Keyword |
Reference(s) |
Comments/Notes |
GENERAL KEYWORDS |
EXTNAME |
See FITS standards document |
FITS convention for naming table extension spectral container |
EQUINOX |
The original WUPPE data used 1950 coordinates (see primary header keywords). These values were precessed using the routine PRECESS from the ASTRON IDL library. |
Comments here |
RADECSYS |
FK5 coordinates were calculated by the PRECESS routine from the IDL ASTRON library. |
FK5 |
TIMESYS |
? |
UTC? Time system |
MJDREF |
0.00000 |
[d] MJD zero point for times |
SPECSYS |
|
topocent, no heliocentric-correction? |
VOCLASS |
'SPECTRUM V1.0' |
VO Data Model |
VOSEGT |
'SPECTRUM' |
Segment type |
DATALEN |
derived from data |
[ ] Number of points in spectrum |
DSSOURCE |
'POINTED' |
Survey or Pointed |
DATA ID KEYWORDS |
DATE |
from DATE keyword |
Processing-Creation Date |
VODATE |
from IDL "today" command |
Curation Date |
VOREF |
'http://archive.stsci.edu/vodocs/wuppe' |
URL for Documentation |
DS_IDENT |
derived from filename |
Publishers Data Set ID |
VERSION |
'1.0' |
Processing Version |
COLLECT |
'ASTRO/WUPPE' |
Data Set Collection |
INSTRUME |
from OBSERVAT keyword |
Instrument |
TELESCOP |
'WUPPE' |
Telescope |
FILENAME |
derived from FILENAME keyword |
File Name |
CR_IDENT |
derived from FILENAME keyword |
Internal dataset ID |
CRETYPE |
'Archival' |
Not an on-the-fly dataset |
CURATION KEYWORDS |
VOPUB |
'MAST' |
VO Publishing Authority |
AUTHOR |
'WUPPE project' |
Creator |
VOPUBID |
'ivo://mast.stsci.edu' |
URI for VO Publisher |
VOLOGO |
'http://archive.stsci.edu/images/100.mastlogo.gif' |
MAST logo |
VOVER |
'1.0' |
VO Curation version |
VORIGHTS |
'PUBLIC' |
Data is public |
CONTRIB1 |
Arthur D. Code |
Principal Investigator |
CONTACT |
'archive help desk' |
Comments here |
EMAIL |
'archive@stsci.edu' |
Comments here |
TARGET KEYWORDS |
OBJECT |
from OBJECT keyword |
proposer's target name |
TITLE |
derived from filename and target name |
Program Identification |
RA_TARG |
precessed from RA keyword |
[deg] right ascension of target |
DEC_TARG |
precessed from DEC keyword |
[deg] declination of target |
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 |
COVERAGE: SPATIAL |
RA |
precessed from RA keyword |
[deg] project-defined right ascension |
DEC |
precessed from DEC keyword |
[deg] project-defined declination |
APERTURE |
derived from APERTURE keyword |
[arcsec] Aperture (radius or lengthxwidth) |
COVERAGE: TEMPORAL |
DATE-OBS |
derived from DATE-OBS and GMTSTART keywords |
UT observation start time (only specified to nearest minute) |
EXPOSURE |
from EXPOSURE keyword |
[s] exposure duration |
TSTART |
derived from DATE-OBS and GMTSTART converted to MJD using JULDATE procedure from IDL ASTRON library |
[d] MJD exposure start time |
TSTOP |
derived from DATE-OBS, GMTSTART + EXPOSURE keywords converted to MJD using JULDATE procedure from IDL ASTRON library |
[d] MJD exposure stop time |
TMID |
average of TSTART and TSTOP derived values |
[d] MJD exposure mid time |
COVERAGE: SPECTRAL |
SPECSDIM |
'1.0E-10 L' |
Comments here |
SPEC_CAL |
|
Calibrated spectral coordinate |
SPEC_ERR |
6 A resolution(?) from http://www.sal.wisc.edu/WUPPE/instrument/instrument.html |
[angstrom] Wavelength statistical error |
SPECBAND |
based on derived wavelength range and classifications by Paolo Padovani using the MAST program vo_specband |
Far-UV, Near-UV Spectral Band(s) |
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 |
400(?) |
[ ] average resolving power W/dW |
COVERAGE: OBSERVABLE |
FLUXSDIM |
'1.0E+7 ML-1T-3' |
Flux SIDim |
FLUX_CAL |
private commnication from marilyn Meade and from comments in FITS header |
Fluxes are relative |
STAT_ERR |
from http://www.sal.wisc.edu/WUPPE/calibration/calibration.html |
Note from WUPPE web page http://www.sal.wisc.edu/WUPPE/calibration/calibration.html: due to pointing system problems the absolute fluxes of some targets observed through smaller apertures are low by up to a factor of two. |
DER_SNR |
derived value. See der_snr.pdf |
[ ] 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 (Wmax-Wmin)/npts |
[angstrom/pixel] Dispersion |