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LIBRIS Formathandbok (Information om MARC21)
| Fältnamn | Indikatorer | Metadata |
|---|---|---|
| 000 | 07736naa a2201885 4500 | |
| 001 | oai:DiVA.org:su-130165 | |
| 003 | SwePub | |
| 008 | 160509s2016 | |||||||||||000 ||eng| | |
| 009 | oai:DiVA.org:kth-187719 | |
| 024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-1301652 URI |
| 024 | 7 | a https://doi.org/10.1103/PhysRevLett.116.1511052 DOI |
| 024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-1877192 URI |
| 040 | a (SwePub)sud (SwePub)kth | |
| 041 | a engb eng | |
| 042 | 9 SwePub | |
| 072 | 7 | a ref2 swepub-contenttype |
| 072 | 7 | a art2 swepub-publicationtype |
| 100 | 1 | a Ackermann, M.4 aut |
| 245 | 1 0 | a Resolving the Extragalactic gamma-Ray Background above 50 GeV with the Fermi Large Area Telescope |
| 264 | 1 | b American Physical Society,c 2016 |
| 338 | a print2 rdacarrier | |
| 500 | a QC 20160527 | |
| 520 | a The Fermi Large Area Telescope (LAT) Collaboration has recently released a catalog of 360 sources detected above 50 GeV (2FHL). This catalog was obtained using 80 months of data re-processed with Pass 8, the newest event-level analysis, which significantly improves the acceptance and angular resolution of the instrument. Most of the 2FHL sources at high Galactic latitude are blazars. Using detailed Monte Carlo simulations, we measure, for the first time, the source count distribution, dN= dS, of extragalactic.-ray sources at E > 50 GeV and find that it is compatible with a Euclidean distribution down to the lowest measured source flux in the 2FHL (8 x 10(-12) ph cm(-2) s(-1)). We employ a one-point photon fluctuation analysis to constrain the behavior of dN= dS below the source detection threshold. Overall, the source count distribution is constrained over three decades in flux and found compatible with a broken power law with a break flux, Sb, in the range [8 x 10-12; 1.5 x 10-11] ph cm(-2) s(-1) and power-law indices below and above the break of a 2. [1.60; 1.75] and a 1 +/- 2.49 +/- 0.12, respectively. Integration of dN= dS shows that point sources account for at least 86_16 -14 % of the total extragalactic gamma-ray background. The simple form of the derived source count distribution is consistent with a single population (i. e., blazars) dominating the source counts to the minimum flux explored by this analysis. We estimate the density of sources detectable in blind surveys that will be performed in the coming years by the Cherenkov Telescope Array. | |
| 650 | 7 | a NATURVETENSKAPx Fysik0 (SwePub)1032 hsv//swe |
| 650 | 7 | a NATURAL SCIENCESx Physical Sciences0 (SwePub)1032 hsv//eng |
