# For each defined redshift, eval the photometry and store on the database.
db_m = db.get('/%s/%s/%s' % (filterid, ccd, 'library'))
i_z = 0
for z in np.arange(z_from, z_to, z_step):
if z == 0:
d_L = 3.08567758e19 # 10 parsec in cm
else:
d_L = cosmocalc.cosmocalc(z)['DL_cm']
k_cosmo = L_sun / ( 4 * np.pi * np.power(d_L,2) )
O = zcor(obs_spec, z)
O['flux'] = O['flux'] * k_cosmo
x = spec2filterset(f.filterset, O, dlambda_eff = 3.0)
# print 'z', z
# print aux0[i_base]
#
# plt.figure(1)
# plt.clf()
# plt.plot(O['wl'][kk], O['flux'][kk])
# plt.figure(2)
# plt.clf()
# plt.plot(f.filteravgwls, x, '.')
db_m[i_z, i_base + aux_basesize*i_av] = x
i_z = i_z + 1
pystarlight.io.starlighttable.__file__
)
ts = atpy.TableSet(obs_test_file, type="starlight_input")
obs_spec = np.copy(
ts.starlight_input.data.view(dtype=np.dtype([("wl", "<f8"), ("flux", "<f8"), ("error", "<f8"), ("flag", "<i8")]))
)
model_spec["flux"] = model_spec["flux"] * tm.keywords["fobs_norm"] * 1e-17
obs_spec["flux"] = obs_spec["flux"] * 1e-17
obs_spec["error"] = obs_spec["error"] * 1e-17
# print spec2filter(filter, obs_spec, model_spec, log_level=logging.DEBUG)
plt.clf()
c = photoconv()
x = spec2filterset(f.filterset, obs_spec, model_spec, dlambda_eff=3.0)
plt.plot(f.filteravgwls, x["m_ab"])
for z in np.arange(0.1, 1, 0.2):
print "z ==", z
O = zcor(obs_spec, z)
M = zcor(model_spec, z)
x = spec2filterset(f.filterset, O, M, dlambda_eff=3.0)
plt.plot(f.filteravgwls, x["m_ab"])
if z > 0.3:
plt.plot(O["wl"], -2.5 * np.log10(O["flux"] * (O["wl"] ** 2) / c_AngSec) - 48.6, color="black", alpha=0.3)
plt.plot(M["wl"], -2.5 * np.log10(M["flux"] * (M["wl"] ** 2) / c_AngSec) - 48.6, color="blue", alpha=0.3)
raw_input()
print "test 1"
raw_input("Enter for next test...")
print c.fromStarlight(f.filterset, ts, tm, dlambda_eff=3.0)