def get_radec_ephemeris(eph_json_single, start_time, end_time, interval,
observing_facility, observing_site):
observing_facility_class = facility.get_service_class(observing_facility)
sites = observing_facility_class().get_observing_sites()
observer = None
for site_name in sites:
obs_site = sites[site_name]
if obs_site['sitecode'] == observing_site:
observer = coordinates.EarthLocation(
lat=obs_site.get('latitude') * units.deg,
lon=obs_site.get('longitude') * units.deg,
height=obs_site.get('elevation') * units.m)
if observer is None:
# this condition occurs if the facility being requested isn't in the site list provided.
return (None, None, None, None, -1)
ra = []
dec = []
mjd = []
for i in range(len(eph_json_single)):
ra.append(float(eph_json_single[i]['R']))
dec.append(float(eph_json_single[i]['D']))
mjd.append(float(eph_json_single[i]['t']))
ra = np.array(ra)
dec = np.array(dec)
mjd = np.array(mjd)
fra = interp.interp1d(mjd, ra)
fdec = interp.interp1d(mjd, dec)
start = Time(start_time)
end = Time(end_time)
time_range = time_grid_from_range(time_range=[start, end],
time_resolution=interval * units.hour)
tr_mjd = time_range.mjd
airmasses = []
sun_alts = []
for i in range(len(tr_mjd)):
c = SkyCoord(fra(time_range[i].mjd),
fdec(time_range[i].mjd),
frame="icrs",
unit="deg")
t = Time(tr_mjd[i], format='mjd')
sun = coordinates.get_sun(t)
altaz = c.transform_to(AltAz(obstime=t, location=observer))
sun_altaz = sun.transform_to(AltAz(obstime=t, location=observer))
airmass = altaz.secz
airmasses.append(airmass)
sun_alts.append(sun_altaz.alt.value)
airmasses = np.array(airmasses)
sun_alts = np.array(sun_alts)
if np.min(tr_mjd) >= np.min(mjd) and np.max(tr_mjd) <= np.max(mjd):
return (tr_mjd, fra(tr_mjd), fdec(tr_mjd), airmasses, sun_alts)
else:
return (None, None, None, None, -2)
def get_astroplan_sun_and_time(start_time, end_time, interval):
"""
Uses astroplan's time_grid_from_range to generate
an astropy Time object covering the time range.
Uses astropy's get_sun to generate sun positions over
that time range.
If time range is small and interval is coarse, approximates
the sun at a fixed position from the middle of the
time range to speed up calculations.
Since the sun moves ~4 minutes a day, this approximation
happens when the number of days covered by the time range
* 4 is less than the interval (in minutes) / 2.
:param start_time: start of the window for which to calculate the airmass
:type start_time: datetime
:param end_time: end of the window for which to calculate the airmass
:type end_time: datetime
:param interval: time interval, in minutes, at which to calculate airmass within the given window
:type interval: int
:returns: ra/dec positions of the sun over the time range,
time range between start_time and end_time at interval
:rtype: astropy SkyCoord, astropy Time
"""
start = Time(start_time)
end = Time(end_time)
time_range = time_grid_from_range(time_range=[start, end],
time_resolution=interval * units.minute)
number_of_days = end.mjd - start.mjd
if number_of_days * 4 < float(interval) / 2:
# Hack to speed up calculation by factor of ~3
sun_coords = get_sun(time_range[int(len(time_range) / 2)])
sun = FixedTarget(name='sun',
coord=SkyCoord(sun_coords.ra,
sun_coords.dec,
unit='deg'))
else:
sun = get_sun(time_range)
return sun, time_range
def get_forecast_window(start=None,
size=30 * units.day,
cadence=2 * units.min):
"""
Get an array of times in JD to forecast transits.
Defaults to an array covering the next 30 days at 2-min cadence.
Parameters
----------
start : `~astropy.time.Time`, optional
Start of the forecast window. `None` defaults to now.
size : float or `~astropy.units.Quantity`, optional
Size of the forecast window. Defaults to days if unit not specified.
cadence : float or `~astropy.units.Quantity`, optional
Cadence of the times in the forecast window. Defaults to 2-min if
unit not specfied.
Returns
-------
tforecast : `~astropy.time.Time`
Array of times.
