CDROM/AJ/V107/P0751 EUVE Bright Light Source List (Malina+ 1994) ================================================================================ The Extreme Ultraviolet Explorer Bright Source List Roger F. Malina, Herman L. Marshall, Behram Antia, Carol A. Christian, Carl A. Dobson, David S. Finley, Antonella Fruscione, Forrest R. Girouard, Isabel Hawkins, Patrick Jelinsky, James W. Lewis, J. S. McDonald, Kelley McDonald, Robert J. Patterer, Vincent W. Saba, Martin M. Sirk, Brett A. Stroozas, John V. Vallerga, Peter W. Vedder, Alexandria Wiercigroch, and Stuart Bowyer <1994, AJ, 107, 751> =1994AJ....107..751M ================================================================================ Abstract: Initial results from the analysis of the Extreme Ultraviolet Explorer (EUVE) all-sky survey (58-740 A) and deep survey (67-364 A) 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 200 A. File Summary: -------------------------------------------------------------------------------- File Name Lrecl Records Explanations -------------------------------------------------------------------------------- table2.dat 166 356 The EUVE bright source list table2.tex 161 523 The EUVE bright source list (LaTeX version) document.tex 73 134 Author-supplied table documentation supertab.sty 74 243 Supertable style file (used by table2.tex) decalign.sty 76 77 Decimal alignment style (used by table2.tex) art8.sty 74 152 Article style for 8pt (used by table2.tex) -------------------------------------------------------------------------------- Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 16 A16 --- EUVE EUVE name based on J2000 coordinates 17- 19 I3 h RAh Right ascension (J2000) 20- 22 I3 min RAm R.A. 23- 25 I3 s RAs R.A. 26 1X --- --- Blank 27 A1 --- DE- Sign of declination (J2000) 28- 29 I2 deg DEd Declination 30- 32 I3 arcmin DEm Dec. 33- 35 I3 arcsec DEs Dec. 36- 41 F6.1 deg Glon Galactic longitude 42- 47 F6.1 deg Glat Galactic latitude 48- 53 I6 ct/ks Lex []? Count rate in Lexan/B filter 54- 55 A2 --- n_Lex *[*] Note for Lex field 56- 61 I6 ct/ks AlC []? Count rate in Al/Ti/C filter 62- 63 A2 --- n_AlC *[*] Note for AlC field 64- 69 I6 ct/ks Dag []? Count rate in Dagwood filter 70- 71 A2 --- n_Dag *[*] Note for Dag field 72- 77 I6 ct/ks Tin []? Count rate in tin filter 78- 79 A2 --- n_Tin *[*] Note for Tin field 80- 85 I6 ct/ks DSL []? Count rate, Deep Survey Lexan/B filter 86- 87 A2 --- n_DSL *[*] Note for DSL field 88- 93 I6 ct/ks DSA []? Count rate, Deep Survey Al/C filter 94- 95 A2 --- n_DSA *[*] Note for DSA field 96 1X --- --- Blank 97-110 A14 --- ID Possible optical counterpart of source 111-124 A14 --- Other Alternate name for possible counterpart 125-138 A14 --- Type *Source or Spectral type 139-144 F6.2 mag mv []? Visual magnitude 145 1X --- --- Blank 146-155 A10 --- WFC Name in ROSAT WFC Bright Source Catalog 156 1X --- --- Blank 157-166 A10 --- Notes *General notes or comments -------------------------------------------------------------------------------- Notes for file: table1.dat -------------------------------------------------------------------------------- n_Lex, n_AlC, n_Dag, n_Tin, n_DSL, n_DSA: 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 Type: Source or spectral type of the optical candidate. 'CSPN' indicates the central star of a planetary nebula, 'XRB' an x-ray binary system, and 'LMXB' a low mass x-ray binary. Notes: Individual coded notes, separated by commas, as follows: A Source A Source verified using only the skymaps. B Calibration target. C Serendipitous source observed during a calibration pointing. D# Private communication from: 1.H. Marshall, T. Carone, & A. Fruscione; 2.J. Vallerga; 3.P. Vedder; 4.G. Stringfellow. 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. -------------------------------------------------------------------------------- ================================================================================ (End) Lee Brotzman [ADS] 19-Apr-1994