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A Decade of Multiwavelength Observations of the TeV Blazar 1ES 1215+303: Extreme Shift of the Synchrotron Peak Frequency and Long-term Optical–Gamma-Ray Flux Increase

Valverde, Janeth and Horan, Deirdre and Bernard, Denis and Fegan, Stephen and Abeysekara, A. U. and Archer, A. and Benbow, W. and Bird, R. and Brill, A. and Brose, R. and Buchovecky, M. and Buckley, J. H. and Christiansen, J. L. and Cui, W. and Falcone, A. and Feng, Q. and Finley, J. P. and Fortson, L. and Furniss, A. and Gent, A. and Gillanders, G. H. and Giuri, C. and Gueta, O. and Hanna, D. and Hassan, T. and Hervet, O. and Holder, J. and Hughes, G. and Humensky, T. B. and Kaaret, P. and Kelley-Hoskins, N. and Kertzman, M. and Kieda, D. and Krause, M. and Krennrich, F. and Lang, M. J. and Maier, G. and Moriarty, P. and Mukherjee, R. and Nieto, D. and Nievas-Rosillo, M. and O’Brien, S. and Ong, R. A. and Otte, A. N. and Park, N. and Petrashyk, A. and Pfrang, K. and Pichel, A. and Pohl, M. and Prado, R. R. and Pueschel, E. and Quinn, J. and Ragan, K. and Reynolds, P. T. and Ribeiro, D. and Richards, G. T. and Roache, E. and Sadeh, I. and Santander, M. and Scott, S. S. and Sembroski, G. H. and Shahinyan, K. and Shang, R. and Sushch, I. and Vassiliev, V. V. and Weinstein, A. and Wells, R. M. and Wilcox, P. and Wilhelm, A. and Williams, D. A. and Williamson, T. J and Noto, Giuliana and Edwards, P. G. and Piner, B. G. and Ramazani, V. Fallah and Hovatta, T. and Jormanainen, J. and Lindfors, E. and Nilsson, K. and Takalo, L. and Kovalev, Y. Y. and Lister, M. L. and Pushkarev, A. B. and Savolainen, T. and Kiehlmann, S. and Max-Moerbeck, W. and Readhead, A. C. S. and Lähteenmäki, A. and Tornikoski, M. (2020) A Decade of Multiwavelength Observations of the TeV Blazar 1ES 1215+303: Extreme Shift of the Synchrotron Peak Frequency and Long-term Optical–Gamma-Ray Flux Increase. Astrophysical Journal, 891 (2). Art. No. 170. ISSN 1538-4357. https://resolver.caltech.edu/CaltechAUTHORS:20200317-133828509

