Swift BAT, Fermi LAT, and the Blazar Sequence
arXiv:0912.2721 · doi:10.1088/0004-637X/710/1/24
Abstract
Using public \fermi LAT and \swift BAT observations, we constructed the first sample of blazars selected at both hard X-rays and gamma-rays. Studying its spectral properties, we find a luminosity dependence of the spectral slopes at both energies. Specifically, luminous blazars, generally classified as FSRQs, have {\it hard} continua in the medium-hard X-ray range but {\it soft} continua in the LAT gamma-ray range (photon indices \ltsima 2 and \gtsima 2), while lower luminosity blazars, classified as BL Lacs, have opposite behavior, i.e., {\it soft} X-ray and {\it hard} gamma-ray continua ( \gtsima 2.4 and ). The trends are confirmed by detailed Monte Carlo simulations explicitly taking into account the observational biases of both instruments. Our results support the so-called ``blazar sequence'' which was originally based on radio samples of blazars and radio luminosities. We also argue that the X-ray-to-gamma-ray continua of blazars may provide independent insights into the physical conditions around the jet, complementing/superseding the ambiguities of the traditional classification based on optical properties.
Accepted by ApJ
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Cited by in corpus (13)
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- Similarity of the Optical-IR and Gamma-Ray Time Variability of Fermi Blazars
- Planck early results. XV. Spectral energy distributions and radio continuum spectra of northern extragalactic radio sources
- Bethe-Heitler emission in BL Lacs: filling the gap between X-rays and -rays
- The Atacama Cosmology Telescope: Dusty Star-Forming Galaxies and Active Galactic Nuclei in the Southern Survey
- Hard X-ray properties of NuSTAR blazars
- Blazars at the Cosmic Dawn
- Basic properties of Fermi blazars and the "blazar sequence"
- Radio-Optical-Gamma-Ray properties of MOJAVE AGN detected by Fermi/LAT
- Fermi/LAT Observations of Swift/BAT Seyferts: on the Contribution of Radio-quiet AGN to the Extragalactic Gamma-ray Background
- High energy emission component, population, and contribution to the extragalactic gamma-ray background of gamma-ray emitting radio galaxies
- Gamma-Ray Burst Afterglows as Analogues of High Frequency-Peaked BL Lac Objects
- Multiple inverse Compton scatterings and the blazar sequence