def test_rectifiedSED(self):
"""
Check for an extreme case that the SN seds are being rectified. This is
done by setting up an extreme case where there will be negative seds, and
checking that this is indeed the case, and checking that they are not
negative if rectified.
"""
snobj = SNObject(ra=30., dec=-60., source='salt2')
snobj.set(z=0.96, t0=self.mjdobs, x1=-3., x0=1.8e-6)
snobj.rectifySED = False
times = np.arange(self.mjdobs - 50., self.mjdobs + 150., 1.)
badTimes = []
for time in times:
sed = snobj.SNObjectSED(time=time,
bandpass=self.lsstBandPass['r'])
if any(sed.flambda < 0.):
badTimes.append(time)
# Check that there are negative SEDs
assert(len(badTimes) > 0)
snobj.rectifySED = True
for time in badTimes:
sed = snobj.SNObjectSED(time=time,
bandpass=self.lsstBandPass['r'])
self.assertGreaterEqual(sed.calcADU(bandpass=self.lsstBandPass['r'],
photParams=self.rectify_photParams), 0.)
self.assertFalse(any(sed.flambda < 0.))
def load_SNsed(self):
"""
returns a list of SN seds in `lsst.sims.photUtils.Sed` observed within
the spatio-temporal range specified by obs_metadata
"""
c, x1, x0, t0, _z, ra, dec = self.column_by_name('c'),\
self.column_by_name('x1'),\
self.column_by_name('x0'),\
self.column_by_name('t0'),\
self.column_by_name('redshift'),\
self.column_by_name('raJ2000'),\
self.column_by_name('decJ2000')
SNobject = SNObject()
raDeg = np.degrees(ra)
decDeg = np.degrees(dec)
sedlist = []
for i in range(self.numobjs):
SNobject.set(z=_z[i], c=c[i], x1=x1[i], t0=t0[i], x0=x0[i])
SNobject.setCoords(ra=raDeg[i], dec=decDeg[i])
SNobject.mwEBVfromMaps()
sed = SNobject.SNObjectSED(time=self.mjdobs,
bandpass=self.lsstBandpassDict,
applyExitinction=True)
sedlist.append(sed)
return sedlist
def get_snbrightness(self):
"""
getters for brightness related parameters of sn
"""
if self._sn_object_cache is None or len(
self._sn_object_cache) > 1000000:
self._sn_object_cache = {}
c, x1, x0, t0, _z, ra, dec = self.column_by_name('c'),\
self.column_by_name('x1'),\
self.column_by_name('x0'),\
self.column_by_name('t0'),\
self.column_by_name('redshift'),\
self.column_by_name('raJ2000'),\
self.column_by_name('decJ2000')
raDeg = np.degrees(ra)
decDeg = np.degrees(dec)
ebv = self.column_by_name('EBV')
id_list = self.column_by_name('snid')
bandname = self.obs_metadata.bandpass
if isinstance(bandname, list):
raise ValueError('bandname expected to be string, but is list\n')
bandpass = self.lsstBandpassDict[bandname]
# Initialize return array so that it contains the values you would get
# if you passed through a t0=self.badvalues supernova
vals = np.array([[0.0] * len(t0), [np.inf] * len(t0),
[np.nan] * len(t0), [np.inf] * len(t0),
[0.0] * len(t0)]).transpose()
for i in np.where(
np.logical_and(
np.isfinite(t0),
np.abs(self.mjdobs - t0) < self.maxTimeSNVisible))[0]:
if id_list[i] in self._sn_object_cache:
SNobject = self._sn_object_cache[id_list[i]]
else:
SNobject = SNObject()
SNobject.set(z=_z[i], c=c[i], x1=x1[i], t0=t0[i], x0=x0[i])
SNobject.setCoords(ra=raDeg[i], dec=decDeg[i])
SNobject.set_MWebv(ebv[i])
self._sn_object_cache[id_list[i]] = SNobject
if self.mjdobs <= SNobject.maxtime(
) and self.mjdobs >= SNobject.mintime():
# Calculate fluxes
fluxinMaggies = SNobject.catsimBandFlux(
time=self.mjdobs, bandpassobject=bandpass)
mag = SNobject.catsimBandMag(time=self.mjdobs,
fluxinMaggies=fluxinMaggies,
bandpassobject=bandpass)
vals[i, 0] = fluxinMaggies
vals[i, 1] = mag
