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The Third Fermi Large Area Telescope Catalog of Gamma-Ray Pulsars

Title:	The Third Fermi Large Area Telescope Catalog of Gamma-Ray Pulsars
Authors:	Smith, DA; Abdollahi, S; Ajello, M; Bailes, M; Baldini, L; Ballet, J; Baring, MG; Bassa, C; Gonzalez, JB; Bellazzini, R; Berretta, A; Bhattacharyya, B; Bissaldi, E; Bonino, R; Bottacini, E; Bregeon, J; Bruel, P; Burgay, M; Burnett, TH; Cameron, RA; Camilo, F; Caputo, R; Caraveo, PA; Cavazzuti, E; Chiaro, G; Ciprini, S; Clark, CJ; Cognard, I; Corongiu, A; Orestano, PC; Crnogorcevic, M; Cuoco, A; Cutini, S; D'Ammando, F; de Angelis, A; DeCesar, ME; De Gaetano, S; de Menezes, R; Deneva, J; de Palma, F; Di Lalla, N; Dirirsa, F; Di Venere, L; Domínguez, A; Dumora, D; Fegan, SJ; Ferrara, EC; Fiori, A; Fleischhack, H; Flynn, C; Franckowiak, A; Freire, PCC; Fukazawa, Y; Fusco, P; Galanti, G; Gammaldi; Gargano, F; Gasparrini, D; Giacchino, F; Giglietto, N; Giordano, F; Giroletti, M; Green, D; Grenier, IA; Guillemot, L; Guiriec, S; Gustafsson, M; Harding, AK; Hays, E; Hewitt, JW; Horan, D; Hou, X; Jankowski, F; Johnson, RP; Johnson, TJ; Johnston, S; Kataoka, J; Keith, MJ; Kerr, M; Kramer, M; Kuss, M; Latronico, L; Lee, SH; Li, D; Li, J; Limyansky, B; Longo, F; Loparco, F; Lorusso, L; Lovellette, MN; Lower, M; Lubrano, P; Lyne, AG; Maan, Y; Maldera, S; Manchester, RN; Manfreda, A; Marelli, M; Martí-Devesa, G; Mazziotta, MN; McEnery, JE; Mereu; Michelson, PF; Mickaliger, M; Mitthumsiri, W; Mizuno, T; Moiseev, AA; Monzani, ME; Morselli, A; Negro, M; Nemmen, R; Nieder, L; Nuss, E; Omodei, N; Orienti, M; Orlando, E; Ormes, JF; Palatiello, M; Paneque, D; Panzarini, G; Parthasarathy, A; Persic, M; Pesce-Rollins, M; Pillera, R; Poon, H; Porter, TA; Possenti, A; Principe, G; Rainò, S; Rando, R; Ransom, SM; Ray, PS; Razzano, M; Razzaque, S; Reimer, A; Reimer, O; Renault-Tinacci, N; Romani, RW; Sánchez-Conde, M; Parkinson, PMS; Scotton, L; Serini, D; Sgrò, C; Shannon, R; Sharma, V; Shen, Z; Siskind, EJ; Spandre, G; Spinelli, P; Stappers, BW; Stephens, TE; Suson, DJ; Tabassum, S; Tajima, H; Tak, D; Theureau, G; Thompson, DJ; Tibolla, O; Torres, DF; Valverde, J; Venter, C; Wadiasingh, Z; Wang, N; Wang, P; Weltevrede, P; Wood, K; Yan, J; Zaharijas, G; Zhang, C; Zhu, W
Contributors:	Smith, Da; Abdollahi, S; Ajello, M; Bailes, M; Baldini, L; Ballet, J; Baring, Mg; Bassa, C; Gonzalez, Jb; Bellazzini, R; Berretta, A; Bhattacharyya, B; Bissaldi, E; Bonino, R; Bottacini, E; Bregeon, J; Bruel, P; Burgay, M; Burnett, Th; Cameron, Ra; Camilo, F; Caputo, R; Caraveo, Pa; Cavazzuti, E; Chiaro, G; Ciprini, S; Clark, Cj; Cognard, I; Corongiu, A; Orestano, Pc; Crnogorcevic, M; Cuoco, A; Cutini, S; D'Ammando, F; de Angelis, A; Decesar, Me; De Gaetano, S; de Menezes, R; Deneva, J; de Palma, F; Di Lalla, N; Dirirsa, F; Di Venere, L; Domínguez, A; Dumora, D; Fegan, Sj; Ferrara, Ec; Fiori, A; Fleischhack, H; Flynn, C; Franckowiak, A; Freire, Pcc; Fukazawa, Y; Fusco, P; Galanti, G; Gammaldi; Gargano, F; Gasparrini, D; Giacchino, F; Giglietto, N; Giordano, F; Giroletti, M; Green, D; Grenier, Ia; Guillemot, L; Guiriec, S; Gustafsson, M; Harding, Ak; Hays, E; Hewitt, Jw; Horan, D; Hou, X; Jankowski, F; Johnson, Rp; Johnson, Tj; Johnston, S; Kataoka, J; Keith, Mj; Kerr, M; Kramer, M; Kuss, M; Latronico, L; Lee, Sh; Li, D; Li, J; Limyansky, B; Longo, F; Loparco, F; Lorusso, L; Lovellette, Mn; Lower, M; Lubrano, P; Lyne, Ag; Maan, Y; Maldera, S; Manchester, Rn; Manfreda, A; Marelli, M; Martí-Devesa, G; Mazziotta, Mn
Publication Year:	2023
Collection:	Politecnico di Bari: Iris POLIBA (Catalogo dei prodotti della Ricerca)
Description:	We present 294 pulsars found in GeV data from the Large Area Telescope (LAT) on the Fermi Gamma-ray Space Telescope. Another 33 millisecond pulsars (MSPs) discovered in deep radio searches of LAT sources will likely reveal pulsations once phase-connected rotation ephemerides are achieved. A further dozen optical and/or X-ray binary systems colocated with LAT sources also likely harbor gamma-ray MSPs. This catalog thus reports roughly 340 gamma-ray pulsars and candidates, 10% of all known pulsars, compared to = 236 are bright enough above 50 MeV to fit the pulse profile, the energy spectrum, or both. For the common two-peaked profiles, the gamma-ray peak closest to the magnetic pole crossing generally has a softer spectrum. The spectral energy distributions tend to narrow as the spindown power E decreases to its observed minimum near 1033 erg s-1, approaching the shape for synchrotron radiation from monoenergetic electrons. We calculate gamma-ray luminosities when distances are available. Our all-sky gamma-ray sensitivity map is useful for population syntheses. The electronic catalog version provides gamma-ray pulsar ephemerides, properties, and fit results to guide and be compared with modeling results.
Document Type:	article in journal/newspaper
Language:	English
Relation:	info:eu-repo/semantics/altIdentifier/wos/WOS:001117603900001; volume:958; issue:2; journal:THE ASTROPHYSICAL JOURNAL; https://hdl.handle.net/11589/264401
DOI:	10.3847/1538-4357/acee67
Availability:	https://hdl.handle.net/11589/264401; https://doi.org/10.3847/1538-4357/acee67
Accession Number:	edsbas.22CA5CD8
Database:	BASE