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J/ApJ/733/60      Accretion rate of AGNs from COSMOS surveys      (Trump+, 2011)

Accretion rate and the physical nature of unobscured active galaxies. Trump J.R., Impey C.D., Kelly B.C., Civano F., Gabor J.M., Diamond-Stanic A.M., Merloni A., Urry C.M., Hao H., Jahnke K., Nagao T., Taniguchi Y., Koekemoer A.M., Lanzuisi G., Liu C., Mainieri V., Salvato M., Scoville N.Z. <Astrophys. J., 733, 60 (2011)> =2011ApJ...733...60T
ADC_Keywords: Active gal. nuclei ; Accretion ; Redshifts Keywords: accretion, accretion disks - galaxies: active - galaxies: nuclei - galaxies: Seyfert - quasars: emission lines - quasars: general Abstract: We show how accretion rate governs the physical properties of a sample of unobscured broad-line, narrow-line, and lineless active galactic nuclei (AGNs). We avoid the systematic errors plaguing previous studies of AGN accretion rates by using accurate intrinsic accretion luminosities (Lint) from well-sampled multiwavelength spectral energy distributions from the Cosmic Evolution Survey, and accurate black hole masses derived from virial scaling relations (for broad-line AGNs) or host-AGN relations (for narrow-line and lineless AGNs). Description: We select a sample of 348 AGNs from the COSMOS (Scoville et al. 2007ApJS..172...38S) field, which is based on the 1.7deg2 Hubble Space Telescope (HST)/Advanced Camera for Surveys (ACS) mosaic. These AGNs have multiwavelength data in the form of Spitzer/IRAC, HST/ACS, Subaru/Suprime-Cam, GALEX, XMM-Newton, and Chandra observations. The sample is selected from the parent catalog of 1651 XMM-COSMOS point sources with optical counterparts (Brusa et al. 2010, Cat. J/ApJ/716/348). File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table2.dat 80 348 Catalog of AGNs
See also: J/A+A/542/A16 : X-ray detection of radio-selected SF galaxies (Ranalli+, 2012) J/A+A/535/A80 : Type-2 QSOs in XMM-COSMOS (Mainieri+, 2011) J/A+A/534/A110 : Type-2 AGN from XMM-COSMOS bolometric output (Lusso+, 2011) J/ApJ/742/61 : AGN from XMM- and C-COSMOS (Salvato+, 2011) J/ApJ/716/348 : The XMM-Newton survey of the COSMOS field (Brusa+, 2010) J/A+A/512/A34 : XMM-COSMOS Type 1 AGNs (Lusso+, 2010) J/ApJ/696/1195 : COSMOS AGN spectroscopic survey. I. (Trump+, 2009) J/A+A/497/635 : XMM-Newton wide-field survey in COSMOS (Cappelluti+, 2009) J/ApJS/172/383 : AGN candidates in the COSMOS field (Trump+, 2007) J/ApJS/172/368 : XMM-Newton survey in COSMOS field. IV. (Mainieri+, 2007) J/ApJS/172/70 : zCOSMOS-bright catalog (Lilly+, 2007) J/ApJS/172/29 : XMM-Newton survey in COSMOS field. I. (Hasinger+, 2007) Byte-by-byte Description of file: table2.dat
Bytes Format Units Label Explanations
1- 2 I2 h RAh Hour of Right Ascension (J2000) 4- 5 I2 min RAm Minute of Right Ascension (J2000) 7- 11 F5.2 s RAs Second of Right Ascension (J2000) 13 A1 --- DE- Sign of the Declination (J2000) 14- 15 I2 deg DEd Degree of Declination (J2000) 17- 18 I2 arcmin DEm Arcminute of Declination (J2000) 20- 23 F4.1 arcsec DEs Arcsecond of Declination (J2000) 25- 26 A2 --- Type Object type (1) 28- 31 F4.2 --- z Redshift 33 A1 --- r_z Spectrum source (2) 35- 39 F5.2 [10-7W] logL Log of the accretion luminosity; in erg/s 41- 44 F4.2 [10-7W] e_logL Lower 1σ error in logL 46- 49 F4.2 [10-7W] E_logL Upper 1σ error in logL 51- 54 F4.2 [Msun] logM Log of the black hole mass 56- 59 F4.2 [Msun] e_logM Lower 1σ error in logM 61- 64 F4.2 [Msun] E_logM Upper 1σ error in logM 66- 70 F5.2 [-] logAcc Log of accretion rate; log(Lint/LEdd) 72- 75 F4.2 [-] e_logAcc Lower 1σ error in logAcc 77- 80 F4.2 [-] E_logAcc Upper 1σ error in logAcc
Note (1): Object type as follows: BL = broad emission line (Type 1 AGN); NL = narrow emission line (Type 2 AGN); OD = absorption line (lineless or optically dull AGN). Note (2): Spectrum source as follows: S = SDSS archive; I = Magellan/IMACS campaign (Trump et al. 2009, Cat. J/ApJ/696/1195); Z = zCOSMOS VLT/VIMOS campaign (Lilly et al. 2007, Cat. J/ApJS/172/70).
History: From electronic version of the journal
(End) Greg Schwarz [AAS], Emmanuelle Perret [CDS] 07-Nov-2012
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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