WFRF:(Do Couto e Silva E.)
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| Fältnamn | Indikatorer | Metadata |
|---|---|---|
| 000 | 08235naa a2202089 4500 | |
| 001 | oai:DiVA.org:kth-160744 | |
| 003 | SwePub | |
| 008 | 150227s2015 | |||||||||||000 ||eng| | |
| 009 | oai:DiVA.org:su-114389 | |
| 024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-1607442 URI |
| 024 | 7 | a https://doi.org/10.1088/0004-637X/799/1/862 DOI |
| 024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-1143892 URI |
| 040 | a (SwePub)kthd (SwePub)su | |
| 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 The spectrum of isotropic diffuse gamma-ray emission between 100 MeV and 820 GeV |
| 264 | 1 | c 2015 |
| 338 | a print2 rdacarrier | |
| 500 | a QC 20150203 | |
| 500 | a AuthorCount:144; | |
| 520 | a The gamma-ray sky can be decomposed into individually detected sources, diffuse emission attributed to the interactions of Galactic cosmic rays with gas and radiation fields, and a residual all-sky emission component commonly called the isotropic diffuse gamma-ray background (IGRB). The IGRB comprises all extragalactic emissions too faint or too diffuse to be resolved in a given survey, as well as any residual Galactic foregrounds that are approximately isotropic. The first IGRB measurement with the Large Area Telescope (LAT) on board the Fermi Gamma-ray Space Telescope (Fermi) used 10 months of sky-survey data and considered an energy range between 200 MeV and 100 GeV. Improvements in event selection and characterization of cosmic-ray backgrounds, better understanding of the diffuse Galactic emission (DGE), and a longer data accumulation of 50 months allow for a refinement and extension of the IGRB measurement with the LAT, now covering the energy range from 100 MeV to 820 GeV. The IGRB spectrum shows a significant high-energy cutoff feature and can be well described over nearly four decades in energy by a power law with exponential cutoff having a spectral index of 2.32 +/- 0.02 and a break energy of (279 +/- 52) GeV using our baseline DGE model. The total intensity attributed to the IGRB is (7.2 +/- 0.6) x 10(-6) cm(-2) s(-1) sr(-1) above 100 MeV, with an additional +15%/-30% systematic uncertainty due to the Galactic diffuse foregrounds. | |
| 650 | 7 | a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe |
| 650 | 7 | a NATURAL SCIENCESx Physical Sciencesx Astronomy, Astrophysics and Cosmology0 (SwePub)103052 hsv//eng |
| 653 | a diffuse radiation | |
| 653 | a gamma rays: diffuse background | |
| 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 Bottacini, E.4 aut |
| 700 | 1 | a Brandt, T. J.4 aut |
| 700 | 1 | a Bregeon, J.4 aut |
| 700 | 1 | a Bruel, P.4 aut |
| 700 | 1 | a Buehler, R.4 aut |
| 700 | 1 | a Buson, S.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 Claus, R.4 aut |
| 700 | 1 | a Cohen-Tanugi, J.4 aut |
| 700 | 1 | a Conrad, Janu Stockholms universitet,KTH,Fysik,Stockholm University, Sweden,Fysikum,Oskar Klein-centrum för kosmopartikelfysik (OKC),Royal Swedish Academy of Sciences, Sweden4 aut0 (Swepub:su)conrad |
| 700 | 1 | a Cuoco, A.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 Dermer, C. D.4 aut |
| 700 | 1 | a Digel, S. W.4 aut |
| 700 | 1 | a do Couto e Silva, E.4 aut |
| 700 | 1 | a Drell, P. S.4 aut |
| 700 | 1 | a Favuzzi, C.4 aut |
| 700 | 1 | a Ferrara, E. C.4 aut |
| 700 | 1 | a Focke, W. B.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 Germani, S.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 Gomez-Vargas, G. A.4 aut |
| 700 | 1 | a Grenier, I. A.4 aut |
| 700 | 1 | a Guiriec, S.4 aut |
| 700 | 1 | a Gustafsson, M.4 aut |
| 700 | 1 | a Hadasch, D.4 aut |
| 700 | 1 | a Hayashi, K.4 aut |
| 700 | 1 | a Hays, E.4 aut |
| 700 | 1 | a Hewitt, J. W.4 aut |
| 700 | 1 | a Ippoliti, P.4 aut |
| 700 | 1 | a Jogler, T.4 aut |
| 700 | 1 | a Johannesson, G.4 aut |
| 700 | 1 | a Johnson, A. S.4 aut |
| 700 | 1 | a Johnson, W. N.4 aut |
| 700 | 1 | a Kamae, T.4 aut |
| 700 | 1 | a Kataoka, J.4 aut |
| 700 | 1 | a Knoedlseder, J.4 aut |
| 700 | 1 | a Kuss, M.4 aut |
| 700 | 1 | a Larsson, Stefanu Stockholms universitet,Fysikum,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC)4 aut0 (Swepub:su)slars |
