5858
p4 = 16.7498
A = []
for i in range(4):
A.append(self.AlbedoConstants['a%d' % i](self.Results['wl']) *
(moon_phase**i))
#for j in range(1,4):
# A.append(AlbedoConstants['b%s'%str(j)](wave)*(data_table['SOLAR_SELENO']**(2*j-1)))
A.append(self.AlbedoConstants['d1'](self.Results['wl']) *
np.exp(-moon_phase / p1))
A.append(self.AlbedoConstants['d2'](self.Results['wl']) *
np.exp(-moon_phase / p2))
A.append(self.AlbedoConstants['d3'](self.Results['wl']) * np.cos(
(moon_phase - p3) / p4))
lnA = np.sum(A, axis=0)
Albedo = np.exp(lnA)
return Albedo
def create_features(self):
obs_time = self.tai / 86400.
start_time = Time(obs_time, scale='tai', format='mjd', location=APACHE)
self.mjd = start_time.mjd
sun_rise = self.apache.sun_rise_time(start_time, which='next')
sun_set = self.apache.sun_set_time(start_time, which='previous')
hour = ((start_time - sun_set).sec) / 3600
month_frac = start_time.datetime.month + start_time.datetime.day / 30.
hour_frac = hour / (
(Time(sun_rise, format='mjd') - Time(sun_set, format='mjd')).sec /
3600.)
MONTHS = np.zeros(12)
mm = np.rint(month_frac)
if mm == 13:
mm = 1
MONTHS[int(mm - 1)] = 1
self.MONTHS = np.array(MONTHS)
HOURS = np.zeros(6)
levels = np.linspace(0, 1, 7)
idx = np.argmin(np.abs(levels - hour_frac))
HOURS[idx] = 1
self.HOURS = np.array(HOURS)
def get_cont_model(self):
self.create_features()
solarF = self.Results[
'sol'] * self.SOLARFLUX #self.solar_flux(self.mjd-self.Results['I'])
zodi = self.Results['c_zodi'] * self.zodi
airmass = self.Results['c_am'] * self.airmass
months = self.Results['feb'] * self.MONTHS[1] + self.Results[
'mar'] * self.MONTHS[2] + self.Results['apr'] * self.MONTHS[
3] + self.Results['may'] * self.MONTHS[4] + self.Results[
'jun'] * self.MONTHS[5] + self.Results['jul'] * self.MONTHS[
6] + self.Results['sep'] * self.MONTHS[
8] + self.Results['oct'] * self.MONTHS[
9] + self.Results['nov'] * self.MONTHS[
10] + self.Results['dec'] * self.MONTHS[11]
hours = self.Results['c2'] * self.HOURS[1] + self.Results[
'c3'] * self.HOURS[2] + self.Results['c4'] * self.HOURS[
3] + self.Results['c5'] * self.HOURS[4] + self.Results[
'c6'] * self.HOURS[5]
twi = (self.Results['t0'] * np.abs(self.sun_alt) + self.Results['t1'] *
(np.abs(self.sun_alt))**2 +
self.Results['t2'] * np.abs(self.sun_sep)**2 +
self.Results['t3'] * np.abs(self.sun_sep)) * np.exp(
-self.Results['t4'] * self.airmass)
ALB = self.albedo(self.moon_phase)
moon = (self.Results['m0'] * self.moon_alt**2 + self.Results['m1'] *
self.moon_alt + self.Results['m2'] * self.moon_ill**2 +
self.Results['m3'] * self.moon_ill +
self.Results['m4'] * self.moon_sep**2 +
self.Results['m5'] * self.moon_sep) * np.exp(
-self.Results['m6'] * self.airmass) * ALB
if self.sun_alt > -20:
self.model = (self.Results['c0'] + solarF + months + hours +
airmass + zodi +
self.Results['c_isl'] * self.isl) * self.tput + twi
elif self.no_zodi:
self.model = (self.Results['c0'] + solarF + months + hours +
airmass +
self.Results['c_isl'] * self.isl) * self.tput + moon
else:
self.model = (self.Results['c0'] + solarF + months + hours +
airmass + zodi +
self.Results['c_isl'] * self.isl) * self.tput + moon
def get_cont_spectrum(self):
self.get_cont_model()
wl = np.array(self.Results['wl'])
sort = np.argsort(wl)
func = interp1d(wl[sort],
self.model[sort],
bounds_error=False,
fill_value='extrapolate')
wave = np.linspace(360, 1000, (1001 - 360))
return wl[sort], func(wl[sort])
results = []
mjd = mjd_start + 0
counter = 0
names = [
'night', 'sunset', 'sun_n12_setting', 'sun_n18_setting', 'sun_n18_rising',
'sun_n12_rising', 'sunrise', 'moonrise', 'moonset'
]
types = [int]
types.extend([float] * (len(names) - 1))
base_al = np.zeros(1, dtype=list(zip(names, types)))
while mjd < (mjd_start + duration):
times = Time(mjd, format='mjd')
sunsets = observer.sun_set_time(times, which='next')
times = sunsets
almanac = base_al.copy()
almanac['sunset'] = sunsets.mjd
almanac['moonset'] = observer.moon_set_time(times, which='next').mjd
almanac['moonrise'] = observer.moon_rise_time(times, which='next').mjd
almanac['sun_n12_setting'] = observer.twilight_evening_nautical(
times, which='next').mjd
times = observer.twilight_evening_astronomical(times, which='next')
almanac['sun_n18_setting'] = times.mjd
almanac['sun_n18_rising'] = observer.twilight_morning_astronomical(
times, which='next').mjd
almanac['sun_n12_rising'] = observer.twilight_morning_nautical(
times, which='next').mjd
targets = astropy.table.unique(targets, keys=["objectID"])
location = EarthLocation.from_geodetic(-111.5967*u.deg, 31.9583*u.deg,
2096*u.m)
kp = Observer(location=location, name="Kitt Peak",timezone="US/Arizona")
observe_time = Time.now()
observe_time = observe_time + np.linspace(deltat_start, deltat_end, 90)*u.hour
tstart, tend = observe_time[0],observe_time[-1]
frame = AltAz(obstime=observe_time, location=location)
global_constraints = [AirmassConstraint(max = opts.airmass,
boolean_constraint = False),
AtNightConstraint.twilight_civil()]
