Sökning: WFRF:(Parkinson P. M. Saz) > Fermi large area te...
Fältnamn | Indikatorer | Metadata |
---|---|---|
000 | 11778naa a2203229 4500 | |
001 | oai:DiVA.org:kth-95260 | |
003 | SwePub | |
008 | 120521s2012 | |||||||||||000 ||eng| | |
009 | oai:DiVA.org:su-80734 | |
024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-952602 URI |
024 | 7 | a https://doi.org/10.1088/0067-0049/199/2/312 DOI |
024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-807342 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 Nolan, P. L.4 aut |
245 | 1 0 | a Fermi large area telescope second source catalog |
264 | c 2012-03-28 | |
264 | 1 | b American Astronomical Society,c 2012 |
338 | a print2 rdacarrier | |
500 | a QC 20120521 | |
500 | a AuthorCount:237; | |
520 | a We present the second catalog of high-energy gamma-ray sources detected by the Large Area Telescope (LAT), the primary science instrument on the Fermi Gamma-ray Space Telescope (Fermi), derived from data taken during the first 24 months of the science phase of the mission, which began on 2008 August 4. Source detection is based on the average flux over the 24 month period. The second Fermi-LAT catalog (2FGL) includes source location regions, defined in terms of elliptical fits to the 95% confidence regions and spectral fits in terms of power-law, exponentially cutoff power-law, or log-normal forms. Also included are flux measurements in five energy bands and light curves on monthly intervals for each source. Twelve sources in the catalog are modeled as spatially extended. We provide a detailed comparison of the results from this catalog with those from the first Fermi-LAT catalog (1FGL). Although the diffuse Galactic and isotropic models used in the 2FGL analysis are improved compared to the 1FGL catalog, we attach caution flags to 162 of the sources to indicate possible confusion with residual imperfections in the diffuse model. The 2FGL catalog contains 1873 sources detected and characterized in the 100 MeV to 100 GeV range of which we consider 127 as being firmly identified and 1171 as being reliably associated with counterparts of known or likely gamma-ray-producing source classes. | |
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 catalogs | |
653 | a gamma rays: general | |
700 | 1 | a Abdo, A. A.4 aut |
700 | 1 | a Ackermann, M.4 aut |
700 | 1 | a Ajello, M.4 aut |
700 | 1 | a Allafort, A.4 aut |
700 | 1 | a Antolini, E.4 aut |
700 | 1 | a Atwood, W. B.4 aut |
700 | 1 | a Axelsson, Magnusu Stockholms universitet,KTH,Partikel- och astropartikelfysik,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC)4 aut0 (Swepub:su)aaxe |
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 Belfiore, A.4 aut |
700 | 1 | a Bellazzini, R.4 aut |
700 | 1 | a Berenji, B.4 aut |
700 | 1 | a Bignami, G. F.4 aut |
700 | 1 | a Blandford, R. D.4 aut |
700 | 1 | a Bloom, E. D.4 aut |
700 | 1 | a Bonamente, E.4 aut |
700 | 1 | a Bonnell, J.4 aut |
700 | 1 | a Borgland, A. W.4 aut |
700 | 1 | a Bottacini, E.4 aut |
700 | 1 | a Bouvier, A.4 aut |
700 | 1 | a Brandt, T. J.4 aut |
700 | 1 | a Bregeon, J.4 aut |
700 | 1 | a Brigida, M.4 aut |
700 | 1 | a Bruel, P.4 aut |
700 | 1 | a Buehler, R.4 aut |
700 | 1 | a Burnett, T. H.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 Campana, R.4 aut |
