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Journal Articles Astrophys.J. Year : 2023

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

D.A Smith (1, 2) , S Abdollahi (3) , M Ajello , M Bailes , L Baldini , J Ballet (4) , M.G Baring , C Bassa , J. Becerra Gonzalez , R Bellazzini , A Berretta , B Bhattacharyya , E Bissaldi , R Bonino , E Bottacini , J Bregeon (5) , P Bruel (6) , M Burgay , T.H Burnett , R.A Cameron , F Camilo , R Caputo , P.A Caraveo , E Cavazzuti , G Chiaro , S Ciprini , C.J Clark , I Cognard (7, 8) , A Corongiu , P. Cristarella Orestano , M Crnogorcevic , A Cuoco , S Cutini , F d'Ammando , A de Angelis , M.E Decesar , S de Gaetano , R de Menezes , J Deneva , F de Palma , N Di Lalla , F Dirirsa , L Di Venere , A Domínguez , D Dumora (1) , S.J Fegan (6) , E.C Ferrara , A Fiori , H Fleischhack , C Flynn , A Franckowiak , P.C.C Freire , Y Fukazawa , P Fusco , G Galanti , V Gammaldi , F Gargano , D Gasparrini , F Giacchino , N Giglietto , F Giordano , M Giroletti , D Green , I.A Grenier (4) , L Guillemot (7, 8) , S Guiriec , M Gustafsson , A.K Harding , E Hays , J.W Hewitt , D Horan (6) , X Hou , F Jankowski (7) , R.P Johnson , T.J Johnson , S Johnston , J Kataoka , M.J Keith , M Kerr , M Kramer , M Kuss , L Latronico , S.-H Lee , D Li , J Li , B Limyansky , F Longo , F Loparco , L Lorusso , M.N Lovellette , M Lower , P Lubrano , A.G Lyne , Y Maan , S Maldera , R.N Manchester , A Manfreda , M Marelli , G Martí-Devesa , M.N Mazziotta , J.E Mcenery , I Mereu , P.F Michelson , M Mickaliger , W Mitthumsiri , T Mizuno , A.A Moiseev , M.E Monzani , A Morselli , M Negro , R Nemmen , L Nieder , E Nuss (9) , N Omodei , M Orienti , E Orlando , J.F Ormes , M Palatiello , D Paneque , G Panzarini , A Parthasarathy , M Persic , M Pesce-Rollins , R Pillera , H Poon , T.A Porter , A Possenti , G Principe , S Raino , R Rando , S.M Ransom , P.S Ray , M Razzano , S Razzaque , A Reimer , O Reimer , N Renault-Tinacci (4) , R.W Romani , M Sanchez-Conde , P.M. Saz Parkinson , L Scotton (9) , D Serini , C Sgro , R Shannon , V Sharma , Z Shen , E.J Siskind , G Spandre , P Spinelli , B.W Stappers , T.E Stephens , D.J Suson , S Tabassum , H Tajima , D Tak , G Theureau (7, 8) , D.J Thompson , O Tibolla , D.F Torres , J Valverde , C Venter , Z Wadiasingh , N Wang , P Wang , P Weltevrede , K Wood , J Yan , G Zaharijas , C Zhang , W Zhu
M Ajello
  • Function : Author
M Bailes
  • Function : Author
L Baldini
  • Function : Author
M.G Baring
  • Function : Author
C Bassa
  • Function : Author
J. Becerra Gonzalez
  • Function : Author
R Bellazzini
  • Function : Author
A Berretta
  • Function : Author
B Bhattacharyya
  • Function : Author
E Bissaldi
  • Function : Author
R Bonino
  • Function : Author
E Bottacini
  • Function : Author
M Burgay
  • Function : Author
T.H Burnett
  • Function : Author
R.A Cameron
  • Function : Author
F Camilo
  • Function : Author
R Caputo
  • Function : Author
P.A Caraveo
  • Function : Author
E Cavazzuti
  • Function : Author
G Chiaro
  • Function : Author
S Ciprini
  • Function : Author
C.J Clark
  • Function : Author
A Corongiu
  • Function : Author
P. Cristarella Orestano
  • Function : Author
M Crnogorcevic
  • Function : Author
A Cuoco
  • Function : Author
S Cutini
  • Function : Author
F d'Ammando
  • Function : Author
A de Angelis
  • Function : Author
M.E Decesar
  • Function : Author
S de Gaetano
  • Function : Author
R de Menezes
  • Function : Author
J Deneva
  • Function : Author
F de Palma
  • Function : Author
N Di Lalla
  • Function : Author
F Dirirsa
  • Function : Author
L Di Venere
  • Function : Author
A Domínguez
  • Function : Author
E.C Ferrara
  • Function : Author
A Fiori
  • Function : Author
H Fleischhack
  • Function : Author
C Flynn
  • Function : Author
A Franckowiak
  • Function : Author
P.C.C Freire
  • Function : Author
Y Fukazawa
  • Function : Author
P Fusco
  • Function : Author
G Galanti
  • Function : Author
V Gammaldi
  • Function : Author
F Gargano
  • Function : Author
D Gasparrini
  • Function : Author
F Giacchino
  • Function : Author
N Giglietto
  • Function : Author
F Giordano
  • Function : Author
M Giroletti
  • Function : Author
D Green
