J/ApJS/253/46       Optical spectroscopy of Fermi blazars       (Paliya+, 2021)

The central engines of Fermi blazars. Paliya V.S., Dominguez A., Ajello M., Olmo-Garcia A., Hartmann D. <Astrophys. J. Suppl. Ser., 253, 46 (2021)> =2021ApJS..253...46P 2021ApJS..253...46P
ADC_Keywords: BL Lac objects; Spectra, optical; Redshifts; Gamma rays; Velocity dispersion; Black holes Keywords: BL Lacertae objects ; Black holes ; Blazars ; Radio loud quasars ; Supermassive black holes ; Spectral line identification Abstract: We present a catalog of central engine properties, i.e., black hole mass (MBH) and accretion luminosity (Ldisk), for a sample of 1077 blazars detected with the Fermi Large Area Telescope. This includes broad emission-line systems and blazars whose optical spectra lack emission lines but are dominated by the absorption features arising from the host galaxy. The average MBH for the sample is <logMBH,allM☉_≥8.60, and there is evidence suggesting the association of more massive black holes with absorption-line systems. Our results indicate a bimodality of Ldisk in Eddington units (Ldisk/LEdd) with broad-line objects tend to have a higher accretion rate (Ldisk/LEdd>0.01). We have found that Ldisk/LEdd and Compton dominance (CD; the ratio of the inverse Compton to synchrotron peak luminosities) are positively correlated at the >5σ confidence level, suggesting that the latter can be used to reveal the state of accretion in blazars. Based on this result, we propose a CD-based classification scheme. Sources with CD>1 can be classified as high-Compton-dominated or HCD blazars, whereas those with CD≲1 are low-Compton-dominated (LCD) objects. This scheme is analogous to that based on the mass accretion rate proposed in the literature; however, it overcomes the limitation imposed by the difficulty in measuring Ldisk and MBH for objects with quasi-featureless spectra. We conclude that the overall physical properties of Fermi blazars are likely to be controlled by the accretion rate in Eddington units. Description: A good fraction of the 1077 γ-ray-detected blazars in our sample have optical spectrum taken from the SDSS-DR16; however, we do not use the emission-/absorption-line measurements obtained with the automatic SDSS data reduction pipeline. During the data analysis, every optical spectrum was individually analyzed rather than by running any automatic pipeline. See Section 3. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table2.dat 41 54 The spectral parameters associated with the Hα emission line table3.dat 55 173 The spectral parameters associated with the Hβ emission line table4.dat 54 492 The spectral parameters associated with the MgII emission line table5.dat 55 193 The spectral parameters associated with the CIV emission line table6.dat 38 346 The stellar velocity dispersion and line luminosity upper limit measurements for 346 blazars table7.dat 67 684 The central engine and SED properties of emission line blazars table8.dat 67 346 The central engine and SED properties of absorption line blazars table10.dat 91 1077 References used in this work -------------------------------------------------------------------------------- See also: III/175 : Optical spectroscopy of radio sources (Stickel+, 1989-94) VIII/34 : Parkes Half-Jansky Flat-Spectrum Sample (Drinkwater + 1997) VII/250 : The 2dF Galaxy Redshift Survey (2dFGRS) (2dFGRS Team, 1998-2003) VII/259 : 6dF galaxy survey final redshift release (Jones+, 2009) IX/67 : Incremental Fermi LAT 4th cat. 