J/ApJ/941/46 X-ray to FIR observations for an AGN sample (Spinoglio+, 2022)
The high-ionization IR fine structure lines as bolometric indicators of the AGN
power: study of the complete 12um AGN Sample.
Spinoglio L., Fernandez-Ontiveros J.A., Malkan M.A.
<Astrophys. J., 941, 46 (2022)>
=2022ApJ...941...46S 2022ApJ...941...46S
ADC_Keywords: Active gal. nuclei ; Galaxies, Seyfert ; Redshifts; Optical;
X-ray sources ; Spectra, infrared ; Black holes
Keywords: Active galaxies ; AGN host galaxies ; Infrared galaxies ;
Seyfert galaxies ; Starburst galaxies ; Infrared spectroscopy ;
X-ray active galactic nuclei ; X-ray observatories
Abstract:
The high-ionization mid-IR lines, excited in the narrow-line regions
of active galactic nuclei (AGN), barely affected by stellar excitation
and dust extinction, trace the AGN bolometric power. We used the
complete 12um sample of Seyfert galaxies, for which 100/116 objects
have reliable 2-10keV observations. The [NeV] and [OIV] mid-IR lines
linearly correlate with several AGN bolometric indicators (intrinsic
2-10keV and observed 14-195keV X-ray emission, compact nuclear 12um
emission, [OIII]λ5007Å line emission) in terms of both flux
and luminosity. No evidence of systematic differences in these
correlations is found among the Seyfert populations, including types 1
and 2 and Compton-thick and Compton-thin AGN. Nevertheless, we find
that a sequence of high-to-low Eddington ratios together with strong-
to-weak line excitation (traced by the [OIV]/[NeII] line ratio)
encompasses from type 1 through type 2 AGN to low-ionization nuclear
emission-line region galaxies, showing intrinsic differences in these
three AGN populations. A positive correlation between the black hole
accretion rate (BHAR) and the star formation rate (SFR) is found, but
no correlation between the specific SFR and the ratio BHAR/MBH,
simply reflecting the fact that the more massive a galaxy is, the more
it is forming stars and feeding its central black hole. The JWST, just
beginning operations, will allow large samples of AGN to be observed
in these lines in the nearby universe (z<0.9).
Description:
Our study is based on the 12um Seyfert galaxy sample (53 Seyfert 1s
and 63 Seyfert 2s) extracted from the Infrared Astronomical Satellite
(IRAS) 12um galaxy sample (Rush+ 1993ApJS...89....1R 1993ApJS...89....1R, VII/157).
The multifrequency observations that we use in our analysis include
the hard X-ray observations in the 2-10 and 14-195keV bands from
Ricci+ 2017, J/ApJS/233/17 and Oh+ 2018, J/ApJS/235/4 which include
the broadband X-ray (0.3-150keV) characteristics of the BAT-detected
AGN, obtained by combining XMM-Newton, Swift/XRT, ASCA, Chandra, and
Suzaku observations in the soft X-ray band, in addition to the
Swift-BAT AGN 70 month catalog (Baumgartner+, 2013, J/ApJS/207/19).
We also use the optical spectroscopy from Malkan+ (2017ApJ...846..102M 2017ApJ...846..102M)
and the 12um nuclear fluxes from Asmus+ 2014, J/MNRAS/439/1648, as
well as the Spitzer spectroscopic data Tommasin+ (2008ApJ...676..836T 2008ApJ...676..836T);
Wu+ (2009ApJ...701..658W 2009ApJ...701..658W); Gallimore+ (2010ApJS..187..172G 2010ApJS..187..172G);
Tommasin+ 2010, J/ApJ/709/1257 and the Herschel PACS spectra
Fernandez-Ontiveros+ 2016, J/ApJS/226/19.