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Abstract

Blazars are known for their variability on a wide range of timescales at all wavelengths. Most studies of TeV gamma-ray blazars focus on short timescales, especially during flares. With a decade of observations from the Fermi-LAT and VERITAS, we present an extensive study of the long-term multiwavelength radio-to-gamma-ray flux-density variability, with the addition of a couple of short-time radio-structure and optical polarization observations of the blazar 1ES 1215+303 (z = 0.130), with a focus on its gamma-ray emission from 100 MeV to 30 TeV. Multiple strong GeV gamma-ray flares, a long-term increase in the gamma-ray and optical flux baseline, and a linear correlation between these two bands are observed over the ten-year period. Typical HBL behaviors are identified in the radio morphology and broadband spectrum of the source. Three stationary features in the innermost jet are resolved by Very Long Baseline Array at 43.1, 22.2, and 15.3 GHz. We employ a two-component synchrotron self-Compton model to describe different flux states of the source, including the epoch during which an extreme shift in energy of the synchrotron peak frequency from infrared to soft X-rays is observed.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.3847/1538-4357/ab765dDOIArticle
ORCID:
AuthorORCID
Valverde, Janeth0000-0002-8090-6528
Benbow, W.0000-0003-2098-170X
Bird, R.0000-0002-4596-8563
Christiansen, J. L.0000-0002-8035-4778
Cui, W.0000-0002-6324-5772
Feng, Q.0000-0001-6674-4238
Fortson, L.0000-0002-1067-8558
Furniss, A.0000-0003-1614-1273
Gillanders, G. H.0000-0001-8763-6252
Hanna, D.0000-0002-8513-5603
Hervet, O.0000-0003-3878-1677
Kaaret, P.0000-0002-3638-0637
Kieda, D.0000-0003-4785-0101
Maier, G.0000-0001-9868-4700
Mukherjee, R.0000-0002-3223-0754
Otte, A. N.0000-0002-5955-6383
Pohl, M.0000-0001-7861-1707
Pueschel, E.0000-0002-0529-1973
Richards, G. T.0000-0002-1408-807X
Santander, M.0000-0001-7297-8217
Shahinyan, K.0000-0001-5128-4160
Sushch, I.0000-0002-2814-1257
Piner, B. G.0000-0003-4379-3250
Hovatta, T.0000-0002-2024-8199
Nilsson, K.0000-0002-1445-8683
Kovalev, Y. Y.0000-0001-9303-3263
Lister, M. L.0000-0003-1315-3412
Pushkarev, A. B.0000-0002-9702-2307
Savolainen, T.0000-0001-6214-1085
Kiehlmann, S.0000-0001-6314-9177
Readhead, A. C. S.0000-0001-9152-961X
Tornikoski, M.0000-0003-1249-6026
Additional Information:© 2020 The American Astronomical Society. Received 2019 October 2; Accepted 2020 February 7; Published 2020 March 17. The Fermi-LAT Collaboration acknowledges generous ongoing support from a number of agencies and institutes that have supported both the development and the operation of the LAT as well as scientific data analysis. These include the National Aeronautics and Space Administration and the Department of Energy in the United States; the Commissariat à l'Energie Atomique and the Centre National de la Recherche Scientifique/Institut National de Physique Nucléaire et de Physique des Particules in France; the Agenzia Spaziale Italiana and the Istituto Nazionale di Fisica Nucleare in Italy; the Ministry of Education, Culture, Sports, Science and Technology (MEXT), High Energy Accelerator Research Organization (KEK), and Japan Aerospace Exploration Agency (JAXA) in Japan; and the KA Wallenberg Foundation, the Swedish Research Council, and the Swedish National Space Board in Sweden. Additional support for science analysis during the operations phase is gratefully acknowledged from the Istituto Nazionale di Astrofisica in Italy and the Centre National d'Études Spatiales in France. This work performed in part under DOE Contract DE- AC02-76SF00515. This research is supported by grants from the U.S. Department of Energy Office of Science, the U.S. National Science Foundation and the Smithsonian Institution, and by NSERC in Canada. This research used resources provided by the Open Science Grid, which is supported by the National Science Foundation and the U.S. Department of Energy's Office of Science, and resources of the National Energy Research Scientific Computing Center (NERSC), a U.S. Department of Energy Office of Science User Facility operated under Contract No. DE-AC02-05CH11231. We acknowledge the excellent work of the technical support staff at the Fred Lawrence Whipple Observatory and at the collaborating institutions in the construction and operation of VERITAS. This research has made use of data from the MOJAVE database, which is maintained by the MOJAVE team (Lister et al. 2018). The MOJAVE program is supported under NASA-Fermi grant NNX15AU76G. The National Radio Astronomy Observatory is a facility of the National Science Foundation, operated under cooperative agreement by Associated Universities, Inc. 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. This research has made use of data from the OVRO 40 m monitoring program (Richards et al. 2011), which is supported in part by NASA grants NNX08AW31G, NNX11A043G, and NNX14AQ89G, as well as by NSF grants AST-0808050 and AST-1109911. J.V. was partially supported by the Alliance program, a partnership between Columbia University, NY, USA, and three major French institutions: École Polytechnique, Paris 1 Panthéon-Sorbonne University, and Science Po. T.S. was supported by the Academy of Finland projects 274477, 284495, and 312496. W.M. acknowledge support from CONICYT project Basal AFB-170002. Y.Y.K. and A.B.P. were supported by the Russian Foundation for Basic Research (project 17-02-00197), the government of the Russian Federation (agreement 05.Y09.21.0018), and the Alexander von Humboldt Foundation. S.K. acknowledges support from the European Research Council under the European Union's Horizon 2020 research and innovation program, under grant agreement No 771282. Software: AIPS (Greisen 2003), DIFMAP (Shepherd 1997), Fermi Science Tools (Fermi Science Support development team 2019).
Group:Astronomy Department
Funders:
Funding AgencyGrant Number
Department of Energy (DOE)DE-AC02-76SF00515
Commissariat a l'Energie Atomique (CEA)UNSPECIFIED
Centre National de la Recherche Scientifique (CNRS)UNSPECIFIED
Institut National de Physique Nucléaire et de Physique des Particules (IN2P3)UNSPECIFIED
Agenzia Spaziale Italiana (ASI)UNSPECIFIED
Istituto Nazionale di Fisica Nucleare (INFN)UNSPECIFIED
Ministry of Education, Culture, Sports, Science and Technology (MEXT)UNSPECIFIED
High Energy Accelerator Research Organization (KEK)UNSPECIFIED
Japan Aerospace Exploration Agency (JAXA)UNSPECIFIED
Knut and Alice Wallenberg FoundationUNSPECIFIED
Swedish Research CouncilUNSPECIFIED
Swedish National Space Board (SNSB)UNSPECIFIED
Istituto Nazionale di Astrofisica (INAF)UNSPECIFIED
Centre National d'Études Spatiales (CNES)UNSPECIFIED
Smithsonian InstitutionUNSPECIFIED
Natural Sciences and Engineering Research Council of Canada (NSERC)UNSPECIFIED
Department of Energy (DOE)DE-AC02-05CH11231
NASANNX15AU76G
NASA/JPL/CaltechUNSPECIFIED
NASANNX08AW31G
NASANNX11A043G
NASANNX14AQ89G
NSFAST-0808050
NSFAST-1109911
Columbia UniversityUNSPECIFIED
École PolytechniqueUNSPECIFIED
Paris 1 Panthéon-Sorbonne UniversityUNSPECIFIED
Science PoUNSPECIFIED
Academy of Finland274477
Academy of Finland284495
Academy of Finland312496
BASAL-CATAAFB-170002
Russian Foundation for Basic Research17-02-00197
Russian Federation05.Y09.21.0018
Alexander von Humboldt FoundationUNSPECIFIED
European Research Council (ERC)771282
Subject Keywords:Active galaxies ; Jets ; Gamma-rays ; Blazars ; BL Lacertae objects
Issue or Number:2
Classification Code:Unified Astronomy Thesaurus concepts: Active galaxies (17); Jets (870); Gamma-rays (637); Blazars (164); BL Lacertae objects (158)
Record Number:CaltechAUTHORS:20200317-133828509
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20200317-133828509
Official Citation:Janeth Valverde et al 2020 ApJ 891 170
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:101946
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:17 Mar 2020 21:04
Last Modified:17 Mar 2020 21:04

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