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IUE FITS Keywords

References and comments on FITS keywords are listed below. See main page for background.


Keyword Reference(s) Comments/Notes
GENERAL KEYWORDS
EXTNAME 'Spectral Container' Name given to binary table extension contained in MAST VO spectral container files
EQUINOX NEWSIPS Manual, Ch. 14.2 Comments here
RADECSYS CDS, NEWSIPS Manual Ch. 14.2 FK4
TIMESYS Telescope Operations office checked synchronization of their UT with USNO time service (per Scott Snell) Time system was UTC
MJDREF 0.00000 [d] MJD zero point for times
SPECSYS NEWSIPS Manual Ch. 14.2 Low dispersion: topocentric, High dispersion: heliocentric
VOCLASS 'SPECTRUM V1.0' VO Data Model
VOSEGT 'SPECTRUM' Segment type
DATALEN 563 [ ] Number of points in spectrum
DSSOURCE 'POINTED' Survey or Pointed
DATA ID KEYWORDS
DATE from IUE keyword DATE Processing-Creation Date
VODATE from IDL "today" command Curation Date
VOREF 'http://archive.stsci.edu/vodocs/iue' URL for Documentation
DS_IDENT 'ads/sa.iue#lwp09671mxlo' Data Set Identifier
VERSION '1.0' Processing Version
COLLECT mission/instrument from IUE keyword CAMERA Data Set Collection (e.g., IUE/LWP)
INSTRUME from IUE keyword CAMERA Instrument
TELESCOP 'IUE' Internation Ultraviolet Explorer (IUE)
FILENAME from IUE keywords CAMERA and IMAGE File Name such as lwp0967mxlo_vo.fits
CR_IDENT same as for filename Internal dataset ID
CRETYPE 'Archival' Not an on-the-fly dataset
CURATION KEYWORDS
VOPUB 'MAST' VO Publishing Authority
AUTHOR 'IUE project' Creator
VOPUBID 'ivo://mast.stsci.edu' URI for VO Publisher
VOLOGO 'http://archive.stsci.edu/images/100.mastlogo.gif' MAST logo
CONTRIB1 from IUE keyword PGM-ID which lists the IUE observing program ID See http://archive.stsci.edu/iue/prog.html
CONTACT 'archive help desk'
EMAIL STScI help desk: 'archive@stsci.edu'
TARGET KEYWORDS
OBJECT from IUE keyword (L/S)TARGET Supplied by GO (proposer's target name)
SRCLASS from keyword (L/S)IUECLAS and converted from number to string title in MAST IDL routine ssap_header_iue.pro See also NEWSIPS manual Ch. 14.2
TITLE 'lwp09671mxlo_vo.fits, L2 PUP' Title is comprised of dataset name, target
RA_TARG taken from IUE keyword (L/S)TARGRA [deg] right ascension of target provided by GO
DEC_TARG taken from IUE keyword (L/S)TARDEC [deg] declination of target provided by GO
WCS Paper 3 Keywords
1S2_1 'WAVE' Column name with spectral coordinates
1CYTP2 'WAVE-TAB' Spectral coordinate is wavelength
1S3_1 'WAVE' Column name with spectral coordinates
1CYTP3 'WAVE-TAB' Spectral coordinate is wavelength
1S4_1 'WAVE' Column name with spectral coordinates
1CYTP4 'WAVE-TAB' Spectral coordinate is wavelength
COVERAGE: SPATIAL
RA taken from IUE keyword (L/S)TARGRA Comments here
DEC taken from IUE keyword (L/S)TARGDEC [deg] project-defined declination provided by GO
APERTURE NEWSIPS manual Ch. 2.2, Tbl 2.1 based on IUE keyword APERTURE [arcsec] radius or lengthxwidth
COVERAGE: TEMPORAL
DATE-OBS from IUE keywords (L/S)DATEOBS and (L/S)TIMEOBS Comments here
EXPOSURE from IUE keyword (L/S)EXPTIME [s] eff. exposure duration
TSTART from IUE keyword (L/S)JD-OBS - 2400000. [d] MJD exposure start time
TSTOP 2 * TMID - TSTART [d] MJD exposure stop time
TMID from IUE keyword (L/S)JD-MID - 2400000. [d] MJD exposure mid time
COVERAGE: SPECTRAL
SPECSDIM '1.0E-10 L' Comments here
SPEC_CAL 'Calibrated' Calibrated spectral coordinate
SPEC_ERR 2.50000 [angstrom] Wavelength statistical error
SPECBAND Based on classification by Paolo Padovani using MAST IDL program vo_specband See http://archive.stsci.edu/genlinks_help.html#data
SPEC_VAL Derived from data [angstrom] Mean Wavelength
SPEC_BW Derived from data [angstrom] Bandpass Width Wmax - Wmin
SPEC_FIL 1.00000 [ ] No gaps between points
SPEC_RP NEWSIPS Manual Ch. 2.3 average resolving power W/dW varies with camera, dispersion and aperture
COVERAGE: OBSERVABLE
FLUXSDIM '1.0E+7 ML-1T-3' Comments here
FLUX_CAL 'Calibrated' Calibrated Fluxes
STAT_ERR 10 [ ] flux error in percent
DER_SNR Stoehr et al. 2007 Space Telescope Coordination Fac. NL, 42, 4 Derived signal-to-noise ratio
FLUXAVG Derived from data [erg/cm**2/s/angstrom] Average Flux
FLUXMAX2 Derived from Data [erg/cm**2/s/angstrom] 98% Maximum Flux
SPECDISP derived from data as (Wmax - Wmin)/npts [angstrom/pixel] Dispersion