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J/ApJ/660/1072      Unified model of active galactic nuclei  (Wang+, 2007)

The unified model of active galactic nuclei. II. Evolutionary connection. Wang J.-M., Zhang E.-P. <Astrophys. J., 660, 1072-1092 (2007)> =2007ApJ...660.1072W
ADC_Keywords: Active gal. nuclei ; Keywords: accretion, accretion disks - black hole physics - galaxies: active - galaxies: Seyfert - polarization - stars: formation Abstract: We assemble a sample composed of 243 nearby Seyfert galaxies with redshifts z≤0.05 to test the unification scheme. The sample contains 94 broad emission line Seyfert 1 galaxies (BLS1s), 44 narrow emission line Seyfert 1s (NLS1s), 36 X-ray-absorbed hidden broad line region Seyfert 2s (HBLR S2s), 42 X-ray-absorbed non-HBLR S2s, and 27 X-ray-unabsorbed Seyfert 2s (unabsorbed non-HBLR S2s and HBLR S2s). We find that (1) NLS1s have less massive black hole masses than BLS1s, (2) HBLR S2s have the same mass distribution of black holes as BLS1s, (3) absorbed non-HBLR S2s have less massive black holes than HBLR S2s, and (4) unabsorbed non-HBLR S2s have the most massive black holes. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table3.dat 109 94 The broad-line Seyfert 1 sample table4.dat 108 36 The X-ray absorbed hidden broad-line region (HBLR) Seyfert 2 sample table5.dat 110 27 The unabsorbed Seyfert 2 sample (7 HBLR and 20 non-HBLR) table12.dat 147 44 The narrow-line Seyfert 1 sample (table 2 of Paper I) table13.dat 129 42 The non-hidden broad-line Seyfert 2 sample (table 3 of Paper I) refs.dat 93 139 References
See also: J/ApJ/614/91 : Black hole mass and accretion rate of AGNs (Wu+, 2004) J/ApJ/641/L21 : Black hole mass & velocity dispersion relation (Greene+, 2006) J/ApJ/645/890 : Radio and X-ray-emitting broad-line AGNs (Wang+, 2006) J/ApJ/669/791 : Quasar black hole masses (Wilhite+, 2007) J/ApJ/667/131 : Mass function of active black holes (Greene+, 2007) J/ApJ/670/92 : New sample of low-mass black holes in AGN (Greene+, 2007) J/ApJS/168/1 : Black hole mass estimates (Kelly+, 2007) J/A+A/492/637 : Eddington ratios of faint AGN (Gavignaud+, 2008) J/ApJ/680/169 : SDSS DR5 virial black hole masses (Shen+, 2008) J/ApJS/176/355 : AGN X-Ray emission and black holes (Kelly+, 2008) J/other/ChA+A/32.351 : Accretion rate distributions of AGNs (Bao+, 2008) Byte-by-byte Description of file: table3.dat
Bytes Format Units Label Explanations
1- 16 A16 --- Name Source name 17 A1 --- n_Name [*] * for objects from the 12um sample 19- 23 F5.3 --- z Redshift 25- 39 A15 --- MType ?=--- Hubble type 41- 46 F6.2 mag BMAG ?=- Bulge absolute magnitude in B band 48- 52 I5 km/s FWHMHb ?=- FWHM of Hβ line 54- 57 F4.2 [solMass] logMBHb ?=- Mass of black hole (calculated with Hβ) 59- 63 F5.2 [-] logEddb ?=- Eddington ratio (Lbol=9*L5100Å) 65- 67 I3 km/s FWHMO ?=- FWHM of [OIII] line 69- 72 F4.2 [solMass] logMBHO ?=- Mass of black hole, calculated with [OIII] 74- 78 F5.2 [-] logEddO ?=- Eddington ratio (Lbol=3500*L[OIII]) 80- 84 F5.2 [10-7W] logL[O3] ?=- Luminosity of [OIII] λ5007Å emission line 86- 89 F4.2 -- Gam.h ?=- Hard X-ray (2-10keV) photon index 91- 94 F4.2 --- e_Gam.h ? rms uncertainty on Gam.h 96- 97 I2 --- r_MType ? Reference for MType, in refs.dat file 99-100 I2 --- r_BMAG ? Reference for BMAG, in refs.dat file 102-103 I2 --- r_FWHMHb ? Reference for FWHMHb, in refs.dat file 105-106 I2 --- r_FWHMO ? Reference for FWHMO, in refs.dat file 108-109 I2 --- r_Gam.h ? Reference for Gam.h, in refs.dat file
