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J/A+AS/132/341      ROSAT GPS optical identification (Motch+ 1998)

Identification of selected sources for the ROSAT Galactic Plane Survey. I. Motch C., Guillout P., Haberl F., Krautter J., Pakull M.W., Pietsh W., Reinsch K., Voges W., Zickgraf F.-J. <Astron. Astrophys. Suppl. Ser. 132, 341 (1998)> =1998A&AS..132..341M (SIMBAD/NED BibCode)
ADC_Keywords: X-ray sources ; Cross identifications Mission_Name: ROSAT Keywords: X-ray: general - X-ray: stars - X-rays: galaxies - surveys Abstract: We report on optical searches in the error circles of 93 ROSAT survey sources located at low galactic latitudes (|b|<20°). These sources were extracted from the ROSAT Galactic Plane Survey using various selection criteria on hardness ratio, X-ray and optical brightness and integrated galactic absorption in the direction of the source. We find optical identifications in 76 cases, among which are 25 new AGN, 6 new CVs and a new Be/X-ray binary. In order to illustrate the relevance of the source selections applied here, we cross-correlated the ROSAT all-sky survey bright source list with SIMBAD. Different classes of X-ray emitters populate distinct regions of a multi dimensional parameter space involving flux ratios, galactic latitude and NH. This relatively good segregation offers the possibility to build source samples with enhanced probability of identification with a given class. Complete optical identification of such subsamples could eventually be used to compute meaningful probabilities of identification for all sources using as basis a restricted set of multi-wavelength information. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table4.dat 99 93 X-ray characteristics of ROSAT survey sources derived from the SASS as in October 1991 table5.dat 96 93 Optical identifications of ROSAT survey sources
See also: IX/10 : ROSAT All-Sky Bright Source Catalogue (1RXS) (Voges+ 1996) J/A+A/318/111 : ROSAT Galactic Plane Survey (Motch+ 1997) Byte-by-byte Description of file: table4.dat
Bytes Format Units Label Explanations
1- 15 A15 --- RXJ Source name 17 A1 --- Source [XAOBS] Source selection origin (1) 19- 20 I2 h RAh Right ascension (J2000.0) 22- 23 I2 min RAm Right ascension (J2000.0) 25- 28 F4.1 s RAs Right ascension (J2000.0) 30 A1 --- DE- Declination sign 31- 32 I2 deg DEd Declination (J2000.0) 34- 35 I2 arcmin DEm Declination (J2000.0) 37- 38 I2 arcsec DEs Declination (J2000.0) 40- 43 F4.1 arcsec r90 ? 90% confidence radius 45- 49 F5.3 ct/s Count Count rate 51- 55 F5.3 ct/s e_Count rms uncertainty on Count 57- 61 F5.2 --- HR1 Hard ratio 1 63- 66 F4.2 --- e_HR1 ? rms uncertainty on HR1 68- 72 F5.2 --- HR2 Hard ratio 2 74- 77 F4.2 --- e_HR2 ? rms uncertainty on HR2 79- 99 A21 --- 1RXS 1RXS (Cat. IX/10) designation
Note (1): X: X-ray binary like S: Soft white dwarf candidate A: Absorption supersoft candidate B: X-ray bright source O: Other remaining source
Byte-by-byte Description of file: table5.dat
Bytes Format Units Label Explanations
1- 15 A15 --- RXJ Source name 17 A1 --- Sel [XAOBS] Source selection origin (1) 19- 22 F4.2 --- Dist ? X-ray to optical distance in units of the 90% confidence radius 24- 25 I2 h RAh ? Right ascension (J2000.0) 27- 28 I2 min RAm ? Right ascension (J2000.0) 30- 34 F5.2 s RAs ? Right ascension (J2000.0) 36 A1 --- DE- Declination sign 37- 38 I2 deg DEd ? Declination (J2000.0) 40- 41 I2 arcmin DEm ? Declination (J2000.0) 43- 46 F4.1 arcsec DEs ? Declination (J2000.0) 48- 67 A20 --- IdOpt Optical identification 69- 73 F5.2 mag Vmag ? V magnitude 75- 79 F5.2 mag Bmag ? B magnitude 81- 84 A4 --- Class Class (2) 87- 94 A8 --- Mtype Spectral or morphological type 96 A1 --- Chart [Y] Y: a finding chart is provided
Note (1): X: X-ray binary like S: Soft white dwarf candidate A: Absorption supersoft candidate B: X-ray bright source O: Other remaining source Note (2): AC: active corona Gal: Normal galaxy AGN: Active galactic nucleus Be/X: Be/X-ray binary UNID: Unidentified WD: Isolated white dwarf
Acknowledgements: Christian Motch
(End) Patricia Bauer [CDS] 08-Oct-1998
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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