def to_mags_old(self, b, z=0., d=None, magnification=1.):
from pystella.rf.star import Star
from pystella.rf import band
# from pystella.rf.lc import LightCurve, SetLightCurve
if b is None:
raise ValueError("Band must be defined.")
if not self.is_time:
return ValueError("No spectral time points.")
# mags = np.zeros(len(self.Time))
times = []
mags = []
for k, t in enumerate(self.Time):
try:
star = Star(k, self.get_spec(k), is_flux_eq_luminosity=True)
star.set_distance(d)
star.set_redshift(z)
star.set_magnification(magnification)
# mag = star.flux_to_mag(b)
if b.Name == band.Band.NameBol:
mag = star.magBol(b)
else:
mag = star.magAB(b)
times.append(t)
mags.append(mag)
except ValueError as ex:
logger.error("Could not compute mag {} for band {} at {} due to {}.".
format(self.Name, b.Name, t, ex))
return times, mags
def to_mag(self, b, z=0., d=phys.pc2cm(10.), magnification=1.):
"""
Compute the magnitude for the band
:param b: photometric band
:param z: redshift, default: 0
:param d: distance [cm], default: 10 pc
:param magnification: , default: 1
:return:
"""
if b is None:
raise ValueError("Band must be defined.")
from pystella.rf.star import Star
from pystella.rf import band
star = Star('', self, is_flux_eq_luminosity=True)
star.set_distance(d)
star.set_redshift(z)
star.set_magnification(magnification)
# mag = star.flux_to_mag(b)
if b.Name in [band.Band.NameBol, band.Band.NameBolQuasi, band.Band.NameUBVRI]:
mag = star.magBol(b)
else:
mag = star.magAB(b)
return mag
def flux_to_mags(self, b, z=0., d=0., magnification=1.):
from pystella.rf.star import Star
if b is None:
raise ValueError("Band must be defined.")
if not self.is_time:
return ValueError("No spectral time points.")
mags = np.zeros(len(self.Time))
for k, t in enumerate(self.Time):
star = Star(k, self.get_spec(k))
star.set_distance(d)
star.set_redshift(z)
star.set_magnification(magnification)
# mag = star.flux_to_mag(b)
mag = star.magAB(b)
mags[k] = mag
# if self.times[k] > 50:
# spec.plot_spec(title="t=%f, mag=%f" % (self.times[k], mag))
return mags
def flux_to_mags(self, b, z=0., d=0., magnification=1.):
if b is None:
return None
if not self.is_time:
return None
mags = np.zeros(len(self.Time))
for k in range(len(self.Time)):
star = Star(k, self.get_spec(k))
star.set_distance(d)
star.set_redshift(z)
star.set_magnification(magnification)
# mag = star.flux_to_mag(b)
mag = star.magAB(b)
mags[k] = mag
# if self.times[k] > 50:
# spec.plot_spec(title="t=%f, mag=%f" % (self.times[k], mag))
return mags
def epsilon(theta, freq, mag, bands, radius, dist, z):
temp_color, zeta = theta
e = 0
if temp_color < 0 or zeta < 0:
for b in bands:
e += mag[b] ** 2
return e
# sp = spectrum.SpectrumDilutePlanck(freq, temp_color, W=zeta**2)
sp = spectrum.SpectrumDilutePlanck(freq, temp_color, W=zeta ** 2)
# sp.correct_zeta(zeta)
star = Star("bb", sp)
star.set_radius_ph(radius)
star.set_distance(dist)
star.set_redshift(z)
mag_bb = {b: star.magAB(band.band_by_name(b)) for b in bands}
for b in bands:
e += (mag[b] - mag_bb[b]) ** 2
return e