  • Function : Author
S Guiriec
  • Function : Author
M Gustafsson
  • Function : Author
A.K Harding
  • Function : Author
E Hays
  • Function : Author
J.W Hewitt
  • Function : Author
X Hou
  • Function : Author
R.P Johnson
  • Function : Author
T.J Johnson
  • Function : Author
S Johnston
  • Function : Author
J Kataoka
  • Function : Author
M.J Keith
  • Function : Author
M Kerr
  • Function : Author
M Kramer
  • Function : Author
M Kuss
  • Function : Author
L Latronico
  • Function : Author
S.-H Lee
  • Function : Author
D Li
  • Function : Author
J Li
  • Function : Author
B Limyansky
  • Function : Author
F Longo
  • Function : Author
F Loparco
  • Function : Author
L Lorusso
  • Function : Author
M.N Lovellette
  • Function : Author
M Lower
  • Function : Author
P Lubrano
  • Function : Author
A.G Lyne
  • Function : Author
Y Maan
  • Function : Author
S Maldera
  • Function : Author
R.N Manchester
  • Function : Author
A Manfreda
  • Function : Author
M Marelli
  • Function : Author
G Martí-Devesa
  • Function : Author
M.N Mazziotta
  • Function : Author
J.E Mcenery
  • Function : Author
I Mereu
  • Function : Author
P.F Michelson
  • Function : Author
M Mickaliger
  • Function : Author
W Mitthumsiri
  • Function : Author
T Mizuno
  • Function : Author
A.A Moiseev
  • Function : Author
M.E Monzani
  • Function : Author
A Morselli
  • Function : Author
M Negro
  • Function : Author
R Nemmen
  • Function : Author
L Nieder
  • Function : Author
N Omodei
  • Function : Author
M Orienti
  • Function : Author
E Orlando
  • Function : Author
J.F Ormes
  • Function : Author
M Palatiello
  • Function : Author
D Paneque
  • Function : Author
G Panzarini
  • Function : Author
A Parthasarathy
  • Function : Author
M Persic
  • Function : Author
M Pesce-Rollins
  • Function : Author
R Pillera
  • Function : Author
H Poon
  • Function : Author
T.A Porter
  • Function : Author
A Possenti
  • Function : Author
G Principe
  • Function : Author
S Raino
  • Function : Author
R Rando
  • Function : Author
S.M Ransom
  • Function : Author
P.S Ray
  • Function : Author
M Razzano
  • Function : Author
S Razzaque
  • Function : Author
A Reimer
  • Function : Author
O Reimer
  • Function : Author
R.W Romani
  • Function : Author
M Sanchez-Conde
  • Function : Author
P.M. Saz Parkinson
  • Function : Author
D Serini
  • Function : Author
C Sgro
  • Function : Author
R Shannon
  • Function : Author
V Sharma
  • Function : Author
Z Shen
  • Function : Author
E.J Siskind
  • Function : Author
G Spandre
  • Function : Author
P Spinelli
  • Function : Author
B.W Stappers
  • Function : Author
T.E Stephens
  • Function : Author
D.J Suson
  • Function : Author
S Tabassum
  • Function : Author
H Tajima
  • Function : Author
D Tak
  • Function : Author
D.J Thompson
  • Function : Author
O Tibolla
  • Function : Author
D.F Torres
  • Function : Author
J Valverde
  • Function : Author
C Venter
  • Function : Author
Z Wadiasingh
  • Function : Author
N Wang
  • Function : Author
P Wang
  • Function : Author
P Weltevrede
  • Function : Author
K Wood
  • Function : Author
J Yan
  • Function : Author
G Zaharijas
  • Function : Author
C Zhang
  • Function : Author
W Zhu
  • Function : Author

Abstract

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 co-located 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 $\leq 11$ known before Fermi. Half of the gamma-ray pulsars are young. Of these, the half that are undetected in radio have a broader Galactic latitude distribution than the young radio-loud pulsars. The others are MSPs, with 6 undetected in radio. Overall, >235 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 $\dot E$ decreases to its observed minimum near $10^{33}$ 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.
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Dates and versions

hal-04179157 , version 1 (12-02-2024)

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D.A Smith, S Abdollahi, M Ajello, M Bailes, L Baldini, et al.. The Third Fermi Large Area Telescope Catalog of Gamma-ray Pulsars. Astrophys.J., 2023, 958 (2), pp.191. ⟨10.3847/1538-4357/acee67⟩. ⟨hal-04179157⟩
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