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000 | 09849naa a2202833 4500 | |
001 | oai:DiVA.org:kth-27355 | |
003 | SwePub | |
008 | 101213s2010 | |||||||||||000 ||eng| | |
009 | oai:DiVA.org:su-51369 | |
024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-273552 URI |
024 | 7 | a https://doi.org/10.1103/PhysRevD.82.0920042 DOI |
024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-513692 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 Fermi LAT observations of cosmic-ray electrons from 7 GeV to 1 TeV |
264 | 1 | c 2010 |
338 | a print2 rdacarrier | |
500 | a QC 20101214 | |
500 | a authorCount :195 | |
520 | a We present the results of our analysis of cosmic-ray electrons using about 8 x 10(6) electron candidates detected in the first 12 months on-orbit by the Fermi Large Area Telescope. This work extends our previously published cosmic-ray electron spectrum down to 7 GeV, giving a spectral range of approximately 2.5 decades up to 1 TeV. We describe in detail the analysis and its validation using beam-test and on-orbit data. In addition, we describe the spectrum measured via a subset of events selected for the best energy resolution as a cross-check on the measurement using the full event sample. Our electron spectrum can be described with a power law proportional to E-3.08+/-0.05 with no prominent spectral features within systematic uncertainties. Within the limits of our uncertainties, we can accommodate a slight spectral hardening at around 100 GeV and a slight softening above 500 GeV. | |
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 large-area telescope | |
653 | a space-telescope | |
653 | a energy-spectra | |
653 | a solar minimum | |
653 | a positrons | |
653 | a propagation | |
653 | a modulation | |
653 | a spectrometer | |
653 | a galaxy | |
653 | a Physics | |
653 | a Fysik | |
700 | 1 | a Ajello, M.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 |
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700 | 1 | a Bechtol, K.4 aut |
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700 | 1 | a Belli, F.4 aut |
700 | 1 | a Berenji, B.4 aut |
700 | 1 | a Blandford, R. D.4 aut |
700 | 1 | a Bloom, E. D.4 aut |
700 | 1 | a Ripken, Joachimu Stockholms universitet,Fysikum4 aut0 (Swepub:su)ripken |
700 | 1 | a Bonamente, E.4 aut |
700 | 1 | a Borgland, A. W.4 aut |
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700 | 1 | a Garde, Maja Llenau Stockholms universitet,Fysikum4 aut0 (Swepub:su)mgarde |
700 | 1 | a Longo, F.4 aut |
700 | 1 | a Loparco, F.4 aut |
700 | 1 | a Lott, B.4 aut |
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700 | 1 | a Siskind, E. J.4 aut |
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700 | 1 | a Spinelli, P.4 aut |
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700 | 1 | a Wood, K. S.4 aut |
700 | 1 | a Yang, Zhaoyuu Stockholms universitet,Fysikum4 aut0 (Swepub:su)zhaoyu |
700 | 1 | a Ylinen, Tomiu KTH,Partikel- och astropartikelfysik4 aut0 (Swepub:kth)u1vmovqg |
700 | 1 | a Ziegler, M.4 aut |
710 | 2 | a Stockholms universitetb Fysikum4 org |
773 | 0 | t PHYSICAL REVIEW Dg 82:9, s. 092004-q 82:9<092004-x 1550-7998 |
773 | 0 | t Physical Review D. Particles and fieldsg 82:9, s. 092004-q 82:9<092004-x 0556-2821x 1089-4918 |
856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-27355 |
856 | 4 8 | u https://doi.org/10.1103/PhysRevD.82.092004 |
856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-51369 |
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