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Broadband Observations of High Redshift Blazars

Paliya, Vaidehi S. and Parker, M. L. and Fabian, A. C. and Stalin, C. S. (2016) Broadband Observations of High Redshift Blazars. Astrophysical Journal, 825 (1). Art. No. 74. ISSN 0004-637X. https://resolver.caltech.edu/CaltechAUTHORS:20160501-095905412

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Abstract

We present a multi-wavelength study of four high redshift blazars, S5 0014+81 (z = 3.37), CGRaBS J0225+1846 (z = 2.69), BZQ J1430+4205 (z = 4.72), and 3FGL J1656.2−3303 (z = 2.40) using quasi-simultaneous data from the Swift, Nuclear Spectroscopic Telescope Array (NuSTAR) and the Fermi-Large Area Telescope (LAT) and also archival XMM-Newton observations. Other than 3FGL J1656.2−3303, none of the sources were known as γ-ray emitters, and our analysis of ~7.5 yr of LAT data reveals the first time detection of statistically significant γ-ray emission from CGRaBS J0225+1846. We generate the broadband spectral energy distributions (SED) of all the objects, centering at the epoch of NuSTAR observations and reproduce them using a one-zone leptonic emission model. The optical−UV emission in all the objects can be explained by radiation from the accretion disk, whereas the X-ray to γ-ray windows of the SEDs are found to be dominated by inverse Compton scattering off the broad line region photons. All of them host black holes that are billions of solar masses. Comparing the accretion disk luminosity and the jet power of these sources with a large sample of blazars, we find them to occupy a high disk luminosity–jet power regime. We also investigate the X-ray spectral properties of the sources in detail with a major focus on studying the causes of soft X-ray deficit, a feature generally seen in high redshift radio-loud quasars. We summarize that this feature could be explained based on the intrinsic curvature in the jet emission rather than being due to the external effects predicted in earlier studies, such as host galaxy and/or warm absorption.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.3847/0004-637X/825/1/74DOIArticle
http://arxiv.org/abs/1604.08566arXivDiscussion Paper
ORCID:
AuthorORCID
Paliya, Vaidehi S.0000-0001-7774-5308
Parker, M. L.0000-0002-8466-7317
Fabian, A. C.0000-0002-9378-4072
Stalin, C. S.0000-0002-4998-1861
Additional Information:© 2016 The American Astronomical Society. Received 2016 April 12; revised 2016 April 25; accepted 2016 April 28; published 2016 June 29. We are grateful to the referee for constructive comments on the manuscript. A.C.F. thanks Greg Madejski for discussions on the curvature of blazar X-ray spectra and acknowledges support from ERC Advanced Grant 340442. This research has made use of data, software, and/or web tools obtained from NASAs High Energy Astrophysics Science Archive Research Center (HEASARC), a service of Goddard Space Flight Center and the Smithsonian Astrophysical Observatory. Part of this work is based on archival data, software, or online services provided by the ASI Science Data Center (ASDC). This research has made use of the XRT Data Analysis Software (XRTDAS) developed under the responsibility of the ASDC, Italy. This research has also made use of the NuSTAR Data Analysis Software (NuSTARDAS) jointly developed by the ASI Science Data Center (ASDC, Italy) and the California Institute of Technology (Caltech, USA). This research has made use of the NASA/IPAC Extragalactic Database (NED) which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration. Funding for SDSS-III has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Science Foundation, and the U.S. Department of Energy Office of Science. The SDSS-III web site is http://www.sdss3.org/. SDSS-III is managed by the Astrophysical Research Consortium for the Participating Institutions of the SDSS-III Collaboration including the University of Arizona, the Brazilian Participation Group, Brookhaven National Laboratory, Carnegie Mellon University, University of Florida, the French Participation Group, the German Participation Group, Harvard University, the Instituto de Astrofisica de Canarias, the Michigan State/Notre Dame/JINA Participation Group, Johns Hopkins University, Lawrence Berkeley National Laboratory, Max Planck Institute for Astrophysics, Max Planck Institute for Extraterrestrial Physics, New Mexico State University, New York University, Ohio State University, Pennsylvania State University, University of Portsmouth, Princeton University, the Spanish Participation Group, University of Tokyo, University of Utah, Vanderbilt University, University of Virginia, University of Washington, and Yale University.
Group:NuSTAR, Infrared Processing and Analysis Center (IPAC)
Funders:
Funding AgencyGrant Number
NASA/JPL/CaltechUNSPECIFIED
Alfred P. Sloan FoundationUNSPECIFIED
Participating InstitutionsUNSPECIFIED
NSFUNSPECIFIED
Department of Energy (DOE)UNSPECIFIED
Subject Keywords:galaxies: active – galaxies: jets – gamma rays: galaxies
Issue or Number:1
Record Number:CaltechAUTHORS:20160501-095905412
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20160501-095905412
Official Citation:Vaidehi S. Paliya et al 2016 ApJ 825 74
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:66567
Collection:CaltechAUTHORS
Deposited By: Joy Painter
Deposited On:01 May 2016 23:34
Last Modified:03 Oct 2019 09:57

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