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(Landt+, 2001) J/ApJS/140/143 : HST FOS spectral atlas (Bechtold+, 2002) J/ApJS/145/199 : Optical sp. atlas of low-redshift AGN (Marziani+, 2003) J/ApJ/590/109 : Gamma-ray blazar in northern sky (Sowards-Emmerd+, 2003) J/ApJ/609/564 : Blazar counterparts for 3EG sources (Sowards-Emmerd+, 2004) J/MNRAS/371/703 : MILES library of empirical spectra (Sanchez-Blazquez+, 2006) J/A+A/470/787 : High energy peaked BL Lacs optical sp. (Piranomonte+, 2007) J/ApJS/175/97 : CGRaBS: γ-ray blazar candidates (Healey+, 2008) J/A+A/488/867 : Synchrotron peak frequency of 135 AGN (Nieppola+, 2008) J/ApJS/180/67 : Phot. selection of quasars from SDSS. II. (Richards+, 2009) J/MNRAS/404/1639 : MILES base models & new line index system (Vazdekis+, 2010) J/ApJ/740/98 : Synchroton peak for blazars & radio galaxies (Meyer+, 2011) J/ApJS/194/45 : QSO properties from SDSS-DR7 (Shen+, 2011) J/ApJ/748/49 : Opt. spectroscopy of 1LAC broad-line blazars (Shaw+, 2012) J/other/RMxAA/48.9 : Optical sp. atlas of MOJAVE AGNs (Torrealba+, 2012) J/ApJ/767/14 : MASIV survey III. Optical identifications (Pursimo+, 2013) J/ApJ/764/135 : Spectroscopic redshifts of BL Lac objects (Shaw+, 2013) J/AJ/146/10 : Sp. of 120 emission-line ICRF2 candidates (Titov+, 2013) J/ApJ/780/73 : Redshifts of BL Lac objects from Fermi (Ajello+, 2014) J/other/Nat/515.376 : Power of relativistic jets in blazars (Ghisellini+, 2014) J/MNRAS/451/4193 : Fermi/non-Fermi blazars jet power & accretion (Chen+, 2015) J/A+A/591/A21 : Optical flux behaviour of Fermi blazars (Marchesini+, 2016) J/MNRAS/460/3202 : Radio-loud AGNs (Olguin-Iglesias+, 2016) J/ApJ/835/L38 : Fermi blazars with Doppler factors (Fan+, 2017) J/ApJ/850/74 : Swift/BAT AGN Spectroscopic Survey. I. (Koss+, 2017) J/ApJ/851/33 : Multi-wavelength analysis of CGRaBS blazars (Paliya+, 2017) J/AJ/153/157 : Cand. ICRF flat-spectrum radio sources. III. (Titov+, 2017) J/A+A/615/A167 : Catalog of NLS1s galaxies in 6dFGS survey (Chen+, 2018) J/ApJ/861/130 : BL Lac objects GTC low resolution sp. (Landoni+, 2018) J/ApJ/881/154 : BAT AGN spectroscopic survey. XVI. Blazars (Paliya+, 2019) J/ApJS/247/33 : Fermi LAT fourth source catalog (4FGL) (Abdollahi+, 2020) J/A+A/643/A103 : Fermi-LAT low-energy counterparts (Pena-Herazo+, 2020) J/ApJ/914/42 : Radio data of 4FGL-DR2 unassoc. sources (Bruzewski+, 2021) http://fermi.gsfc.nasa.gov/ssc/data/access/lat/10yr_catalog/ : 4FGL-DR2 Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 12 A12 --- 4FGL 4FGL-DR2 catalog identifier 14- 18 F5.3 --- z [0.027/0.55] Spectroscopic redshift 20- 23 I4 km/s FWHM [1384/8991] Full-Width at Half-Maximum of Hα 25- 28 I4 km/s e_FWHM [52/5494] Uncertainty in FWHM 30- 35 F6.3 [10-7W] logLHa [40.89/44.41] log Hα luminosity in erg/s 37- 41 F5.3 [10-7W] e_logLHa [0.004/0.4] Uncertainty in logLHa -------------------------------------------------------------------------------- Byte-by-byte Description of file: table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 12 A12 --- 4FGL 4FGL-DR2 catalog identifier 14- 18 F5.3 --- z [0.048/1.52] Spectroscopic redshift 20- 25 F6.3 [10-7W] logL5100 [42.97/47.42] log 5100Å continuum luminosity (1) 27- 31 F5.3 [10-7W] e_logL5100 [0.001/0.3] Uncertainty in logL5100 (1) 33- 37 I5 km/s FWHM [1200/12528] Full-Width at Half-Maximum of Hβ 39- 42 I4 km/s e_FWHM [0/4699] Uncertainty in FWHM 44- 49 F6.3 [10-7W] logLHb [40.79/44.56] log Hβ luminosity (1) 51- 55 F5.3 [10-7W] e_logLHb [0.003/0.4] Uncertainty in logLHb (1) -------------------------------------------------------------------------------- Note (1): In units of erg/s. -------------------------------------------------------------------------------- Byte-by-byte Description of file: table4.