2010ApJS..187..460A


C.D.S. - SIMBAD4 rel 1.7 - 2020.06.02CEST05:06:08

2010ApJS..187..460A - Astrophys. J., Suppl. Ser., 187, 460-494 (2010/April-0)

The first Fermi Large Area Telescope catalog of gamma-ray pulsars.

ABDO A.A., ACKERMANN M., AJELLO M., ATWOOD W.B., AXELSSON M., BALDINI L., BALLET J., BARBIELLINI G., BARING M.G., BASTIERI D., BAUGHMAN B.M., BECHTOL K., BELLAZZINI R., BERENJI B., BLANDFORD R.D., BLOOM E.D., BONAMENTE E., BORGLAND A.W., BREGEON J., BREZ A., BRIGIDA M., BRUEL P., BURNETT T.H., BUSON S., CALIANDRO G.A., CAMERON R.A., CAMILO F., CARAVEO P.A., CASANDJIAN J.M., CECCHI C., CELIK O., CHARLES E., CHEKHTMAN A., CHEUNG C.C., CHIANG J., CIPRINI S., CLAUS R., COGNARD I., COHEN-TANUGI J., COMINSKY L.R., CONRAD J., CORBET R., CUTINI S., DEN HARTOG P.R., DERMER C.D., DE ANGELIS A., DE LUCA A., DE PALMA F., DIGEL S.W., DORMODY M., DO COUTO E SILVA E., DRELL P.S., DUBOIS R., DUMORA D., ESPINOZA C., FARNIER C., FAVUZZI C., FEGAN S.J., FERRARA E.C., FOCKE W.B., FORTIN P., FRAILIS M., FREIRE P.C.C., FUKAZAWA Y., FUNK S., FUSCO P., GARGANO F., GASPARRINI D., GEHRELS N., GERMANI S., GIAVITTO G., GIEBELS B., GIGLIETTO N., GIOMMI P., GIORDANO F., GLANZMAN T., GODFREY G., GOTTHELF E.V., GRENIER I.A., GRONDIN M.-H., GROVE J.E., GUILLEMOT L., GUIRIEC S., GWON C., HANABATA Y., HARDING A.K., HAYASHIDA M., HAYS E., HUGHES R.E., JACKSON M.S., JOHANNESSON G., JOHNSON A.S., JOHNSON R.P., JOHNSON T.J., JOHNSON W.N., JOHNSTON S., KAMAE T., KANBACH G., KASPI V.M., KATAGIRI H., KATAOKA J., KAWAI N., KERR M., KNODLSEDER J., KOCIAN M.L., KRAMER M., KUSS M., LANDE J., LATRONICO L., LEMOINE-GOUMARD M., LIVINGSTONE M., LONGO F., LOPARCO F., LOTT B., LOVELLETTE M.N., LUBRANO P., LYNE A.G., MADEJSKI G.M., MAKEEV A., MANCHESTER R.N., MARELLI M., MAZZIOTTA M.N., McCONVILLE W., McENERY J.E., McGLYNN S., MEURER C., MICHELSON P.F., MINEO T., MITTHUMSIRI W., MIZUNO T., MOISEEV A.A., MONTE C., MONZANI M.E., MORSELLI A., MOSKALENKO I.V., MURGIA S., NAKAMORI T., NOLAN P.L., NORRIS J.P., NOUTSOS A., NUSS E., OHSUGI T., OMODEI N., ORLANDO E., ORMES J.F., OZAKI M., PANEQUE D., PANETTA J.H., PARENT D., PELASSA V., PEPE M., PESCE-ROLLINS M., PIRON F., PORTER T.A., RAINO S., RANDO R., RANSOM S.M., RAY P.S., RAZZANO M., REA N., REIMER A., REIMER O., REPOSEUR T., RITZ S., RODRIGUEZ A.Y., ROMANI R.W., ROTH M., RYDE F., SADROZINSKI H.F.-W., SANCHEZ D., SANDER A., SAZ PARKINSON P.M., SCARGLE J.D., SCHALK T.L., SELLERHOLM A., SGRO C., SISKIND E.J., SMITH D.A., SMITH P.D., SPANDRE G., SPINELLI P., STAPPERS B.W., STARCK J.-L., STRIANI E., STRICKMAN M.S., STRONG A.W., SUSON D.J., TAJIMA H., TAKAHASHI H., TAKAHASHI T., TANAKA T., THAYER J.B., THAYER J.G., THEUREAU G., THOMPSON D.J., THORSETT S.E., TIBALDO L., TIBOLLA O., TORRES D.F., TOSTI G., TRAMACERE A., UCHIYAMA Y., USHER T.L., VAN ETTEN A., VASILEIOU V., VENTER C., VILCHEZ N., VITALE V., WAITE A.P., WANG P., WANG N., WATTERS K., WELTEVREDE P., WINER B.L., WOOD K.S., YLINEN T. and ZIEGLER M.

