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Gamma rays from the quasar PKS 1441+25: story of an escape
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 escap...
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creator | Abeysekara, A U Archambault, S Archer, A Aune, T Barnacka, A Benbow, W Bird, R Biteau, J Buckley, J H Bugaev, V Cardenzana, J V Cerruti, M Chen, X Christiansen, J L Ciupik, L Connolly, M P Coppi, P Cui, W Dickinson, H J Eisch, J D Errando, M Falcone, A Feng, Q Finley, J P Fleischhack, H Flinders, A tin, P tson, L Furniss, A Griffin, S Grube, J Gyuk, G Hütten, M Håkansson, N Hanna, D Holder, J Humensky, T B Johnson, C A Kaaret, P Kar, P Kelley-Hoskins, N Khassen, Y Kieda, D Krause, M Krennrich, F Kumar, S Lang, M J Maier, G McArthur, S McCann, A Meagher, K Moriarty, P Mukherjee, R Nieto, D A O'Faoláin de Bhróithe Ong, R A Otte, A N Park, N Perkins, J S Petrashyk, A Pohl, M Pueschel, E Quinn, J Ragan, K Ratliff, G Reynolds, P T Richards, G T Roache, E Santander, M Shahinyan, K Smith, A W Staszak, D Telezhinsky, I Todd, N W Tucci, J V Tyler, J Vassiliev, V V Vincent, S Wakely, S P Weiner, O M Weinstein, A Wilhelm, A Williams, D A Zitzer, B Smith, P S Holoien, T W -S Kochanek, C S Stanek, K Z Shappee, B Hovatta, T Max-Moerbeck, W Pearson, T J Reeves, R A Richards, J L Readhead, A C S Madejski, G M Djorgovski, S G Drake, A J Graham, M J Mahabal, A |
description | 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. |
doi_str_mv | 10.48550/arxiv.1512.04434 |
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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. 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A</creatorcontrib><creatorcontrib>Otte, A N</creatorcontrib><creatorcontrib>Park, N</creatorcontrib><creatorcontrib>Perkins, J S</creatorcontrib><creatorcontrib>Petrashyk, A</creatorcontrib><creatorcontrib>Pohl, M</creatorcontrib><creatorcontrib>Pueschel, E</creatorcontrib><creatorcontrib>Quinn, J</creatorcontrib><creatorcontrib>Ragan, K</creatorcontrib><creatorcontrib>Ratliff, G</creatorcontrib><creatorcontrib>Reynolds, P T</creatorcontrib><creatorcontrib>Richards, G T</creatorcontrib><creatorcontrib>Roache, E</creatorcontrib><creatorcontrib>Santander, M</creatorcontrib><creatorcontrib>Shahinyan, K</creatorcontrib><creatorcontrib>Smith, A W</creatorcontrib><creatorcontrib>Staszak, D</creatorcontrib><creatorcontrib>Telezhinsky, I</creatorcontrib><creatorcontrib>Todd, N W</creatorcontrib><creatorcontrib>Tucci, J V</creatorcontrib><creatorcontrib>Tyler, J</creatorcontrib><creatorcontrib>Vassiliev, V V</creatorcontrib><creatorcontrib>Vincent, S</creatorcontrib><creatorcontrib>Wakely, S P</creatorcontrib><creatorcontrib>Weiner, O M</creatorcontrib><creatorcontrib>Weinstein, A</creatorcontrib><creatorcontrib>Wilhelm, A</creatorcontrib><creatorcontrib>Williams, D A</creatorcontrib><creatorcontrib>Zitzer, B</creatorcontrib><creatorcontrib>Smith, P S</creatorcontrib><creatorcontrib>Holoien, T W -S</creatorcontrib><creatorcontrib>Kochanek, C S</creatorcontrib><creatorcontrib>Stanek, K Z</creatorcontrib><creatorcontrib>Shappee, B</creatorcontrib><creatorcontrib>Hovatta, T</creatorcontrib><creatorcontrib>Max-Moerbeck, W</creatorcontrib><creatorcontrib>Pearson, T J</creatorcontrib><creatorcontrib>Reeves, R