rise_time = kp.sun_rise_time(tstart, which=u'next', horizon=-12*u.deg).iso
set_time = kp.sun_set_time(tstart, which=u'next', horizon=-12*u.deg).iso
blocks = []
read_out = 10.0 * u.s
nexp = 1
for ii, target in enumerate(targets):
bandpass = target["filter"]
exposure_time = int(target["exposure_time"]) * u.s
priority = target["sig"]
b = ObservingBlock.from_exposures(target["target"],priority,
exposure_time, nexp, read_out,
configuration = {'filter': bandpass})
blocks.append(b)
# Initialize a transitioner object with the slew rate and/or the
def astroplan_test():
'''
'''
currentDate = time.strftime("%Y-%m-%d")
currentTime = time.strftime("%H:%M:%S")
print('\n Today is ', currentDate, ' time is ', currentTime, '\n')
longitude = '36d56m29.000s'
latitude = '+49d38m10.000s'
elevation = 156 * u.m
location = EarthLocation.from_geodetic(longitude, latitude, elevation)
observer = Observer(
name='UTR-2 radio telescope',
location=location,
pressure=0.615 * u.bar,
relative_humidity=0.11,
temperature=0 * u.deg_C,
timezone=timezone('Europe/Kiev'),
description=
"UTR-2 radio telescope, Volokhiv Yar village Kharkiv region Ukraine")
print(' Observer:', observer.name)
coordinates = SkyCoord('20h41m25.9s', '+45d16m49.3s', frame='icrs')
deneb = FixedTarget(name='Deneb', coord=coordinates)
obs_time = Time('2019-08-06 23:00:00')
#utr2 = Observer.at_site(observer)
#obs_time = Time(currentDate +' '+ currentTime) # Pay attention, not UTC, local time!
print(' At', obs_time, ' Night is: ', observer.is_night(obs_time))
print(' Is Deneb on the sky: ', observer.target_is_up(obs_time, deneb))
sunset_tonight = observer.sun_set_time(obs_time, which='nearest')
sunrise_tonight = observer.sun_rise_time(obs_time, which='nearest')
print(' Sunset:', sunset_tonight.iso, ' Sunrise: ', sunrise_tonight.iso)
# Plotting
deneb_rise = observer.target_rise_time(obs_time, deneb) + 5 * u.minute
deneb_set = observer.target_set_time(obs_time, deneb) - 5 * u.minute
print(' Deneb is up from ', deneb_rise, 'till', deneb_set)
deneb_style = {'color': 'r'}
'''
start = Time('2019-08-06 12:00:00')
end = Time('2019-08-07 12:00:00')
time_window = start + (end - start) * np.linspace(0, 1, 20)
plot_sky(deneb, observer, time_window, style_kwargs=deneb_style)
plt.legend(loc='center left', bbox_to_anchor=(1.25, 0.5))
plt.show()
'''
start_time = Time('2019-08-06 18:00:00')
end_time = Time('2019-08-07 09:00:00')
delta_t = end_time - start_time
observe_time = start_time + delta_t * np.linspace(0, 1, 75)
plot_altitude(deneb, observer, observe_time)
plt.grid(b=True, which='both', color='silver', linestyle='-')
plt.show()
return
location = EarthLocation.from_geodetic(longitude, latitude, elevation)
# lokasi = Observer(name='Tilong',location=location,timezone=timezone('Asia/Makassar')) # lokasi pengamat
lokasi = Observer(name='Siak', location=location) #GMS
time = Time('2019-12-26') #UTC
midnight = Time(lokasi.midnight(time).iso)
delta_md = np.linspace(-5, 5, 22) * u.hour
win_time = midnight + delta_md
night = win_time
# day = (midnight + 12*u.hour) + delta_md
day = (midnight + 12 * u.hour) + np.linspace(0, 3, 30) * u.hour # GMS
op = pd.read_csv('op.csv', index_col='nama')
ra = op.ra
dec = op.dec
sunset = lokasi.sun_set_time(time)
sunrise = lokasi.sun_rise_time(time)
moonrise = lokasi.moon_rise_time(time)
moonset = lokasi.moon_set_time(time)
moon_ill = lokasi.moon_illumination(time)
moonaltaz = lokasi.moon_altaz(time)
moonaltaz.name = 'moon'
sunaltaz = lokasi.sun_altaz(time)
sunaltaz.name = 'sun'
def objek(nama, ra, dec):
op = SkyCoord(ra, dec, frame='icrs', unit='deg')
op_name = FixedTarget(coord=op, name=nama)
# betelgeus = SkyCoord.from_name('betelgeuse')
# altaz_frame = lokasi.altaz(time) # ubah lokasi pengamat ke altaz frame
def plan_when_transits_will_occur(
filename='targets.txt',
observatory='Southern African Large Telescope',
start='2017-06-22',
end='2017-06-28',
airmass_limit=2.5,
moon_distance=10,
do_secondary=True,
method='by_night'):
'''
Plan when targets will be visibile and transiting from a site.
Inputs
------
filename : str
A plain text file with the following columns:
target : The name of the target (e.g. J0555-57).
RA : The right ascension of the target (e.g. 05h55m32.62s).
DEC : The declination of the target (e.g. -57d17m26.1s).
epoch* : The epoch of the transit. Youc can either use:
epoch_HJD-2400000 : HJD - 24500000
epoch_BJD-2455000 : MJD
Period : The period of the system (days).
Secondary : can be True or False depending on whether you want
to see when the secondary transits will be.
observatory : str
The observatory you are observing from. See later for list of available
observatories (accepted by astropy).
start : str
The first night of observation (e.g. 2017-08-31).
end : str
The last night of observation (e.g. 2017-09-10).
airmass_limit : float
The maximum airmass you want to observe through.
moon_distance : float
The closest the target can be t the moon in arcmins.
do_secondary = True:
Look for secondary eclipses assuming circularised orbits.
