Spectral Energy Distributions of Hard X-Ray Selected Active Galactic Nuclei in the XMM-Newton Medium Deep Survey

By M. Polletta, M. Tajer, L. Maraschi, G. Trinchieri, C. Lonsdale, L. Chiappetti, S. Andreon, M. Pierre, O. Fèvre, G. Zamorani and 11 more. 2007

606 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/920e26e14abbb1d49abc36d18c108823a60145f9

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1. D. M. Alexander
2. P. Hopkins
3. L. Hernquist
4. P. V. van Dokkum
5. R. Somerville
6. C. Conroy
7. R. Dav'e
8. M. Franx

Citations in the corpus

• The Herschel* PEP/HerMES luminosity function - I. Probing the evolution of PACS selected Galaxies to z ≃ 4 (2013, methodology): “…to derive the SEDs of our PEP sources, which we interpreted and classified by performing a χ2 fit (using the Le Phare code2; Arnouts et al. 2002 and Ilbert et al. 2006) with the semi-empirical template library of Polletta et al. (2007), representative of different classes of IR galaxies and AGN.”
• Unveiling Obscured Accretion in the Chandra Deep Field-South (2007, methodology): “Comparing the global observed Spectral Energy Distribution (SED) to AGN and galaxy templates proved to be more efficient in selecting AGN samples (Polletta et al. 2006, 2007).”
• The WIRCam Deep Survey I. Counts, colours, and mass-functions derived from near-infrared imaging in the CFHTLS deep fields (2011, methodology): “As in Ilbert et al. (2009), we use a combination of the Polletta et al. (2007) templates with the additional templates generated by Ilbert et al. (2009) to account for starbursts with ages of 0.3 to 3 Gyr.”
• Fitting the integrated spectral energy distributions of galaxies (2010, methodology): “Polletta et al. (2007) published a set templates that combine the SEDs of galaxies with those of AGN and thus fill an important hole in many SED fitting template sets.2 The library contains 20 templates including 1 elliptical, 7 spirals, 3 starbursts, 6 AGNs, and 3 composite (starburst + AGN)…”
• CHARACTERIZING THE MID-INFRARED EXTRAGALACTIC SKY WITH WISE AND SDSS (2012, methodology): “Figure 10 shows the W1 − W2 and W2 − W3 color tracks as a function of redshift calculated using the set of SED templates of Assef et al. (2010), the Arp 220 SED template of Polletta et al. (2007) and the IRAS15250+3609 template of Vega et al. (2008).”
• PHAT: PHoto-z Accuracy Testing (2010, methodology): “The 9 galaxy templates of Polletta et al. (2007) include 3 SEDs of elliptical galaxies and 6 templates of spiral galaxies (S0, Sa, Sb, Sc, Sd, Sdm).”
• Cosmic X-ray surveys of distant active galaxies (2015, background): “…a broad variety of star-formation indicators, including optical spectroscopy, MIR data, and submillimeter (submm) observations (e.g., Alexander et al 2005b; Polletta et al 2007; Silverman et al 2009b; Trichas et al 2009; Mullaney et al 2010; Lutz et al 2010; Xue et al 2010; Rafferty et al 2011).”
• AN ATLAS OF GALAXY SPECTRAL ENERGY DISTRIBUTIONS FROM THE ULTRAVIOLET TO THE MID-INFRARED (2013, methodology): “We compare the performance of our templates with those from Coleman et al. (1980), Kinney et al. (1996) and Polletta et al. (2007), which have been used by a large variety of K-correction and photometric redshift codes over the past two decades (e.g., Fernández-Soto et al. 1999; Beńıtez 2000;…”
• The Star Formation Rate Density and Dust Attenuation Evolution over 12 Gyr with the VVDS Surveys (2011, methodology): “For this purpose, we computed them again using different template sets, like PEGASE.2 templates (Fioc & Rocca-Volmerange 1997) or a mixed set with Bruzual & Charlot (2003) and Polletta et al. (2007) templates, as used in Ilbert et al. (2009).”
• A HIGHLY CONSISTENT FRAMEWORK FOR THE EVOLUTION OF THE STAR-FORMING “MAIN SEQUENCE” FROM z ∼ 0–6 (2014, neutral): “…compilation presented here13 are taken from Fioc & Rocca-Volmerange (1997, 1999) (PEGASE.2), Bruzual & Charlot (2003) (BC03), Maraston (2005) (M05), Charlot & Bruzual (2007, 2011) (CB07, CB11)14, Polletta et al. (2007) (P07), Rowan-Robinson et al. (2008) (R08), and Gruppioni et al. (2010) (G10).”
• The VISTA deep extragalactic observations (VIDEO) survey (2012, methodology): “The AGN templates are those used and described in detail in Polletta et al. (2007), the library consists of empirically determined spectra for three Type 1 AGNs, five Type 2 AGNs and two composite AGNs and starburst galaxies.”
• THE COSMOS-WIRCam NEAR-INFRARED IMAGING SURVEY. I. BzK-SELECTED PASSIVE AND STAR-FORMING GALAXY CANDIDATES AT z ≳ 1.4 (2009, methodology): “A set of templates generated by Polletta et al. (2007) using the GRASIL code Silva et al. (1998) are used .”
• The mean star formation rate of X-ray selected active galaxies and its evolution from z~2.5: results from PEP-Herschel (2012, methodology): “For the SF templates, we consider the five basis SEDs from Mullaney et al. (2011) and add an M82like and Arp220-like SED from the SWIRE template library 2 available from http://sites.google.com/site/decompir/ (Polletta et al. 2007) to incorporate strongly star-bursting and ULIRG-like systems.”
• Defining the intrinsic AGN infrared spectral energy distribution and measuring its contribution to the infrared output of composite galaxies (2011, methodology): “…rely on either observed AGN SEDs that likely include considerable amounts of host-galaxy contamin tion at infrared wavelengths or predictions from radiative transfer models which are often poorly constrained (e.g. Polletta et al.2007; Fiore et al. 2008, 2009; Pozzi et al. 2010; Hatziminaoglou etal.”
• THE NEXT GENERATION ATLAS OF QUASAR SPECTRAL ENERGY DISTRIBUTIONS FROM RADIO TO X-RAYS (2011, background): “Other investigations of SEDs have focused on subclasses, like broad absorption line (BAL) quasars (e.g., Gallagher et al. 2007), 2MASS red quasars (Kuraszkiewicz et al. 2009), hard X-ray selected quasars (Polletta et al. 2000, 2007), or on individual objects (e.g., Zheng et al. 2001).”
• Panchromatic spectral energy distributions of Herschel sources (2013, methodology): “8 show the same color-redshift tracks for the Polletta et al. (2007) template set.”
• A CENSUS OF STAR-FORMING GALAXIES IN THE Z ∼ 9–10 UNIVERSE BASED ON HST+SPITZER OBSERVATIONS OVER 19 CLASH CLUSTERS: THREE CANDIDATE Z ∼ 9–10 GALAXIES AND IMPROVED CONSTRAINTS ON THE STAR FORMATION RATE DENSITY AT Z ∼ 9.2 (2012, methodology): “…PHARE were the same ones as optimized for the COSMOS survey (Scoville et al. 2007) and included three elliptical and six spiral SEDs as generated by Polletta et al. (2007) using the GRASIL code (Silva et al. 1998) as well as 12 starburst galaxies ranging in age from 30 Myr to 3 Gyr using the…”