flux_err = SNobject.catsimBandFluxError(
time=self.mjdobs,
bandpassobject=bandpass,
m5=self.obs_metadata.m5[bandname],
photParams=self.photometricparameters,
fluxinMaggies=fluxinMaggies,
magnitude=mag)
mag_err = SNobject.catsimBandMagError(
time=self.mjdobs,
bandpassobject=bandpass,
m5=self.obs_metadata.m5[bandname],
photParams=self.photometricparameters,
magnitude=mag)
sed = SNobject.SNObjectSED(time=self.mjdobs,
bandpass=self.lsstBandpassDict,
applyExtinction=True)
adu = sed.calcADU(bandpass,
photParams=self.photometricparameters)
vals[i, 2] = flux_err
vals[i, 3] = mag_err
vals[i, 4] = adu
return (vals[:, 0], vals[:, 1], vals[:, 2], vals[:, 3], vals[:, 4])
class SNObject_tests(unittest.TestCase):
@classmethod
def tearDownClass(cls):
sims_clean_up()
def setUp(self):
"""
Setup tests
SN_blank: A SNObject with no MW extinction
"""
mydir = get_config_dir()
print('===============================')
print('===============================')
print (mydir)
print('===============================')
print('===============================')
# A range of wavelengths in Ang
self.wave = np.arange(3000., 12000., 50.)
# Equivalent wavelenths in nm
self.wavenm = self.wave / 10.
# Time to be used as Peak
self.mjdobs = 571190
# Check that we can set up a SED
# with no extinction
self.SN_blank = SNObject()
self.SN_blank.setCoords(ra=30., dec=-60.)
self.SN_blank.set(z=0.96, t0=571181, x1=2.66, c=0.353, x0=1.796e-6)
self.SN_blank.set_MWebv(0.)
self.SN_extincted = SNObject(ra=30., dec=-60.)
self.SN_extincted.set(z=0.96, t0=571181, x1=2.66, c=0.353,
x0=1.796112e-06)
self.SNCosmoModel = self.SN_extincted.equivalentSNCosmoModel()
self.rectify_photParams = PhotometricParameters()
self.lsstBandPass = BandpassDict.loadTotalBandpassesFromFiles()
self.SNCosmoBP = sncosmo.Bandpass(wave=self.lsstBandPass['r'].wavelen,
trans=self.lsstBandPass['r'].sb,
wave_unit=astropy.units.Unit('nm'),
name='lsst_r')
def tearDown(self):
del self.SNCosmoBP
del self.SN_blank
del self.SN_extincted
def test_SNstatenotEmpty(self):
"""
Check that the state of SNObject, stored in self.SNstate has valid
entries for all keys and does not contain keys with None type Values.
"""
myDict = self.SN_extincted.SNstate
for key in myDict:
assert myDict[key] is not None
def test_attributeDefaults(self):
"""
Check the defaults and the setter properties for rectifySED and
modelOutSideRange
"""
snobj = SNObject(ra=30., dec=-60., source='salt2')
self.assertEqual(snobj.rectifySED, True)
self.assertEqual(snobj.modelOutSideTemporalRange, 'zero')
snobj.rectifySED = False
self.assertFalse(snobj.rectifySED, False)
self.assertEqual(snobj.modelOutSideTemporalRange, 'zero')
def test_raisingerror_forunimplementedmodelOutSideRange(self):
"""
check that correct error is raised if the user tries to assign an
un-implemented model value to
`sims.catUtils.supernovae.SNObject.modelOutSideTemporalRange`
"""
snobj = SNObject(ra=30., dec=-60., source='salt2')
assert snobj.modelOutSideTemporalRange == 'zero'
with self.assertRaises(ValueError) as context:
snobj.modelOutSideTemporalRange = 'False'
self.assertEqual('Model not implemented, defaulting to zero method\n',
context.exception.args[0])
def test_rectifiedSED(self):
"""
Check for an extreme case that the SN seds are being rectified. This is
done by setting up an extreme case where there will be negative seds, and
checking that this is indeed the case, and checking that they are not
negative if rectified.