Byte-by-byte Description of file: table4.dat
Bytes Format Units Label Explanations
1- 16 A16 --- Name Source name 17 A1 --- n_Name [*] * for objects from the 12um sample 19- 23 F5.3 --- z Redshift 25- 39 A15 --- MType ?=--- Hubble type 41- 46 F6.2 mag BMAG ?=- Bulge absolute magnitude in B band 48- 50 I3 km/s FWHMO ?=- FWHM of [OIII] line 52- 55 F4.2 [solMass] logMBHO ?=- Mass of black hole (calculated with [OIII]) 57- 61 F5.2 [-] logEddO ?=- Eddington ratio (Lbol=3500*L[OIII]) 63- 67 F5.2 [10-7W] logL[O3] ?=- Luminosity of [OIII] λ5007 emission line 69 A1 --- l_logNH Limit flag on logNH 70- 74 F5.2 [cm-2] logNH ?=- H column density 76- 80 F5.2 [10-7W] logLPAH ?=- PAH luminosity 82- 85 F4.2 -- Gam.h ?=- Hard X-ray (2-10keV) photon index 87- 90 F4.2 --- e_Gam.h ? rms uncertainty on Gam.h 92- 93 I2 --- r_BMAG Reference for BMAG in refs.dat file 95- 96 I2 --- r_FWHMO ? Reference for FWHMO, in refs.dat file 98- 99 I2 --- r_logL[O3] ? Reference for logL[O3], in refs.dat file 101-102 I2 --- r_logNH ? Reference for logNH, in refs.dat file 104-105 I2 --- r_logLPAH ? Reference for logLPAH, in refs.dat file 107-108 I2 --- r_Gam.h ? Reference for Gam.h, in refs.dat file
Byte-by-byte Description of file: table5.dat
Bytes Format Units Label Explanations
1 A1 --- f_Name [HN] H for HBLR, N for non-HBLR Seyfert 2 3- 18 A16 --- Name Source name 19- 23 A5 --- m_Name (pol) for polarized broad lines 24 A1 --- n_Name [*] * for objects from the 12um sample 26- 30 F5.3 --- z Redshift 32- 45 A14 --- MType ?=--- Hubble type 47- 52 F6.2 mag BMAG ?=- Bulge absolute magnitude in B band 54- 56 I3 km/s sigma ?=- Velocity dispersion 58- 60 I3 km/s FWHMO ?=- FWHM of [OIII] line 62- 65 F4.2 [solMass] logMBHO ?=- Mass of black hole, calculated with [OIII] 66 A1 --- n_logMBHO [a] MBH is deduced from Mbul 67- 71 F5.2 [-] logEddO ?=- Eddington ratio (Lbol=3500*L[OIII]) 72 A1 --- n_logEddO [b] Bolometric luminosity is deduced from LX(2-10keV) (1) 73- 77 F5.2 [10-7W] logL[O3] ?=- Luminosity of [OIII] λ5007 emission line 79- 80 A2 --- l_logNH [≤ ] Limit flag on logNH 81- 85 F5.2 [cm-2] logNH ?=- Column density 87 A1 --- l_logLPAH Limit flag on logLPAH 88- 92 F5.2 [10-7W] logLPAH ?=- PAH luminosity 94- 95 I2 --- r_BMAG Reference for BMAG in refs.dat file 97- 98 I2 --- r_sigma ? Reference for sigma, in refs.dat file 100-101 I2 --- r_FWHMO ? Reference for FWHMO, in refs.dat file 103-104 I2 --- r_logMBHO ? Reference for logMBHO, in refs.dat file 106-107 I2 --- r_logNH ? Reference for logNH, in refs.dat file 109-110 I2 --- r_logLPAH ? Reference for logLPAH, in refs.dat file
Note (1): We have : IRAS 01428-0404, logLX=41.38 (Panessa & Bassani, 2002A&A...394..435P) NGC 5995, logLX=43.52 (Panessa & Bassani, 2002A&A...394..435P) NGC 6251, logLX=41.38 (Panessa & Bassani, 2002A&A...394..435P) NGC 7679, logLX=42.42 (Della Ceca et al., 2001A&A...375..781D)
Byte-by-byte Description of file: table12.dat
Bytes Format Units Label Explanations
