Using gamma-ray data collected by the Astro-rivelatore Gamma ad Immagini LEggero (AGILE) satellite over a period of almost one year (from 2007 July to 2008 June), we searched for pulsed signals from 35 potentially interesting radio pulsars, ordered according to F(gamma) alpha root(E) over dot d(-2) and for which contemporary or recent radio data were available. AGILE detected three new top-ranking nearby and Vela-like pulsars with good confidence both through timing and spatial analysis. Among the newcomers we find pulsars with very high rotational energy losses, such as the remarkable PSR B1509-58 with a magnetic field in excess of 10(13) Gauss, and PSR J2229+6114 providing a reliable identification for the previously unidentified EGRET source 3EG 2227+6122. Moreover, the powerful millisecond pulsar B1821-24, in the globular cluster M28, is detected during a fraction of the observations. Four other promising gamma-ray pulsar candidates, among which is the notable J2043+2740 with an age in excess of 1 million years, show a possible detection in the timing analysis only and deserve confirmation.

DISCOVERY OF NEW GAMMA-RAY PULSARS WITH AGILE

PREST, MICHELA;
2009-01-01

Abstract

Using gamma-ray data collected by the Astro-rivelatore Gamma ad Immagini LEggero (AGILE) satellite over a period of almost one year (from 2007 July to 2008 June), we searched for pulsed signals from 35 potentially interesting radio pulsars, ordered according to F(gamma) alpha root(E) over dot d(-2) and for which contemporary or recent radio data were available. AGILE detected three new top-ranking nearby and Vela-like pulsars with good confidence both through timing and spatial analysis. Among the newcomers we find pulsars with very high rotational energy losses, such as the remarkable PSR B1509-58 with a magnetic field in excess of 10(13) Gauss, and PSR J2229+6114 providing a reliable identification for the previously unidentified EGRET source 3EG 2227+6122. Moreover, the powerful millisecond pulsar B1821-24, in the globular cluster M28, is detected during a fraction of the observations. Four other promising gamma-ray pulsar candidates, among which is the notable J2043+2740 with an age in excess of 1 million years, show a possible detection in the timing analysis only and deserve confirmation.
2009
http://iopscience.iop.org/article/10.1088/0004-637X/695/1/L115?fromSearchPage=true
Agile; radio pulsar
Pellizzoni, A; Pilia, M; Possenti, A; Chen, A; Giuliani, A; Trois, A; Caraveo, P; Del Monte, E; Fornari, F; Fuschino, F; Mereghetti, S; Tavani, Marco; Argan, A; Burgay, M; Cognard, I; Corongiu, A; Costa, E; D'Amico, N; De Luca, Andrea; Esposito, Paolo; Evangelista, Y; Feroci, M; Johnston, S; Kramer, M; Longo, Francesco; Marisaldi, M; Theureau, G; Weltevrede, P; Barbiellini Amidei, Guido; Boffelli, Fabrizio; Bulgarelli, A; Cattaneo Paolo, Walter; Cocco, V; D'Ammando, F; De Paris, G; Di Cocco, G; Donnarumma, I; Fiorini, Massimiliano; Froysland Tom, Vidar; Galli, M; Gianotti, F; Labanti, C; Lapshov, I; Lazzarotto, F; Lipari, Paolo; Mineo, T; Morselli, Aldo; Pacciani, L; Perotti, F; Piano, Giovanni; Picozza, Piergiorgio; Prest, Michela; Pucella, G; Rapisarda, M; Rappoldi, Andrea; Sabatini, Sabina; Soffitta, P; Trifoglio, M; Vallazza Erik, Silvio; Vercellone, S; Vittorini, V; Zambra, A; Zanello, Dino; Pittori, C; Verrecchia, F; Preger, B; Santolamazza, P; Giommi, P; Salotti, L; Bignami, Gf
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11383/1737423
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