File Summary:
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FileName Lrecl Records Explanations
--------------------------------------------------------------------------------
ReadMe 80 . This file
table1.dat 101 117 The AGN sample: names, coordinates, redshift, types
table2.dat 100 117 X-ray properties of the AGN sample: SWIFT
identifiers, X-ray fluxes and luminosities
table3.dat 60 21 Observed and absorption corrected 2-10keV fluxes
and luminosities for Compton thick objects
table4.dat 116 117 Observed properties of the local galaxy sample:
AGN types, IR lines and continuum fluxes
table5.dat 86 117 Observed properties of the local galaxy sample:
AGN types, K-band fluxes, galaxy and BH masses and
bolometric luminosities
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See also:
VII/157 : The Extended 12um galaxy sample (Rush+ 1993)
J/ApJ/453/616 : JHKL photometry of 12 micron galaxy sample (Spinoglio+ 1995)
J/ApJS/112/315 : Spectroscopic parameters of Seyfert nuclei (Ho+ 1997)
J/ApJS/121/473 : A diagnostic diagram for Seyfert 2 Galaxies (Bassani+, 1999)
J/ApJS/161/185 : GIS catalog project : source catalog II (Ueda+, 2005)
J/ApJ/648/111 : Chandra sources near AGNs (Levenson+, 2006)
J/ApJ/679/140 : IR measurement of quasar obscuration (Treister+, 2008)
J/A+A/524/A64 : The 54-month Palermo BAT-survey catalogue (Cusumano+, 2010)
J/ApJ/709/1257 : Spitzer-IRS sp. of Seyfert galaxies. II. (Tommasin+, 2010)
J/MNRAS/413/1206 : XMM survey of 12um selected galaxies (Brightman+, 2011)
J/ApJ/728/58 : Swift-BAT survey of AGNs (Burlon+, 2011)
J/A+A/533/A119 : GOODS-Herschel North and South catalogs (Elbaz+, 2011)
J/ApJS/207/19 : Swift-BAT 2004-2010 hard X-ray survey (Baumgartner+, 2013)
J/MNRAS/439/1648 : Subarcsecond mid-infrared atlas of local AGN (Asmus+, 2014)
J/ApJ/788/45 : Luminosity and redshift of gal. from WISE/SDSS (Toba+, 2014)
J/MNRAS/454/766 : Mid-infrared-X-ray correlation for local AGNs (Asmus+, 2015)
J/ApJ/815/L13 : Compton-thick AGNs from 70-mth Swift/BAT cat. (Ricci+, 2015)
J/ApJS/226/19 : FIR sp. of AGN from Herschel (Fernandez-Ontiveros+, 2016)
J/ApJ/835/74 : IR phot. of AGNs in Swift/BAT 70-month (Ichikawa+, 2017)
J/ApJS/233/17 : Swift/BAT AGN spectroscopic survey. V. X-ray (Ricci+, 2017)
J/MNRAS/475/788 : GAMA blue spheroids within 87 Mpc (Mahajan+, 2018)
J/ApJS/235/4 : The 105-mth Swift-BAT all-sky hard X-ray survey (Oh+, 2018)
J/ApJ/876/102 : Reverberation mapping of the Seyfert Zw I 1 (Huang+, 2019)
J/ApJ/870/31 : BAT AGN spectroscopic survey. XI. IR phot. (Ichikawa+, 2019)
J/ApJ/884/136 : PAH features of star-forming gal. using Spitzer (Xie+, 2019)
J/ApJ/876/49 : 10yr reverberation mapping campaign for 3C273 (Zhang+, 2019)
J/MNRAS/504/5726 : IR lines of AGNs accretion disk (Fernandez-Ontiveros+, 2021)
Byte-by-byte Description of file: table1.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 3 I3 -- Seq [1/117] Sequential Catalog number
