Commit ebbb6019 authored by Zhang Xin's avatar Zhang Xin
Browse files

fix redshift calculation method

parent 4ce9fe3e
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+8 −8
Original line number Diff line number Diff line
@@ -239,7 +239,7 @@ def getObservedSED(sedCat, redshift=0.0, av=0.0, redden=0):
    sw, sf = sedCat[:,0], sedCat[:,1]
    # reddening
    sf = reddening(sw, sf, av=av, model=redden)
    sw, sf = sw*z, sf*(z**3)
    sw, sf = sw*z, sf/z
    # lyman forest correction
    sf = lyman_forest(sw, sf, redshift)
    isedObs = (sw.copy(), sf.copy())
@@ -482,6 +482,8 @@ def produceGalSED_C6( gal_id_s = '03593100052300144566', gal_z = 1.6927,mag_norm
    pcs = pcs['pcs'][()]

    cosmo = FlatLambdaCDM(H0=67.66, Om0=0.3111)
    factor=1
    if gal_z != 0:
        factor = 10**(-.4 * cosmo.distmod(gal_z).value)
    flux = np.matmul(pcs, coeff) * factor

@@ -501,11 +503,12 @@ def produceGalSED_C6( gal_id_s = '03593100052300144566', gal_z = 1.6927,mag_norm
    all_sed = y * lamb / (cons.h.value * cons.c.value) * 1e-13
    orig_spec_phot = Table(np.array([lamb, all_sed]).T, names=('WAVELENGTH', 'FLUX'))

    
    sedNormFactor=1.0
    if mag_norm != -99:
        normThr = Table.read(norm_filter_thr_fn)
        # orig_spec = Table(np.array([wave,flux]).T,  names=(['WAVELENGTH', 'FLUX']))
        norm_thr_rang_ids = normThr['SENSITIVITY'] > 0.001
    sedNormFactor=1.0
    if mag_norm != -99:
        sedNormFactor = getNormFactorForSpecWithABMAG(ABMag=mag_norm, spectrum=orig_spec_phot,
                                                    norm_thr=normThr,
                                                    sWave=np.floor(normThr[norm_thr_rang_ids][0][0]),
@@ -516,10 +519,8 @@ def produceGalSED_C6( gal_id_s = '03593100052300144566', gal_z = 1.6927,mag_norm

    return norm_spec, norm_spec_phot


fileDir = os.getcwd()


#normlization filter star
# star_norm_fn = '/Users/zhangxin/Work/SlitlessSim/sed/produceSED_bycatfile/data/throughputs/SDSS/SLOAN_SDSS.g.fits'
star_norm_fn = os.path.join(fileDir, "data/throughputs/SDSS/SLOAN_SDSS.g.fits")
@@ -562,4 +563,3 @@ gal_spec, gal_spec_photo = produceGalSED_C6(gal_id_s = '03490800052300010462', g
#     mag = getABMAG(spec_p, throughput_dir+fi+'.Throughput.fits')
#     print(fi,mag)