J/ApJ/502/558       Catalog of ROSAT galaxy clusters          (Vikhlinin+ 1998)

A catalog of 200 galaxy clusters serendipitously detected in the ROSAT PSPC pointed observations. Vikhlinin A., McNamara B.R., Forman W., Jones C., Quintana H., Hornstrup A. <Astrophys. J. 502, 558 (1998)> =1998ApJ...502..558V 1998ApJ...502..558V
ADC_Keywords: Clusters, galaxy ; X-ray sources ; Redshifts Mission_Name: ROSAT Keywords: catalogs - galaxies: clusters: general - surveys - X-rays: galaxies Abstract: We present a catalog of 203 clusters of galaxies serendipitously detected in 647 ROSAT PSPC high Galactic latitude pointings covering 158deg2. This is one of the largest X-ray-selected cluster samples, comparable in size only to the ROSAT All-Sky Survey sample of nearby clusters (Ebeling et al., 1997ApJ...479L.101E 1997ApJ...479L.101E). We detect clusters in the inner 175 of the ROSAT PSPC field of view using the spatial extent of their X-ray emission. Fluxes of detected clusters range from 1.6x10-14 to 8x10-12ergs/s/cm2 in the 0.52keV energy band. X-ray luminosities range from 1042ergs/s, corresponding to very poor groups, to ∼5x1044ergs/s, corresponding to rich clusters. The cluster redshifts range from z=0.015 to z>0.5. The catalog lists X-ray fluxes, core radii, and spectroscopic redshifts for 73 clusters and photometric redshifts for the remainder. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table3.dat 67 223 Cluster catalog notes.dat 79 41 Notes to table3.dat -------------------------------------------------------------------------------- See also: IX/11 : ROSAT Source Catalog (Voges+ 1994) Byte-by-byte Description of file: table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 I3 --- [VMF98] Sequential number 5- 6 I2 h RAh X-ray centroid right ascension (J2000) 8- 9 I2 min RAm X-ray centroid right ascension (J2000) 11- 14 F4.1 s RAs X-ray centroid right ascension (J2000) 16 A1 --- DE- X-ray centroid declination sign (J2000) 17- 18 I2 deg DEd X-ray centroid declination (J2000) 20- 21 I2 arcmin DEm X-ray centroid declination (J2000) 23- 24 I2 arcsec DEs X-ray centroid declination (J2000) 26- 30 F5.1 10-17W/m2 FX Total unabsorbed X-ray flux in the 0.5-2keV energy band (in 10-14erg/s/cm2) 32- 35 F4.1 10-17W/m2 e_FX rms uncertainty on FX 37- 39 I3 arcsec Rc Angular core radius 41- 42 I2 arcsec e_Rc rms uncertainty on Rc 44- 48 F5.3 --- z ? Heliocentric spectroscopic or photometric redshift (1) 50- 53 F4.2 --- zmin ? Photometric redshift 90% confidence interval 54 A1 --- --- [-] 55- 58 F4.2 --- zmax ? Photometric redshift 90% confidence interval 59- 61 A3 --- n_zmax [dss ] dss: Digited Sky Survey redshift 63- 64 I2 arcsec errPos 90% X-ray position error circle 65 A1 --- detFlag [UF] Uncertain or False detections (2) 66- 67 I2 --- Note ? Note detailed in file "notes.dat" -------------------------------------------------------------------------------- Note (1): If the redshift is spectroscopic, no error interval is given Note (2): the 'U' flag is set for clusters that show clear concentrations of galaxies near the X-ray position, but the choice of BCG is uncertain because of the large cluster angular size. No photometric redshift are given. -------------------------------------------------------------------------------- Byte-by-byte Description of file: notes.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 2 I2 --- Note Note number 4- 79 A76 --- Text Text of the note -------------------------------------------------------------------------------- History: From ApJ electronic version * 18-Dec-2001: Thanks to checks by Stephen A. Drake (), the flux units have corrected.
(End) James Marcout, Patricia Bauer [CDS] 22-Sep-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