A SEARCH FOR VERY HIGH ENERGY GAMMA RAYS FROM THE MISSING LINK BINARY PULSAR J1023+0038 WITH VERITAS
dc.contributor.author | Aliu, E. | |
dc.contributor.author | Archambault, S. | |
dc.contributor.author | Archer, A. | |
dc.contributor.author | Benbow, W. | |
dc.contributor.author | Bird, R. | |
dc.contributor.author | Biteau, J. | |
dc.contributor.author | Buchovecky, M. | |
dc.contributor.author | Buckley, J. H. | |
dc.contributor.author | Bugaev, V. | |
dc.contributor.author | Byrum, K. | |
dc.contributor.author | Cardenzana, J. V. | |
dc.contributor.author | Cerruti, M. | |
dc.contributor.author | Chen, X. | |
dc.contributor.author | Ciupik, L. | |
dc.contributor.author | Connolly, M. P. | |
dc.contributor.author | Cui, W. | |
dc.contributor.author | Dickinson, H. J. | |
dc.contributor.author | Eisch, J. D. | |
dc.contributor.author | Falcone, A. | |
dc.contributor.author | Feng, Q. | |
dc.contributor.author | Finley, J. P. | |
dc.contributor.author | Fleischhack, H. | |
dc.contributor.author | Flinders, A. | |
dc.contributor.author | Fortin, P. | |
dc.contributor.author | Fortson, L. | |
dc.contributor.author | Furniss, A. | |
dc.contributor.author | Gillanders, G. H. | |
dc.contributor.author | Griffin, S. | |
dc.contributor.author | Grube, J. | |
dc.contributor.author | Gyuk, G. | |
dc.contributor.author | Huetten, M. | |
dc.contributor.author | Hakansson, N. | |
dc.contributor.author | Holder, J. | |
dc.contributor.author | Humensky, T. B. | |
dc.contributor.author | Johnson, C. A. | |
dc.contributor.author | Kaaret, P. | |
dc.contributor.author | Kar, P. | |
dc.contributor.author | Kelley-Hoskins, N. | |
dc.contributor.author | Kertzman, M. | |
dc.contributor.author | Kieda, D. | |
dc.contributor.author | Krause, M. | |
dc.contributor.author | Lang, M. J. | |
dc.contributor.author | Loo, A. | |
dc.contributor.author | Maier, G. | |
dc.contributor.author | McArthur, S. | |
dc.contributor.author | McCann, A. | |
dc.contributor.author | Meagher, K. | |
dc.contributor.author | Moriarty, P. | |
dc.contributor.author | Mukherjee, R. | |
dc.contributor.author | Nguyen, T. | |
dc.contributor.author | Nieto, D. | |
dc.contributor.author | De Bhroithe, A. O'Faolain | |
dc.contributor.author | Ong, R. A. | |
dc.contributor.author | Otte, A. N. | |
dc.contributor.author | Pandel, D. | |
dc.contributor.author | Park, N. | |
dc.contributor.author | Pelassa, V. | |
dc.contributor.author | Petrashyk, A. | |
dc.contributor.author | Pohl, M. | |
dc.contributor.author | Popkow, A. | |
dc.contributor.author | Pueschel, E. | |
dc.contributor.author | Quinn, J. | |
dc.contributor.author | Ragan, K. | |
dc.contributor.author | Reynolds, P. T. | |
dc.contributor.author | Richards, G. T. | |
dc.contributor.author | Roache, E. | |
dc.contributor.author | Rulten, C. | |
dc.contributor.author | Santander, M. | |
dc.contributor.author | Sembroski, G. H. | |
dc.contributor.author | Shahinyan, K. | |
dc.contributor.author | Smith, A. W. | |
dc.contributor.author | Staszak, D. | |
dc.contributor.author | Telezhinsky, I. | |
dc.contributor.author | Tucci, J. V. | |
dc.contributor.author | Tyler, J. | |
dc.contributor.author | Varlotta, A. | |
dc.contributor.author | Vincent, S. | |
dc.contributor.author | Wakely, S. P. | |
dc.contributor.author | Weiner, O. M. | |
dc.contributor.author | Weinstein, A. | |
dc.contributor.author | Wilhelm, A. | |
dc.contributor.author | Williams, D. A. | |
dc.contributor.author | Zitzer, B. | |
dc.contributor.author | Chernyakova, M. | |
dc.contributor.author | Roberts, M. S. E. | |
dc.contributor.other | Columbia University | |
dc.contributor.other | McGill University | |
dc.contributor.other | Washington University (WUSTL) | |
dc.contributor.other | Harvard University | |
dc.contributor.other | Smithsonian Institution | |
dc.contributor.other | University College Dublin | |
dc.contributor.other | University of California System | |
dc.contributor.other | University of California Santa Cruz | |
dc.contributor.other | University of California Los Angeles | |
dc.contributor.other | United States Department of Energy (DOE) | |
dc.contributor.other | Argonne National Laboratory | |
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 | Ollscoil na Gaillimhe-University of Galway | |
dc.contributor.other | Purdue University System | |
dc.contributor.other | Purdue University | |
dc.contributor.other | Purdue University West Lafayette Campus | |
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 | Utah System of Higher Education | |
dc.contributor.other | University of Utah | |
dc.contributor.other | University of Minnesota System | |
dc.contributor.other | University of Minnesota Twin Cities | |
dc.contributor.other | California State University System | |
