Published December 15, 2015 | Version Submitted + Published
Journal Article Open

Gamma rays from the quasar PKS 1441+25: story of an escape

Creators

  • 1. ROR icon University of Utah
  • 2. ROR icon McGill University
  • 3. ROR icon Washington University in St. Louis
  • 4. ROR icon University of California, Los Angeles
  • 5. ROR icon Harvard-Smithsonian Center for Astrophysics
  • 6. ROR icon University College Dublin
  • 7. ROR icon University of California, Santa Cruz
  • 8. ROR icon University of Paris-Saclay
  • 9. ROR icon Iowa State University
  • 10. ROR icon Laboratoire de Physique Nucléaire et de Hautes Énergies
  • 11. ROR icon University of Potsdam
  • 12. ROR icon Deutsches Elektronen-Synchrotron DESY
  • 13. ROR icon California Polytechnic State University
  • 14. ROR icon Adler Planetarium
  • 15. ROR icon National University of Ireland, Galway
  • 16. ROR icon Yale University
  • 17. ROR icon Purdue University West Lafayette
  • 18. ROR icon University of Minnesota
  • 19. ROR icon Columbia University
  • 20. ROR icon Pennsylvania State University
  • 21. ROR icon California State University, East Bay
  • 22. ROR icon University of Delaware
  • 23. ROR icon University of Iowa
  • 24. ROR icon Georgia Institute of Technology
  • 25. ROR icon University of Chicago
  • 26. ROR icon Goddard Space Flight Center
  • 27. ROR icon Munster Technological University
  • 28. ROR icon University of Maryland, College Park
  • 29. ROR icon Argonne National Laboratory
  • 30. ROR icon The Ohio State University
  • 31. ROR icon Diego Portales University
  • 32. ROR icon Millennium Institute of Astrophysics
  • 33. ROR icon Carnegie Observatories
  • 34. ROR icon Aalto University
  • 35. ROR icon National Radio Astronomy Observatory
  • 36. ROR icon California Institute of Technology
  • 37. ROR icon University of Concepción
  • 38. ROR icon Stanford University

Abstract

Outbursts from gamma-ray quasars provide insights on the relativistic jets of active galactic nuclei and constraints on the diffuse radiation fields that fill the Universe. The detection of significant emission above 100 GeV from a distant quasar would show that some of the radiated gamma rays escape pair-production interactions with low-energy photons, be it the extragalactic background light (EBL), or the radiation near the supermassive black hole lying at the jet's base. VERITAS detected gamma-ray emission up to 200 GeV from PKS 1441+25 (z=0.939) during April 2015, a period of high activity across all wavelengths. This observation of PKS 1441+25 suggests that the emission region is located thousands of Schwarzschild radii away from the black hole. The gamma-ray detection also sets a stringent upper limit on the near-ultraviolet to near-infrared EBL intensity, suggesting that galaxy surveys have resolved most, if not all, of the sources of the EBL at these wavelengths.

Additional Information

© 2015. The American Astronomical Society. Received 2015 August 10; accepted 2015 November 17; published 2015 December 15. 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, with additional support from NASA Swift GI grant NNX15AR38G. 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 the instrument. The VERITAS Collaboration is grateful to Trevor Weekes for his seminal contributions and leadership in the field of VHE gamma-ray astrophysics, which made this study possible. ASAS-SN thanks LCOGT, NSF, Mt. Cuba Astronomical Foundation, OSU/CCAPP and MAS/Chile for their support. The observations at Steward Observatory are funded through NASA Fermi GI grant NNX12AO93G. CRTS is supported by the NSF grants AST-1313422 and AST-1413600. The OVRO 40-m monitoring program is supported in part by NASA grants NNX08AW31G and NNX11A043G, and NSF grants AST-0808050 and AST-1109911. The National Radio Astronomy Observatory is a facility of NSF operated under cooperative agreement by Associated Universities, Inc. This research has made use of data from the MOJAVE database that is maintained by the MOJAVE team (Lister et al. 2009).

Attached Files

Published - Abeysekara_2015pL22.pdf

Submitted - 1512.04434v1.pdf

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Additional details

Identifiers

Eprint ID
64197
Resolver ID
CaltechAUTHORS:20160203-120802229

Related works

Funding

Department of Energy (DOE)
Smithsonian Institution
Natural Sciences and Engineering Research Council of Canada (NSERC)
NASA
NNX15AR38G
NASA
NNX12AO93G
NSF
AST-1313422
NSF
AST-1413600
NASA
NNX08AW31G
NASA
NNX11A043G
NASA
AST-0808050
NASA
AST-1109911
Associated Universities, Inc
Las Cumbres Observatory Global Telescope Network
Mt. Cuba Astronomical Foundation
Ohio State University
Instituto Milenio de Astrofísica (MAS)

Dates

Created
2016-02-03
Created from EPrint's datestamp field
Updated
2023-03-16
Created from EPrint's last_modified field

Caltech Custom Metadata

Caltech groups
NuSTAR, Space Radiation Laboratory, Owens Valley Radio Observatory