| 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 Manfreda, A.4 aut |
| 700 | 1 | a Massaro, F.4 aut |
| 700 | 1 | a Mayer, M.4 aut |
| 700 | 1 | a Mazziotta, M. N.4 aut |
| 700 | 1 | a McEnery, J. E.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 Nemmen, R.4 aut |
| 700 | 1 | a Nuss, E.4 aut |
| 700 | 1 | a Ohsugi, T.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 Panetta, J. H.4 aut |
| 700 | 1 | a Perkins, J. S.4 aut |
| 700 | 1 | a Pesce-Rollins, M.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 Ritz, S.4 aut |
| 700 | 1 | a Romani, R. W.4 aut |
| 700 | 1 | a Sanchez-Conde, M.4 aut |
| 700 | 1 | a Schaal, M.4 aut |
| 700 | 1 | a Schulz, A.4 aut |
| 700 | 1 | a Sgro, C.4 aut |
| 700 | 1 | a Siskind, E. J.4 aut |
| 700 | 1 | a Spandre, G.4 aut |
| 700 | 1 | a Spinelli, P.4 aut |
| 700 | 1 | a Strong, A. W.4 aut |
| 700 | 1 | a Suson, D. J.4 aut |
| 700 | 1 | a Takahashi, H.4 aut |
| 700 | 1 | a Thayer, J. G.4 aut |
| 700 | 1 | a Thayer, J. B.4 aut |
| 700 | 1 | a Tibaldo, L.4 aut |
| 700 | 1 | a Tinivella, M.4 aut |
| 700 | 1 | a Torres, D. F.4 aut |
| 700 | 1 | a Tosti, G.4 aut |
| 700 | 1 | a Troja, E.4 aut |
| 700 | 1 | a Uchiyama, Y.4 aut |
| 700 | 1 | a Vianello, G.4 aut |
| 700 | 1 | a Werner, M.4 aut |
| 700 | 1 | a Winer, B. L.4 aut |
| 700 | 1 | a Wood, K. S.4 aut |
| 700 | 1 | a Wood, M.4 aut |
| 700 | 1 | a Zaharijas, G.4 aut |
| 700 | 1 | a Zimmer, Stephanu Stockholms universitet,Fysikum,Oskar Klein-centrum för kosmopartikelfysik (OKC)4 aut0 (Swepub:su)stzi0820 |
| 710 | 2 | a KTHb Fysik4 org |
| 773 | 0 | t Astrophysical Journalg 799:1, s. 86-q 799:1<86-x 0004-637Xx 1538-4357 |
| 856 | 4 | u https://arxiv.org/abs/1410.3696y arXiv:1410.3696 |
| 856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-160744 |
| 856 | 4 8 | u https://doi.org/10.1088/0004-637X/799/1/86 |
| 856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-114389 |
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- Ackermann, M.
- Ajello, M.
- Albert, A.
- Atwood, W. B.
- Baldini, L.
- Ballet, J.
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- Barbiellini, G.
- Bastieri, D.
- Bechtol, K.
- Bellazzini, R.
- Bissaldi, E.
- Blandford, R. D.
- Bloom, E. D.
- Bottacini, E.
- Brandt, T. J.
- Bregeon, J.
- Bruel, P.
- Buehler, R.
- Buson, S.
- Caliandro, G. A.
- Cameron, R. A.
- Caragiulo, M.
- Caraveo, P. A.
- Cavazzuti, E.
- Cecchi, C.
- Charles, E.
- Chekhtman, A.
- Chiang, J.
- Chiaro, G.
- Ciprini, S.
- Claus, R.
- Cohen-Tanugi, J.
- Conrad, Jan
- Cuoco, A.
- Cutini, S.
- D'Ammando, F.
- de Angelis, A.
- de Palma, F.
- Dermer, C. D.
- Digel, S. W.
- do Couto e Silva ...
- Drell, P. S.
- Favuzzi, C.
- Ferrara, E. C.
- Focke, W. B.
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- Funk, S.
- Fusco, P.
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- Giordano, F.
- Giroletti, M.
- Godfrey, G.
- Gomez-Vargas, G. ...
- Grenier, I. A.
- Guiriec, S.
- Gustafsson, M.
- Hadasch, D.
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- Hays, E.
- Hewitt, J. W.
- Ippoliti, P.
- Jogler, T.
- Johannesson, G.
- Johnson, A. S.
- Johnson, W. N.
- Kamae, T.
- Kataoka, J.
- Knoedlseder, J.
- Kuss, M.
- Larsson, Stefan
- Latronico, L.
- Li, J.
- Li, L.
- Longo, F.
- Loparco, F.
- Lott, B.
- Lovellette, M. N ...
- Lubrano, P.
- Madejski, G. M.
- Manfreda, A.
- Massaro, F.
- Mayer, M.
- Mazziotta, M. N.
- McEnery, J. E.
- Michelson, P. F.
- Mitthumsiri, W.
- Mizuno, T.
- Moiseev, A. A.
- Monzani, M. E.
- Morselli, A.
- Moskalenko, I. V ...
- Murgia, S.
- Nemmen, R.
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- Ohsugi, T.
- Omodei, N.
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- Porter, T. A.
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- Reimer, O.
- Reposeur, T.
- Ritz, S.
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- Sanchez-Conde, M ...
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- Schulz, A.
- Sgro, C.
- Siskind, E. J.
- Spandre, G.
- Spinelli, P.
- Strong, A. W.
- Suson, D. J.
- Takahashi, H.
- Thayer, J. G.
- Thayer, J. B.
- Tibaldo, L.
- Tinivella, M.
- Torres, D. F.
- Tosti, G.
- Troja, E.
- Uchiyama, Y.
- Vianello, G.
- Werner, M.
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- Wood, K. S.
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