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dc.date.accessioned | 2019-12-16T16:14:45Z | |
dc.date.available | 2019-12-16T16:14:45Z | |
dc.date.issued | 2017-03-09 | |
dc.identifier.uri | http://sedici.unlp.edu.ar/handle/10915/87493 | |
dc.description.abstract | Simultaneous measurements of air showers with the fluorescence and surface detectors of the Pierre Auger Observatory allow a sensitive search for EeV photon point sources. Several Galactic and extragalactic candidate objects are grouped in classes to reduce the statistical penalty of many trials from that of a blind search and are analyzed for a significant excess above the background expectation. The presented search does not find any evidence for photon emission at candidate sources, and combined p-values for every class are reported. Particle and energy flux upper limits are given for selected candidate sources. These limits significantly constrain predictions of EeV proton emission models from non-transient Galactic and nearby extragalactic sources, as illustrated for the particular case of the Galactic center region. | en |
dc.language | en | es |
dc.subject | astroparticle physics | es |
dc.subject | cosmic rays | es |
dc.subject | methods: data analysis | es |
dc.title | A Targeted Search for Point Sources of EeV Photons with the Pierre Auger Observatory | en |
dc.type | Articulo | es |
sedici.identifier.other | doi:10.3847/2041-8213/aa61a5 | es |
sedici.identifier.other | eid:2-s2.0-85016166402 | es |
sedici.identifier.issn | 2041-8205 | es |
sedici.creator.person | Dova, María Teresa | es |
sedici.creator.person | Hansen, Patricia María | es |
sedici.creator.person | Mariazzi, Analisa Gabriela | es |
sedici.creator.person | Sciutto, Sergio Juan | es |
sedici.creator.person | Vergara Quispe, Indira Dajhana | es |
sedici.creator.person | Wahlberg, Hernán Pablo | es |
sedici.description.note | La lista completa de autores que integran el documento puede consultarse en el archivo | es |
sedici.subject.materias | Física | es |
sedici.subject.materias | Ciencias Exactas | es |
sedici.description.fulltext | true | es |
mods.originInfo.place | Instituto de Física La Plata | es |
sedici.subtype | Articulo | es |
sedici.rights.license | Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) | |
sedici.rights.uri | http://creativecommons.org/licenses/by-nc-sa/4.0/ | |
sedici.description.peerReview | peer-review | es |
sedici.relation.journalTitle | Astrophysical Journal Letters | es |
sedici.relation.journalVolumeAndIssue | vol. 837, no. 2 | es |
sedici.rights.sherpa | * Color: green * Pre-print del autor: si * Post-print del autor: si * Versión de editor/PDF:si * Condiciones: >>On any website, arXiv, scientific social networks (except Research Gate) or non-commercial open access repository. >>Publisher's version/PDF may be used on any website or authors' institutional repository >>Publisher copyright and source must be acknowledged >>Must link to publisher version >>Publisher's version/PDF may be used >>Authors depositing in arXiv must they choose the first licence statement offered by arXiv when uploading their article � a "non-exclusive licence to distribute" >>Publisher last contacted on 10/02/2016 >>Publisher last reviewed on 15/08/2017 * Link a Sherpa: http://sherpa.ac.uk/romeo/issn/2041-8205/es/ |