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 12 A12 --- 4FGL 4FGL-DR2 catalog identifier 14- 18 F5.3 --- z [0.29/2.37] Spectroscopic redshift 20- 25 F6.3 [10-7W] logL3000 [42.55/46.9] log 3000Å continuum luminosity (1) 27- 31 F5.3 [10-7W] e_logL3000 [0.001/0.04] Uncertainty in logL3000 (1) 33- 36 I4 km/s FWHM [1367/8372] Full-Width at Half-Maximum of MgII 38- 41 I4 km/s e_FWHM [41/5074] Uncertainty in FWHM 43- 48 F6.3 [10-7W] logLMgII [40.97/44.8] log MgII luminosity (1) 50- 54 F5.3 [10-7W] e_logLMgII [0.003/0.42] Uncertainty in logLMgII -------------------------------------------------------------------------------- Note (1): In units of erg/s. -------------------------------------------------------------------------------- Byte-by-byte Description of file: table5.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 12 A12 --- 4FGL 4FGL-DR2 catalog identifier 14- 18 F5.3 --- z [0.21/4.32] Spectroscopic redshift 20- 25 F6.3 [10-7W] logL1350 [43.89/47.72] log 1350Å continuum luminosity (1) 27- 31 F5.3 [10-7W] e_logL1350 [0/0.14] Uncertainty in logL1350 (1) 33- 37 I5 km/s FWHM [1204/13253] Full-Width at Half-Maximum of CIV 39- 42 I4 km/s e_FWHM [43/6544] Uncertainty in FWHM 44- 49 F6.3 [10-7W] logLCIV [42.63/45.48] log CIV luminosity (1) 51- 55 F5.3 [10-7W] e_logLCIV [0.004/0.31] Uncertainty in logLCIV (1) -------------------------------------------------------------------------------- Note (1): In units of erg/s. -------------------------------------------------------------------------------- Byte-by-byte Description of file: table6.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 12 A12 --- 4FGL 4FGL-DR2 catalog identifier 14- 18 F5.3 --- z [0.024/0.85] Spectroscopic redshift 20- 25 F6.2 km/s sigma [123/586] Stellar velocity dispersion 27- 32 F6.2 km/s e_sigma [1.3/113] Uncertainty in sigma 34- 38 F5.2 [10-7W] logLUp [0/42.65] Upper 3σ limit in log line luminosity in erg/s (1) -------------------------------------------------------------------------------- Note (1): For the Hβ line except for sources 4FGL J0006.4+0135, 4FGL J0204.0-3334, and 4FGL J1146.0-0638, for which we quote the MgII line luminosity upper limit. -------------------------------------------------------------------------------- Byte-by-byte Description of file: table[78].dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 12 A12 --- 4FGL 4FGL-DR2 catalog identifier 14- 18 F5.2 [Msun] logMBH [6.3/10.2] log central black hole mass 20- 23 F4.2 [Msun] e_logMBH [0/0.9] Uncertainty in log MBH 25- 29 F5.2 [10-7W] logLd [0/47.5] log accretion disk luminosity in erg/s units 31- 34 F4.2 [10-7W] e_logLd [0/0.5]? Uncertainty in logLd (only for Table 7) 36- 40 F5.2 [Hz] lognuSyn [11.3/19.4] log synchrotron peak frequency 42- 47 F6.2 [mW/m2] lognuFSyn [-13/-9.7] log synchrotron peak flux in erg/s/cm2 units 49- 53 F5.2 [Hz] lognuIC [19.6/26] log inverse Compton peak frequency 55- 60 F6.2 [mW/m2] lognuFIC [-13.3/-9.3] log inverse Compton peak flux in erg/s/cm2 units 62- 67 F6.2 --- CD [0.04/118] Compton Dominance -------------------------------------------------------------------------------- Byte-by-byte Description of file: table10.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 12 A12 --- 4FGL 4FGL-DR2 catalog identifier 15- 40 A26 --- Auth First author's name of the reference 49- 67 A19 --- BibCode Bibcode of the reference 69- 91 A23 --- Comm VizieR catalog reference; column added by CDS -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Prepared by [AAS], Emmanuelle Perret [CDS] 29-Jun-2021
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