5- 19 A15 --- Name Galaxy Name used in other tables
21- 45 A25 --- NEDName NED preferred name
47- 48 I2 h RAh Hour of Right Ascension (J2000)
50- 51 I2 min RAm Minute of Right Ascension (J2000)
53- 56 F4.1 s RAs Second of Right Ascension (J2000)
58- 58 A1 -- DE- Sign of the Declination (J2000)
59- 60 I2 deg DEd Degree of Declination (J2000)
62- 63 I2 arcmin DEm Arcminute of Declination (J2000)
65- 66 I2 arcsec DEs Arcsecond of Declination (J2000)
68- 75 F8.5 --- z [-0.00013/0.2] Redshift from NED
77- 83 A7 --- Type AGN Classification
85-101 A17 --- OName Other Name(s)
--------------------------------------------------------------------------------
Byte-by-byte Description of file: table2.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
2- 4 I3 --- Seq [1/117] Sequential catalog number
6- 20 A15 --- Name Galaxy Name used in other tables
22- 28 A7 --- Type AGN classification
30- 30 A1 --- l_logNH Limit flag on logNH
32- 36 F5.2 [cm-2] logNH [19.7/25.1]? Log of Hydrogen
column density
38- 38 A1 --- CT Compton thick flag
40- 51 A12 --- SWIFT SWIFT name (JHHMM.m+DDMM)
53- 53 A1 --- r_Name Reference of SWIFT name (1)
55- 55 A1 --- l_F2-10keV Limit flag on F2-10keV
56- 63 F8.3 10-15W/m2 F2-10keV [0.005/1068]? Intrinsic 2-10keV
X-ray flux in 10-12erg/s/cm2
65- 70 F6.2 10-15W/m2 F14-195keV [4.0/619]? Observed 14-195keV
X-ray flux in 10-12erg/s/cm2
from Oh+ 2018, J/ApJS/235/4
72- 72 A1 --- l_logL2-10keV Limit flag on logL2-10keV
74- 78 F5.2 [10-7W] logL2-10keV [37.9/45.8]? Log of intrinsic
2-10keV X-ray luminosity
80- 84 F5.2 [10-7W] logL14-195keV [38.6/46.4]? Log of observed
14-195keV X-ray luminosity in erg/s
86- 90 F5.2 [10-7W] logLBol(X) [41.17/46.21]? Log of bolometric
luminosity (from 2-10keV)
92-100 A9 --- Ref References and notes (2)
--------------------------------------------------------------------------------
Note (1): SWIFT name from Ricci+ 2017, J/ApJS/233/17; or from
Cusumano+ 2010, J/A+A/524/A64 if flagged.
Note (2): References for the X-ray observations and hydrogen column
densities, no X: means that no x-rays observations are available.
Flag as follows:
1 = Ichikawa+ (2019ApJ...870..31I), J/ApJ/870/31
2 = Ghosh & Soundararajaperumal (1992MNRAS.259..175G 1992MNRAS.259..175G)
3 = Ricci et al. 2017, J/ApJS/233/17
4 = Brightman & Nandra. 2011 J/MNRAS/413/1206
5 = Brightman & Nandra (2008MNRAS.390.1241B 2008MNRAS.390.1241B)
6 = Bassani et al. 1999, J/ApJS/121/473
7 = Grupe, Mathur & Komossa (2004AJ...127..3161G 2004AJ...127..3161G)
8 = Akylas & Georgantopoulos (2009A&A...500..999A 2009A&A...500..999A)
9 = Cusumano et al. 2010, J/A+A/524/A64
10 = Risaliti et al. (2000A&A...357...13R 2000A&A...357...13R)
11 = Risaliti, Maiolino & Salvati (1999ApJ...522..157R 1999ApJ...522..157R)
12 = Guainazzi, Matt & Perola (2005A&A...444..119G 2005A&A...444..119G)
13 = Strickland (2007MNRAS.376..523S 2007MNRAS.376..523S)
14 = Gonzalez-Martin+ (2009A&A...506.1107G 2009A&A...506.1107G)
