def generate_blobs(nside,
nexp=1,
exptime=30.,
filter1s=['u', 'u', 'g', 'r', 'i', 'z', 'y'],
filter2s=['g', 'r', 'r', 'i', 'z', 'y', 'y'],
pair_time=22.,
camera_rot_limits=[-80., 80.],
n_obs_template=3,
season=300.,
season_start_hour=-4.,
season_end_hour=2.,
shadow_minutes=60.,
max_alt=76.,
moon_distance=30.,
ignore_obs='DD',
m5_weight=6.,
footprint_weight=0.6,
slewtime_weight=3.,
stayfilter_weight=3.,
template_weight=12.,
footprints=None):
"""
Generate surveys that take observations in blobs.
Parameters
----------
nside : int (32)
The HEALpix nside to use
nexp : int (1)
The number of exposures to use in a visit.
exptime : float (30.)
The exposure time to use per visit (seconds)
filter1s : list of str
The filternames for the first set
filter2s : list of str
The filter names for the second in the pair (None if unpaired)
pair_time : float (22)
The ideal time between pairs (minutes)
camera_rot_limits : list of float ([-80., 80.])
The limits to impose when rotationally dithering the camera (degrees).
n_obs_template : int (3)
The number of observations to take every season in each filter
season : float (300)
The length of season (i.e., how long before templates expire) (days)
season_start_hour : float (-4.)
For weighting how strongly a template image needs to be observed (hours)
sesason_end_hour : float (2.)
For weighting how strongly a template image needs to be observed (hours)
shadow_minutes : float (60.)
Used to mask regions around zenith (minutes)
max_alt : float (76.
The maximium altitude to use when masking zenith (degrees)
moon_distance : float (30.)
The mask radius to apply around the moon (degrees)
ignore_obs : str or list of str ('DD')
Ignore observations by surveys that include the given substring(s).
m5_weight : float (3.)
The weight for the 5-sigma depth difference basis function
footprint_weight : float (0.3)
The weight on the survey footprint basis function.
slewtime_weight : float (3.)
The weight on the slewtime basis function
stayfilter_weight : float (3.)
The weight on basis function that tries to stay avoid filter changes.
template_weight : float (12.)
The weight to place on getting image templates every season
"""
blob_survey_params = {
'slew_approx': 7.5,
'filter_change_approx': 140.,
'read_approx': 2.,
'min_pair_time': 15.,
'search_radius': 30.,
'alt_max': 85.,
'az_range': 90.,
'flush_time': 30.,
'smoothing_kernel': None,
'nside': nside,
'seed': 42,
'dither': True,
'twilight_scale': True
}
surveys = []
times_needed = [pair_time, pair_time * 2]
for filtername, filtername2 in zip(filter1s, filter2s):
detailer_list = []
detailer_list.append(
detailers.Camera_rot_detailer(min_rot=np.min(camera_rot_limits),
max_rot=np.max(camera_rot_limits)))
detailer_list.append(detailers.Close_alt_detailer())
# List to hold tuples of (basis_function_object, weight)
bfs = []
if filtername2 is not None:
bfs.append(
(bf.M5_diff_basis_function(filtername=filtername,
nside=nside), m5_weight / 2.))
bfs.append(
(bf.M5_diff_basis_function(filtername=filtername2,
nside=nside), m5_weight / 2.))
else:
bfs.append((bf.M5_diff_basis_function(filtername=filtername,
nside=nside), m5_weight))
if filtername2 is not None:
bfs.append((bf.Footprint_basis_function(filtername=filtername,
footprint=footprints,
out_of_bounds_val=np.nan,
nside=nside),
footprint_weight / 2.))
bfs.append((bf.Footprint_basis_function(filtername=filtername2,
footprint=footprints,
out_of_bounds_val=np.nan,
nside=nside),
footprint_weight / 2.))
else:
bfs.append(
(bf.Footprint_basis_function(filtername=filtername,
footprint=footprints,
out_of_bounds_val=np.nan,
nside=nside), footprint_weight))
bfs.append((bf.Slewtime_basis_function(filtername=filtername,
nside=nside), slewtime_weight))
bfs.append((bf.Strict_filter_basis_function(filtername=filtername),
stayfilter_weight))
if filtername2 is not None:
bfs.append((bf.N_obs_per_year_basis_function(
filtername=filtername,
nside=nside,
footprint=footprints.get_footprint(filtername),
n_obs=n_obs_template,
season=season,
season_start_hour=season_start_hour,
season_end_hour=season_end_hour), template_weight / 2.))