"""
snobj = SNObject(ra=30., dec=-60., source='salt2')
snobj.set(z=0.96, t0=self.mjdobs, x1=-3., x0=1.8e-6)
snobj.rectifySED = False
times = np.arange(self.mjdobs - 50., self.mjdobs + 150., 1.)
badTimes = []
for time in times:
sed = snobj.SNObjectSED(time=time,
bandpass=self.lsstBandPass['r'])
if any(sed.flambda < 0.):
badTimes.append(time)
# Check that there are negative SEDs
assert(len(badTimes) > 0)
snobj.rectifySED = True
for time in badTimes:
sed = snobj.SNObjectSED(time=time,
bandpass=self.lsstBandPass['r'])
self.assertGreaterEqual(sed.calcADU(bandpass=self.lsstBandPass['r'],
photParams=self.rectify_photParams), 0.)
self.assertFalse(any(sed.flambda < 0.))
def test_ComparebandFluxes2photUtils(self):
"""
The SNObject.catsimBandFlux computation uses the sims.photUtils.sed
band flux computation under the hood. This test makes sure that these
definitions are in sync
"""
snobject_r = self.SN_extincted.catsimBandFlux(
bandpassobject=self.lsstBandPass['r'],
time=self.mjdobs)
# `sims.photUtils.Sed`
sed = self.SN_extincted.SNObjectSED(time=self.mjdobs,
bandpass=self.lsstBandPass['r'])
sedflux = sed.calcFlux(bandpass=self.lsstBandPass['r'])
np.testing.assert_allclose(snobject_r, sedflux / 3631.0)
def test_CompareBandFluxes2SNCosmo(self):
"""
Compare the r band flux at a particular time computed in SNObject and
SNCosmo for MW-extincted SEDs. While the underlying sed is obtained
from SNCosmo the integration with the bandpass is an independent
calculation in SNCosmo and catsim
"""
times = self.mjdobs
catsim_r = self.SN_extincted.catsimBandFlux(
bandpassobject=self.lsstBandPass['r'],
time=times)
sncosmo_r = self.SNCosmoModel.bandflux(band=self.SNCosmoBP,
time=times, zpsys='ab',
zp=0.)
np.testing.assert_allclose(sncosmo_r, catsim_r)
def test_CompareBandMags2SNCosmo(self):
"""
Compare the r band flux at a particular time computed in SNObject and
SNCosmo for MW-extincted SEDs. Should work whenever the flux comparison
above works.
"""
times = self.mjdobs
catsim_r = self.SN_extincted.catsimBandMag(
bandpassobject=self.lsstBandPass['r'],
time=times)
sncosmo_r = self.SNCosmoModel.bandmag(band=self.SNCosmoBP,
time=times, magsys='ab')
np.testing.assert_allclose(sncosmo_r, catsim_r)
def test_CompareExtinctedSED2SNCosmo(self):
"""
Compare the extincted SEDS in SNCosmo and SNObject. Slightly more
non-trivial than comparing unextincted SEDS, as the extinction in
SNObject uses different code from SNCosmo. However, this is still
using the same values of MWEBV, rather than reading it off a map.
"""
SNObjectSED = self.SN_extincted.SNObjectSED(time=self.mjdobs,
wavelen=self.wavenm)
SNCosmoSED = self.SNCosmoModel.flux(time=self.mjdobs, wave=self.wave) \
* 10.
np.testing.assert_allclose(SNObjectSED.flambda, SNCosmoSED,
rtol=1.0e-7)
def test_CompareUnextinctedSED2SNCosmo(self):
"""
Compares the unextincted flux Densities in SNCosmo and SNObject. This
is mereley a sanity check as SNObject uses SNCosmo under the hood.