700 | 1 | a Canadas, B.4 aut |
700 | 1 | a Cannon, A.4 aut |
700 | 1 | a Caraveo, P. A.4 aut |
700 | 1 | a Casandjian, J. M.4 aut |
700 | 1 | a Cavazzuti, E.4 aut |
700 | 1 | a Ceccanti, M.4 aut |
700 | 1 | a Cecchi, C.4 aut |
700 | 1 | a Celik, Oe4 aut |
700 | 1 | a Charles, E.4 aut |
700 | 1 | a Chekhtman, A.4 aut |
700 | 1 | a Cheung, C. C.4 aut |
700 | 1 | a Chiang, J.4 aut |
700 | 1 | a Chipaux, R.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 Cominsky, L. R.4 aut |
700 | 1 | a Conrad, Janu Stockholms universitet,Fysikum,Oskar Klein-centrum för kosmopartikelfysik (OKC)4 aut0 (Swepub:su)conrad |
700 | 1 | a Corbet, R.4 aut |
700 | 1 | a Cutini, S.4 aut |
700 | 1 | a D'Ammando, F.4 aut |
700 | 1 | a Davis, D. S.4 aut |
700 | 1 | a de Angelis, A.4 aut |
700 | 1 | a DeCesar, M. E.4 aut |
700 | 1 | a DeKlotz, M.4 aut |
700 | 1 | a De Luca, A.4 aut |
700 | 1 | a den Hartog, P. R.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 Drlica-Wagner, A.4 aut |
700 | 1 | a Dubois, R.4 aut |
700 | 1 | a Dumora, D.4 aut |
700 | 1 | a Enoto, T.4 aut |
700 | 1 | a Escande, L.4 aut |
700 | 1 | a Fabiani, D.4 aut |
700 | 1 | a Falletti, L.4 aut |
700 | 1 | a Favuzzi, C.4 aut |
700 | 1 | a Fegan, S. J.4 aut |
700 | 1 | a Ferrara, E. C.4 aut |
700 | 1 | a Focke, W. B.4 aut |
700 | 1 | a Fortin, P.4 aut |
700 | 1 | a Frailis, M.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 Gehrels, N.4 aut |
700 | 1 | a Germani, S.4 aut |
700 | 1 | a Giebels, B.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 Glanzman, T.4 aut |
700 | 1 | a Godfrey, G.4 aut |
700 | 1 | a Grenier, I. A.4 aut |
700 | 1 | a Grondin, M. -H4 aut |
700 | 1 | a Grove, J. E.4 aut |
700 | 1 | a Guillemot, L.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 Hanabata, Y.4 aut |
700 | 1 | a Harding, A. K.4 aut |
700 | 1 | a Hayashida, M.4 aut |
700 | 1 | a Hays, E.4 aut |
700 | 1 | a Hill, A. B.4 aut |
700 | 1 | a Horan, D.4 aut |
700 | 1 | a Hou, X.4 aut |
700 | 1 | a Hughes, R. E.4 aut |
700 | 1 | a Iafrate, G.4 aut |
700 | 1 | a Itoh, R.4 aut |
700 | 1 | a Johannesson, G.4 aut |
700 | 1 | a Johnson, R. P.4 aut |
700 | 1 | a Johnson, T. E.4 aut |
700 | 1 | a Johnson, A. S.4 aut |
700 | 1 | a Johnson, T. J.4 aut |
700 | 1 | a Kamae, T.4 aut |
700 | 1 | a Katagiri, H.4 aut |
700 | 1 | a Kataoka, J.4 aut |
700 | 1 | a Katsuta, J.4 aut |
700 | 1 | a Kawai, N.4 aut |
700 | 1 | a Kerr, M.4 aut |
700 | 1 | a Knoedlseder, J.4 aut |
700 | 1 | a Kocevski, D.4 aut |
700 | 1 | a Kuss, M.4 aut |
700 | 1 | a Lande, J.4 aut |
700 | 1 | a Landriu, D.4 aut |
700 | 1 | a Latronico, L.4 aut |
700 | 1 | a Lemoine-Goumard, M.4 aut |
700 | 1 | a Lionetto, A. M.4 aut |
700 | 1 | a Garde, Maja Llenau Stockholms universitet,Fysikum,Oskar Klein-centrum för kosmopartikelfysik (OKC)4 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 |
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 Marelli, M.4 aut |
700 | 1 | a Massaro, E.4 aut |
700 | 1 | a Mazziotta, M. N.4 aut |
700 | 1 | a McConville, W.4 aut |
700 | 1 | a McEnery, J. E.4 aut |
700 | 1 | a Mehault, J.4 aut |
700 | 1 | a Michelson, P. F.4 aut |
700 | 1 | a Minuti, M.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 Mongelli, M.4 aut |
700 | 1 | a Monte, C.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 Nakamori, T.4 aut |
