GAMMA-RAYS FROM THE QUASAR PKS 1441+25: STORY OF AN ESCAPE
dc.contributor.author | VERITAS | |
dc.contributor.author | SPOL | |
dc.contributor.author | ASAS-SN | |
dc.contributor.author | OVRO | |
dc.contributor.author | NuSTAR | |
dc.contributor.author | CRTS | |
dc.contributor.other | Utah System of Higher Education | |
dc.contributor.other | University of Utah | |
dc.contributor.other | McGill University | |
dc.contributor.other | Washington University (WUSTL) | |
dc.contributor.other | University of California System | |
dc.contributor.other | University of California Los Angeles | |
dc.contributor.other | Harvard University | |
dc.contributor.other | Smithsonian Astrophysical Observatory | |
dc.contributor.other | Smithsonian Institution | |
dc.contributor.other | University College Dublin | |
dc.contributor.other | University of California Santa Cruz | |
dc.contributor.other | Iowa State University | |
dc.contributor.other | University of Potsdam | |
dc.contributor.other | Helmholtz Association | |
dc.contributor.other | Deutsches Elektronen-Synchrotron (DESY) | |
dc.contributor.other | California State University System | |
dc.contributor.other | California Polytechnic State University San Luis Obispo | |
dc.contributor.other | Ollscoil na Gaillimhe-University of Galway | |
dc.contributor.other | Yale University | |
dc.contributor.other | Purdue University System | |
dc.contributor.other | Purdue University | |
dc.contributor.other | Purdue University West Lafayette Campus | |
dc.contributor.other | University of Minnesota System | |
dc.contributor.other | University of Minnesota Twin Cities | |
dc.contributor.other | Columbia University | |
dc.contributor.other | Pennsylvania Commonwealth System of Higher Education (PCSHE) | |
dc.contributor.other | Pennsylvania State University | |
dc.contributor.other | Pennsylvania State University - University Park | |
dc.contributor.other | University of Delaware | |
dc.contributor.other | University of Iowa | |
dc.contributor.other | University System of Georgia | |
dc.contributor.other | Georgia Institute of Technology | |
dc.contributor.other | University of Chicago | |
dc.contributor.other | National Aeronautics & Space Administration (NASA) | |
dc.contributor.other | NASA Goddard Space Flight Center | |
dc.contributor.other | Cork Institute of Technology | |
dc.contributor.other | University System of Maryland | |
dc.contributor.other | University of Maryland College Park | |
dc.contributor.other | United States Department of Energy (DOE) | |
dc.contributor.other | Argonne National Laboratory | |
dc.contributor.other | University of Arizona | |
dc.contributor.other | University System of Ohio | |
dc.contributor.other | Ohio State University | |
dc.contributor.other | University Diego Portales | |
dc.contributor.other | Carnegie Institution for Science | |
dc.contributor.other | Aalto University | |
dc.contributor.other | National Radio Astronomy Observatory (NRAO) | |
dc.contributor.other | California Institute of Technology | |
dc.contributor.other | Universidad de Concepcion | |
dc.contributor.other | Stanford University | |
dc.contributor.other | SLAC National Accelerator Laboratory | |
dc.contributor.other | University of Alabama Tuscaloosa | |
dc.date.accessioned | 2019-06-27T21:14:49Z | |
dc.date.available | 2019-06-27T21:14:49Z | |
dc.date.issued | 2015-12-15 | |
dc.description.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 similar to 200 GeV from PKS 1441+25 (z = 0.939) during 2015 April, 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. | en_US |