Available observator names are:
'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',
'Gemini South',
'Hale Telescope',
'Haleakala Observatories',
'Happy Jack',
'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',
'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',
'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',
'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',
'gemini_north',
'gemini_south',
'gemn',
'gems',
'greenwich',
'haleakala',
'irtf',
'keck',
'kpno',
'lapalma',
'lasilla',
'lbt',
'lco',
'lick',
'lowell',
'mcdonald',
'mdm',
'medicina',
'mmt',
'mro',
'mso',
'mtbigelow',
'mwo',
'noto',
'ohp',
'paranal',
'salt',
'sirene',
'spm',
'srt',
'sso',
'tona',
'vbo',
'vla'.
'''
###################
# Try reading table
###################
try:
target_table = Table.read(filename, format='ascii')
except:
raise ValueError(
'I cant open the target file (make sure its ascii with the following first line:\ntarget RA DEC epoch_HJD-2400000 Period Secondary'
)
##############################
# try reading observation site
##############################
try:
observation_site = coord.EarthLocation.of_site(observatory)
observation_handle = Observer(location=observation_site)
observation_handle1 = Observer.at_site(observatory)
except:
print(coord.EarthLocation.get_site_names())
raise ValueError('The site is not understood')
###################################
# Try reading start and end times
###################################
try:
start_time = Time(start + ' 12:01:00', location=observation_site)
end_time = Time(end + ' 12:01:00', location=observation_site)
number_of_nights = int(end_time.jd - start_time.jd)
time_range = Time([start + ' 12:01:00', end + ' 12:01:00'])
print('Number of nights: {}'.format(number_of_nights))
except:
raise ValueError('Start and end times not understood')
#####################
# Now do constraints
#####################
#try:
constraints = [
AltitudeConstraint(0 * u.deg, 90 * u.deg),
AirmassConstraint(3),
AtNightConstraint.twilight_civil()
]
#except:
# raise ValueError('Unable to get set constraints')
if method == 'by_night':
for i in range(number_of_nights):
start_time_tmp = start_time + TimeDelta(
i,
format='jd') # get start time (doesent need to be accurate)
end_time_tmp = start_time + TimeDelta(
i + 1,
format='jd') # get start time (doesent need to be accurate)
print('#' * 80)
start_time_tmpss = start_time_tmp.datetime.ctime().split(
) # ['Fri', 'Dec', '24', '12:00:00', '2010']
print('Night {} - {} {} {} {}'.format(i + 1, start_time_tmpss[0],
start_time_tmpss[2],
start_time_tmpss[1],
start_time_tmpss[-1]))
print('#' * 80)
# Now print Almnac information (sunset and end of evening twilight
print('Almnac:')
sun_set = observation_handle.sun_set_time(start_time_tmp,
which='next')
print('Sunset:\t\t\t\t\t\t\t' + sun_set.utc.datetime.ctime())
twilight_evening_astronomical = observation_handle.twilight_evening_astronomical(
start_time_tmp, which='next') # -18
twilight_evening_nautical = observation_handle.twilight_evening_nautical(
start_time_tmp, which='next') # -12
twilight_evening_civil = observation_handle.twilight_evening_civil(
start_time_tmp, which='next') # -6 deg
print('Civil evening twilight (-6 deg) (U.T.C):\t\t' +
twilight_evening_civil.utc.datetime.ctime())
print('Nautical evening twilight (-12 deg) (U.T.C):\t\t' +
twilight_evening_nautical.utc.datetime.ctime())
print('Astronomical evening twilight (-18 deg) (U.T.C):\t' +
twilight_evening_astronomical.utc.datetime.ctime())
print('\n')
twilight_morning_astronomical = observation_handle.twilight_morning_astronomical(
start_time_tmp, which='next') # -18
twilight_morning_nautical = observation_handle.twilight_morning_nautical(
start_time_tmp, which='next') # -12
twilight_morning_civil = observation_handle.twilight_morning_civil(
start_time_tmp, which='next') # -6 deg
print('Astronomical morning twilight (-18 deg) (U.T.C):\t' +
twilight_morning_astronomical.utc.datetime.ctime())
print('Nautical morning twilight (-12 deg) (U.T.C):\t\t' +
twilight_morning_nautical.utc.datetime.ctime())
print('Civil morning twilight (-6 deg) (U.T.C):\t\t' +
twilight_morning_civil.utc.datetime.ctime())
sun_rise = observation_handle.sun_rise_time(start_time_tmp,
which='next')
print('Sunrise:\t\t\t\t\t\t' + sun_rise.utc.datetime.ctime())
print('\n')
# stuff for creating plot
plot_mids = []
plot_names = []
plot_widths = []
for j in range(len(target_table)):
# Extract information
star_coordinates = coord.SkyCoord('{} {}'.format(
target_table['RA'][j], target_table['DEC'][j]),
unit=(u.hourangle, u.deg),
frame='icrs')
star_fixed_coord = FixedTarget(coord=star_coordinates,
name=target_table['target'][j])
####################
# Get finder image
####################
'''
plt.close()
try:
finder_image = plot_finder_image(star_fixed_coord,reticle=True,fov_radius=10*u.arcmin)
except:
pass
plt.savefig(target_table['target'][j]+'_finder_chart.eps')
'''
P = target_table['Period'][j]
Secondary_transit = target_table['Secondary'][j]
transit_half_width = TimeDelta(
target_table['width'][j] * 60 * 60 / 2,
format='sec') # in seconds for a TimeDelta
# now convert T0 to HJD -> JD -> BJD so we can cout period
if 'epoch_HJD-2400000' in target_table.colnames:
#print('Using HJD-2400000')
T0 = target_table['epoch_HJD-2400000'][j]
T0 = Time(T0 + 2400000, format='jd') # HJD given by WASP
ltt_helio = T0.light_travel_time(star_coordinates,
'heliocentric',
location=observation_site)
T0 = T0 - ltt_helio # HJD -> JD
ltt_bary = T0.light_travel_time(star_coordinates,
'barycentric',
location=observation_site)
T0 = T0 + ltt_bary # JD -> BJD
elif 'epoch_BJD-2455000' in target_table.colnames:
#print('Using BJD-2455000')
T0 = target_table['epoch_BJD-2455000'][j] + 2455000
T0 = Time(T0, format='jd') # BJD
else:
print('\n\n\n\n FAILE\n\n\n\n')
continue
##########################################################
# Now start from T0 and count in periods to find transits
##########################################################
# convert star and end time to BJD
ltt_bary_start_time = start_time_tmp.light_travel_time(
