GMOS Data Reduction

More documents

Recommendations

Info

Final normalized spectral image. Minimal fringing is visible inCCD2 and CCD3, and the GCALflat image has beenreproduced, displaced 1536 pixels below the original, simulatinga shuffled GCALflat.
gsreduce (N&S)gsreduce N20051118S0305.fits logfile=gmos.logfilerawpath="rawdata$” fl_over+ fl_trim+nbiascontam=4 fl_bias+ bias=“sciencebias” fl_dark+dark=“Nsdark” fl_flat- fl_gmosaic- fl_fixpixfl_gsappwave-fl_cut- ovs_flinter+ fl_vardq+N20051118S0305.fits: raw science image (810nm)fl_gmosaic-: do not mosaic, leave the detectors as separate extensionsfl_gsappwave-: do not apply a first order wavelength solution based on theheaderfl_cut-: do not cut the slits into separate extensions (superfluous forlongslit)ovs_flinter+: examine fits to overscan region interactively** attempting to fl_flat+ in the first gsreduce call produces an error, willdiscuss this with the experts and clean it up before posting cookbook **
Page 1 and 2:
Reducing GMOSSpectroscopic dataRica
Page 3 and 4:
General Principles• Record everyt
Page 5:
Notes on Bias and Dark• Standard
Page 8 and 9:
Overscan “Spillover”R400 gratin
Page 10: Reduced combined 2x1 biasimage, con
Page 13 and 14: Difference image of two reduced sta
Page 15 and 16: Flatfield Correction• Flats may b
Page 17 and 18: gsflatgsflat @flatfiles_460 out=Fla
Page 19 and 20: gsflatFitting the overscan region:
Page 21 and 22: gsflatFitting the “response” fu
Page 23 and 24: gsflatλRed flat field along the sp
Page 25 and 26: gsflatThere is a trade off between,
Page 27 and 28: Alignment starsGMOS MOS Spectra
Page 29 and 30: GMOS MOS reductionThe yoffset param
Page 31 and 32: gswavelengthgswavelenth @gsNarcfile
Page 33 and 34: gswavelengthDetermine wavelength so
Page 35 and 36: gswavelengthAutomatic line identifi
Page 37 and 38: gswavelengthFinding the wavelength
Page 39 and 40: gswavelengthOutput after fitting wa
Page 41 and 42: gswavelengthFinding the 2D waveleng
Page 43 and 44: gstransformgstransform gsNarcfile.f
Page 45 and 46: gsextractgsextract @tgsNsciencefile
Page 48 and 49: Raw Longslit N&SSpectrum
Page 50 and 51: Observing Tool N&SComponent2010B
Page 52 and 53: N&S Dark Correction• N&S darks ta
Page 54 and 55: Overscan fit for CCD1. By utilizing
Page 56 and 57: Zoom of reduced spectral image wher
Page 58 and 59: Flatfield Correction• GCALflats f
Page 62 and 63: N&S Sky Subtraction• Sky subtract
Page 64 and 65: Bias corrected, dark subtracted, fl
Page 66: Bias Correction• Not talking abou
show all

GMOS Data Reduction

Create successful ePaper yourself

Delete template?

Save as template?