J/MNRAS/407/2399 AGN activity and black hole mass (McKernan+, 2010)
Black hole mass, host galaxy classification and AGN activity.
McKernan B., Ford K.E.S., Reynolds C.S.
<Mon. Not. R. Astron. Soc., 407, 2399-2410 (2010)>
=2010MNRAS.407.2399M 2010MNRAS.407.2399M
ADC_Keywords: Active gal. nuclei ; Galaxies, IR ; X-ray sources
Keywords: accretion, accretion discs - galaxies: active - galaxies: nuclei -
galaxies: Seyfert - infrared: galaxies - X-rays: galaxies
Abstract:
We investigate the role of host galaxy classification and black hole
mass (MBH) in a heterogeneous sample of 276 mostly nearby (z<0.1)
X-ray and IR-selected active galactic nuclei (AGN).
File Summary:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
table1.dat 90 276 The AGN in our sample
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See also:
VII/248 : Quasars and Active Galactic Nuclei (12th Ed.) (Veron+ 2006)
VII/258 : Quasars and Active Galactic Nuclei (13th Ed.) (Veron+ 2010)
Byte-by-byte Description of file: table1.dat
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Bytes Format Units Label Explanations
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1 I1 --- Group [1/2] AGN group (1)
3- 7 A5 --- Note Note on redshift for group 1 AGN
9- 23 A15 --- Name AGN name
25- 31 F7.2 Mpc Dlum Luminosity distance listed in NED
33- 39 F7.4 10-14W/m2 FX Mean observed 2-10keV X-ray flux
(in 10-11erg/cm2/s)
41- 46 F6.3 Jy F12um Mean observed 12um flux
48- 61 A14 --- Class Host galaxy classification
(from NED notes and RC3 (VII/155))
63- 75 A13 --- Aclass Activity classification according to NED and
Veron-Cetty & Veron (2006, VII/248) with (in
brackets) Group 1 or 2 identification. (2)
78- 81 F4.2 Msun Mbh ?=- Central black hole mass estimate
82 A1 --- --- [-]
83 I1 Msun Mbh2 ? Upper limit of central black hole mass
estimate when interval
86- 90 A5 --- Ref References for data (3)
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Note (1):
* Group 1 AGN are Seyfert 1.X AGN (X=0-9) or quasi-stellar objects.
* Group 2 AGN are everything else (Seyfert 2s, LINERs, low-luminosity
AGN, starburst/AGN, cross-classified AGN)
Note (2): Activity classification is denoted according to Veron-Cetty and
Veron (2006A&A...455..773V 2006A&A...455..773V, Cat. VII/248) except:
we write Sy3 as L(LINERS) with S3b,S3h denoted by L1 and L2,
respectively, and S1n are written as NLSy1 (narrow-line Sy1). Other
classifications include SB = starburst, U = ULIRG.
Note (3): References as follows:
N = NED
1 = Satyapal et al. (2005ApJ...633...86S 2005ApJ...633...86S)
2 = Winter et al. (2009ApJ...690.1322W 2009ApJ...690.1322W)
3 = Ho (1999ApJ...516..672H 1999ApJ...516..672H)
4 = Krips et al. (2007A&A...464..553K 2007A&A...464..553K)
5 = Yuan et al. (2009ApJ...703.1034Y 2009ApJ...703.1034Y)
6 = Lewis & Eracleous (2006ApJ...642..711L 2006ApJ...642..711L)
7 = Graham (2008PASA...25..167G 2008PASA...25..167G)
8 = Dong & De Robertis (2006)
9 = Krongold (2005ApJ...620..165K 2005ApJ...620..165K)
10 = Kim et al. (2008ApJ...687..767K 2008ApJ...687..767K)
11 = Gonzalez-Martin (2006A&A...460...45G 2006A&A...460...45G)
12 = Weaver et al. (2002ApJ...576L..19W 2002ApJ...576L..19W)
13 = Satyapal, Sambruna & Dudik (2004, Cat. J/A+A/414/825)
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History:
From electronic version of the journal
(End) Patricia Vannier [CDS] 31-Mar-2011