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J/ApJ/566/744       EEMSS new X-ray clusters                 (Lewis+, 2002)

New X-ray clusters in the EINSTEIN Extended Medium-Sensitivity Survey. I. Modifications to the X-ray luminosity function. Lewis A.D., Stocke J.T., Ellingson E., Gaidos E.J. <Astrophys. J. 566, 744 (2002)> =2002ApJ...566..744L
ADC_Keywords: Clusters, galaxy ; X-ray sources Keywords: galaxies: clusters: general - surveys - X-rays: general Abstract: The complete ensemble of Einstein Imaging Proportional Counter (IPC) X-ray images has been reprocessed and reanalyzed using a multiaperture source detection algorithm. A catalog of 772 new source candidates detected within the 38' diameter central regions of the 1435 IPC fields comprising the Extended Medium-Sensitivity Survey (EMSS) has been compiled. By comparison, 478 EMSS sources fall within the same area of sky. A randomly selected subsample of 133 fields was examined; 73 sources were detected and compared with 49 original EMSS sources in the same region of sky. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table3.dat 62 74 New sources in the randomly selected subset of 133 EMSS (Extended Medium-Sensitivity Survey) IPC fields table7.dat 62 13 X-ray data for sources from the ramp subsample table9.dat 62 20 X-ray data for sources observed in the high flux and S/N subsample
See also: IX/15 : Einstein EMSS Survey (Gioia+ 1990, Stocke+ 1991) Byte-by-byte Description of file: table3.dat table7.dat table9.dat
Bytes Format Units Label Explanations
1- 4 I4 --- [LSE2002] Sequential number 5 A1 --- n_[LSE2002] [b] b: Source was removed from the random subsample; see Section 3.2 of paper 7- 8 I2 h RAh Right ascension (J2000) 10- 11 I2 min RAm Right ascension (J2000) 13- 17 F5.2 s RAs Right ascension (J2000) 19 A1 --- DE- Declination sign (J2000) 20- 21 I2 deg DEd Declination (J2000) 23- 24 I2 arcmin DEm Declination (J2000) 26- 29 F4.1 arcsec DEs Declination (J2000) 31- 35 I5 --- Seq Sequence number 37- 38 I2 10-3s-1 CR1 First Count rate in the 0.3-3.5 keV band 40- 41 I2 10-3s-1 CR2 Second Count rate in the 0.3-3.5 keV band 43- 44 I2 10-3s-1 CR3 Third Count rate in the 0.3-3.5 keV band 46- 49 F4.2 10-3s-1 e_CR1 rms uncertainty on CR1 (1) 51- 54 F4.2 10-3s-1 e_CR2 rms uncertainty on CR2 (1) 56- 59 F4.2 10-3s-1 e_CR3 rms uncertainty on CR3 (1) 61- 62 A2 --- Type Identification of the source (2)
Note (1): An entry of zero indicates a value less than the detection threshold limit of 2.5. Note (2): Identification based on all the data in Tables 4-6 as follows: C = cluster of galaxies X = not a cluster of galaxies; C: = possible cluster of galaxies If there is no entry, no definitive determination is possible at this time.
Table 4: Identifications or Counterparts for Random Subsample Sources -------------------------------------------------------------------------------- No ID or Counterpart E Reference -------------------------------------------------------------------------------- 64 Radio: NVSS 002349.97 +171717; 17mJy 97 Radio: 87GB 00352.2+291502 1991, Cat. VIII/14, Gregory & Condon 97 Galaxy group: NGC 0181/0183/0184 (z=0.018) C 1976ApJS...31..187D, Dressel & Condon 163 QSO: 0050+0123 (z=1.439) A 1995AJ....109.1498H, Hewett et al. 299 Star: PPM 183386 (V=10.0) S 299 Radio: PMN J0123-0348 1995, Cat. VIII/38, Griffith et al. 1955 AGN: EXO 1156.3+3239 (z=0.215) A 1991ApJ...378...77G, Giommi et al. 2282 Star: HD 112221 (GV, V=9.10, B-V=0.45) S 1994, Cat. J/A+AS/106/257 Olsen 4359 Galaxy group related to A665 (z=0.20) C this paper Source was removed from the random subsample, for being target related; see Chap. 3.2 5101 Star: SAO 17771 (K2, V=9.3, B-V=1.4) S 5187 IRAS: 21586-5652; probable AGN A 1990, Cat. II/156, Moshir et al. 5208 Star: EXO 2251.1-1737 (V=16) S 1991ApJ...378...77G, Giommi et al. 5223 QSO: HB89 2314-423 (z=0.27) A 1987ApJS...63....1H, Hewitt & Burbidge 5341 Star: Gliese 1416 K2 double (V=9.8, B-V=1.2) S 1994, Cat. J/A+AS/106/377 Couteau & Gili -------------------------------------------------------------------------------- Note: E: Identification of the source based on the information available: C = cluster of galaxies A = AGN S = star History: From electronic version of the journal
(End) James Marcout, Patricia Bauer [CDS] 19-Apr-2002
The document above follows the rules of the Standard Description for Astronomical Catalogues.From this documentation it is possible to generate f77 program to load files into arrays or line by line

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