| 653 | a Intelligent systems | |
| 700 | 1 | a Ajello, M.4 aut |
| 700 | 1 | a Albert, A.4 aut |
| 700 | 1 | a Atwood, W. B.4 aut |
| 700 | 1 | a Baldini, L.4 aut |
| 700 | 1 | a Ballet, J.4 aut |
| 700 | 1 | a Barbiellini, G.4 aut |
| 700 | 1 | a Bastieri, D.4 aut |
| 700 | 1 | a Bechtol, K.4 aut |
| 700 | 1 | a Bellazzini, R.4 aut |
| 700 | 1 | a Bissaldi, E.4 aut |
| 700 | 1 | a Blandford, R. D.4 aut |
| 700 | 1 | a Bloom, E. D.4 aut |
| 700 | 1 | a Bonino, R.4 aut |
| 700 | 1 | a Bregeon, J.4 aut |
| 700 | 1 | a Britto, R. J.4 aut |
| 700 | 1 | a Bruel, P.4 aut |
| 700 | 1 | a Buehler, R.4 aut |
| 700 | 1 | a Caliandro, G. A.4 aut |
| 700 | 1 | a Cameron, R. A.4 aut |
| 700 | 1 | a Caragiulo, M.4 aut |
| 700 | 1 | a Caraveo, P. A.4 aut |
| 700 | 1 | a Cavazzuti, E.4 aut |
| 700 | 1 | a Cecchi, C.4 aut |
| 700 | 1 | a Charles, E.4 aut |
| 700 | 1 | a Chekhtman, A.4 aut |
| 700 | 1 | a Chiang, J.4 aut |
| 700 | 1 | a Chiaro, G.4 aut |
| 700 | 1 | a Ciprini, S.4 aut |
| 700 | 1 | a Cohen-Tanugi, J.4 aut |
| 700 | 1 | a Li, L.u KTH,Partikel- och astropartikelfysik,Oskar Klein Centre for Cosmoparticle Physics, Sweden4 aut0 (Swepub:kth)- |
| 700 | 1 | a Costanza, F.4 aut |
| 700 | 1 | a Cutini, S.4 aut |
| 700 | 1 | a D'Ammando, F.4 aut |
| 700 | 1 | a de Angelis, A.4 aut |
| 700 | 1 | a de Palma, F.4 aut |
| 700 | 1 | a Desiante, R.4 aut |
| 700 | 1 | a Digel, S. W.4 aut |
| 700 | 1 | a Di Mauro, M.4 aut |
| 700 | 1 | a Di Venere, L.4 aut |
| 700 | 1 | a Dominguez, A.4 aut |
| 700 | 1 | a Drell, P. S.4 aut |
| 700 | 1 | a Favuzzi, C.4 aut |
| 700 | 1 | a Fegan, S. J.4 aut |
| 700 | 1 | a Ferrara, E. C.4 aut |
| 700 | 1 | a Franckowiak, A.4 aut |
| 700 | 1 | a Fukazawa, Y.4 aut |
| 700 | 1 | a Funk, S.4 aut |
| 700 | 1 | a Fusco, P.4 aut |
| 700 | 1 | a Gargano, F.4 aut |
| 700 | 1 | a Gasparrini, D.4 aut |
| 700 | 1 | a Giglietto, N.4 aut |
| 700 | 1 | a Giommi, P.4 aut |
| 700 | 1 | a Giordano, F.4 aut |
| 700 | 1 | a Giroletti, M.4 aut |
| 700 | 1 | a Godfrey, G.4 aut |
| 700 | 1 | a Green, D.4 aut |
| 700 | 1 | a Grenier, I. A.4 aut |
| 700 | 1 | a Guiriec, S.4 aut |
| 700 | 1 | a Hays, E.4 aut |
| 700 | 1 | a Horan, D.4 aut |
| 700 | 1 | a Iafrate, G.4 aut |
| 700 | 1 | a Jogler, T.4 aut |
| 700 | 1 | a Johannesson, G.4 aut |
| 700 | 1 | a Kuss, M.4 aut |
| 700 | 1 | a La Mura, G.4 aut |
| 700 | 1 | a Larsson, Stefanu KTH,Partikel- och astropartikelfysik,Oskar Klein Centre for Cosmoparticle Physics, Sweden4 aut0 (Swepub:kth)u1xfjjbn |
| 700 | 1 | a Latronico, L.4 aut |
| 700 | 1 | a Li, J.4 aut |
| 700 | 1 | a Li, L.4 aut |
| 700 | 1 | a Longo, F.4 aut |
| 700 | 1 | a Loparco, F.4 aut |
| 700 | 1 | a Lott, B.4 aut |