"""
SNCosmoFluxDensity = self.SN_blank.flux(wave=self.wave,
time=self.mjdobs) * 10.
unextincted_sed = self.SN_blank.SNObjectSED(time=self.mjdobs,
wavelen=self.wavenm)
SNObjectFluxDensity = unextincted_sed.flambda
np.testing.assert_allclose(SNCosmoFluxDensity, SNObjectFluxDensity,
rtol=1.0e-7)
def test_redshift(self):
"""
test that the redshift method works as expected by checking that
if we redshift a SN from its original redshift orig_z to new_z where
new_z is smaller (larger) than orig_z:
- 1. x0 increases (decreases)
- 2. source peak absolute magnitude in BesselB band stays the same
"""
from astropy.cosmology import FlatLambdaCDM
cosmo = FlatLambdaCDM(H0=70., Om0=0.3)
orig_z = self.SN_extincted.get('z')
orig_x0 = self.SN_extincted.get('x0')
peakabsMag = self.SN_extincted.source_peakabsmag('BessellB', 'AB', cosmo=cosmo)
lowz = orig_z * 0.5
highz = orig_z * 2.0
# Test Case for lower redshift
self.SN_extincted.redshift(z=lowz, cosmo=cosmo)
low_x0 = self.SN_extincted.get('x0')
lowPeakAbsMag = self.SN_extincted.source_peakabsmag('BessellB', 'AB', cosmo=cosmo)
# Test 1.
self.assertGreater(low_x0, orig_x0)
# Test 2.
self.assertAlmostEqual(peakabsMag, lowPeakAbsMag, places=14)
# Test Case for higher redshift
self.SN_extincted.redshift(z=highz, cosmo=cosmo)
high_x0 = self.SN_extincted.get('x0')
HiPeakAbsMag = self.SN_extincted.source_peakabsmag('BessellB', 'AB', cosmo=cosmo)
# Test 1.
self.assertLess(high_x0, orig_x0)
# Test 2.
self.assertAlmostEqual(peakabsMag, HiPeakAbsMag, places=14)
def test_bandFluxErrorWorks(self):
"""
test that bandflux errors work even if the flux is negative
"""
times = self.mjdobs
e = self.SN_extincted.catsimBandFluxError(times,
self.lsstBandPass['r'],
m5=24.5, fluxinMaggies=-1.0)
assert isinstance(e, np.float)
print(e)
assert not(np.isinf(e) or np.isnan(e))
class SNSynthPhotFactory:
"""
Factory class to return the SyntheticPhotometry objects for a SN Ia
as a function of time. This uses the 'salt2-extended' model in
sncosmo as implemented in sims_catUtils.
"""
lsst_bp_dict = BandpassDict.loadTotalBandpassesFromFiles()
def __init__(self, z=0, t0=0, x0=1, x1=0, c=0, snra=0, sndec=0):
"""
Parameters
----------
z: float [0]
Redshift of the SNIa object to pass to sncosmo.
t0: float [0]
Time in mjd of phase=0, corresponding to the B-band
maximum.
x0: float [1]
Normalization factor for the lightcurves.
x1: float [0]
Empirical parameter controlling the stretch in time of the
light curves
c: float [0]
Empirical parameter controlling the colors.
snra: float [0]
RA in degrees of the SNIa.
sndec: float [0]
Dec in degrees of the SNIa.
"""
self.sn_obj = SNObject(snra, sndec)
self.sn_obj.set(z=z,
t0=t0,
x0=x0,
x1=x1,
c=c,
hostebv=0,
hostr_v=3.1,
mwebv=0,
mwr_v=3.1)
self.bp_dict = self.lsst_bp_dict
def set_bp_dict(self, bp_dict):
"""
Set the bandpass dictionary.
Parameters
----------
bp_dict: lsst.sims.photUtils.BandpassDict
Dictionary containing the bandpasses. If None, the standard
LSST total bandpasses will be used.
"""
self.bp_dict = bp_dict
def create(self, mjd):
"""
Return a SyntheticPhotometry object for the specified time in MJD.
Parameters
----------
mjd: float
Observation time in MJD.
Returns
-------
desc.sims_truthcatalog.SyntheticPhotometry
"""
# Create the Sed object. Milky Way extinction will be
# below, so set applyExtinction=False.
sed = self.sn_obj.SNObjectSED(mjd,
bandpass=self.bp_dict,
applyExtinction=False)
# The redshift was applied to the model SED computed by
# sncosmo in the __init__ function, so set redshift=0 here.
synth_phot = SyntheticPhotometry.create_from_sed(sed, redshift=0)
synth_phot.add_MW_dust(*np.degrees(self.sn_obj.skycoord).flatten())
return synth_phot
def __getattr__(self, attr):
# Pass any attribute access requests to the SNObject instance.
return getattr(self.sn_obj, attr)