dc.format.mimetype | application/pdf | |
dc.identifier.citation | Abeysekara, A. U., et al. (2015): Gamma-Rays from the Quasar PKS 1441+ 25: Story of an Escape. The Astrophysical Journal Letters, 815(2). DOI: http://dx.doi.org/10.1088/2041-8205/815/2/L22 | |
dc.identifier.doi | 10.1088/2041-8205/815/2/L22 | |
dc.identifier.orcid | https://orcid.org/0000-0002-5955-6383 | |
dc.identifier.orcid | https://orcid.org/0000-0001-6674-4238 | |
dc.identifier.orcid | https://orcid.org/0000-0002-2126-2419 | |
dc.identifier.orcid | https://orcid.org/0000-0002-5491-5244 | |
dc.identifier.orcid | https://orcid.org/0000-0001-7891-699X | |
dc.identifier.orcid | https://orcid.org/0000-0001-5213-6231 | |
dc.identifier.orcid | https://orcid.org/0000-0003-3343-0755 | |
dc.identifier.orcid | https://orcid.org/0000-0002-5491-5244 | |
dc.identifier.orcid | https://orcid.org/0000-0001-5704-271X | |
dc.identifier.orcid | https://orcid.org/0000-0001-7861-1707 | |
dc.identifier.orcid | https://orcid.org/0000-0002-6324-5772 | |
dc.identifier.orcid | https://orcid.org/0000-0002-1067-8558 | |
dc.identifier.orcid | https://orcid.org/0000-0002-1432-7771 | |
dc.identifier.orcid | https://orcid.org/0000-0001-7297-8217 | |
dc.identifier.orcid | https://orcid.org/0000-0003-4641-4201 | |
dc.identifier.orcid | https://orcid.org/0000-0001-9604-2325 | |
dc.identifier.orcid | https://orcid.org/0000-0003-4785-0101 | |
dc.identifier.orcid | https://orcid.org/0000-0001-7595-0914 | |
dc.identifier.orcid | https://orcid.org/0000-0002-4837-5253 | |
dc.identifier.orcid | https://orcid.org/0000-0002-0529-1973 | |
dc.identifier.orcid | https://orcid.org/0000-0003-4631-1149 | |
dc.identifier.orcid | https://orcid.org/0000-0002-5167-1221 | |
dc.identifier.orcid | https://orcid.org/0000-0002-4596-8563 | |
dc.identifier.orcid | https://orcid.org/0000-0002-2133-5251 | |
dc.identifier.orcid | https://orcid.org/0000-0002-2024-8199 | |
dc.identifier.orcid | https://orcid.org/0000-0001-9868-4700 | |
dc.identifier.orcid | https://orcid.org/0000-0003-1072-2712 | |
dc.identifier.orcid | https://orcid.org/0000-0002-8006-9854 | |
dc.identifier.orcid | https://orcid.org/0000-0002-5221-6669 | |
dc.identifier.orcid | https://orcid.org/0000-0002-0794-8780 | |
dc.identifier.orcid | https://orcid.org/0000-0002-4855-2694 | |
dc.identifier.orcid | https://orcid.org/0000-0002-1853-863X | |
dc.identifier.orcid | https://orcid.org/0000-0003-3967-1533 | |
dc.identifier.orcid | https://orcid.org/0000-0003-2098-170X | |
dc.identifier.orcid | https://orcid.org/0000-0001-9206-3460 | |
dc.identifier.uri | http://ir.ua.edu/handle/123456789/5856 | |
dc.language | English | |
dc.language.iso | en_US | |
dc.publisher | IOP Publishing | |
dc.subject | cosmology: observations | |
dc.subject | diffuse radiation | |
dc.subject | gamma rays: galaxies | |
dc.subject | quasars: individual (PKS 1441+25-VER J1443+250) | |
dc.subject | radiation mechanisms: non-thermal | |
dc.subject | EXTRAGALACTIC BACKGROUND LIGHT | |
dc.subject | COMPLETE SAMPLE | |
dc.subject | BLAZARS | |
dc.subject | TELESCOPE | |
dc.subject | RADIATION | |
dc.subject | SPECTRA | |
dc.subject | VARIABILITY | |
dc.subject | ABSORPTION | |
dc.subject | DISCOVERY | |
dc.subject | EMISSION | |
dc.subject | Astronomy & Astrophysics | |
dc.title | GAMMA-RAYS FROM THE QUASAR PKS 1441+25: STORY OF AN ESCAPE | en_US |
dc.type | text | |
dc.type | Article |
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