15 = Winter+ (2008ApJ...674..686W 2008ApJ...674..686W)
16 = Lee+ (2013MNRAS.430.2650L 2013MNRAS.430.2650L)
17 = Lutz et al. 2004, J/A+A/418/465
18 = Deluit & Courvoisier (2003A&A...399...77D 2003A&A...399...77D)
19 = Cusumano et al. 2010, J/A+A/524/A64
20 = Tan+ (2012ApJ...747L..11T 2012ApJ...747L..11T)
21 = Iyomoto+ (1996PASJ...48..231I 1996PASJ...48..231I)
22 = Polletta et al. 1996, J/ApJS/106/399
23 = Iwasawa+ (2011A&A...529A.106I 2011A&A...529A.106I)
24 = Liu+ (2014ApJ...783..106L 2014ApJ...783..106L)
25 = Singh, Shastri & Risaliti (2011A&A...532A..84S 2011A&A...532A..84S)
26 = Ueda et al. 2001, J/ApJS/133/1
27 = Bianchi et al. 2009, J/A+A/495/421
28 = Ueda et al. 2005, J/ApJS/161/185
29 = Bianchi+ (2008MNRAS.386..105B 2008MNRAS.386..105B)
30 = Teng+ (2009ApJ...691..261T 2009ApJ...691..261T)
31 = Shu, Liu & Wang (2010ApJ...722...96S 2010ApJ...722...96S)
32 = Bianchi+ (2005A&A...442..185B 2005A&A...442..185B)
33 = Bi, Feng & Ho 2020, J/ApJ/900/124
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Byte-by-byte Description of file: table3.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 3 I3 --- Seq [9/116] Sequential catalog number
5- 19 A15 --- Name Galaxy name used in other tables
21- 23 A3 --- OType AGN classification
25- 25 A1 --- l_logNH Limit flag on logNH
27- 31 F5.2 [cm-2] logNH [23.55/25.1] Log of the Hydrogen
intrinsic absorption column density
33- 36 F4.2 10-15W/m2 FX(OBS) [0.08/4.9] Observed 2-10keV flux in
10-12erg/s/cm2
38- 43 F6.2 10-15W/m2 FX(COR) [4.6/120] Absorption corrected
2-10keV flux, 10-12erg/s/cm2
45- 49 F5.2 [10-7W] logLX(OBS) [39.28/42.07] Log of the observed
2-10keV luminosity, erg/s
51- 55 F5.2 [10-7W] logLX(COR) [40.2/43.69] Log of the absorption
corrected 2-10keV luminosity, erg/s
57- 60 A4 --- Ref References (1)
--------------------------------------------------------------------------------
Note (1): Flag as follows:
1 = observed and corrected 2-10keV fluxes and luminosities from
extrapolated 14-150keV data by Ricci+ 2017, J/ApJS/233/17
2 = Guainazzi+ 2005A&A...444..119G 2005A&A...444..119G
3 = observed 2-10keV fluxes and luminosities from
LaMassa+ 2011ApJ...729...52L 2011ApJ...729...52L
4 = Ueda et al. 2005, J/ApJS/161/185
5 = Brightman & Nandra 2011, J/MNRAS/413/1206
6 = Yamada+ 2020ApJ...897..107Y 2020ApJ...897..107Y
7 = Levenson et al. 2006, J/ApJ/648/111
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Byte-by-byte Description of file: table4.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 3 I3 --- Seq [1/117] Sequential Catalog number
5- 19 A15 --- Name Galaxy Name used in other tables
21- 28 F8.5 --- z [-0.00013/0.2] Redshift from NED
30- 36 A7 --- Type AGN Classification
38- 38 A1 --- l_F[NeII] Limit flag for F[NeII]
40- 45 F6.2 10-17W/m2 F[NeII] [0.2/520]? Flux of [NeII]12.8um (1)
47- 47 A1 --- l_F[NeV]1 Limit flag for F[NeV]1
49- 55 F7.2 10-17W/m2 F[NeV]1 [0.38/1110]? Flux of [NeV]14.3um (1)