bfs.append((bf.N_obs_per_year_basis_function(
filtername=filtername2,
nside=nside,
footprint=footprints.get_footprint(filtername2),
n_obs=n_obs_template,
season=season,
season_start_hour=season_start_hour,
season_end_hour=season_end_hour), template_weight / 2.))
else:
bfs.append((bf.N_obs_per_year_basis_function(
filtername=filtername,
nside=nside,
footprint=footprints.get_footprint(filtername),
n_obs=n_obs_template,
season=season,
season_start_hour=season_start_hour,
season_end_hour=season_end_hour), template_weight))
# Masks, give these 0 weight
bfs.append((bf.Zenith_shadow_mask_basis_function(
nside=nside,
shadow_minutes=shadow_minutes,
max_alt=max_alt,
penalty=np.nan,
site='LSST'), 0.))
bfs.append(
(bf.Moon_avoidance_basis_function(nside=nside,
moon_distance=moon_distance),
0.))
filternames = [
fn for fn in [filtername, filtername2] if fn is not None
]
bfs.append(
(bf.Filter_loaded_basis_function(filternames=filternames), 0))
if filtername2 is None:
time_needed = times_needed[0]
else:
time_needed = times_needed[1]
bfs.append(
(bf.Time_to_twilight_basis_function(time_needed=time_needed), 0.))
bfs.append((bf.Not_twilight_basis_function(), 0.))
bfs.append((bf.Planet_mask_basis_function(nside=nside), 0.))
# unpack the basis functions and weights
weights = [val[1] for val in bfs]
basis_functions = [val[0] for val in bfs]
if filtername2 is None:
survey_name = 'blob, %s' % filtername
else:
survey_name = 'blob, %s%s' % (filtername, filtername2)
if filtername2 is not None:
detailer_list.append(
detailers.Take_as_pairs_detailer(filtername=filtername2))
surveys.append(
Blob_survey(basis_functions,
weights,
filtername1=filtername,
filtername2=filtername2,
exptime=exptime,
ideal_pair_time=pair_time,
survey_note=survey_name,
ignore_obs=ignore_obs,
nexp=nexp,
detailers=detailer_list,
**blob_survey_params))
return surveys
def gen_greedy_surveys(nside=32,
nexp=1,
exptime=30.,
filters=['r', 'i', 'z', 'y'],
camera_rot_limits=[-80., 80.],
shadow_minutes=60.,
max_alt=76.,
moon_distance=30.,
ignore_obs='DD',
m5_weight=3.,
footprint_weight=0.3,
slewtime_weight=3.,
stayfilter_weight=3.,
footprints=None):
"""
Make a quick set of greedy surveys
This is a convienence function to generate a list of survey objects that can be used with
lsst.sims.featureScheduler.schedulers.Core_scheduler.
To ensure we are robust against changes in the sims_featureScheduler codebase, all kwargs are
explicitly set.
Parameters
----------
nside : int (32)
The HEALpix nside to use
nexp : int (1)
The number of exposures to use in a visit.
exptime : float (30.)
The exposure time to use per visit (seconds)
filters : list of str (['r', 'i', 'z', 'y'])
Which filters to generate surveys for.
camera_rot_limits : list of float ([-80., 80.])
The limits to impose when rotationally dithering the camera (degrees).
shadow_minutes : float (60.)
Used to mask regions around zenith (minutes)
max_alt : float (76.
The maximium altitude to use when masking zenith (degrees)
moon_distance : float (30.)
The mask radius to apply around the moon (degrees)
ignore_obs : str or list of str ('DD')
Ignore observations by surveys that include the given substring(s).
m5_weight : float (3.)
The weight for the 5-sigma depth difference basis function
footprint_weight : float (0.3)
The weight on the survey footprint basis function.
slewtime_weight : float (3.)
The weight on the slewtime basis function
stayfilter_weight : float (3.)
The weight on basis function that tries to stay avoid filter changes.