A</creatorcontrib><creatorcontrib>Richards, J L</creatorcontrib><creatorcontrib>Readhead, A C S</creatorcontrib><creatorcontrib>Madejski, G M</creatorcontrib><creatorcontrib>Djorgovski, S G</creatorcontrib><creatorcontrib>Drake, A J</creatorcontrib><creatorcontrib>Graham, M J</creatorcontrib><creatorcontrib>Mahabal, A</creatorcontrib><title>Gamma rays from the quasar PKS 1441+25: story of an escape</title><title>arXiv.org</title><description>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.</description><subject>Active galactic nuclei</subject><subject>Background radiation</subject><subject>Diffuse radiation</subject><subject>Emission</subject><subject>Galaxies</subject><subject>Gamma rays</subject><subject>Outbursts</subject><subject>Photons</subject><subject>Quasars</subject><subject>Supermassive black 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Humensky, T B ; Johnson, C A ; Kaaret, P ; Kar, P ; Kelley-Hoskins, N ; Khassen, Y ; Kieda, D ; Krause, M ; Krennrich, F ; Kumar, S ; Lang, M J ; Maier, G ; McArthur, S ; McCann, A ; Meagher, K ; Moriarty, P ; Mukherjee, R ; Nieto, D ; A O'Faoláin de Bhróithe ; Ong, R A ; Otte, A N ; Park, N ; Perkins, J S ; Petrashyk, A ; Pohl, M ; Pueschel, E ; Quinn, J ; Ragan, K ; Ratliff, G ; Reynolds, P T ; Richards, G T ; Roache, E ; Santander, M ; Shahinyan, K ; Smith, A W ; Staszak, D ; Telezhinsky, I ; Todd, N W ; Tucci, J V ; Tyler, J ; Vassiliev, V V ; Vincent, S ; Wakely, S P ; Weiner, O M ; Weinstein, A ; Wilhelm, A ; Williams, D A ; Zitzer, B ; Smith, P S ; Holoien, T W -S ; Kochanek, C S ; Stanek, K Z ; Shappee, B ; Hovatta, T ; Max-Moerbeck, W ; Pearson, T J ; Reeves, R A ; Richards, J L ; Readhead, A C S ; Madejski, G M ; Djorgovski, S G ; Drake, A J ; Graham, M J ; Mahabal, 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D</creatorcontrib><creatorcontrib>A O'Faoláin de Bhróithe</creatorcontrib><creatorcontrib>Ong, R A</creatorcontrib><creatorcontrib>Otte, A N</creatorcontrib><creatorcontrib>Park, N</creatorcontrib><creatorcontrib>Perkins, J S</creatorcontrib><creatorcontrib>Petrashyk, A</creatorcontrib><creatorcontrib>Pohl, M</creatorcontrib><creatorcontrib>Pueschel, E</creatorcontrib><creatorcontrib>Quinn, J</creatorcontrib><creatorcontrib>Ragan, K</creatorcontrib><creatorcontrib>Ratliff, G</creatorcontrib><creatorcontrib>Reynolds, P T</creatorcontrib><creatorcontrib>Richards, G T</creatorcontrib><creatorcontrib>Roache, E</creatorcontrib><creatorcontrib>Santander, M</creatorcontrib><creatorcontrib>Shahinyan, K</creatorcontrib><creatorcontrib>Smith, A W</creatorcontrib><creatorcontrib>Staszak, D</creatorcontrib><creatorcontrib>Telezhinsky, I</creatorcontrib><creatorcontrib>Todd, N W</creatorcontrib><creatorcontrib>Tucci, J V</creatorcontrib><creatorcontrib>Tyler, 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J</creatorcontrib><creatorcontrib>Graham, M J</creatorcontrib><creatorcontrib>Mahabal, A</creatorcontrib><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>Materials Science & Engineering Collection</collection><collection>ProQuest Central (Alumni)</collection><collection>ProQuest Central</collection><collection>ProQuest Central Essentials</collection><collection>ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central</collection><collection>SciTech