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J/ApJ/688/826        Radio and X-ray-emitting broad-line AGNs        (Li+, 2008)

The black hole fundamental plane: revisited with a larger sample of radio and X-ray-emitting broad-line AGNs. Li Z.-Y., Wu X.-B., Wang R. <Astrophys. J., 688, 826-836 (2008)> =2008ApJ...688..826L
ADC_Keywords: Active gal. nuclei ; Galaxies, radio ; X-ray sources Keywords: accretion, accretion disks - black hole physics - galaxies: active - galaxies: nuclei - radio continuum: galaxies - X-rays: galaxies Abstract: We use a recently released SDSS catalog of X-ray-emitting AGNs in conjunction with the FIRST radio survey to investigate the black hole (BH) fundamental plane relationship between the 1.4GHz radio luminosity (Lr), 0.1-2.4keV X-ray luminosity (LX), and black hole mass (M), namely, logLrRXlogLXRMlogM+constant. For this purpose, we compile a large sample of 725 broad-line AGNs, which consists of 498 radio-loud sources and 227 radio-quiet sources. We confirm that radio-loud objects have a steeper slope (ξRX) with respect to radio-quiet objects and that the dependence of the BH fundamental plane on the BH mass (ξRM) is weak. Description: Our sample is selected based on the cross-identification of the newly published X-ray-emitting SDSS AGN catalog (Anderson et al. 2007, Cat. J/AJ/133/313) and the catalog of the FIRST 20cm radio survey (White et al. 1997, Cat. VIII/71). File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 63 725 The sample of AGNs
See also: VIII/71 : The FIRST Survey Catalog, Version 03Apr11 (Becker+ 2003) J/A+A/356/445 : ROSAT-FIRST AGN correlation (Brinkmann+, 2000) J/AJ/126/2209 : X-ray AGN from RASS and SDSS (Anderson+, 2003) J/MNRAS/362/9 : Radio-loud AGN in SDSS (Best+, 2005) J/AJ/132/1475 : SDSS AGN from ROSAT PSPC (Suchkov+, 2006) J/ApJ/645/890 : Radio and X-ray-emitting broad-line AGNs (Wang+, 2006) J/AJ/133/313 : AGN from RASS and SDSS DR5 (Anderson+, 2007) J/ApJS/176/355 : AGN X-Ray emission and black holes (Kelly+, 2008) Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 4 A4 --- --- [SDSS] 6- 24 A19 --- SDSS AGN designation (JHHMMSS.ss+DDMMSS.s) 26- 30 F5.3 --- z SDSS spectroscopic redshift 32- 36 F5.2 [10-7W] logLX Log of (0.1-2.4keV) soft X-ray luminosity 38- 42 F5.2 [10-7W] logLr Log of rest-frame 1.4GHz radio luminosity 44- 49 F6.3 [-] logR Log of radio-loudness 51- 55 F5.2 [Msun] logM Log of black hole mass 57- 61 F5.2 [10-7W] logLbl Log of broad emission line luminosity (1) 63 I1 --- n_logLbl Line used for the broad-line luminosity (2)
Note (1): Represented by the Hbeta broad component luminosity or the MgII emission line luminosity (when Hbeta is unavailable). Note (2): Flags as follows: 1 = Hβ broad component luminosity is used to represent the broad emission line luminosity. 0 = MgII emission line luminosity is used to represent the broad emission line luminosity.
History: From electronic version of the journal References: Wang et al. The black hole fundamental plane from a uniform sample of radio and X-ray-emitting broad-line AGNs. 2006ApJ...645..890W Cat. J/ApJ/645/890
(End) Greg Schwarz [AAS], Emmanuelle Perret [CDS] 17-Jan-2011
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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