"""
# Define the extra parameters that are used in the greedy survey. I
# think these are fairly set, so no need to promote to utility func kwargs
greed_survey_params = {
'block_size': 1,
'smoothing_kernel': None,
'seed': 42,
'camera': 'LSST',
'dither': True,
'survey_name': 'greedy'
}
surveys = []
detailer = detailers.Camera_rot_detailer(min_rot=np.min(camera_rot_limits),
max_rot=np.max(camera_rot_limits))
for filtername in filters:
bfs = []
bfs.append((bf.M5_diff_basis_function(filtername=filtername,
nside=nside), m5_weight))
bfs.append(
(bf.Footprint_basis_function(filtername=filtername,
footprint=footprints,
out_of_bounds_val=np.nan,
nside=nside), footprint_weight))
bfs.append((bf.Slewtime_basis_function(filtername=filtername,
nside=nside), slewtime_weight))
bfs.append((bf.Strict_filter_basis_function(filtername=filtername),
stayfilter_weight))
# Masks, give these 0 weight
bfs.append((bf.Zenith_shadow_mask_basis_function(
nside=nside, shadow_minutes=shadow_minutes, max_alt=max_alt), 0))
bfs.append(
(bf.Moon_avoidance_basis_function(nside=nside,
moon_distance=moon_distance), 0))
bfs.append(
(bf.Filter_loaded_basis_function(filternames=filtername), 0))
bfs.append((bf.Planet_mask_basis_function(nside=nside), 0))
weights = [val[1] for val in bfs]
basis_functions = [val[0] for val in bfs]
surveys.append(
Greedy_survey(basis_functions,
weights,
exptime=exptime,
filtername=filtername,
nside=nside,
ignore_obs=ignore_obs,
nexp=nexp,
detailers=[detailer],
**greed_survey_params))
return surveys
def generate_twilight_neo(nside,
night_pattern=None,
nexp=1,
exptime=1,
camera_rot_limits=[-80., 80.],
footprint_weight=0.1,
slewtime_weight=3.,
stayfilter_weight=3.):
# XXX finish eliminating magic numbers and document this one
slew_estimate = 4.5
filters = 'riz'
survey_name = 'twilight_neo'
footprint = ecliptic_target(nside=nside)
footprints = {}
for filtername in filters:
footprints[filtername] = footprint
sum_footprints = 0
for key in footprints:
sum_footprints += np.sum(footprints[key])
surveys = []
for filtername in filters:
detailer_list = []
detailer_list.append(
detailers.Camera_rot_detailer(min_rot=np.min(camera_rot_limits),
max_rot=np.max(camera_rot_limits)))
detailer_list.append(detailers.Close_alt_detailer())
detailer_list.append(
detailers.Twilight_triple_detailer(slew_estimate=slew_estimate,
n_repeat=3))
bfs = []
bfs.append(
(bf.Footprint_basis_function(filtername=filtername,
footprint=footprints[filtername],
out_of_bounds_val=np.nan,
nside=nside,
all_footprints_sum=sum_footprints),
footprint_weight))
bfs.append((bf.Slewtime_basis_function(filtername=filtername,
nside=nside), slewtime_weight))
bfs.append((bf.Strict_filter_basis_function(filtername=filtername),
stayfilter_weight))
# Need a toward the sun, reward high airmass, with an airmass cutoff basis function.
bfs.append((bf.Near_sun_twilight_basis_function(nside=nside,
max_airmass=2.), 0))
bfs.append((bf.Zenith_shadow_mask_basis_function(nside=nside,
shadow_minutes=60.,
max_alt=76.), 0))
bfs.append((bf.Moon_avoidance_basis_function(nside=nside,
moon_distance=30.), 0))
bfs.append(
(bf.Filter_loaded_basis_function(filternames=filtername), 0))
bfs.append((bf.Planet_mask_basis_function(nside=nside), 0))
bfs.append((bf.Sun_alt_limit_basis_function(), 0))
bfs.append((bf.Time_in_twilight_basis_function(time_needed=5.), 0))
bfs.append((bf.Night_modulo_basis_function(pattern=night_pattern), 0))
# unpack the basis functions and weights
weights = [val[1] for val in bfs]
basis_functions = [val[0] for val in bfs]
# Set huge ideal pair time and use the detailer to cut down the list of observations to fit twilight?
surveys.append(
Blob_survey(basis_functions,
weights,
filtername1=filtername,
filtername2=None,
ideal_pair_time=3.,
nside=nside,
exptime=exptime,
survey_note=survey_name,
ignore_obs=['DD', 'greedy', 'blob'],
dither=True,
nexp=nexp,
detailers=detailer_list,
az_range=180.,
twilight_scale=False))
return surveys
