Sökning: WFRF:(Lande J. D.) > Fermi Observations ...
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000 | 11931naa a2203481 4500 | |
001 | oai:DiVA.org:hik-2829 | |
003 | SwePub | |
008 | 100223s2009 | |||||||||||000 ||eng| | |
009 | oai:DiVA.org:su-26499 | |
009 | oai:DiVA.org:kth-32187 | |
024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:hik:diva-28292 URI |
024 | 7 | a https://doi.org/10.1126/science.11691012 DOI |
024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-264992 URI |
024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-321872 URI |
040 | a (SwePub)lnud (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 Abdo, A. A.4 aut |
245 | 1 0 | a Fermi Observations of High-Energy Gamma-Ray Emission from GRB 080916C |
264 | 1 | b American Association for the Advancement of Science (AAAS),c 2009 |
338 | a print2 rdacarrier | |
500 | a QC 20110408 | |
520 | a Gamma-ray bursts (GRBs) are highly energetic explosions signaling the death of massive stars in distant galaxies. The Gamma-ray Burst Monitor and Large Area Telescope onboard the Fermi Observatory together record GRBs over a broad energy range spanning about 7 decades of gamma-ray energy. In September 2008, Fermi observed the exceptionally luminous GRB 080916C, with the largest apparent energy release yet measured. The high-energy gamma rays are observed to start later and persist longer than the lower energy photons. A simple spectral form fits the entire GRB spectrum, providing strong constraints on emission models. The known distance of the burst enables placing lower limits on the bulk Lorentz factor of the outflow and on the quantum gravity mass. | |
650 | 7 | a NATURVETENSKAPx Fysik0 (SwePub)1032 hsv//swe |
650 | 7 | a NATURAL SCIENCESx Physical Sciences0 (SwePub)1032 hsv//eng |
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 Fysik | |
653 | a Physics | |
653 | a High energy astrophysics | |
653 | a Astronomy | |
653 | a BURST SPECTRA | |
653 | a Astronomy and astrophysics | |
700 | 1 | a Ackermann, M.4 aut |
700 | 1 | a Arimoto, M.4 aut |
700 | 1 | a Asano, K.4 aut |
700 | 1 | a Atwood, W. B.4 aut |
700 | 1 | a Axelsson, M.u Stockholms universitet,Institutionen för astronomi4 aut |
700 | 1 | a Baldini, L.4 aut |
700 | 1 | a Ballet, J.4 aut |
700 | 1 | a Band, D. L.4 aut |
700 | 1 | a Barbiellini, G.4 aut |
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700 | 1 | a Bastieri, D.4 aut |
700 | 1 | a Battelino, Milanu KTH,Partikel- och astropartikelfysik4 aut0 (Swepub:kth)u18q1oud |
700 | 1 | a Baughman, B. M.4 aut |
700 | 1 | a Bechtol, K.4 aut |
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700 | 1 | a Brigida, M.4 aut |
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710 | 2 | a Stockholms universitetb Institutionen för astronomi4 org |
773 | 0 | t Scienced : American Association for the Advancement of Science (AAAS)g 323:5922, s. 1688-1693q 323:5922<1688-1693x 0036-8075x 1095-9203 |
856 | 4 | u https://www.osti.gov/biblio/1357451 |
856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:hik:diva-2829 |
856 | 4 8 | u https://doi.org/10.1126/science.1169101 |
856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-26499 |
856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-32187 |
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