Premium Collection</collection><collection>ProQuest Engineering Collection</collection><collection>Engineering Database</collection><collection>Publicly Available Content Database</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central China</collection><collection>Engineering Collection</collection><jtitle>arXiv.org</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Abeysekara, A U</au><au>Archambault, S</au><au>Archer, A</au><au>Aune, T</au><au>Barnacka, A</au><au>Benbow, W</au><au>Bird, R</au><au>Biteau, J</au><au>Buckley, J H</au><au>Bugaev, V</au><au>Cardenzana, J V</au><au>Cerruti, M</au><au>Chen, X</au><au>Christiansen, J L</au><au>Ciupik, L</au><au>Connolly, M P</au><au>Coppi, P</au><au>Cui, W</au><au>Dickinson, H J</au><au>Eisch, J D</au><au>Errando, M</au><au>Falcone, A</au><au>Feng, Q</au><au>Finley, J P</au><au>Fleischhack, H</au><au>Flinders, A</au><au>tin, P</au><au>tson, L</au><au>Furniss, A</au><au>Griffin, S</au><au>Grube, J</au><au>Gyuk, G</au><au>Hütten, M</au><au>Håkansson, N</au><au>Hanna, D</au><au>Holder, J</au><au>Humensky, T B</au><au>Johnson, C A</au><au>Kaaret, P</au><au>Kar, P</au><au>Kelley-Hoskins, N</au><au>Khassen, Y</au><au>Kieda, D</au><au>Krause, M</au><au>Krennrich, F</au><au>Kumar, S</au><au>Lang, M J</au><au>Maier, G</au><au>McArthur, S</au><au>McCann, A</au><au>Meagher, K</au><au>Moriarty, P</au><au>Mukherjee, R</au><au>Nieto, D</au><au>A O'Faoláin de Bhróithe</au><au>Ong, R A</au><au>Otte, A N</au><au>Park, N</au><au>Perkins, J S</au><au>Petrashyk, A</au><au>Pohl, M</au><au>Pueschel, E</au><au>Quinn, J</au><au>Ragan, K</au><au>Ratliff, G</au><au>Reynolds, P T</au><au>Richards, G T</au><au>Roache, E</au><au>Santander, M</au><au>Shahinyan, K</au><au>Smith, A W</au><au>Staszak, D</au><au>Telezhinsky, I</au><au>Todd, N W</au><au>Tucci, J V</au><au>Tyler, J</au><au>Vassiliev, V V</au><au>Vincent, S</au><au>Wakely, S P</au><au>Weiner, O M</au><au>Weinstein, A</au><au>Wilhelm, A</au><au>Williams, D A</au><au>Zitzer, B</au><au>Smith, P S</au><au>Holoien, T W -S</au><au>Kochanek, C S</au><au>Stanek, K Z</au><au>Shappee, B</au><au>Hovatta, T</au><au>Max-Moerbeck, W</au><au>Pearson, T J</au><au>Reeves, R A</au><au>Richards, J L</au><au>Readhead, A C S</au><au>Madejski, G M</au><au>Djorgovski, S G</au><au>Drake, A J</au><au>Graham, M J</au><au>Mahabal, A</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Gamma rays from the quasar PKS 1441+25: story of an escape</atitle><jtitle>arXiv.org</jtitle><date>2015-12-14</date><risdate>2015</risdate><eissn>2331-8422</eissn><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.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><doi>10.48550/arxiv.1512.04434</doi><oa>free_for_read</oa></addata></record> |
fulltext | fulltext |
identifier | EISSN: 2331-8422 |
ispartof | arXiv.org, 2015-12 |
issn | 2331-8422 |
language | eng |
recordid | cdi_proquest_journals_2083823896 |
source | Publicly Available Content Database |
subjects | Active galactic nuclei Background radiation Diffuse radiation Emission Galaxies Gamma rays Outbursts Photons Quasars Supermassive black holes Universe Wavelengths |
title | Gamma rays from the quasar PKS 1441+25: story of an escape |
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