J/AJ/107/751 EUVE bright sources list (Malina+, 1994)
The extreme ultraviolet explorer bright source list
Malina R.F., Marshall H.L., Antia B., Christian C.A., Dobson C.A.,
Finley D.S., Fruscione A., Girouard F.R., Hawkins I., Jelinsky P.,
Lewis J.W., McDonald J.S., McDonald K., Patterer R.J., Saba V.W.,
Sirk M.M., Stroozas B.A., Vallerga J.V., Vedder P.W., Wiercigroch A.,
Bowyer S.
<Astron. J. 107, 751 (1994)>
=1994AJ....107..751M 1994AJ....107..751M (SIMBAD/NED Reference)
ADC_Keywords: EUV sources
Mission_Name: EUVE
Abstract:
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.
Addresses:
Center for EUV Astrophysics, 2150 Kittredge Street,
University of California, Berkeley, CA 94720
See also:
J/ApJS/93/569 : First EUVE source catalogue (Bowyer+, 1994)
II/203 : Second EUVE Source Catalog (Craig+ 1996)
http://www.cea.berkeley.edu/HomePage.html (Center for EUV Astrophysics)
File Summary:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
table2.dat 165 356 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)
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Byte-per-byte Description of file: table2.dat
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Bytes Format Units Label Explanations
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1- 16 A16 --- Name EUVE name based on J2000 coordinates
18- 19 I2 h RAh Right ascension J2000
21- 22 I2 min RAm Right ascension J2000
24- 25 I2 s RAs Right ascension J2000
27 A1 --- DE- Declination sign
28- 29 I2 deg DEd Declination J2000
31- 32 I2 arcmin DEm Declination J2000
34- 35 I2 arcsec DEs Declination J2000
37- 41 F5.1 deg GLON Galactic longitude
43- 47 F5.1 deg GLAT Galactic latitude
49- 53 I5 ct/ks Lex []? Count rate in Lexan/B filter (1)
54 A1 --- n_Lex [*] Note for Lex field (2)
57- 61 I5 ct/ks AlC []? Count rate in Al/Ti/C filter (1)
62- 63 A2 --- n_AlC [* ] Note for AlC field (2)
66- 69 I4 ct/ks Dag []? Count rate in Dagwood filter (1)
71 A1 --- n_Dag [*] Note for Dag field (2)
73- 77 I5 ct/ks Tin []? Count rate in tin filter (1)
79 A1 --- n_Tin [* ] Note for Tin field (2)
81- 85 I5 ct/ks DSL []? Count rate, Deep Survey
Lexan/B filter (1)
86 A1 --- n_DSL [* ] Note for DSL field (2)
90- 93 I4 ct/ks DSA []? Count rate, Deep Survey
Al/C filter (1)
94 A1 --- n_DSA [* ] Note for DSA field (2)
97-109 A13 --- Id Possible optical counterpart of source
111-123 A13 --- OtherId Alternate name for possible counterpart
125-138 A14 --- Type Source or Spectral type of the optical
candidate (3)
140-144 F5.2 mag Vmag []? Visual magnitude
146-155 A10 --- ROSAT Name in ROSAT WFC Bright Source Catalog
157-166 A10 --- Notes General notes or comments (4)
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Note (1): Lex, AlC, Dag, Tin, DSL, DSA: Count rate fields are in units of
counts/kilosecond.
Note (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
Note (3): 'CSPN' indicates the central star of a planetary nebula,
'XRB' an X-ray binary system, and
'LMXB' a low mass X-ray binary.
Note (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. =1993ApJ...410L.119V 1993ApJ...410L.119V
2. Marshall, Carone, & Fruscione =1993ApJ...414L..53M 1993ApJ...414L..53M
3. Patterer et al. =1993ApJ...414L..57P 1993ApJ...414L..57P
4. Vedder et al. =1993ApJ...414L..61V 1993ApJ...414L..61V
5. Cully et al. =1993ApJ...414L..49C 1993ApJ...414L..49C
6. Vallerga, Vedder, & Welsh =1993ApJ...414L..65V 1993ApJ...414L..65V
7. Warren et al. =1993ApJ...414L..69W 1993ApJ...414L..69W
8. Finley et al. =1993ApJ...417..259F 1993ApJ...417..259F
9. Stringfellow & Bowyer =1993IAUC.5803....1S 1993IAUC.5803....1S
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.
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Origin: AAS CD-ROM series, Volume 2, 1994
(End) Lee Brotzman [ADS] 19-Apr-1994, Patricia Bauer [CDS] 21-Oct-1994