"""
if start is None:
start = Time.now()
if type(size) is units.Quantity:
size = size.to(units.day)
else:
size = size * units.day
if type(cadence) is units.Quantity:
cadence = cadence.to(units.day)
else:
cadence = cadence * units.day
tforecast = ap.time_grid_from_range([start, start + size], cadence)
return tforecast
def get_24hr_airmass(target, interval, airmass_limit):
plot_data = []
start = Time(datetime.datetime.utcnow())
end = Time(start.datetime + datetime.timedelta(days=1))
time_range = time_grid_from_range(
time_range = [start, end],
time_resolution = interval*u.minute)
time_plot = time_range.datetime
fixed_target = FixedTarget(name = target.name,
coord = SkyCoord(
target.ra,
target.dec,
unit = 'deg'
)
)
#Hack to speed calculation up by factor of ~3
sun_coords = get_sun(time_range[int(len(time_range)/2)])
fixed_sun = FixedTarget(name = 'sun',
coord = SkyCoord(
sun_coords.ra,
sun_coords.dec,
unit = 'deg'
)
)
#Colors to match SNEx1
colors = {
'Siding Spring': '#3366cc',
'Sutherland': '#dc3912',
'Teide': '#8c6239',
'Cerro Tololo': '#ff9900',
'McDonald': '#109618',
'Haleakala': '#990099'
}
for observing_facility in facility.get_service_classes():
observing_facility_class = facility.get_service_class(observing_facility)
sites = observing_facility_class().get_observing_sites()
for site, site_details in sites.items():
observer = Observer(
longitude = site_details.get('longitude')*u.deg,
latitude = site_details.get('latitude')*u.deg,
elevation = site_details.get('elevation')*u.m
)
sun_alt = observer.altaz(time_range, fixed_sun).alt
obj_airmass = observer.altaz(time_range, fixed_target).secz
bad_indices = np.argwhere(
(obj_airmass >= airmass_limit) |
(obj_airmass <= 1) |
(sun_alt > -18*u.deg) #between astro twilights
)
obj_airmass = [np.nan if i in bad_indices else float(x)
for i, x in enumerate(obj_airmass)]
label = '({facility}) {site}'.format(
facility = observing_facility, site = site
)
plot_data.append(
go.Scatter(x=time_plot, y=obj_airmass, mode='lines', name=label, marker=dict(color=colors.get(site)))
)
return plot_data
def get_24hr_airmass(target, interval, airmass_limit):
plot_data = []
start = Time(datetime.datetime.utcnow())
end = Time(start.datetime + datetime.timedelta(days=1))
time_range = time_grid_from_range(time_range=[start, end],
time_resolution=interval * u.minute)
time_plot = time_range.datetime
fixed_target = FixedTarget(name=target.name,
coord=SkyCoord(target.ra,
target.dec,
unit='deg'))
#Hack to speed calculation up by factor of ~3
sun_coords = get_sun(time_range[int(len(time_range) / 2)])
fixed_sun = FixedTarget(name='sun',
coord=SkyCoord(sun_coords.ra,
sun_coords.dec,
unit='deg'))
for observing_facility in facility.get_service_classes():
if observing_facility != 'LCO':
continue
observing_facility_class = facility.get_service_class(
observing_facility)
sites = observing_facility_class().get_observing_sites()
for site, site_details in sites.items():
observer = Observer(longitude=site_details.get('longitude') *
u.deg,
latitude=site_details.get('latitude') * u.deg,
elevation=site_details.get('elevation') * u.m)
sun_alt = observer.altaz(time_range, fixed_sun).alt
obj_airmass = observer.altaz(time_range, fixed_target).secz
bad_indices = np.argwhere(
(obj_airmass >= airmass_limit) | (obj_airmass <= 1)
| (sun_alt > -18 * u.deg) #between astro twilights
)
obj_airmass = [
np.nan if i in bad_indices else float(x)
for i, x in enumerate(obj_airmass)
]
label = '({facility}) {site}'.format(facility=observing_facility,
site=site)
plot_data.append(
go.Scatter(
x=time_plot,
y=obj_airmass,
mode='lines',
name=label,
))
return plot_data
def make_obs_table(obs_info, source_list, save=True, min_uptime=10):
tab = Table.read(source_list, format="ascii.csv")