57- 63 F7.2 10-17W/m2 F[NeIII] [0.6/2100]? Flux of [NeIII]15.5um (1)
65- 65 A1 --- l_F[NeV]2 Limit flag for F[NeV]2
67- 72 F6.2 10-17W/m2 F[NeV]2 [0/800]? Flux of [NeV] 24.3um (1)
74- 74 A1 --- l_F[OIV] Limit flag for F[OIV]
76- 82 F7.2 10-17W/m2 F[OIV] [0.6/2200]? Flux of [OIV]25.9um (1)
84- 84 A1 --- l_F(PAH11.3) Limit flag for F(PAH11.3)
86- 91 F6.1 10-17W/m2 F(PAH11.3) [4.5/1200]? Flux of PAH11.3um (2)
93- 99 F7.2 10-17W/m2 F[CII] [1.6/1361]? Flux of [CII]158um (3)
101-107 F7.2 10-17W/m2 F[OIII]5007 [0.16/1630]? Flux of [OIII]5007Å (4)
109-109 A1 --- l_F12um Limit flag for F12um
110-116 F7.1 mJy F12um [3.7/10206]? Nuclear Flux at 12um (5)
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Note (1): The IR line fluxes have been taken from
Tommasin+ 2008ApJ...676..836T 2008ApJ...676..836T and Tommasin+ 2010, J/ApJ/709/1257
Note (2): PAH11.3um flux from Wu+ 2009ApJ...701..658W 2009ApJ...701..658W, where available,
otherwise from Tommasin+ 2008ApJ...676..836T 2008ApJ...676..836T and
Tommasin+ 2010, J/ApJ/709/1257
Note (3): [CII]158um flux from Fernandez-Ontiveros et al. 2016, J/ApJS/226/19
Note (4): [OIII]5007Å flux from Malkan+ 2017ApJ...846..102M 2017ApJ...846..102M
Note (5): Nuclear 12um flux from Asmus+ 2014, J/MNRAS/439/1648
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Byte-by-byte Description of file: table5.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 3 I3 --- Seq [1/117] Sequential Catalog number
5- 19 A15 --- Name Galaxy Name used in other tables
22- 29 F8.5 --- z [-0.00013/0.2] Redshift from NED
31- 37 A7 --- Type AGN Classification
39- 46 A8 Jy F(K)GAL Galaxy K band flux density
48- 55 A8 Jy F(K)TOT Total K band flux density
57- 64 A8 Jy F(K)NUC Nuclear K band flux density
66- 70 F5.2 [Msun] logMgal [8.5/11.3]? Log of galaxy mass
in solar units
72- 72 A1 --- r_logMgal Reference for logMgal (1)
74- 78 F5.2 [10-7W] logLBol(IR) [41.28/46]? Log of bolometric
luminosity (2)
80- 83 F4.2 [Msun] logMBH [5.8/9]? Log of black hole mass (3)
86- 86 A1 --- r_logMBH Reference for logMBH (1)
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Note (1): Flag as follows:
1 = Galaxy mass estimated from HST observations of Kim+ 2017ApJS...232..21K 2017ApJS...232..21K
2 = Galaxy mass estimated from Zhang+ 2019, J/ApJ/876/49
3 = Black hole mass estimated from Huang+ 2019, J/ApJ/876/102
4 = Black hole mass estimated from Kim+ 2017ApJS...232..21K 2017ApJS...232..21K
5 = Black hole mass estimated from Lee+ 2013MNRAS.430.2650L 2013MNRAS.430.2650L
Note (2): Bolometric luminosity from Mordini+ 2021A&A...653A..36M 2021A&A...653A..36M and
bolometric correction of Lusso+ 2012MNRAS.425..623L 2012MNRAS.425..623L
Note (3): Unless otherwise noted in r_logMBH, the black hole mass is from
Fernandez-Ontiveros & Munoz-Darias 2021, J/MNRAS/504/5726
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History:
From electronic version of the journal
(End) Prepared by [AAS], Katia van der Woerd [CDS] 20-Jan-2025