Zobrazeno 1 - 4
of 4
pro vyhledávání: '"Venere, LD"'
Autor:
Ajello, M, Baldini, L, Barbiellini, G, Bastieri, D, Bellazzini, R, Bissaldi, E, Bloom, ED, Bonino, R, Bottacini, E, Brandt, TJ, Bregeon, J, Bruel, P, Buehler, R, Caliandro, GA, Cameron, RA, Caragiulo, M, Cavazzuti, E, Charles, E, Chekhtman, A, Ciprini, S, Cohen-Tanugi, J, Condon, B, Costanza, F, Cutini, S, D'Ammando, F, Palma, FD, Desiante, R, Lalla, ND, Mauro, MD, Venere, LD, Drell, PS, Dubner, G, Dumora, D, Duvidovich, L, Favuzzi, C, Focke, WB, Fusco, P, Gargano, F, Gasparrini, D, Giacani, E, Giglietto, N, Glanzman, T, Green, DA, Grenier, IA, Guiriec, S, Hays, E, Hewitt, JW, Hill, AB, Horan, D, Jogler, T, Jóhannesson, G, Jung-Richardt, I, Kensei, S, Kuss, M, Larsson, S, Latronico, L, Lemoine-Goumard, M, Li, J, Li, L, Longo, F, Loparco, F, Lovellette, MN, Lubrano, P, Magill, J, Maldera, S, Manfreda, A, Mayer, M, Mazziotta, MN, McEnery, JE, Michelson, PF, Mitthumsiri, W, Mizuno, T, Monzani, ME, Morselli, A, Moskalenko, IV, Negro, M, Nuss, E, Orienti, M, Orlando, E, Ormes, JF, Paneque, D, Perkins, JS, Pesce-Rollins, M, Piron, F, Pivato, G, Porter, TA, Rainò, S, Rando, R, Razzano, M, Reimer, A, Reimer, O, Reposeur, T, Schmid, J, Schulz, A, Sgrò, C, Simone, D, Siskind, EJ, Spada, F, Spandre, G, Spinelli, P
RCW 86 is a young supernova remnant (SNR) showing a shell-type structure at several wavelengths and is thought to be an efficient cosmic-ray (CR) accelerator. Earlier \textit{Fermi} Large Area Telescope results reported the detection of $\gamma$-ray
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______109::d592d655977ec702a42e43bd81265b9e
https://www.repository.cam.ac.uk/handle/1810/253526
https://www.repository.cam.ac.uk/handle/1810/253526
Autor:
Ackermann, M, Ajello, M, Albert, A, Atwood, WB, Baldini, L, Barbiellini, G, Bastieri, D, Bechtol, K, Bellazzini, R, Bissaldi, E, Bloom, ED, Bonino, R, Bottacini, E, Brandt, TJ, Bregeon, J, Bruel, P, Buehler, R, Buson, S, Caliandro, GA, Cameron, RA, Caputo, R, Caragiulo, M, Caraveo, PA, Casandjian, JM, Cavazzuti, E, Cecchi, C, Charles, E, Chekhtman, A, Chiaro, G, Ciprini, S, Cohen-Tanugi, J, Conrad, J, Cutini, S, D'Ammando, F, Angelis, AD, Palma, FD, Desiante, R, Digel, SW, Venere, LD, Drell, PS, Favuzzi, C, Fegan, SJ, Focke, WB, Franckowiak, A, Fukazawa, Y, Funk, S, Fusco, P, Gargano, F, Gasparrini, D, Giglietto, N, Giordano, F, Giroletti, M, Glanzman, T, Godfrey, G, Gomez-Vargas, GA, Grenier, IA, Guiriec, S, Gustafsson, M, Hewitt, JW, Hill, AB, Horan, D, Jeltema, TE, Jogler, T, Johnson, AS, Kuss, M, Larsson, S, Latronico, L, Li, J, Li, L, Longo, F
Publikováno v:
Ackermann, M; Ajello, M; Albert, A; Atwood, WB; Baldini, L; Barbiellini, G; et al.(2015). SEARCH for EXTENDED GAMMA-RAY EMISSION from the VIRGO GALAXY CLUSTER with FERMI-LAT. Astrophysical Journal, 812(2). doi: 10.1088/0004-637X/812/2/159. UC Irvine: Retrieved from: http://www.escholarship.org/uc/item/6k35b8wv
© 2015. The American Astronomical Society. All rights reserved.. Galaxy clusters are one of the prime sites to search for dark matter (DM) annihilation signals. Depending on the substructure of the DM halo of a galaxy cluster and the cross sections
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______325::abe90c6d197635c085acf3704ff85037
http://www.escholarship.org/uc/item/6k35b8wv
http://www.escholarship.org/uc/item/6k35b8wv
Autor:
Acero, F, Ackermann, M, Ajello, M, Albert, A, Atwood, WB, Axelsson, M, Baldini, L, Ballet, J, Barbiellini, G, Bastieri, D, Belfiore, A, Bellazzini, R, Bissaldi, E, Blandford, RD, Bloom, ED, Bogart, JR, Bonino, R, Bottacini, E, Bregeon, J, Britto, RJ, Bruel, P, Buehler, R, Burnett, TH, Buson, S, Caliandro, GA, Cameron, RA, Caputo, R, Caragiulo, M, Caraveo, PA, Casandjian, JM, Cavazzuti, E, Charles, E, Chaves, RCG, Chekhtman, A, Cheung, CC, Chiang, J, Chiaro, G, Ciprini, S, Claus, R, Cohen-Tanugi, J, Cominsky, LR, Conrad, J, Cutini, S, D'Ammando, F, Angelis, AD, Deklotz, M, Palma, FD, Desiante, R, Digel, SW, Venere, LD, Drell, PS, Dubois, R, Dumora, D, Favuzzi, C, Fegan, SJ, Ferrara, EC, Finke, J, Franckowiak, A, Fukazawa, Y, Funk, S, Fusco, P, Gargano, F, Gasparrini, D, Giebels, B, Giglietto, N, Giommi, P, Giordano, F, Giroletti, M, Glanzman, T, Godfrey, G, Grenier, IA, Grondin, MH, Grove, JE, Guillemot, L, Guiriec, S, Hadasch, D, Harding, AK, Hays, E, Hewitt, JW, Hill, AB, Horan, D, Iafrate, G, Jogler, T, Jóhannesson, G, Johnson, RP, Johnson, AS, Johnson, TJ, Johnson, WN, Kamae, T, Kataoka, J, Katsuta, J, Kuss, M, Mura, GL, Landriu, D, Larsson, S, Latronico, L, Lemoine-Goumard, M, Li, J, Li, L, Longo, F
Publikováno v:
The Astrophysical Journal Supplement Series, vol 218, iss 2
Astrophysical Journal, Supplement Series, vol 218, iss 2
Astrophysical Journal, Supplement Series, vol 218, iss 2
We present the third Fermi Large Area Telescope (LAT) source catalog (3FGL) of sources in the 100 MeV-300 GeV range. Based on the first 4 yr of science data from the Fermi Gamma-ray Space Telescope mission, it is the deepest yet in this energy range.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::a504e8a5030d4b11fd51deb3006e3c2d
https://escholarship.org/uc/item/75g478r8
https://escholarship.org/uc/item/75g478r8
Autor:
Acero, F, Ackermann, M, Ajello, M, Allafort, A, Baldini, L, Ballet, J, Barbiellini, G, Bastieri, D, Bechtol, K, Bellazzini, R, Blandford, RD, Bloom, ED, Bonamente, E, Bottacini, E, Brandt, TJ, Bregeon, J, Brigida, M, Bruel, P, Buehler, R, Buson, S, Caliandro, GA, Cameron, RA, Caraveo, PA, Cecchi, C, Charles, E, Chaves, RCG, Chekhtman, A, Chiang, J, Chiaro, G, Ciprini, S, Claus, R, Cohen-Tanugi, J, Conrad, J, Cutini, S, Dalton, M, D'Ammando, F, De Palma, F, Dermer, CD, Venere, LD, Silva, EDCE, Drell, PS, Drlica-Wagner, A, Falletti, L, Favuzzi, C, Fegan, SJ, Ferrara, EC, Focke, WB, Franckowiak, A, Fukazawa, Y, Funk, S, Fusco, P, Gargano, F, Gasparrini, D, Giglietto, N, Giordano, F, Giroletti, M, Glanzman, T, Godfrey, G, Grégoire, T, Grenier, IA, Grondin, MH, Grove, JE, Guiriec, S, Hadasch, D, Hanabata, Y, Harding, AK, Hayashida, M, Hayashi, K, Hays, E, Hewitt, J, Hill, AB, Horan, D, Hou, X, Hughes, RE, Inoue, Y, Jackson, MS, Jogler, T, Jóhannesson, G, Johnson, AS, Kamae, T, Kawano, T, Kerr, M, Knödlseder, J, Kuss, M, Lande, J, Larsson, S, Latronico, L, Lemoine-Goumard, M, Longo, F, Loparco, F, Lovellette, MN, Lubrano, P, Marelli, M, Massaro, F, Mayer, M, Mazziotta, MN, McEnery, JE, Mehault, J, Michelson, PF, Mitthumsiri, W
Publikováno v:
The Astrophysical Journal, vol 773, iss 1
Astrophysical Journal, vol 773, iss 1
Astrophysical Journal, vol 773, iss 1
Pulsar wind nebulae (PWNe) have been established as the most populous class of TeV γ-ray emitters. Since launch, the Fermi Large Area Telescope (LAT) has identified five high-energy (100 MeV < E < 100 GeV) γ-ray sources as PWNe and detected a large
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::8852fadbd9c6a52dca1bf5453e158eee
https://escholarship.org/uc/item/7dn390t6
https://escholarship.org/uc/item/7dn390t6