star_coordinates, 'barycentric',
location=observation_site) # + TimeDelta(i,format='jd')
start_time_bary = start_time_tmp + ltt_bary_start_time # + TimeDelta(i,format='jd') # convert start time to BJD
ltt_bary_end_time_tmp = end_time_tmp.light_travel_time(
star_coordinates, 'barycentric',
location=observation_site) # + TimeDelta(i,format='jd')
end_time_bary = end_time_tmp + ltt_bary_start_time #+ TimeDelta(i+1,format='jd') # convert end time to BJD and add 1 day 12pm -> 12pm the next day
elapsed = end_time_bary - start_time_bary # now this is 24 hours from the start day 12:00 pm
# now count transits
time = Time(T0.jd, format='jd') # make a temporary copy
transits = []
primary_count, secondary_count = 0, 0
while time.jd < end_time_bary.jd:
if (time.jd > start_time_bary.jd) and (time.jd <
end_time_bary.jd):
if is_observable(constraints,
observation_handle,
[star_fixed_coord],
times=[time])[0] == True:
transits.append(time)
primary_count += 1
if Secondary_transit == 'yes':
timesecondary = time + TimeDelta(P / 2, format='jd')
if (timesecondary.jd > start_time_bary.jd) and (
timesecondary.jd < end_time_bary.jd):
if is_observable(constraints,
observation_handle,
[star_fixed_coord],
times=[timesecondary])[0] == True:
transits.append(timesecondary)
secondary_count += 1
time = time + TimeDelta(P,
format='jd') # add another P to T0
# Now find visible transits
transits = [
i for i in transits
if is_observable(constraints,
observation_handle, [star_fixed_coord],
times=[i])[0] == True
]
if len(transits) == 0:
message = '{} has no transits.'.format(
target_table['target'][j])
print('-' * len(message))
print(message)
print('-' * len(message))
print('\n')
plt.close()
continue
else:
message = '{} has {} primary transits and {} secondary transits.'.format(
target_table['target'][j], primary_count,
secondary_count)
print('-' * len(message))
print(message)
print('RA: {}'.format(target_table['RA'][j]))
print('DEC: {}'.format(target_table['DEC'][j]))
print('Epoch: 2000')
print('T0 (BJD): {}'.format(T0.jd))
print('Period: {}'.format(P))
print('Transit width (hr): {}'.format(
target_table['width'][j]))
print('-' * len(message))
print('\n')
for i in transits:
# currently transit times are in BJD (need to convert to HJD to check
ltt_helio = i.light_travel_time(star_coordinates,
'barycentric',
location=observation_site)
ii = i - ltt_helio
ltt_helio = ii.light_travel_time(star_coordinates,
'heliocentric',
location=observation_site)
ii = ii + ltt_helio
transit_1 = i - transit_half_width - TimeDelta(
7200, format='sec') # ingress - 2 hr
transit_2 = i - transit_half_width - TimeDelta(
3600, format='sec') # ingress - 2 hr
transit_3 = i - transit_half_width # ingress
transit_4 = i + transit_half_width # egress
transit_5 = i + transit_half_width + TimeDelta(
3600, format='sec') # ingress - 2 hr
transit_6 = i + transit_half_width + TimeDelta(
7200, format='sec') # ingress - 2 hr
if (((i.jd - time.jd) / P) - np.floor(
(i.jd - time.jd) / P) < 0.1) or ((
(i.jd - time.jd) / P) - np.floor(
(i.jd - time.jd) / P) > 0.9):
print('Primary Transit:')
print('-' * len('Primary Transit'))
if 0.4 < ((i.jd - time.jd) / P) - np.floor(
(i.jd - time.jd) / P) < 0.6:
print('Secondary Transit')
print('-' * len('Secondary Transit'))
##################
# now get sirmass
##################
altaz = star_coordinates.transform_to(
AltAz(obstime=transit_1, location=observation_site))
hourangle = observation_handle1.target_hour_angle(
transit_1, star_coordinates)
hourangle = 24 * hourangle.degree / 360
if hourangle > 12:
hourangle -= 24
print('Ingress - 2hr (U.T.C):\t\t\t\t\t' +
transit_1.utc.datetime.ctime() +
'\tAirmass: {:.2f}\tHA:{:.2f}'.format(
altaz.secz, hourangle))
altaz = star_coordinates.transform_to(
AltAz(obstime=transit_2, location=observation_site))
hourangle = observation_handle1.target_hour_angle(
transit_2, star_coordinates)
hourangle = 24 * hourangle.degree / 360
if hourangle > 12:
hourangle -= 24
print('Ingress - 1hr (U.T.C):\t\t\t\t\t' +
transit_2.utc.datetime.ctime() +
'\tAirmass: {:.2f}\tHA:{:.2f}'.format(
altaz.secz, hourangle))
altaz = star_coordinates.transform_to(
AltAz(obstime=transit_3, location=observation_site))
hourangle = observation_handle1.target_hour_angle(
transit_3, star_coordinates)
hourangle = 24 * hourangle.degree / 360
if hourangle > 12:
hourangle -= 24
print('Ingress (U.T.C):\t\t\t\t\t' +
transit_3.utc.datetime.ctime() +
'\tAirmass: {:.2f}\tHA:{:.2f}'.format(
altaz.secz, hourangle))
altaz = star_coordinates.transform_to(
AltAz(obstime=i, location=observation_site))
hourangle = observation_handle1.target_hour_angle(
i, star_coordinates)
hourangle = 24 * hourangle.degree / 360
if hourangle > 12:
hourangle -= 24
print('Mid transit (U.T.C):\t\t\t\t\t' +
i.utc.datetime.ctime() +
'\tAirmass: {:.2f}\tHA:{:.2f}'.format(
altaz.secz, hourangle))
altaz = star_coordinates.transform_to(
AltAz(obstime=transit_4, location=observation_site))
hourangle = observation_handle1.target_hour_angle(
transit_4, star_coordinates)
hourangle = 24 * hourangle.degree / 360
if hourangle > 12:
hourangle -= 24
print('Egress (U.T.C):\t\t\t\t\t\t' +
transit_4.utc.datetime.ctime() +
'\tAirmass: {:.2f}\tHA:{:.2f}'.format(
altaz.secz, hourangle))
altaz = star_coordinates.transform_to(
AltAz(obstime=transit_5, location=observation_site))
hourangle = observation_handle1.target_hour_angle(
transit_5, star_coordinates)
hourangle = 24 * hourangle.degree / 360
if hourangle > 12:
hourangle -= 24
print('Egress + 1hr (U.T.C):\t\t\t\t\t' +
transit_5.utc.datetime.ctime() +
'\tAirmass: {:.2f}\tHA:{:.2f}'.format(
altaz.secz, hourangle))
altaz = star_coordinates.transform_to(
AltAz(obstime=transit_6, location=observation_site))
hourangle = observation_handle1.target_hour_angle(
transit_6, star_coordinates)
hourangle = 24 * hourangle.degree / 360
if hourangle > 12:
hourangle -= 24
print('Egress + 2hr (U.T.C):\t\t\t\t\t' +
transit_6.utc.datetime.ctime() +
'\tAirmass: {:.2f}\tHA:{:.2f}'.format(
altaz.secz, hourangle))
print('HJD {} (to check with http://var2.astro.cz/)\n'.
