/
mmirs_longslit_template.v1.txt
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/
mmirs_longslit_template.v1.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/2013/2013.0622/'
R_DIR = '/d1/data1/mmirs/preproc/2013/2013.0622/'
W_DIR = '/d1/data1/mmirs/reduced/2013/2013.0622/2pixel_O1.0315_HK_HK/01/'
RAWEXT = '.gz'
INSTRUME= 'MMIRS' / spectrograph name
SLIT = '2_pixel' / slit name or MOS
GRISM = 'HK' / grism
FILTER = 'HK' / filter
BRIGHT = 0 / bright source 1=Yes 0=No
SCI = 'O1.0315_longslit.4161' / science frame (only one)
SCI2 = 'O1.0315_longslit.4162' / second science frame (only one)
DITHPOS = 0.0000 / current dithering position in arcsec
DITHPOS2= 7.0000 / dithering position for the second frame
DARKSCI = 'dark.4513,dark.4514,dark.4515,dark.4516,dark.4517' / dark frame(s) for science
ARC = 'comp.4179' / arc frames
DARKARC = 'dark.4488,dark.4489,dark.4490,dark.4491,dark.4492' / dark frame(s) for arc
FLAT = 'flat.4182'
DARKFLAT= 'dark.4478,dark.4479,dark.4480,dark.4481,dark.4482' / dark frame(s) for flat
STAR01 = 'HD148749_longslit.4133,HD148749_longslit.4134'
DARKST01= 'dark.4508,dark.4509,dark.4510,dark.4511,dark.4512'
STTYPE01= 'a0v'
STAR02 = 'HD148749_longslit.4177,HD148749_longslit.4178'
DARKST02= 'dark.4503,dark.4504,dark.4505,dark.4506,dark.4507'
STTYPE02= 'a0v'
STAR03 = 'HD148749_longslit.4288,HD148749_longslit.4289'
DARKST03= 'dark.4508,dark.4509,dark.4510,dark.4511,dark.4512'
STTYPE03= 'a0v'
STAR04 = 'HD148749_longslit.4369,HD148749_longslit.4370'
DARKST04= 'dark.4508,dark.4509,dark.4510,dark.4511,dark.4512'
STTYPE04= 'a0v'
STAR05 = 'HD148749_longslit.4398,HD148749_longslit.4399'
DARKST05= 'dark.4508,dark.4509,dark.4510,dark.4511,dark.4512'
STTYPE05= '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