J/ApJ/824/70    UV-FIR SED results of SDSS QSOs and their hosts    (Dong+, 2016)

Herschel observed stripe 82 quasars and their host galaxies: connections between AGN activity and host galaxy star formation. Dong X.Y., Wu X.-B. <Astrophys. J., 824, 70-70 (2016)> =2016ApJ...824...70D 2016ApJ...824...70D (SIMBAD/NED BibCode)
ADC_Keywords: Active gal. nuclei ; QSOs ; Redshifts ; Surveys ; Infrared sources Keywords: galaxies: active; galaxies: evolution; galaxies: starburst; galaxies: star formation; quasars: general; techniques: photometric Abstract: In this work, we present a study of 207 quasars selected from the Sloan Digital Sky Survey quasar catalogs and the Herschel Stripe 82 survey. Quasars within this sample are high-luminosity quasars with a mean bolometric luminosity of 1046.4erg/s. The redshift range of this sample is within z Herschel-SPIRE bands, the quasar sample is complete yet highly biased. Based on the multi-wavelength photometric observation data, we conducted a spectral energy distribution (SED) fitting through UV to FIR. Parameters such as active galactic nucleus (AGN) luminosity, far-IR (FIR) luminosity, stellar mass, as well as many other AGN and galaxy properties are deduced from the SED fitting results. The mean star formation rate (SFR) of the sample is 419M/yr and the mean gas mass is ∼1011.3M. All of these results point to an IR luminous quasar system. Compared with star formation main sequence (MS) galaxies, at least 80 out of 207 quasars are hosted by starburst galaxies. This supports the statement that luminous AGNs are more likely to be associated with major mergers. The SFR increases with the redshift up to z=2. It is correlated with the AGN bolometric luminosity, where LFIR∝LBol0.46±0.03. The AGN bolometric luminosity is also correlated with the host galaxy mass and gas mass. Yet the correlation between LFIR and LBol has higher significant level, implies that the link between AGN accretion and the SFR is more primal. The MBH/M* ratio of our sample is 0.02, higher than the value 0.005 in the local universe. It might indicate an evolutionary trend of the MBH/M* scaling relation. Description: SDSS Stripe 82 covers approximately 270deg2 area on the celestial equator in the south Galactic cap, spanning from 20h to 4h in RA and -1.25°∼1.25° in DEC. It has been repeatedly imaged by SDSS between 1998 and 2007. Besides the optical imaging survey and the spectroscopic survey, SDSS Stripe 82 has also been observed extensively by other surveys from X-ray through UV/optical to IR and radio bandpasses. Among these surveys, HerS (Viero+, 2014, J/ApJS/210/22), an imaging survey conducted by SPIRE on board the Herschel Space Observatory, covers about 79deg2 in area to an average depth of 13.0, 12.9, and 14.8mJy/beam (including a confusion limit of 7mJy) at 250, 350, and 500um, respectively. The quasar sample is selected by cross-identifying the HerS catalog with the Shen et al. (2011, J/ApJS/194/45) quasar catalog, the compiled catalog based on the spectroscopic quasar catalog (Schneider et al. 2010, VII/260) from SDSS Data Release 7 (Abazajian et al. 2009, II/294); and the SDSS quasar catalog from the tenth data release (Paris et al. 2014, VII/270). The search radius is 5 arcsec. See section 2 for further details. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 198 207 The SED fitting results -------------------------------------------------------------------------------- See also: II/319 : UKIDSS-DR9 LAS, GCS and DXS Surveys (Lawrence+ 2012) VII/270 : SDSS quasar catalog: tenth data release (Paris+, 2014) VII/260 : The SDSS-DR7 quasar catalog (Schneider+, 2010) II/294 : The SDSS Photometric Catalog, Release 7 (Adelman-McCarthy+, 2009) VII/233 : The 2MASS Extended sources (IPAC/UMass, 2003-2006) J/ApJ/811/58 : FIR properties of SDSS 0.1<z<5 quasars (Ma+, 2015) J/ApJS/219/18 : LIRAS: LoCuSS IR AGN survey (Xu+, 2015) J/ApJS/210/22 : Herschel Stripe 82 survey (HerS) first catalog (Viero+, 2014) J/MNRAS/434/3104 : QSOs SED shapes from optical to NIR (Hao+, 2013) J/A+A/533/A119 : GOODS-Herschel North and South catalogs (Elbaz+, 2011) J/ApJS/194/45 : QSO properties from SDSS-DR7 (Shen+, 2011) J/ApJ/708/137 : Broad-line AGNs in zCOSMOS survey (Merloni+, 2010) J/ApJ/699/800 : Mass functions of active black holes (Vestergaard+, 2009) J/ApJ/690/20 : Models of the AGN and black hole populations (Shankar+, 2009) J/ApJ/666/806 : SED of Spitzer quasars (QUEST) (Netzer+, 2007) J/ApJ/663/81 : SED of hard X-ray selected AGN in XMDS (Polletta+, 2007) J/ApJS/166/470 : SDSS-Spitzer type I QSOs IR photometry (Richards+, 2006) J/ApJS/95/1 : Atlas of Quasar Energy Distributions (Elvis+ 1994) http://www.sdss.org/ : SDSS home page Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 I3 --- Seq Running sequence number 5- 22 A18 --- SDSS Quasar designation (hhmmss.ss+ddmmss.s; J2000) 24- 32 F9.6 deg RAdeg Right ascension in decimal degrees (J2000), from HerS catalog 34- 45 F12.9 deg DEdeg Declination in decimal degrees (J2000), from HerS catalog 47- 52 F6.4 --- z [0.1/4.1] Redshift, from the SDSS DR7,DR10 54- 56 F3.1 --- fg Host galaxy fraction at 1um 58- 61 F4.2 --- e_fg Uncertainty in fg 63- 65 F3.1 mag Aint [0/0.5] The internal reddening Aint 67- 70 F4.2 mag e_Aint [0/0.3] Uncertainty in Aint 72- 75 A4 --- Morph Host galaxy morphological type; "E" (49 sources) or "Sb" (44 sources) 77- 78 I2 K Tcold [15/50] FIR cold dust temperature Tcold 80- 83 F4.1 K e_Tcold [0.6/17] Uncertainty in Tcold 85- 89 F5.2 --- alpha [-1/1.5] AGN power-law index at UV/optical, α 91- 94 F4.2 --- e_alpha [0/0.5] Uncertainty in alpha 96- 99 F4.1 [10-7W] LFIR [10.9/13.1] FIR luminosity integrated from 8um to 1000um Log(LFIR), erg/s 101-104 F4.2 [10-7W] e_LFIR [0.03/1.2] Uncertainty in Log(LFIR) 106-109 F4.1 [10-7W] LBol [44.5/48.4] Bolometric luminosity Log(LBol), in erg/s units 111-114 F4.2 [10-7W] e_LBol [0/1.1] Uncertainty in Log(LBol) 116-118 F3.1 [Msun/yr] SFR [1.1/3.3] SFR Log(SFR) 120-123 F4.2 [Msun/yr] e_SFR [0.03/1.2] Uncertainty in Log(SFR) 125-128 F4.1 [10-7W] L1300 [43.9/48] Monochromatic luminosity at 1300Å, Log(L1300), erg/s 130-133 F4.2 [10-7W] e_L1300 [0/1.3] Uncertainty in Log(L1300) 135-138 F4.1 [10-7W] L3000 [43.7/47.4] Monochromatic luminosity at 3000Å, Log(L3000), erg/s 140-143 F4.2 [10-7W] e_L3000 [0/1.3] Uncertainty in Log(L3000) 145-148 F4.1 [10-7W] L5100 [43.6/47.2] Monochromatic luminosity at 5100Å, Log(L5100), erg/s 150-153 F4.2 [10-7W] e_L5100 [0/1.3] Uncertainty in Log(L5100) 155-158 F4.1 [10-7W] L250um [43.1/45.7] Monochromatic luminosity at 250um, Log(L250um), erg/s 160-163 F4.2 [10-7W] e_L250um [0.02/1.7] Uncertainty in Log(L250um) 165-168 F4.1 [Msun] MBH [0/11] Black hole mass, Log(MBH) 170-173 F4.2 [Msun] e_MBH [0/1.1] Uncertainty in Log(MBH) 175-178 F4.1 [Msun] Mgas [9.8/12.4] Gas mass, Log(Mgas) 180-183 F4.2 [Msun] e_Mgas [0.03/1.2] Uncertainty in Log(Mgas) 185-188 F4.1 [Msun] Mstar [0/12.1] Host galaxy mass, Log(Mstar) 190-193 F4.2 [Msun] e_Mstar [0/0.4] Uncertainty in Log(Mstar) 195-198 A4 --- Cat SDSS quasar catalog ("DR7" or "DR10") -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Prepared by [AAS], Emmanuelle Perret [CDS] 16-Aug-2016
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