format(ii.jd))
# append stuff for plots
plot_mids.append(i) # astropy Time
plot_names.append(target_table['target'][j])
plot_widths.append(target_table['width'][j])
# Now plot
plt.close()
if len(plot_mids) == 0:
continue
date_formatter = dates.DateFormatter('%H:%M')
#ax.xaxis.set_major_formatter(date_formatter)
# now load dummy transit lightcurves
xp, yp = np.load('lc.npy')
xs, ys = np.load('lcs.npy')
# x = np.linspace(0, 2*np.pi, 400)
# y = np.sin(x**2)
subplots_adjust(hspace=0.000)
number_of_subplots = len(
plot_names) # number of targets transiting that night
time = sun_set + np.linspace(-1, 14,
100) * u.hour # take us to sunset
for i, v in enumerate(xrange(number_of_subplots)):
# exctract params
width = plot_widths[v]
name = plot_names[v]
mid = plot_mids[v]
# now set up dummy lc plot
x_tmp = mid + xp * (width /
2) * u.hour # get right width in hours
# now set up axis
v = v + 1
ax1 = subplot(number_of_subplots, 1, v)
ax1.xaxis.set_major_formatter(date_formatter)
if v == 1:
ax1.set_title(start)
# plot transit model
ax1.plot_date(x_tmp.plot_date, ys, 'k-')
# plot continuum
#xx =time.plot_date
#xx = [uu for uu in xx if (uu<min(x_tmp.plot_date)) or (uu>max(x_tmp.plot_date))]
#ax1.plot_date(xx, np.ones(len(xx)),'k--', alpha=0.3)
ax1.set_xlim(min(time.plot_date), max(time.plot_date))
#ax1.plot_date(mid.plot_date, 0.5, 'ro')
plt.setp(ax1.get_xticklabels(), rotation=30, ha='right')
ax1.set_ylabel(name, rotation=45, labelpad=20)
twilights = [
(sun_set.datetime, 0.0),
(twilight_evening_civil.datetime, 0.1),
(twilight_evening_nautical.datetime, 0.2),
(twilight_evening_astronomical.datetime, 0.3),
(twilight_morning_astronomical.datetime, 0.4),
(twilight_morning_nautical.datetime, 0.3),
(twilight_morning_civil.datetime, 0.2),
(sun_rise.datetime, 0.1),
]
for ii, twii in enumerate(twilights[1:], 1):
ax1.axvspan(twilights[ii - 1][0],
twilights[ii][0],
ymin=0,
ymax=1,
color='grey',
alpha=twii[1])
ax1.grid(alpha=0.5)
ax1.get_yaxis().set_ticks([])
if v != number_of_subplots:
ax1.get_xaxis().set_ticks([])
plt.xlabel('Time [U.T.C]')
#plt.tight_layout()
#plt.savefig('test.eps',format='eps')
plt.show()
def eop(self):
IERS_A_in_cache()
# astroplan.get_IERS_A_or_workaround()
iers.conf.auto_download = False
iers.conf.auto_max_age = None
now = Time.now()
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="IAO Hanle telescopes")
iaohanle
# Calculating the sunset, midnight and sunrise times for our observatory
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')
moon_rise = iaohanle.moon_rise_time(eve_twil_iao, which='nearest')
moon_set = iaohanle.moon_set_time(now, which='nearest')
# moon_alt = iaohanle.moon_altaz(now).alt
# moon_az = iaohanle.moon_altaz(now).az
#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))
Automation.moon_strength = moon_illumination(midnight_iao)
observing_time = (morn_twil_iao - eve_twil_iao).to(u.h)
#print("Total Night hours at IAO tonight {0:.1f} ".format(observing_time))
img = Image.new('RGB', (850, 320), color=(0, 0, 0))
fnt = ImageFont.truetype(
'/var/lib/defoma/gs.d/dirs/fonts/DejaVuSerif.ttf', 15)
d = ImageDraw.Draw(img)
d.text((10, 11),
"IAO Hanle Coordinates: " + str(iaohanle),
font=fnt,
fill=(255, 255, 255))
d.text((10, 71),
"Moon Illumination Strength : " +
str(moon_illumination(midnight_iao)),
font=fnt,
fill=(255, 255, 255))
d.text((10, 101),
"Sunset : " +
Time(sunset_iao, out_subfmt='date_hms').iso + " UTC",
font=fnt,
fill=(255, 255, 255))
d.text((10, 131),
"Astronomical evening twilight : " +
Time(eve_twil_iao, out_subfmt='date_hms').iso + " UTC",
font=fnt,
fill=(255, 255, 255))
d.text((10, 161),
"Astronomical morning twilight : " +
Time(morn_twil_iao, out_subfmt='date_hms').iso + " UTC",
font=fnt,
fill=(255, 255, 255))
d.text((10, 191),
"Sunrise : " +
Time(sunrise_iao, out_subfmt='date_hms').iso + " UTC",
font=fnt,
fill=(255, 255, 255))
d.text((10, 221),
"Moon Rise : " +
Time(moon_rise, out_subfmt='date_hms').iso + " UTC",
font=fnt,
fill=(255, 255, 255))
d.text((10, 251),
"Moon Set : " +
Time(moon_set, out_subfmt='date_hms').iso + " UTC",
font=fnt,
fill=(255, 255, 255))
d.text((10, 281),
"Total Astronomical hours tonight : " +
str(observing_time),
font=fnt,
fill=(255, 255, 255))
img.save('tonight.png')
img.close()
t_start = eve_twil_iao
t_end = morn_twil_iao
