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Re: Sample header info
Doug,
I think that it is very much dependant upon the site and the processing
involved... Dark sky sites ..like Arne has air mass would be very much a
factor...light polluted sites..like we have in the MidWest (with very few
really 'photometric' nights...I don't think airmass would make much of a
difference...but could of course be included for completeness sake...
Of course we would want to include heliocentric JD in all of our 'raw'
image headers...
Best Reguards,
Glenn G.
>From: Doug Welch <welch@physics.mcmaster.ca>
>To: TASS List <tass@listserv.wwa.com>
>Subject: Sample header info
>Date: Mon, 6 Nov 2000 16:27:27 -0500 (EST)
>
>
>Folks,
>
>I think that it would be a mistake to not include easily
>computable information like airmass and heliocentric JD in the
>header at the time of image creation. This removes an inevitable
>impediment to progress later on. I also think that it *is* a
>good idea to record the steps of how the image has been mutilated.
>
>Here is a FITS header from a WIYN image I took a few years back
>for reference. It is overkill, to be sure, but it does illustrate
>what others have done. (I would have added HJD, as well).
>
>Cheers,
>Doug
>
>
>dcd0009.imh[2043,2042][real]: M13 B 15sec
>No bad pixels, min=unknown, max=unknown
>Line storage mode, physdim [2048,2042], length of user area 2512 s.u.
>Created Mon 16:03:34 08-Mar-1999, Last modified Mon 16:03:34 08-Mar-1999
>Pixel file "HDR$dcd0009.pix" [ok]
>'KPNO-IRAF' /
>'15-07-97' /
>New copy of dcd0009.imh
>IRAF-MAX= 0.000000E0 / DATA MAX
>IRAF-MIN= 0.000000E0 / DATA MIN
>IRAF-BPX= 32 / DATA BITS/PIXEL
>IRAFTYPE= 'REAL ' / PIXEL TYPE
>HDR_REV = '1.010 13Jul94 (title @ end of pic; UTSHUT)' /
>ORIGPIC = 'obj0371' / Original picture file name
>OPICNUM = 371 / Original picture number
>NAMPSYX = '1 1' / Num amps in y & x (eg. '2 2'=quad)
>AMPLIST = '11' / Readout order in y,x
>OBSERVAT= 'KPNO' / Origin of data
>TELESCOP= 'WIYN3.5m' / Specific system
>DETECTOR= 's2kb' / Detector (CCD type, photon counter, etc.)
>IMAGETYP= 'OBJECT' / Type of picture (object, dark, etc.)
>PREFLASH= 0.000000 / Preflash time in secs
>CCDSUM = '1 1' / On chip summation (X,Y)
>CCDSEC = '[1:2043,3:2044]' / Section in full CCD for DATASEC
>CAMTEMP = -110.3 / CCD Temperature
>DEWTEMP = -176.2 / Dewar Temperature
>DATE-OBS= '13/07/97' / Date (dd/mm/yy) of observation
>UTSHUT = '16:34:45.0' / UT of shutter open
>EXPTIME = 15.000 / Exposure time in secs
>DARKTIME= 18.247 / Total elapsed time in secs
>DCS_TIME= 3000 / (ns) DCS integrator slope time
>GAIN = '7.5' / electrons per ADU
>RDNOISE = '14' / electrons
>READTIME= 20200 / (ns) unbinned pixel read time
>WAVEFILE= 's2kb Sat Jul 12 16:02:11 1997' /
>RECID = 'wiyn.imager.970715.064520' / archive ID for observation
>UT = ' 6:45:19.02' / universal time
>ST = '18:51:34.34' / sidereal time
>EL = '62:55:40.75' / elevation
>AZ = '-71:26:34.29' / azimuth
>TRACK = 'enabled' / tracking
>COORDS = 'Helio. mean FK5' / coordinate system
>RA = '16:41:49.16' / Telescope RA
>DEC = '36:27:13.16' / Telescope DEC
>RAOFFST = '00:00:0.00' / Telescope RA offset
>DECOFFST= '00:00:0.00' / Telescope DEC offset
>RADECSYS= 'FK5' / coordinate system
>TARGRA = '16:39:54.19' / right ascension
>TARGDEC = '36:33:16.30' / declination
>EQUINOX = 1997.6 / equinox of position
>EPOCH = 1997.6 / same as EQUINOX (for back compat.)
>ZD = 27.112 / zenith distance
>AIRMASS = 1.123176 / airmass at start of exposure
>ROTANGLE= -27.1 / rotator angle, degrees CW from N
>FILTERS = 'Harris_B' / fsa filter name
>FILTNUM = 6 / fsa filter number
>FILTWHEL= 2 / fsa filter wheel
>TRIM = 'Jul 15 15:40 Trim data section is [1:2043,3:2044]'
>OVERSCAN= 'Jul 15 15:40 Overscan section is [2049:2080,1:2048] with
>mean=757.98'
>ZEROCOR = 'Jul 15 15:40 Zero level correction image is Zero'
>CCDPROC = 'Mar 8 16:03 CCD processing done'
>HISTORY New copy of obj0371.imh
>WCSDIM = 2
>LTV2 = -2.
>LTM1_1 = 1.
>LTM2_2 = 1.
>WAT0_001= 'system=physical'
>WAT1_001= 'wtype=linear'
>WAT2_001= 'wtype=linear'
>FLATCOR = 'Mar 8 16:03 Flat field image is FlatHarris_B with
>scale=11798.85'
>
>
>
>
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