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CONTEMPORANEOUS BROADBAND OBSERVATIONS OF THREE HIGH-REDSHIFT BL LAC OBJECTS
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Number of Authors: 104
2016 (English)In: Astrophysical Journal, ISSN 0004-637X, E-ISSN 1538-4357, Vol. 820, no 1, 72Article in journal (Refereed) Published
Abstract [en]

We have collected broadband spectral energy distributions (SEDs) of three BL Lac objects 3FGL J0022.1-1855 (z = 0.689), 3FGL J0630.9-2406 (z greater than or similar to 1.239), and 3FGL J0811.2-7529 (z = 0.774), detected by Fermi with relatively flat gigaelectronvolt spectra. By observing simultaneously in the near-infrared to hard X-ray band, we can well characterize the high end of the synchrotron component of the SED. Thus, fitting the SEDs to synchro-Compton models of the dominant emission from the relativistic jet, we can constrain the underlying particle properties and predict the shape of the gigaelectronvolt Compton component. Standard extragalactic background light (EBL) models explain the high-energy absorption well, with poorer fits for high-ultraviolet models. The fits show clear evidence for EBL absorption in the Fermi spectrum of our highest-redshift source 3FGL J0630.9-2406. While synchrotron self-Compton models adequately describe the SEDs, the situation may be complicated by possible external Compton components. For 3FGL J0811.2-7529, we also discover a nearby serendipitous source in the X-ray data, which is almost certainly another lower synchrotron peak frequency (nu(sy)(pk)) BL Lac, that may contribute flux in the Fermi band. Since our sources are unusual high-luminosity, moderate nu(sy)(pk) BL Lacs, we compare these quantities and the Compton dominance, the ratio of peak inverse Compton to peak synchrotron luminosities (L-pk(IC)/L-pk(sy)), with those of the full Fermi BL Lac population.

Place, publisher, year, edition, pages
2016. Vol. 820, no 1, 72
Keyword [en]
BL Lacertae objects: general, BL Lacertae objects: individual (3FGL J0022.1-1855, 3FGL J0630.9-2406, 3FGL J0811.2-7529), galaxies: active, radiation mechanisms: non-thermal
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Physical Sciences
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URN: urn:nbn:se:su:diva-129676DOI: 10.3847/0004-637X/820/1/72ISI: 000372787000071OAI: oai:DiVA.org:su-129676DiVA: diva2:930275
Available from: 2016-05-23 Created: 2016-04-27 Last updated: 2016-05-23Bibliographically approved

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Larsson, Stefan
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The Oskar Klein Centre for Cosmo Particle Physics (OKC)
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