# We can turn solar system objects into 'pseudo-fixed' targets to plan observations
mercury_midnight = FixedTarget(name='Mercury',
coord=get_body('mercury', midnight_iao))
mercury_midnight.coord
venus_midnight = FixedTarget(name='Venus',
coord=get_body('venus', midnight_iao))
venus_midnight.coord
uranus_midnight = FixedTarget(name='Uranus',
coord=get_body('uranus', midnight_iao))
uranus_midnight.coord
neptune_midnight = FixedTarget(name='Neptune',
coord=get_body('neptune', midnight_iao))
neptune_midnight.coord
saturn_midnight = FixedTarget(name='Saturn',
coord=get_body('saturn', midnight_iao))
saturn_midnight.coord
jupiter_midnight = FixedTarget(name='Jupiter',
coord=get_body('jupiter', midnight_iao))
jupiter_midnight.coord
mars_midnight = FixedTarget(name='Mars',
coord=get_body('mars', midnight_iao))
mars_midnight.coord
targets = [
mercury_midnight, venus_midnight, mars_midnight, jupiter_midnight,
saturn_midnight, uranus_midnight, neptune_midnight
]
targets
#for target in targets:
#print(iaohanle.target_rise_time(now, target, which='next', horizon=10 * u.deg).iso)
# iaohanle.altaz(now, targets[0])
# print(iaohanle.target_rise_time(now, target, which='next', horizon=10 * u.deg).iso)
# iaohanle.altaz(now, targets[0])
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=[1.0, 0])
plt.xlabel('Planets motion tonight')
# plt.ylim(4,0.5)
# plt.legend()
plt.savefig('planets_motion.png')
plt.close()
# plt.legend(loc=[1.1,0])
coords1 = SkyCoord(
'15h58m3s', '-18d10m0.0s',
frame='icrs') # coordinates of Andromeda Galaxy (M32)
tt1 = FixedTarget(name='Moon', coord=coords1)
tt1.coord
t_observe = t_start + (t_end - t_start) * np.linspace(0.0, 1.0, 20)
plot_sky(tt1, iaohanle, t_observe)
plt.xlabel('Moon motion tonight')
plt.savefig('moon_motion.png')
plt.close()
if (eve_twil_iao <= now):
Automation.eve_twilight_flag = 1
Automation.mor_twilight_flag = 0
Automation.moon_setting_flag = 0
elif (morn_twil_iao <= now):
Automation.eve_twilight_flag = 0
Automation.mor_twilight_flag = 1
Automation.moon_setting_flag = 0
elif (Automation.moon_strength > 0.30):
if (moon_rise <= now):
Automation.eve_twilight_flag = 0
Automation.mor_twilight_flag = 0
Automation.moon_setting_flag = 1
elif (moon_set <= now):
Automation.eve_twilight_flag = 1
Automation.mor_twilight_flag = 0
Automation.moon_setting_flag = 0
def make_np(t_now, nb_jours, tel):
telescope = tel
t0 = Time(t_now)
dt = Time('2018-01-02 00:00:00',scale='tcg')-Time('2018-01-01 00:00:00',scale='tcg') # 1 day
for nb_day in range(0,nb_jours):
t_now=Time(t0+ nb_day*dt, scale='utc', out_subfmt='date').tt.datetime.strftime("%Y-%m-%d")
Path = path_spock + '/DATABASE'
p=os.path.join(Path,str(telescope),'Plans_by_date',str(t_now))
if not os.path.exists(p):
os.makedirs(p)
scheduler_table = Table.read(path_spock + '/DATABASE/' + str(telescope) + '/Archive_night_blocks' +
'/night_blocks_'+ str(telescope) +'_' + str(t_now)+'.txt', format='ascii')
if (tel == 'Io') or tel == ('Europa') or (tel == 'Ganymede') or (tel == 'Callisto'):
scheduler_table = dome_rotation(telescope=tel, day_of_night=t_now) # Intentional dome rotation to
# avoid technical pb on Callisto with dome
name=scheduler_table['target']
date_start = scheduler_table['start time (UTC)']
date_end = scheduler_table['end time (UTC)']
ra1=scheduler_table['ra (h)']
ra2=scheduler_table['ra (m)']
ra3=scheduler_table['ra (s)']
dec1=scheduler_table['dec (d)']
dec2=scheduler_table['dec (m)']
dec3=scheduler_table['dec (s)']
config = scheduler_table['configuration']
filt = []
texp = []
scheduler_table.add_index('target')
try:
index_to_delete=scheduler_table.loc['TransitionBlock'].index
scheduler_table.remove_row(index_to_delete)
except KeyError:
print()
for i in range(0,len(scheduler_table)):
if name[i]!='TransitionBlock':
conf = ast.literal_eval(config[i])
filt.append(conf['filt'])
texp.append(conf['texp'])
if telescope != 'Artemis':
if filt[i] == 'z' or filt[i] == 'g' or filt[i] == 'g' or filt[i] == 'i' or filt[i] == 'r':
a = filt[i]
filt[i] = a+'\''
if telescope == 'Artemis':
autofocus = True
else:
autofocus = False
waitlimit = 600
afinterval = 60
count = '5000'
location = EarthLocation.from_geodetic(-70.40300000000002*u.deg, -24.625199999999996*u.deg,
2635.0000000009704*u.m)
paranal = Observer(location=location, name="paranal", timezone="UTC")
t = Time(t_now)