targets = [
FixedTarget(coord=SkyCoord(ra=ra, dec=dec, unit=(u.hourangle, u.deg)),
name=source) for source, ra, dec, _ in tab
]
# Some arecibo specific settings
arecibo_site = E.from_geocentric(x=2390490.0,
y=-5564764.0,
z=1994727.0,
unit=u.meter)
arecibo = Observer(location=arecibo_site, name="AO")
constraints = [
AltitudeConstraint((90 - 19.7) * u.deg, (90 - 1.06) * u.deg)
]
min_alt = (90 - 19.7) * u.deg
max_alt = (90 - 1.06) * u.deg
utc_offset = 4 * u.hour
ast_to_utc_offset = TimezoneInfo(utc_offset=utc_offset)
months = [
'Jan', 'Feb', 'Mar', 'Apr', 'May', 'Jun', 'Jul', 'Aug', 'Sep', 'Oct',
'Nov', 'Dec'
]
tstarts = []
tends = []
for index, row in obs_info.iterrows():
obs_month = row['Month']
for i, month in enumerate(months):
if month == obs_month:
break
i = i + 1
if row['End_time(AST)'] == '24:00':
row['End_time(AST)'] = '23:59'
tstarts.append(
f"{row['Year']}-{i:02d}-{row['Start_date']} {row['Start_time(AST)']}"
)
tends.append(
f"{row['Year']}-{i:02d}-{row['End_date']} {row['End_time(AST)']}")
ots = []
for st, et in zip(tstarts, tends):
#setting up for altitude constraints
tstart_obs = Time(st) + utc_offset
tobs_len = (Time(et) - Time(st)).sec / (60 * 60) #hours
delta_t = np.linspace(0, tobs_len, 100) * u.hour
frame_obs = AltAz(obstime=tstart_obs + delta_t, location=arecibo_site)
#setting up for astroplan observability table
st_utc = str(Time(st).to_datetime(timezone=ast_to_utc_offset))[:-6]
et_utc = str(Time(et).to_datetime(timezone=ast_to_utc_offset))[:-6]
time_range = Time([st_utc, et_utc], scale='utc')
print(f'Making observability table for {st}')
ot = observability_table(constraints,
arecibo,
targets,
times=time_grid_from_range(
time_range, 5 * u.min)).to_pandas()
ot['ever obs'] = ot['ever observable']
ot = ot.drop([
'fraction of time observable', 'ever observable',
'always observable'
],
axis=1)
ot_obs = ot[ot['ever obs']]
ra = []
dec = []
set_time = []
up_time = []
rise_time = []
tstart_observable = []
tend_observable = []
print(f'Processing observability table for {st}')
for i, row in ot_obs.iterrows():
ra.append(targets[i].ra.deg)
dec.append(targets[i].dec.deg)
# manual altitude constraints
target = SkyCoord(ra=targets[i].ra, dec=targets[i].dec)
frame_obs_altaz = target.transform_to(frame_obs)
times_observable = tstart_obs + delta_t[
(frame_obs_altaz.alt > min_alt)
& (frame_obs_altaz.alt < max_alt)]
tstart_observable.append(times_observable.min() - utc_offset)
if Time(times_observable.max()) < Time(et_utc):
tend_observable.append(times_observable.max() - utc_offset)
up_time.append((Time(times_observable.max()) -
Time(times_observable.min())).sec / 60)
else:
tend_observable.append(Time(et_utc) - utc_offset)
up_time.append(
(Time(et_utc) - Time(times_observable.min())).sec / 60)
ot_obs['RA'] = ra
ot_obs['DEC'] = dec
ot_obs['uptime (min)'] = up_time
ot_obs['tstart_obs (AST)'] = tstart_observable
ot_obs['tend_obs (AST)'] = tend_observable
ot_obs = ot_obs[ot_obs['uptime (min)'] > min_uptime]
ot_obs = ot_obs.drop(['ever obs'], axis=1)
ots.append(ot_obs)
if save:
fname = str(Time(st_utc) - utc_offset)
f = open(fname.replace(' ', '_') + '.tab', 'w')
f.write(
f'Observations from {str(Time(st_utc) - utc_offset)} to {str(Time(et_utc) - utc_offset)}\n'
)
f.write(f'Length of observations: {tobs_len:.2f}hr \n')
f.write(
tabulate(ot_obs,
headers='keys',
tablefmt='psql',
showindex="never"))
f.close()
obs_database = {
name: dict(times=[], fluxes=[], model=[], transit=False)
for name in table['spc']
}
for i in range(n_years * 365):
# Simulate weather losses
if np.random.rand() > fraction_cloudy:
time = start_time + i * u.day
night_start = saintex.twilight_evening_nautical(time,
which='previous')
night_end = saintex.twilight_morning_nautical(time, which='next')
