J/AJ/107/751 J/AJ/107/751 EUV Explorer bright sources list R F Malina H L Marshall B Antia C A Christian C A Dobson D S Finley A Fruscione F R Girouard I Hawkins P Jelinsky J W Lewis J S McDonald K McDonald R J Patterer V W Saba M M Sirk B A Stroozas J V Vallerga P W Vedder A Wiercigroch S Bowyer Astron. J. 107 751 1994 1994AJ....107..751M Space observations Ultraviolet Initial results from the analysis of the Extreme Ultraviolet Explorer (EUVE) all-sky survey (58-740A) and deep survey (67-364A) are presented through the EUVE Bright Source List (BSL). The BSL contains 356 confirmed extreme ultraviolet (EUV) point sources with supporting information, including positions, observed EUV count rates, and the identification of possible optical counterparts. One-hundred twenty-six sources have been detected longward of 200A.

EUVE

Name EUVE name based on J2000 coordinates --- RAh Right ascension J2000 h RAm Right ascension J2000 min RAs Right ascension J2000 s DE- Declination sign --- DEd Declination J2000 deg DEm Declination J2000 arcmin DEs Declination J2000 arcsec GLON Galactic longitude deg GLAT Galactic latitude deg Lex Count rate in Lexan/B filter number=1 Lex, AlC, Dag, Tin, DSL, DSA: Count rate fields are in units of counts/kilosecond. ct/ks n_Lex Note for Lex field number=2 The note flags for the count rate fields are as follows: * Count rate derived from the calibration observation ** Count rate from Patterer et al, 1993, ApJ, 414, L57 --- AlC Count rate in Al/Ti/C filter number=1 Lex, AlC, Dag, Tin, DSL, DSA: Count rate fields are in units of counts/kilosecond. ct/ks n_AlC Note for AlC field number=2 The note flags for the count rate fields are as follows: * Count rate derived from the calibration observation ** Count rate from Patterer et al, 1993, ApJ, 414, L57 --- Dag Count rate in Dagwood filter number=1 Lex, AlC, Dag, Tin, DSL, DSA: Count rate fields are in units of counts/kilosecond. ct/ks n_Dag Note for Dag field number=2 The note flags for the count rate fields are as follows: * Count rate derived from the calibration observation ** Count rate from Patterer et al, 1993, ApJ, 414, L57 --- Tin Count rate in tin filter number=1 Lex, AlC, Dag, Tin, DSL, DSA: Count rate fields are in units of counts/kilosecond. ct/ks n_Tin Note for Tin field number=2 The note flags for the count rate fields are as follows: * Count rate derived from the calibration observation ** Count rate from Patterer et al, 1993, ApJ, 414, L57 --- DSL Count rate, Deep Survey Lexan/B filter number=1 Lex, AlC, Dag, Tin, DSL, DSA: Count rate fields are in units of counts/kilosecond. ct/ks n_DSL Note for DSL field number=2 The note flags for the count rate fields are as follows: * Count rate derived from the calibration observation ** Count rate from Patterer et al, 1993, ApJ, 414, L57 --- DSA Count rate, Deep Survey Al/C filter number=1 Lex, AlC, Dag, Tin, DSL, DSA: Count rate fields are in units of counts/kilosecond. ct/ks n_DSA Note for DSA field number=2 The note flags for the count rate fields are as follows: * Count rate derived from the calibration observation ** Count rate from Patterer et al, 1993, ApJ, 414, L57 --- ID Possible optical counterpart of source --- OtherID Alternate name for possible counterpart --- Type Source or Spectral type of the optical candidate number=3 'CSPN' indicates the central star of a planetary nebula, 'XRB' an X-ray binary system, and 'LMXB' a low mass X-ray binary. --- Vmag Visual magnitude mag ROSAT Name in ROSAT WFC Bright Source Catalog --- Notes General notes or comments number=4 Individual coded notes, separated by commas, as follows: A Source verified using only the skymaps. B Calibration target. C Serendipitous source observed during a calibration pointing. D Private communication from: 1. Marshall H., Carone T. & Fruscione A. 2. Vallerga J. 3. Vedder P. 4. Stringfellow G. E Refer to the following papers: 1. Vennes et al. 1993, ApJ, 410, L119; 2. Marshall, Carone, & Fruscione 1993, ApJ, 414, L53; 3. Patterer et al. 1993, ApJ, 414, L57; 4. Vedder et al. 1993, ApJ, 414, L61; 5. Cully et al. 1993, ApJ, 414, L49; 6. Vallerga, Vedder, & Welsh 1993, ApJ, 414, L65; 7. Warren et al. 1993, ApJ, 414, L69; 8. Finley et al. 1993, ApJ, 417, 259; 9. Stringfellow & Bowyer 1993, in IAU Circular No. 5803, V1974 Cygni. F Three stars, including a white dwarf, are very likely optical counterparts (J. Dupuis, private communication). G DS count rates, accurate to 50%, are provided by J. Vallerga. H A and B stars probably detected as a "UV leak" by EUVE but reported as extreme ultraviolet sources in the ROSAT Bright Source Catalog. I Optical ID confirmed via: 1. High signal-to-noise optical spectra by D. Finley; 2. Photometry or spectroscopy by M. Dopita. J The DS count rate includes the flare occurring during the observation. --- table2.texThe EUVE bright source list (LaTeX version) document.texAuthor-supplied table documentation Lee Brotzman ADS 1994, Patricia Bauer [CDS] 21-Oct-1994Apr19Center for EUV Astrophysics, 2150 Kittredge Street, University of California, Berkeley, CA 94720 AAS CD-ROM series, Volume 2, 1994 J_AJ_107_751.xml