dc.contributor.other | California State University East Bay | |
dc.contributor.other | University of Delaware | |
dc.contributor.other | University of Iowa | |
dc.contributor.other | DePauw University | |
dc.contributor.other | University System of Georgia | |
dc.contributor.other | Georgia Institute of Technology | |
dc.contributor.other | Grand Valley State University | |
dc.contributor.other | University of Chicago | |
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 | Dublin City University | |
dc.contributor.other | Dublin Institute for Advanced Studies | |
dc.contributor.other | Eureka Scientific | |
dc.contributor.other | University of Alabama Tuscaloosa | |
dc.date.accessioned | 2019-06-18T13:36:52Z | |
dc.date.available | 2019-06-18T13:36:52Z | |
dc.date.issued | 2016-11-08 | |
dc.description.abstract | The binary millisecond radio pulsar PSR J1023+0038 exhibits many characteristics similar to the gamma-ray binary system PSR B1259-63/LS 2883, making it an ideal candidate for the study of high-energy nonthermal emission. It has been the subject of multiwavelength campaigns following the disappearance of the pulsed radio emission in 2013 June, which revealed the appearance of an accretion disk around the neutron star. We present the results of very high energy (VHE) gamma-ray observations carried out by the Very Energetic Radiation Imaging Telescope Array System before and after this change of state. Searches for steady and pulsed emission of both data sets yield no significant gamma-ray signal above 100 GeV, and upper limits are given for both a steady and pulsed gamma-ray flux. These upper limits are used to constrain the magnetic field strength in the shock region of the PSR J1023+0038 system. Assuming that VHE gamma rays are produced via an inverse Compton mechanism in the shock region, we constrain the shock magnetic field to be greater than similar to 2 G before the disappearance of the radio pulsar and greater than similar to 10 G afterward. | en_US |
dc.format.mimetype | application/pdf | |
dc.identifier.citation | Aliu, E., et al. (2016):A Search for Very High-Energy Gamma Rays from the Missing Link Binary Pulsar J1023+0038 with VERITAS. The Astrophysical Journal, 831(2). DOI: http://dx.doi.org/10.3847/0004-637X/831/2/193 | |
dc.identifier.doi | 10.3847/0004-637X/831/2/193 | |
dc.identifier.orcid | https://orcid.org/0000-0002-5955-6383 | |
dc.identifier.orcid | https://orcid.org/0000-0001-7891-699X | |
dc.identifier.orcid | https://orcid.org/0000-0002-2126-2419 | |
dc.identifier.orcid | https://orcid.org/0000-0001-6674-4238 | |
dc.identifier.orcid | https://orcid.org/0000-0001-7861-1707 | |
dc.identifier.orcid | https://orcid.org/0000-0003-3343-0755 | |
dc.identifier.orcid | https://orcid.org/0000-0002-6324-5772 | |
dc.identifier.orcid | https://orcid.org/0000-0002-4855-2694 | |
dc.identifier.orcid | https://orcid.org/0000-0003-4641-4201 | |
dc.identifier.orcid | https://orcid.org/0000-0001-9868-4700 | |
dc.identifier.orcid | https://orcid.org/0000-0002-0794-8780 | |
dc.identifier.orcid | https://orcid.org/0000-0003-3967-1533 | |
dc.identifier.orcid | https://orcid.org/0000-0002-5221-6669 | |
dc.identifier.orcid | https://orcid.org/0000-0003-4785-0101 | |
dc.identifier.orcid | https://orcid.org/0000-0002-2133-5251 | |
dc.identifier.orcid | https://orcid.org/0000-0001-7483-4348 | |
dc.identifier.orcid | https://orcid.org/0000-0002-4837-5253 | |
dc.identifier.orcid | https://orcid.org/0000-0002-9735-3608 | |
dc.identifier.orcid | https://orcid.org/0000-0002-1432-7771 | |
dc.identifier.orcid | https://orcid.org/0000-0002-9396-9720 | |
dc.identifier.orcid | https://orcid.org/0000-0003-2098-170X | |
dc.identifier.orcid | https://orcid.org/0000-0002-1067-8558 | |
dc.identifier.orcid | https://orcid.org/0000-0003-2085-5586 | |
dc.identifier.orcid | https://orcid.org/0000-0001-7595-0914 | |
dc.identifier.orcid | https://orcid.org/0000-0002-4596-8563 | |
dc.identifier.orcid | https://orcid.org/0000-0001-7297-8217 | |
dc.identifier.uri | http://ir.ua.edu/handle/123456789/5789 | |
dc.language | English | |
dc.language.iso | en_US | |
dc.publisher | IOP Publishing | |
dc.subject | binaries: general | |
dc.subject | gamma rays: general | |
dc.subject | pulsars: general | |
dc.subject | pulsars: individual (PSR J1023+0038) | |
dc.subject | NUSTAR OBSERVATIONS | |
dc.subject | PSR J1023+0038 | |
dc.subject | STATE CHANGE | |
dc.subject | EMISSION | |
dc.subject | TRANSITION | |
dc.subject | PERIASTRON | |
dc.subject | DISCOVERY | |
dc.subject | FERMI | |
dc.subject | Astronomy & Astrophysics | |
dc.title | A SEARCH FOR VERY HIGH ENERGY GAMMA RAYS FROM THE MISSING LINK BINARY PULSAR J1023+0038 WITH VERITAS | en_US |
dc.type | text | |
dc.type | Article |
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