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 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:
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FileName Lrecl Records Explanations
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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 107 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
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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
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Bytes Format Units Label Explanations
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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
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Byte-by-byte Description of file: table4.dat
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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
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Byte-by-byte Description of file: table5.dat
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Bytes Format Units Label Explanations
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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
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Note (1): We have :
IRAS 01428-0404, logLX=41.38 (Panessa & Bassani, 2002A&A...394..435P 2002A&A...394..435P)
NGC 5995, logLX=43.52 (Panessa & Bassani, 2002A&A...394..435P 2002A&A...394..435P)
NGC 6251, logLX=41.38 (Panessa & Bassani, 2002A&A...394..435P 2002A&A...394..435P)
NGC 7679, logLX=42.42 (Della Ceca et al., 2001A&A...375..781D 2001A&A...375..781D)
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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
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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 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)
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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
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Note (1): 5GHz luminosities deduced from:
a = 2.3GHz;
b = 8.4GHz;
c = 8.3GHz;
d = 4.9GHz;
e = 1.5GHz.
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Byte-by-byte Description of file: refs.dat
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Bytes Format Units Label Explanations
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1- 3 I3 --- Ref Reference number
5- 23 A19 --- BibCode BibCode
25- 48 A24 --- Aut Author's name
50- 93 A44 --- Com Comments
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History:
From electronic version of the journal
References:
Zhang and Wang, Paper I 2006ApJ...653..137Z 2006ApJ...653..137Z
(End) Patricia Vannier [CDS] 05-Jun-2010