1- 16 A16 --- Name Source name 17 A1 --- n_Name [*] * for objects from the 12um sample 19- 23 F5.3 --- z Redshift 25- 39 A15 --- MType ?=--- Hubble type 41- 46 F6.2 mag BMAG ?=- Bulge absolute magnitude in B band 48- 51 I4 km/s FWHMHb ?=- FWHM of Hβ line 53- 56 F4.2 [solMass] logMBHb ?=- Mass of black hole (calculated with Hβ) 58- 62 F5.2 [-] logEddb ?=- Eddington ratio (Lbol=9*L5100Å) 64- 66 I3 km/s FWHMO ?=- FWHM of [OIII] line 68- 71 F4.2 [solMass] logMBHO ?=- Mass of black hole (calculated with [OIII]) 73- 77 F5.2 [-] logEddO ?=- Eddington ratio (Lbol=3500*L[OIII]) 79- 83 F5.2 [10-7W] logL[O3] ?=- Luminosity of [OIII] λ5007 emission line 85 A1 --- l_logLrad Limit flag on logLrad 86- 90 F5.2 [10-7W] logLrad ? Luminosity of radio emission at 5GHz 91 A1 --- n_logLrad [a-c] Frequency used for logLrad (1) 92 A1 --- l_F25um Limit flag on F25um 93- 96 F4.2 Jy F25um ?=- Infrared flux at 25um 98 A1 --- l_F60um Limit flag on F60um 99-102 F4.2 Jy F60um ?=- Infrared flux at 60um 104 A1 --- l_F100um Limit flag on F100um 105-109 F5.2 Jy F100um ?=- Infrared flux at 100um 111-114 F4.2 -- Gam.s ?=- Soft X-ray photon index (2) 116-119 F4.2 --- e_Gam.s ? rms uncertainty on Gam.s 121-123 I3 --- r_BMAG Reference for BMAG, in refs.dat file 125-127 I3 --- r_FWHMHb ? Reference for FWHMHb,, in refs.dat file 129-131 I3 --- r_FWHMO ? Reference for FWHMO, in refs.dat file 133-135 I3 --- r_logL[O3] ? Reference for logL[O3], in refs.dat 137-139 I3 --- r_logLrad ? Reference for logLrad, in refs.dat file 141-143 I3 --- r_F25um ? Reference for infrared fluxes, in refs.dat 145-147 I3 --- r_Gam.s ? Reference for Gam.s, in refs.dat file
Note (1): 5GHz luminosities deduced from: a = 8.3GHz b = 2.3GHz c = 8.4GHz Note (2): Photon index of soft X-ray 0.1-2.4 and 0.2-2.0 keV (Grupe et al. 1998A&A...330...25G; 1999, Cat. J/A+A/350/805; 2004, J/AJ/127/156); 0.1-2.0 keV (Xu et al., 2003, Cat. J/ApJ/590/73)
Byte-by-byte Description of file: table13.dat
Bytes Format Units Label Explanations
1- 16 A16 --- Name Source name 17 A1 --- n_Name [*] * for objects from the 12um sample 19- 23 F5.3 --- z Redshift 25- 39 A15 --- MType ?=--- Hubble type 41- 46 F6.2 mag BMAG ?=- Bulge absolute magnitude in B band 48- 50 I3 km/s FWHMHb ?=- FWHM of Hβ line 52 A1 --- l_logMBHb Limit flag on logMBHb 53- 56 F4.2 [solMass] logMBHb ?=- Mass of black hole, (calculated with Hβ) 58 A1 --- l_logEddb Limit flag on logEddb 59- 63 F5.2 [-] logEddb ?=- Eddington ratio (Lbol=9*L5100Å) 65- 69 F5.2 [10-7W] logL[O3] ?=- Luminosity of [OIII] λ5007 emission line 71 A1 --- l_logLrad Limit flag on logLrad 72- 76 F5.2 [10-7W] logLrad ? Luminosity of radio emission (5 GHz) 77 A1 --- n_logLrad [a-e] Frequency used for logLrad (1) 78 A1 --- l_F25um Limit flag on F25um 79- 83 F5.2 Jy F25um ?=- Infrared flux at 25um 85- 91 F7.3 Jy F60um ?=- Infrared flux at 60um 92 A1 --- l_F100um Limit flag on F100um 93- 98 F6.2 Jy F100um ?=- Infrared flux at 100um 100 A1 --- l_logNH Limt flag on logNH 101-105 F5.2 [cm-2] logNH ?=- Column density 107-109 I3 --- r_BMAG Reference for BMAG, in refs.dat file 111-113 I3 --- r_FWHMHb ? Reference for FWHMHb,, in refs.dat file 115-117 I3 --- r_logEddb ? Reference for logEddb, in refs.dat file 119-121 I3 --- r_logL[O3] ? Reference for logL[O3], in refs.dat file 123-125 I3 --- r_logLrad ? Reference for logLrad, in refs.dat file 127-129 I3 --- r_F25um ? Reference for infrared fluxes, in refs.dat
Note (1): 5GHz luminosities deduced from: a = 2.3GHz; b = 8.4GHz; c = 8.3GHz; d = 4.9GHz; e = 1.5GHz.
Byte-by-byte Description of file: refs.dat
Bytes Format Units Label Explanations
1- 3 I3 --- Ref Reference number 5- 23 A19 --- BibCode BibCode 25- 48 A24 --- Aut Author's name 50- 93 A44 --- Com Comments
History: From electronic version of the journal References: Zhang and Wang, Paper I 2006ApJ...653..137Z
(End) Patricia Vannier [CDS] 05-Jun-2010
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