night_duration = night_end - night_start
times = time_grid_from_range((night_start, night_end),
time_resolution=1.6 * u.min)
obs_table = observability_table(constraints,
saintex,
targets,
times=times)
# Prevent memory from getting out of hand by clearing out cache:
saintex._altaz_cache = {}
mask_targets_visible_2hrs = obs_table[
'fraction of time observable'] * night_duration > 6 * u.hr
object_inds_to_observe = np.random.choice(
np.argwhere(mask_targets_visible_2hrs)[:, 0],
size=n_objects_per_night)
target_inds_observed.update(object_inds_to_observe)
#
#
#observability_table = observability_table(constraints, observer, targets[2:],
# time_range=time_range,
# time_grid_resolution=1*u.hour)
#print(observability_table)
## calculate observability of most-observable target
#observability = is_observable(constraints, observer, targets[-1],
# time_range=time_range,
# time_grid_resolution=1*u.hr)
# Create grid of times from ``start_time`` to ``end_time``
# with resolution ``time_resolution``
time_resolution = 7 * u.day
time_grid = time_grid_from_range(time_range, time_resolution=time_resolution)
observability_grid = np.zeros((24, len(time_grid)), dtype='bool')
for targetlon in (-5, 5, 15, 25, 35, 45, 55):
target = coordinates.SkyCoord(targetlon * u.deg,
0 * u.deg,
frame='galactic')
pb = ProgressBar(observability_grid.shape[1])
for ii, day in (enumerate(time_grid)):
day_time_grid = time_grid_from_range(Time(
[day, day + TimeDelta(1 * u.day)]),
time_resolution=1 * u.hour)
assert np.all(np.isfinite(day_time_grid.value))
longitude = -104.2455
latitude = 34.4714
elevation = 0 * u.m
location = EarthLocation.from_geodetic(longitude, latitude, elevation)
observer = Observer(name='Fort Sumner',
location=location,
pressure=0.615 * u.bar,
relative_humidity=0.11,
temperature=0 * u.deg_C,
timezone=timezone('US/Mountain'),
description="Launch")
time_range = Time(["2016-09-16 03:00","2016-09-16 13:00"],scale='utc')
time_grid = time_grid_from_range(time_range)
clean_table = pickle.load(open('data/clean_table.data','r'))
# add ratios
clean_table['R19'] = clean_table['R50_19']/clean_table['R50_cal_19']
clean_table['R31'] = clean_table['R50_31']/clean_table['R50_cal_31']
clean_table['R37'] = clean_table['R50_37']/clean_table['R50_cal_37']
clean_table.sort(['F37','R37'])
clean_table.reverse()
clean_table = clean_table[clean_table['F37']>20]
print clean_table['SOFIA_name','RA','DEC']
#targets = [FixedTarget(coord=SkyCoord(ra=334.82557*u.deg,dec=63.313065*u.deg),name='S140.5')]
prihdr['cmd'] = ('X', 'command sent to filter-wheel box')
prihdr['channel'] = ('X', 'camera type (e.g. B=blue,R=red)')
prihdr['F_T'] = ('X', 'filter type (e.g. N=narrow band, g=SDSS g)')
prihdr['F_I'] = (0, 'index of filter')
prihdr['F_B'] = (0, 'wavelength (A)')
prihdr['exp'] = (0, 'Exposure time (seconds)')
prihdr['ra'] = (179.755936891, 'RA of obj (deg)')
prihdr['dec'] = (-0.524622205172, 'DEC of obj (deg)')
prihdr['ra_hms'] = (c.ra.to_string(unit=u.hourangle,
sep=':'), 'RA of obj (hourangle)')
prihdr['dec_dms'] = (c.dec.to_string(unit=u.deg, sep=':'), 'DEC of obj (deg)')
################################################################
time_range = Time(["2017-09-03 20:00:00", "2017-09-04 08:00"])
#time1=Time("2016-03-04 12:04")
time_grid = time_grid_from_range(time_range, time_resolution=12 * u.min)
#tt=datetime.datetime(2016, 11, 07, 10, 49, 53, 239,tzinfo=pytz.timezone('Asia/Urumqi'))
data = scipy.ndimage.rotate(hdu[0].data, -6, reshape=False)
fig = plt.figure()
plt.imshow(data, origin='lower', vmin=-0.2, vmax=0.2, cmap=plt.cm.viridis)
exp = 1800
#import numpy as np
path = 'data4/'
#for i in xrange(1):
for i in [1, 2, 3, 4, 6]:
# II=np.random.randint(11)
ff = [0, 1, 2, 0, 1, 1, 6, 7]
II = ff[i]
