J/A+AS/109/147 ROSAT AGN content (Brinkmann+, 1995)
The ROSAT AGN content of the 87GB 5GHz survey: bulk properties of previously
optically identified sources
Brinkmann W., Siebert J., Reich W., Fuerst E., Reich P., Voges W.,
Truemper J., Wielebinski R.
<Astron. Astrophys. Suppl. Ser. 109, 147 (1995)>
=1995A&AS..109..147B 1995A&AS..109..147B (SIMBAD/NED Reference)
Mission_Name: ROSAT
ADC_Keywords: Active gal. nuclei ; X-ray sources ; Radio sources
Keywords: galaxies: active - quasars; X-rays: general - radio sources: general
Description:
The cross-correlation of the source list from the ROSAT All-Sky Survey
with the 5 GHz Green Bank survey yields a list of 2127 objects. About
two thirds of them are optically unidentified. The majority of the
objects with known optical counterparts are quasars and radio
galaxies, most of them detected in X-rays for the first time. In this
paper we present a list of the previously optically identified objects
with their main characteristics and discuss their general (bulk)
properties. We find strong correlations between luminosities in the
radio, optical, and X-ray bands which differ for quasars and radio
galaxies.
File Summary:
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File Name Lrecl Records Explanations
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ReadMe 80 . This file
table1 89 617 Catalog of sources from RASS-Condon correlation
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See also:
III/175 : Optical spectroscopy of radio sources (Stickel+, 1989-94)
VIII/14 : 87GB Catalog of radio sources (Gregory et al., 1991)
Byte-by-byte Description of file: table1
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Bytes Format Units Label Explanations
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1- 13 A13 --- ROSAT ROSAT name of source
16- 18 A3 --- Class Object class (reference r_Vmag)
20- 23 A4 --- Type Optical type (4)
25- 40 A16 --- Name Other name of source
41 A1 --- r_Vmag Reference for the optical identification
and data if not from NED (1)
43- 47 F5.2 mag Vmag []? Optical magnitude
49- 54 F6.4 --- z []? Redshift
57- 62 F6.3 Jy F5GHz 5GHz radio flux density
64- 68 F5.3 Jy e_F5GHz []? rms uncertainty on F5GHz
69 I1 --- q_F5GHz []? Error class from Bonn catalog (3)
70 A1 --- r_F5GHz [BC] Reference for radio flux (2)
73- 78 F6.3 10-14W/m2 FX X-ray flux in (0.1-2.4)keV energy band
80- 85 F6.3 10-14W/m2 e_FX rms uncertainty on X-ray flux
88- 89 I2 arcsec Dist Distance between radio and X-ray position
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Note (1): References for optical identification, Vmag and z are:
1: Stickel and Kuehr (1994A&AS..103..349S 1994A&AS..103..349S); in catalog III/175
2: Stickel and Kuehr (1993A&AS..100..395S 1993A&AS..100..395S); in catalog III/175
3: Stickel and Kuehr (1993A&AS..101..521S 1993A&AS..101..521S); in catalog III/175
4: Stickel and Kuehr (1994A&AS..105...67S 1994A&AS..105...67S)
5: Kock A., private communication
6: Bade N., et al. (1994A&A...286..381B 1994A&A...286..381B)
7: Fleming T.A., et al., 1994, ApJ (in press?)
Note (2):
B = Bonn catalog: error class is available (see q_F5GHz)
C = Gregory & Condon 87GB VIII/14 catalog.
Note (3): For the Bonn catalog, the error class on F5GHz is
1: ≤ 9%; 2: 9-14% ; 3: 14-23% ; 4: ≥ 23%
Note (4): the optical type is a defined in NED:
E = Elliptical ; S = Spiral ; I = Irregular ; SY1,2 = Seyfert type 1,2
HP = Highly polarized in the optical ;
0,1,2 = richness class for Clusters of Galaxies
GPA = Galaxy pair ; GTR = Galaxy triple
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(End) Patricia Bauer [CDS] 02-Sep-1994; revised F. Ochsenbein 13-May-1996