sun_set = paranal.sun_set_time(t, which='next')
sun_rise = paranal.sun_rise_time(t, which='next')
location_SNO = EarthLocation.from_geodetic(-16.50583131*u.deg, 28.2999988*u.deg, 2390*u.m)
teide = Observer(location=location_SNO, name="SNO", timezone="UTC")
sun_set_teide=teide.sun_set_time(t, which='next')
sun_rise_teide=teide.sun_rise_time(t+1, which='next')
location_saintex = EarthLocation.from_geodetic(-115.48694444444445*u.deg, 31.029166666666665*u.deg,
2829.9999999997976*u.m)
san_pedro = Observer(location=location_saintex, name="saintex", timezone="UTC")
sun_set_san_pedro=san_pedro.sun_set_time(t+1, which='next')
sun_rise_san_pedro=san_pedro.sun_rise_time(t+1, which='next')
Path=Path_txt_files(telescope)
if telescope.find('Europa') is not -1:
startup(t_now, name[0], sun_set.iso, date_start[0], Path, telescope)
if telescope.find('Ganymede') is not -1:
startup(t_now, name[0], sun_set.iso, date_start[0], Path, telescope)
if telescope.find('Io') is not -1:
startup(t_now, name[0],sun_set.iso, date_start[0], Path, telescope)
if telescope.find('Callisto') is not -1:
startup(t_now, name[0], sun_set.iso, date_start[0], Path, telescope)
if telescope.find('Artemis') is not -1:
startup_artemis(t_now, name[0], sun_set_teide.iso, date_start[0], Path)
if telescope.find('Saint-Ex') is not -1:
startup(t_now, name[0], sun_set_san_pedro.iso, date_start[0], Path, telescope)
for i, nam in enumerate(name):
if nam != 'TransitionBlock':
if len(name) >= 2:
if i == 0:
first_target(t_now, nam, date_start[i], date_end[i], waitlimit, afinterval, autofocus,count,
filt[i], texp[i],ra1[i], ra2[i], ra3[i], dec1[i], dec2[i], dec3[i], name[i+1],
Path, telescope)
if i == 0 and telescope.find('Ganymede') is not -1:
first_target(t_now, nam, date_start[i], date_end[i], waitlimit, afinterval, autofocus,count,
filt[i], texp[i], ra1[i], ra2[i], ra3[i], dec1[i], dec2[i], dec3[i], name[i+1],
Path, telescope)
if i == 0 and telescope.find('Artemis') is not -1:
filt[i] = filt[i].replace('\'', '')
if nam == 'haumea':
SPOCKtxt.haumea(t_now,date_start[i],date_end[i], count, filt='Exo', exptime=240,
name_2=name[i+1], binning=2, Path=Path, telescope='Artemis')
else:
first_target(t_now, nam, date_start[i], date_end[i], waitlimit, afinterval, autofocus,count,
filt[i], texp[i], ra1[i], ra2[i],ra3[i], dec1[i], dec2[i], dec3[i], name[i+1],
Path, telescope='Artemis')
if i == 0 and telescope.find('Saint-Ex') is not -1:
first_target(t_now, nam, date_start[i], date_end[i], waitlimit, afinterval, autofocus,count,
filt[i], texp[i], ra1[i], ra2[i], ra3[i], dec1[i], dec2[i], dec3[i], name[i+1],
Path, telescope='Saint-Ex')
if i == (len(name)-1) and telescope.find('Europa') is not -1:
target(t_now,nam,date_start[i],date_end[i],waitlimit,afinterval, autofocus,count,filt[i],
texp[i],ra1[i],ra2[i],ra3[i],dec1[i],dec2[i],dec3[i], None, Path, telescope)
flatdawn(t_now,date_end[i],sun_rise.iso,Path,telescope)
if i == (len(name)-1) and telescope.find('Callisto') is not -1:
target(t_now,nam,date_start[i],date_end[i],waitlimit,afinterval, autofocus,count,filt[i],
texp[i],ra1[i],ra2[i],ra3[i],dec1[i],dec2[i],dec3[i],None,Path,telescope)
flatdawn(t_now,date_end[i],sun_rise.iso,Path,telescope)
if i == (len(name)-1) and telescope.find('Io') is not -1:
target(t_now,nam,date_start[i],date_end[i],waitlimit,afinterval, autofocus,count,filt[i],
texp[i],ra1[i],ra2[i],ra3[i],dec1[i],dec2[i],dec3[i],None,Path,telescope)
flatdawn(t_now,date_end[i],sun_rise.iso,Path,telescope)
if i==(len(name)-1) and telescope.find('Ganymede') is not -1:
target(t_now,nam,date_start[i],date_end[i],waitlimit,afinterval, autofocus,count,filt[i],
texp[i],ra1[i],ra2[i],ra3[i],dec1[i],dec2[i],dec3[i],None,Path,telescope)
flatdawn(t_now,date_end[i],sun_rise.iso,Path,telescope)
if i == (len(name)-1) and telescope.find('Artemis') is not -1:
filt[i] = filt[i].replace('\'', '')
if nam == 'haumea':
SPOCKtxt.haumea(t_now, date_start[i],date_end[i], count, filt='Exo', exptime=240,
name_2=None, binning=2, Path=Path, telescope='Artemis')
else:
target(t_now,nam,date_start[i],date_end[i],waitlimit,afinterval, autofocus,count,
filt[i].replace('\'',''),texp[i],ra1[i],ra2[i],ra3[i],dec1[i],dec2[i],dec3[i],None,
Path,telescope='Artemis')
flatdawn_artemis(t_now,date_end[i],sun_rise_teide.iso,Path)
if i == (len(name)-1) and telescope.find('Saint-Ex') is not -1:
target(t_now,nam,date_start[i],date_end[i],waitlimit,afinterval, autofocus,count,filt[i],
texp[i],ra1[i],ra2[i],ra3[i],dec1[i],dec2[i],dec3[i],None,Path,telescope='Saint-Ex')
flatdawn(t_now,date_end[i],sun_rise_san_pedro.iso,Path,telescope)
if i < (len(name)-1):
if nam == 'haumea':
SPOCKtxt.haumea(t_now, date_start[i],date_end[i], count, filt='Exo', exptime=240,
name_2=name[i+1], binning=2, Path=Path, telescope='Artemis')
else:
target(t_now,nam,date_start[i],date_end[i],waitlimit,afinterval, autofocus,count,filt[i],
texp[i],ra1[i],ra2[i],ra3[i],dec1[i],dec2[i],dec3[i],name[i+1],Path,telescope=telescope)
else:
if i == (len(name)-1) and telescope.find('Europa') is not -1:
target(t_now,nam,date_start[i],date_end[i],waitlimit,afinterval, autofocus,count,filt[i],
texp[i],ra1[i],ra2[i],ra3[i],dec1[i],dec2[i],dec3[i],None,Path,telescope)
flatdawn(t_now,date_end[i],sun_rise.iso,Path,telescope)
if i==(len(name)-1) and telescope.find('Callisto') is not -1:
target(t_now,nam,date_start[i],date_end[i],waitlimit,afinterval, autofocus,count,filt[i],
texp[i],ra1[i],ra2[i],ra3[i],dec1[i],dec2[i],dec3[i],None,Path,telescope)
flatdawn(t_now,date_end[i],sun_rise.iso,Path,telescope)
if i==(len(name)-1) and telescope.find('Io') is not -1:
target(t_now,nam,date_start[i],date_end[i],waitlimit,afinterval, autofocus,count,filt[i],
texp[i],ra1[i],ra2[i],ra3[i],dec1[i],dec2[i],dec3[i],None,Path,telescope)
flatdawn(t_now,date_end[i],sun_rise.iso,Path,telescope)
if i == (len(name)-1) and telescope.find('Ganymede') is not -1:
target(t_now,nam,date_start[i],date_end[i],waitlimit,afinterval, autofocus,count,filt[i],
texp[i],ra1[i],ra2[i],ra3[i],dec1[i],dec2[i],dec3[i],None,Path,telescope)
flatdawn(t_now,date_end[i],sun_rise.iso,Path,telescope)
if i == (len(name)-1) and telescope.find('Artemis') is not -1:
filt[i] = filt[i].replace('\'', '')
if nam == 'haumea':
SPOCKtxt.haumea(t_now, date_start[i],date_end[i], count, filt='Exo', exptime=240,
name_2=None, binning=2, Path=Path, telescope='Artemis')
else:
target(t_now,nam,date_start[i],date_end[i],waitlimit,afinterval, autofocus,count,
filt[i].replace('\'',''),texp[i],ra1[i],ra2[i],ra3[i],dec1[i],dec2[i],dec3[i],
None,Path,telescope='Artemis')
flatdawn_artemis(t_now,date_end[i],sun_rise_teide.iso,Path)
if i == (len(name)-1) and telescope.find('Saint-Ex') is not -1:
target(t_now,nam,date_start[i],date_end[i],waitlimit,afinterval, autofocus,count,
filt[i],texp[i],ra1[i],ra2[i],ra3[i],dec1[i],dec2[i],dec3[i],
None,Path,telescope='Saint-Ex')
flatdawn(t_now,date_end[i],sun_rise_san_pedro.iso,Path,telescope)
if i < (len(name)-1):
if nam == 'haumea':
SPOCKtxt.haumea(t_now, date_start[i],date_end[i], count, filt='Exo', exptime=240,
name_2=name[i+1], binning=2, Path=Path, telescope='Artemis')
else:
target(t_now,nam,date_start[i],date_end[i],waitlimit,afinterval, autofocus,count,
filt[i],texp[i],ra1[i],ra2[i],ra3[i],dec1[i],dec2[i],dec3[i],name[i+1],
Path, telescope=telescope)
if telescope.find('Callisto') is not -1:
flatexo_calli(Path,t_now,filt,nbu=3,nbB=3,nbz=3,nbV=3,nbr=3,nbi=3,nbg=3,nbIz=7,nbExo=3,nbClear=3)
if telescope.find('Ganymede') is not -1:
flatexo_gany(Path,t_now,filt,nbOIII=3,nbHa=3,nbSII=3,nbz=3,nbr=3,nbi=3,nbg=3,nbIz=7,nbExo=3,nbClear=3)
if telescope.find('Io') is not -1:
flatexo_io(Path,t_now,filt,nbu=3,nbHa=3,nbRc=3,nbz=3,nbr=3,nbi=3,nbg=3,nbIz=7,nbExo=3,nbClear=3)
if telescope.find('Europa') is not -1:
flatexo_euro(Path,t_now,filt,nbRc=3,nbB=3,nbz=3,nbV=3,nbr=3,nbi=3,nbg=3,nbIz=7,nbExo=3,nbClear=3)
if telescope.find('Artemis') is not -1:
flatexo_artemis_evening(Path,t_now,filt,nbu=3,nbz=3,nbr=3,nbi=3,nbg=3,nbIz=7,nbExo=7,nbClear=3)
flatexo_artemis_morning(Path,t_now,filt,nbu=3,nbz=3,nbr=3,nbi=3,nbg=3,nbIz=7,nbExo=7,nbClear=3)
if telescope.find('Saint-Ex') is not -1:
flatexo_saintex(Path,t_now,filt,nbu=3,nbz=3,nbr=3,nbi=3,nbg=3,nbIz=9,nbExo=3,nbClear=3)
if telescope.find('Saint-Ex') is not -1:
list_texps = [texp[i] for i in range(len(texp))]
list_texps = list(dict.fromkeys(list_texps))
biasdark(t_now,Path,telescope,texps=list_texps)
else:
if np.any(name == 'haumea'):
biasdark(t_now, Path, telescope,bining_2=True)
else:
biasdark(t_now, Path, telescope, bining_2=False)
p2 = os.path.join(path_spock + '/DATABASE', str(telescope), 'Zip_files', str(t_now))
shutil.make_archive(p2, 'zip', p)
