示例#1
0
twomassid, id, teff, feh = mcallib.loadSampleOfCalibrators(options.inputsample)

Tcal = []
FeHcal = []
ewcal = []

for file in listOfStarSpectra:

    spc = Spectrum(file)
    objname = spc.object.replace(" ", "").upper()

    if options.verbose:
        print "Processing spectrum: ", file, objname

    if spc.instrument == 'ESPaDOnS' or spc.instrument == 'NARVAL':
        spc.resampling(0.01, 4000, 10400)

    for i in range(len(id)):
        if objname in id[i].upper() or objname in twomassid[i].upper():
            spc.equivalentWidths(override=False, verbose=options.verbose)
            ewcal_tmp = spc.eqwidths
            if not np.any(np.isnan(ewcal_tmp)):
                ewcal.append(ewcal_tmp)
                Tcal.append(teff[i])
                FeHcal.append(feh[i])
                print "Selected Calibrator: ", file, objname, twomassid[i], id[
                    i], teff[i], feh[i]
            else:
                print "Eq. Widths contain NaNs. Ignoring potential calibrator: ", file, objname

mcallib.calibrate_mcal(ewcal, Tcal, FeHcal, options.outputcalibmatrix)
示例#2
0
    print 'File with wavelength ranges: ', options.wavemask

spc = Spectrum(options.input,
               options.spectype,
               options.polar,
               options.telluric,
               options.helio,
               Sort=False)

#spc.binningOrderByOrder(rvsampling_kps=float(options.rvsampling), median=False)

if options.wavemask:
    spc.applyMask(options.wavemask)

spc.sortByWavelength()

if options.output.endswith(".fits"):

    wlsampling = (float(options.rvsampling) * 1000.0 /
                  constants.c) * (spc.wl[-1] + spc.wl[0]) / 2.0
    spc.resampling(wlsampling)
    spc.saveToFile(options.output, format='fits')

elif options.output.endswith(".txt"):

    spc.binning(float(options.rvsampling), median=False)
    spc.saveToFile(options.output, format='ascii')

else:
    spc.printdata(printerrors=False)