Environmental clustering properties of high-energy blazars

Kyle Willett, Thomas Nelson, Lucy F Fortson

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Abstract

The intrinsic properties of the host galaxies of blazars are often unable to be measured due to the high brightness and relativistic beaming of the jet itself. This makes it difficult to determine, for example, whether there is a difference in the parent populations of BL Lacs versus those of flat-spectrum radio quasars (FSRQs). As an alternative to direct observation of the host galaxy, we study the Mpc-scale environments using data from the Sloan Digital Sky Survey. Our study of 757 blazars at 0.05<z<0.75 shows a significant increase in local density over field galaxies. There is no measurable difference, however, between the clustering amplitude of BL Lacs and FSRQs. Similar clustering amplitudes are found for a large sample of powerful radio galaxies. As a result, this data does not rule out a unification model in which BL Lacs and FSRQs are beamed versions of FRI and FRII radio galaxies, respectively. Within the context of the blazar sequence/envelopemodel, our results suggest that the radiative efficiency of accretion, on which the observed properties of jet emission depend, is not affected by the local galactic environment.

Original languageEnglish (US)
Title of host publicationHigh Energy Gamma-Ray Astronomy - 5th International Meeting on High Energy Gamma-Ray Astronomy
Pages558-561
Number of pages4
DOIs
StatePublished - Dec 1 2012
Event5th International Meeting on High Energy Gamma-Ray Astronomy - Heidelberg, Germany
Duration: Jul 9 2012Jul 13 2012

Publication series

NameAIP Conference Proceedings
Volume1505
ISSN (Print)0094-243X
ISSN (Electronic)1551-7616

Other

Other5th International Meeting on High Energy Gamma-Ray Astronomy
CountryGermany
CityHeidelberg
Period7/9/127/13/12

Keywords

  • Blazars
  • Spatial clustering

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