Authors
AA Abdo, Marco Ajello, A Allafort, Luca Baldini, Jean Ballet, Guido Barbiellini, MG Baring, Denis Bastieri, A Belfiore, Rea Bellazzini, B Bhattacharyya, Elisabetta Bissaldi, ED Bloom, E Bonamente, E Bottacini, TJ Brandt, J Bregeon, M Brigida, Pascal Bruel, R Buehler, M Burgay, TH Burnett, Giovanni Busetto, Sara Buson, GA Caliandro, RA Cameron, F Camilo, PA Caraveo, JM Casandjian, C Cecchi, Ö Çelik, E Charles, S Chaty, RCG Chaves, A Chekhtman, AW Chen, J Chiang, G Chiaro, S Ciprini, R Claus, Ismaël Cognard, J Cohen-Tanugi, LR Cominsky, Jan Conrad, S Cutini, Filippo D'Ammando, A De Angelis, ME DeCesar, A De Luca, PR Den Hartog, F De Palma, CD Dermer, G Desvignes, SW Digel, L Di Venere, PS Drell, A Drlica-Wagner, R Dubois, D Dumora, CM Espinoza, L Falletti, C Favuzzi, EC Ferrara, WB Focke, A Franckowiak, PCC Freire, S Funk, P Fusco, F Gargano, D Gasparrini, S Germani, N Giglietto, P Giommi, F Giordano, M Giroletti, T Glanzman, G Godfrey, EV Gotthelf, IA Grenier, M-H Grondin, JE Grove, L Guillemot, S Guiriec, D Hadasch, Y Hanabata, AK Harding, M Hayashida, E Hays, J Hessels, J Hewitt, AB Hill, D Horan, X Hou, RE Hughes, Miranda S Jackson, GH Janssen, T Jogler, G Jóhannesson, RP Johnson, AS Johnson, TJ Johnson, WN Johnson, S Johnston, T Kamae, J Kataoka, M Keith, M Kerr, Jürgen Knödlseder, M Kramer, M Kuss, J Lande, Stefan Larsson, L Latronico, M Lemoine-Goumard, Francesco Longo, F Loparco, MN Lovellette, P Lubrano, AG Lyne, RN Manchester, M Marelli, Francesco Massaro, M Mayer, MN Mazziotta, JE McEnery, MA McLaughlin, J Mehault, PF Michelson, RP Mignani, W Mitthumsiri, T Mizuno, AA Moiseev, ME Monzani, A Morselli, IV Moskalenko, S Murgia, T Nakamori, R Nemmen, E Nuss, M Ohno, T Ohsugi, M Orienti, E Orlando, JF Ormes, D Paneque, JH Panetta, D Parent, JS Perkins, M Pesce-Rollins, M Pierbattista
Publication date
2013/9/19
Journal
The Astrophysical Journal Supplement Series
Volume
208
Issue
2
Pages
17
Publisher
IOP Publishing
Description
This catalog summarizes 117 high-confidence⩾ 0. 1 GeV gamma-ray pulsar detections using three years of data acquired by the Large Area Telescope (LAT) on the Fermi satellite. Half are neutron stars discovered using LAT data through periodicity searches in gamma-ray and radio data around LAT unassociated source positions. The 117 pulsars are evenly divided into three groups: millisecond pulsars, young radio-loud pulsars, and young radio-quiet pulsars. We characterize the pulse profiles and energy spectra and derive luminosities when distance information exists. Spectral analysis of the off-peak phase intervals indicates probable pulsar wind nebula emission for four pulsars, and off-peak magnetospheric emission for several young and millisecond pulsars. We compare the gammaray properties with those in the radio, optical, and X-ray bands. We provide flux limits for pulsars with no observed gamma-ray …
Scholar articles
AA Abdo, M Ajello, A Allafort, L Baldini, J Ballet… - The Astrophysical Journal Supplement Series, 2013