/
mmirs_mos_template.v2.txt
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/
mmirs_mos_template.v2.txt
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SIMPLE = T / FITS-like header
LONGSTRN= 'OGIP 1.0' / The OGIP long string convention may be used.
RAW_DIR = '/data/mmirs/Archive/rawdata/data/MMIRS/2011/2011.1203/'
R_DIR = '/d1/data1/mmirs/preproc/2011/2011.1203/'
W_DIR = '/d1/data1/mmirs/reduced/2011/2011.1203/lei1.a1_mask1_HK_HK/01/'
RAWEXT = '.gz'
INSTRUME= 'MMIRS' / spectrograph name
SLIT = 'mos' / slit name or MOS
GRISM = 'HK' / grism
FILTER = 'HK' / filter
BRIGHT = 0 / bright source 1=Yes 0=No
SCI = 'lei1.a1_mos.8456' / science frame (only one)
SCI2 = 'lei1.a1_mos.8457' / second science frame (only one)
DITHPOS = 1.8000 / current dithering position in arcsec
DITHPOS2= -1.4000 / dithering position for the second frame
DARKSCI = 'dark.8653,dark.8654,dark.8655,dark.8656,dark.8657' / sci darks
ARC = 'comp_mos.8468' / arc frames
DARKARC = 'dark.8638,dark.8639,dark.8640,dark.8641,dark.8642' / arc darks
FLAT = 'flat_mos.8470'
DARKFLAT= 'dark.8628,dark.8629,dark.8630,dark.8631,dark.8632' / flat darks
STAR01 = 'HIP-16904_mos.8491,HIP-16904_mos.8492,HIP-16904_mos.8494,&'
CONTINUE 'HIP-16904_mos.8514,HIP-16904_mos.8516,HIP-16904_mos.8518,&'
CONTINUE 'HIP-16904_mos.8519,HIP-16904_mos.8521'
DARKST01= 'dark.8638,dark.8639,dark.8640,dark.8641,dark.8642'
STTYPE01= 'a0v'
STAR02 = 'HIP-16904_mos.8596,HIP-16904_mos.8597,HIP-16904_mos.8598,&'
CONTINUE 'HIP-16904_mos.8599,HIP-16904_mos.8600,HIP-16904_mos.8601,&'
CONTINUE 'HIP-16904_mos.8602,HIP-16904_mos.8603,HIP-16904_mos.8604,&'
CONTINUE 'HIP-16904_mos.8605,HIP-16904_mos.8606,HIP-16904_mos.8607,&'
CONTINUE 'HIP-16904_mos.8608,HIP-16904_mos.8609,HIP-16904_mos.8610,&'
CONTINUE 'HIP-16904_mos.8611,HIP-16904_mos.8612,HIP-16904_mos.8613,&'
CONTINUE 'HIP-16904_mos.8614,HIP-16904_mos.8615,HIP-16904_mos.8616,&'
CONTINUE 'HIP-16904_mos.8617,HIP-16904_mos.8618'
DARKST02= 'dark.8638,dark.8639,dark.8640,dark.8641,dark.8642'
STTYPE02= 'a0v'
COMMENT flat fielding settings
FFSCFLAT= 0 / subtract scattered light from flat field?
FFSCSCI = 0 / subtract scattered light from science frames?
FFNSLIT = -1 / normalize to slit #N, -1 for per-slit normalization
COMMENT wavelength calibration settings
WLNDEG = 3 / polynomial degree along dispersion
WLYNDEG = 3 / polynomial degree across dispersion
WLDEBUG = 0 / debug setting
WLPLOT = 0 / plot the arc line identification spectrum on the screen
WLADJ = 1 / adjust wavelength solution using all slits
WLOH = 1 / use OH lines to build the wavelength solution
SKIPLINE= ' ' / arc lines NOT to use
COMMENT sky subtraction settings
SSADJWL = 1 / use the adjusted wavelength solution?
SSDIM = 3 / 3-dimension or 2-dimension sky model?
SSDEBUG = 0 / debug for sky subtraction
COMMENT linearisation settings
LINADJWL= 1 / use the adjusted wavelength solution?
LINSSBOX= 1 / sky subtraction in linearized spectra in all "BOX" slits
LINSSTRG= 1 / sky subtraction in linearized spectra in all "TARGET" slits
COMMENT extraction settings
EXTMETH = 1 / 1 - box extraction, 2 - optimal extraction
EXTAPW = 5 / extraction aperture in pixels, window with or gaussian FWHM
EXTDFBOX= 0 / use alignbox star positions to get empirical dithering offset?
EXTBOXEX= 'obj-sky' / image type to use alignbox positions from
COMMENT process the following reduction steps (yes=1/no=0)
S01PROC = 1 / up-the-ramp fitting (if needed) and dark subtraction
S02PROC = 1 / distortion map creation
S03PROC = 1 / flat-fielding and 2D slit extraction
S04PROC = 1 / wavelength calibration
S05PROC = 1 / sky subtraction
S06PROC = 1 / linearisation
S07PROC = 1 / extraction
S08PROC = 1 / telluric star processing
S09PROC = 0 / telluric correction
END