| 700 | 1 | a Lovellette, M. N.4 aut |
| 700 | 1 | a Lubrano, P.4 aut |
| 700 | 1 | a Madejski, G. M.4 aut |
| 700 | 1 | a Magill, J.4 aut |
| 700 | 1 | a Maldera, S.4 aut |
| 700 | 1 | a Manfreda, A.4 aut |
| 700 | 1 | a Mayer, M.4 aut |
| 700 | 1 | a Mazziotta, M. N.4 aut |
| 700 | 1 | a Michelson, P. F.4 aut |
| 700 | 1 | a Mitthumsiri, W.4 aut |
| 700 | 1 | a Mizuno, T.4 aut |
| 700 | 1 | a Moiseev, A. A.4 aut |
| 700 | 1 | a Monzani, M. E.4 aut |
| 700 | 1 | a Morselli, A.4 aut |
| 700 | 1 | a Moskalenko, I. V.4 aut |
| 700 | 1 | a Murgia, S.4 aut |
| 700 | 1 | a Negro, M.4 aut |
| 700 | 1 | a Nuss, E.4 aut |
| 700 | 1 | a Ohsugi, T.4 aut |
| 700 | 1 | a Okada, C.4 aut |
| 700 | 1 | a Omodei, N.4 aut |
| 700 | 1 | a Orlando, E.4 aut |
| 700 | 1 | a Ormes, J. F.4 aut |
| 700 | 1 | a Paneque, D.4 aut |
| 700 | 1 | a Perkins, J. S.4 aut |
| 700 | 1 | a Pesce-Rollins, M.4 aut |
| 700 | 1 | a Petrosian, V.4 aut |
| 700 | 1 | a Piron, F.4 aut |
| 700 | 1 | a Pivato, G.4 aut |
| 700 | 1 | a Porter, T. A.4 aut |
| 700 | 1 | a Raino, S.4 aut |
| 700 | 1 | a Rando, R.4 aut |
| 700 | 1 | a Razzano, M.4 aut |
| 700 | 1 | a Razzaque, S.4 aut |
| 700 | 1 | a Reimer, A.4 aut |
| 700 | 1 | a Reimer, O.4 aut |
| 700 | 1 | a Reposeur, T.4 aut |
| 700 | 1 | a Romani, R. W.4 aut |
| 700 | 1 | a Sanchez-Conde, Miguelu Stockholms universitet,Fysikum,Oskar Klein-centrum för kosmopartikelfysik (OKC)4 aut |
| 700 | 1 | a Schmid, J.4 aut |
| 700 | 1 | a Schulz, A.4 aut |
| 700 | 1 | a Sgro, C.4 aut |
| 700 | 1 | a Simone, D.4 aut |
| 700 | 1 | a Siskind, E. J.4 aut |
| 700 | 1 | a Spada, F.4 aut |
| 700 | 1 | a Spandre, G.4 aut |
| 700 | 1 | a Spinelli, P.4 aut |
| 700 | 1 | a Suson, D. J.4 aut |
| 700 | 1 | a Takahashi, H.4 aut |
| 700 | 1 | a Thayer, J. B.4 aut |
| 700 | 1 | a Tibaldo, L.4 aut |
| 700 | 1 | a Torres, D. F.4 aut |
| 700 | 1 | a Troja, E.4 aut |
| 700 | 1 | a Vianello, G.4 aut |
| 700 | 1 | a Yassine, M.4 aut |
| 700 | 1 | a Zimmer, Stephanu Stockholms universitet,Fysikum,Oskar Klein-centrum för kosmopartikelfysik (OKC)4 aut |
| 710 | 2 | a KTHb Partikel- och astropartikelfysik4 org |
| 773 | 0 | t Physical Review Lettersd : American Physical Societyg 116:15q 116:15x 0031-9007x 1079-7114 |
| 856 | 4 | u https://doi.org/10.1103/PhysRevLett.116.151105y Fulltext |
| 856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-130165 |
| 856 | 4 8 | u https://doi.org/10.1103/PhysRevLett.116.151105 |
| 856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-187719 |
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- Desiante, R.
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- Michelson, P. F.
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