700 | 1 | a Naumann-Godo, M.4 aut |
700 | 1 | a Norris, J. P.4 aut |
700 | 1 | a Nuss, E.4 aut |
700 | 1 | a Nymark, Tanjau KTH,Fysik4 aut0 (Swepub:kth)u14p8rnp |
700 | 1 | a Ohno, M.4 aut |
700 | 1 | a Ohsugi, T.4 aut |
700 | 1 | a Okumura, A.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 Ozaki, M.4 aut |
700 | 1 | a Paneque, D.4 aut |
700 | 1 | a Panetta, J. H.4 aut |
700 | 1 | a Parent, D.4 aut |
700 | 1 | a Perkins, J. S.4 aut |
700 | 1 | a Pesce-Rollins, M.4 aut |
700 | 1 | a Pierbattista, M.4 aut |
700 | 1 | a Pinchera, 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 Racusin, J. L.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 Rochester, L. S.4 aut |
700 | 1 | a Romani, R. W.4 aut |
700 | 1 | a Roth, M.4 aut |
700 | 1 | a Rousseau, R.4 aut |
700 | 1 | a Ryde, Felixu KTH,Partikel- och astropartikelfysik4 aut0 (Swepub:kth)u1tlyg6w |
700 | 1 | a Sadrozinski, H. F. -W4 aut |
700 | 1 | a Salvetti, D.4 aut |
700 | 1 | a Sanchez, D. A.4 aut |
700 | 1 | a Parkinson, P. M. Saz4 aut |
700 | 1 | a Sbarra, C.4 aut |
700 | 1 | a Scargle, J. D.4 aut |
700 | 1 | a Schalk, T. L.4 aut |
700 | 1 | a Sgro, C.4 aut |
700 | 1 | a Shaw, M. S.4 aut |
700 | 1 | a Shrader, C.4 aut |
700 | 1 | a Siskind, E. J.4 aut |
700 | 1 | a Smith, D. A.4 aut |
700 | 1 | a Spandre, G.4 aut |
700 | 1 | a Spinelli, P.4 aut |
700 | 1 | a Stephens, T. E.4 aut |
700 | 1 | a Strickman, M. S.4 aut |
700 | 1 | a Suson, D. J.4 aut |
700 | 1 | a Tajima, H.4 aut |
700 | 1 | a Takahashi, H.4 aut |
700 | 1 | a Takahashi, T.4 aut |
700 | 1 | a Tanaka, T.4 aut |
700 | 1 | a Thayer, J. G.4 aut |
700 | 1 | a Thayer, J. B.4 aut |
700 | 1 | a Thompson, D. J.4 aut |
700 | 1 | a Tibaldo, L.4 aut |
700 | 1 | a Tibolla, O.4 aut |
700 | 1 | a Tinebra, F.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 Vandenbroucke, J.4 aut |
700 | 1 | a Van Etten, A.4 aut |
700 | 1 | a Van Klaveren, B.4 aut |
700 | 1 | a Vasileiou, V.4 aut |
700 | 1 | a Vianello, G.4 aut |
700 | 1 | a Vitale, V.4 aut |
700 | 1 | a Waite, A. P.4 aut |
700 | 1 | a Wallace, E.4 aut |
700 | 1 | a Wang, P.4 aut |
700 | 1 | a Werner, M.4 aut |
700 | 1 | a Winer, B. L.4 aut |
700 | 1 | a Wood, D. L.4 aut |
700 | 1 | a Wood, K. S.4 aut |
700 | 1 | a Wood, M.4 aut |
700 | 1 | a Yang, Zhaoyuu Stockholms universitet,Fysikum,Oskar Klein-centrum för kosmopartikelfysik (OKC)4 aut0 (Swepub:su)zhaoyu |
700 | 1 | a Zimmer, Stephanu Stockholms universitet,Fysikum,Oskar Klein-centrum för kosmopartikelfysik (OKC)4 aut0 (Swepub:su)stzi0820 |
710 | 2 | a KTHb Partikel- och astropartikelfysik4 org |
773 | 0 | t Astrophysical Journal Supplement Seriesd : American Astronomical Societyg 199:2, s. 31-q 199:2<31-x 0067-0049x 1538-4365 |
856 | 4 | u https://bib-pubdb1.desy.de/record/144018/files/Astrophys.J.199.pdf |
856 | 4 | u https://arxiv.org/abs/1108.1435y arXiv:1108.1435 |
856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-95260 |
856 | 4 8 | u https://doi.org/10.1088/0067-0049/199/2/31 |
856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-80734 |
Kungliga biblioteket hanterar dina personuppgifter i enlighet med EU:s dataskyddsförordning (2018), GDPR. Läs mer om hur det funkar här.
Så här hanterar KB dina uppgifter vid användning av denna tjänst.