Detection of 16 Gamma-Ray Pulsars Through Blind Frequency Searches Using the Fermi LAT
- ABDO AA
- ACKERMANN M
- AJELLO M
- ANDERSON B
- ATWOOD WB
- AXELSSON M
- BALDINI L
- BALLET J
- BARBIELLINI G
- BARING MG
- BAUGHMAN BM
- BECHTOL K
- BELLAZZINI R
- BERENJI B
- BIGNAMI GF
- BLANDFORD RD
- BLOOM ED
- BONAMENTE E
- BORGLAND AW
- BREGEON J
- BREZ A
- BRIGIDA M
- BRUEL P
- BURNETT TH
- CALIANDRO GA
- CAMERON RA
- CARAVEO PA
- CASANDJIAN JM
- CECCHI C
- CELIK O
- CHEKHTMAN A
- CHEUNG CC
- CHIANG J
- CIPRINI S
- CLAUS R
- COHEN TANUGI J
- CONRAD J
- CUTINI S
- DERMER CD
- DE ANGELIS A
- DE LUCA A
- DE PALMA F
- DIGEL SW
- DORMODY M
- SILVA EDE
- DRELL PS
- DUBOIS R
- DUMORA D
- FARNIER C
- FAVUZZI C
- FEGAN SJ
- FUKAZAWA Y
- FUNK S
- FUSCO P
- GARGANO F
- GASPARRINI D
- GEHRELS N
- GERMANI S
- GIEBELS B
- GIGLIETTO N
- GIOMMI P
- GIORDANO F
- GLANZMAN T
- GODFREY G
- GRENIER IA
- GRONDIN MH
- GROVE JE
- GUILLEMOT L
- GUIRIEC S
- GWON C
- HANABATA Y
- HARDING AK
- HAYASHIDA M
- HAYS E
- HUGHES RE
- JOHANNESSON G
- JOHNSON RP
- JOHNSON TJ
- JOHNSON WN
- KAMAE T
- KATAGIRI H
- KATAOKA J
- KAWAI N
- KERR M
- KNODLSEDER J
- KOCIAN ML
- KUSS M
- LANDE J
- LATRONICO L
- LEMOINE GOUMARD M
- LONGO F
- LOPARCO F
- LOTT B
- LOVELLETTE MN
- LUBRANO P
- MADEJSKI GM
- MAKEEV A
- MARELLI M
- MAZZIOTTA MN
- MCCONVILLE W
- MCENERY JE
- MEURER C
- MICHELSON PF
- MITTHUMSIRI W
- MIZUNO T
- MONTE C
- MONZANI ME
- MORSELLI A
- MOSKALENKO IV
- MURGIA S
- NOLAN PL
- NORRIS JP
- NUSS E
- OHSUGI T
- OMODEI N
- ORLANDO E
- ORMES JF
- PANEQUE D
- PARENT D
- PELASSA V
- PEPE M
- PESCE ROLLINS M
- PIERBATTISTA M
- PIRON F
- PORTER TA
- PRIMACK JR
- RAINO S
- RAY PS
- RAZZANO M
- REA N
- REIMER A
- REIMER O
- REPOSEUR T
- RITZ S
- ROCHESTER LS
- RODRIGUEZ AY
- ROMANI RW
- RYDE F
- SADROZINSKI HFW
- SANCHEZ D
- SANDER A
- PARKINSON PMS
- SCARGLE JD
- SGRO C
- SISKIND EJ
- SMITH DA
- SMITH PD
- SPANDRE G
- SPINELLI P
- STARCK JL
- STRICKMAN MS
- SUSON DJ
- TAJIMA H
- TAKAHASHI H
- TAKAHASHI T
- TANAKA T
- THAYER JG
- THOMPSON DJ
- TIBOLLA O
- TORRES DF
- TOSTI G
- TRAMACERE A
- UCHIYAMA Y
- USHER TL
- VAN ETTEN A
- VASILEIOU V
- VILCHEZ N
- VITALE V
- WAITE AP
- WANG P
- WATTERS K
- WINER BL
- WOLFF MT
- WOOD KS
- YLINEN T
- ZIEGLER M.
- BASTIERI, DENIS
- RANDO, RICCARDO
- TIBALDO, LUIGI
DOIAbstract
Pulsars are rapidly rotating, highly magnetized neutron stars emitting radiation across the electromagnetic spectrum. Although there are more than 1800 known radio pulsars, until recently only seven were observed to pulse in gamma rays, and these were all discovered at other wavelengths. The Fermi Large Area Telescope (LAT) makes it possible to pinpoint neutron stars through their gamma-ray pulsations. We report the detection of 16 gamma-ray pulsars in blind frequency searches using the LAT. Most of these pulsars are coincident with previously unidentified gamma-ray sources, and many are associated with supernova remnants. Direct detection of gamma-ray pulsars enables studies of emission mechanisms, population statistics, and the energetics...
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