{ "id": "1704.07195", "version": "v1", "published": "2017-04-24T13:00:38.000Z", "updated": "2017-04-24T13:00:38.000Z", "title": "Cosmic-ray electron+positron spectrum from 7 GeV to 2 TeV with the Fermi Large Area Telescope", "authors": [ "Fermi-LAT Collaboration", ":", "S. Abdollahi", "M. Ackermann", "M. Ajello", "W. B. Atwood", "L. Baldini", "G. Barbiellini", "D. Bastieri", "R. Bellazzini", "E. D. Bloom", "R. Bonino", "T. J. Brandt", "J. Bregeon", "P. Bruel", "R. Buehler", "R. A. Cameron", "R. Caputo", "M. Caragiulo", "D. Castro", "E. Cavazzuti", "C. Cecchi", "A. Chekhtman", "S. Ciprini", "J. Cohen-Tanugi", "F. Costanza", "A. Cuoco", "S. Cutini", "F. D'Ammando", "F. de Palma", "R. Desiante", "S. W. Digel", "N. Di Lalla", "M. Di Mauro", "L. Di Venere", "P. S. Drell", "A. Drlica-Wagner", "C. Favuzzi", "W. B. Focke", "S. Funk", "P. Fusco", "F. Gargano", "D. Gasparrini", "N. Giglietto", "F. Giordano", "M. Giroletti", "D. Green", "L. Guillemot", "S. Guiriec", "A. K. Harding", "T. Jogler", "G. Jóhannesson", "T. Kamae", "M. Kuss", "G. La Mura", "L. Latronico", "F. Longo", "F. Loparco", "P. Lubrano", "S. Maldera", "D. Malyshev", "A. Manfreda", "M. N. Mazziotta", "P. F. Michelson", "N. Mirabal", "W. Mitthumsiri", "T. Mizuno", "A. A. Moiseev", "M. E. Monzani", "A. Morselli", "I. V. Moskalenko", "M. Negro", "E. Nuss", "E. Orlando", "D. Paneque", "J. S. Perkins", "M. Pesce-Rollins", "F. Piron", "G. Pivato", "T. A. Porter", "G. Principe", "S. Rainò", "R. Rando", "M. Razzano", "A. Reimer", "O. Reimer", "C. Sgrò", "D. Simone", "E. J. Siskind", "F. Spada", "G. Spandre", "P. Spinelli", "H. Tajima", "J. B. Thayer", "L. Tibaldo", "D. F. Torres", "E. Troja", "M. Wood", "A. Worley", "G. Zaharijas", "S. Zimmer" ], "journal": "Phys. Rev. D 95, 082007 (2017)", "doi": "10.1103/PhysRevD.95.082007", "categories": [ "astro-ph.HE" ], "abstract": "We present a measurement of the cosmic-ray electron+positron spectrum between 7 GeV and 2 TeV performed with almost seven years of data collected with the Fermi Large Area Telescope. We find that the spectrum is well fit by a broken power law with a break energy at about 50 GeV. Above 50 GeV, the spectrum is well described by a single power law with a spectral index of $3.07 \\pm 0.02 \\; (\\text{stat+syst}) \\pm 0.04 \\; (\\text{energy measurement})$. An exponential cutoff lower than 1.8 TeV is excluded at 95\\% CL.", "revisions": [ { "version": "v1", "updated": "2017-04-24T13:00:38.000Z" } ], "analyses": { "keywords": [ "fermi large area telescope", "cosmic-ray", "single power law", "broken power law", "exponential cutoff lower" ], "tags": [ "journal article" ], "publication": { "publisher": "APS", "journal": "Phys. Rev. D" }, "note": { "typesetting": "TeX", "pages": 0, "language": "en", "license": "arXiv", "status": "editable" } } }