Abstract (from CDS):

The dramatic increase in the number of known gamma-ray pulsars since the launch of the Fermi Gamma-ray Space Telescope (formerly GLAST) offers the first opportunity to study a sizable population of these high-energy objects. This catalog summarizes 46 high-confidence pulsed detections using the first six months of data taken by the Large Area Telescope (LAT), Fermi's main instrument. Sixteen previously unknown pulsars were discovered by searching for pulsed signals at the positions of bright gamma-ray sources seen with the LAT, or at the positions of objects suspected to be neutron stars based on observations at other wavelengths. The dimmest observed flux among these gamma-ray-selected pulsars is 6.0x10–8 ph/cm2/s (for E>100 MeV). Pulsed gamma-ray emission was discovered from 24 known pulsars by using ephemerides (timing solutions) derived from monitoring radio pulsars. Eight of these new gamma-ray pulsars are millisecond pulsars. The dimmest observed flux among the radio-selected pulsars is 1.4x10–8 ph/cm2/s (for E>100 MeV). The remaining six gamma-ray pulsars were known since the Compton Gamma Ray Observatory mission, or before. The limiting flux for pulse detection is non-uniform over the sky owing to different background levels, especially near the Galactic plane. The pulsed energy spectra can be described by a power law with an exponential cutoff, with cutoff energies in the range ∼1-5 GeV. The rotational energy-loss rate ({dot}E) of these neutron stars spans five decades, from ∼3x1033 erg/s to 5x1038 erg/s, and the apparent efficiencies for conversion to gamma-ray emission range from ∼0.1% to ∼ unity, although distance uncertainties complicate efficiency estimates. The pulse shapes show substantial diversity, but roughly 75% of the gamma-ray pulse profiles have two peaks, separated by ≳0.2 of rotational phase. For most of the pulsars, gamma-ray emission appears to come mainly from the outer magnetosphere, while polar-cap emission remains plausible for a remaining few. Spatial associations imply that many of these pulsars power pulsar wind nebulae. Finally, these discoveries suggest that gamma-ray-selected young pulsars are born at a rate comparable to that of their radio-selected cousins and that the birthrate of all young gamma-ray-detected pulsars is a substantial fraction of the expected Galactic supernova rate.

Abstract Copyright:

Journal keyword(s): catalogs - gamma rays: general - pulsars: general - stars: neutron

Errata: erratum vol.193, art. 22 (2011)

Status at CDS:  

Simbad objects: 90

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Number of rows : 90

N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2020
#notes
1 PSR J0007+7303 Psr 00 06 34.20 +73 11 06.6           ~ 146 1
2 SNR G119.5+10.2 SNR 00 06.6 +72 47           ~ 233 1
3 EGR J0028+0457 gam 00 28.2 +04 57           ~ 4 0
4 PSR J0030+0451 Psr 00 30 27.4277 +04 51 39.710           ~ 226 1
5 SNR G130.7+03.1 SNR 02 05 37.0 +64 49 42           ~ 562 4
6 PSR J0205+6449 Psr 02 05 37.92 +64 49 42.8           ~ 208 1
7 PSR J0218+42 Psr 02 18 06.3604 +42 32 17.365           ~ 298 2
8 IC 1848 OpC 02 51 06 +60 24.6   6.87 6.5     ~ 443 2
9 NAME Per Arm PoG 03 30 +45.0           ~ 1239 0
10 PSR J0357+32 Psr 03 57 52.161 +32 05 23.63           ~ 75 0
11 PSR J0437-47 Psr 04 37 15.7976203608 -47 15 08.536908257           DC 750 0
12 HESS J0534+220 gam 05 34 +22.0           ~ 3 1
13 V* CM Tau Psr 05 34 31.93830 +22 00 52.1758           ~ 4785 1
14 M 1 SNR 05 34 31.94 +22 00 52.2           ~ 5576 4
15 NAME Gal Anticenter reg 05 46 +28.9           ~ 718 0
16 * 3 Mon ** 06 01 50.42241 -10 35 52.5565 4.24 4.82 4.94     B5III/V 51 1
17 PSR B0613-02.0 Psr 06 13 43.9759 -02 00 47.228           ~ 201 1
18 PSR J0631+10 Psr 06 31 27.369 +10 37 05.63           ~ 102 0
19 LDN 1605 DNe 06 32.8 +10 38           ~ 14 0
20 GeV J0633+0645 gam 06 33 08.8 +06 45 49           ~ 6 1
21 PSR J0633+0632 Psr 06 33 44.136 +06 32 29.48           ~ 58 1
22 NAME Geminga Psr 06 33 54.153 +17 46 12.91           ~ 1088 0
23 PSR B0656+14 Psr 06 59 48.183 +14 14 21.54   24.85 24.90     ~ 754 1
24 PSR B0740-28 Psr 07 42 49.058 -28 22 43.76           ~ 353 0
25 NAME GUM Nebula ISM 07 43 -42.1           ~ 387 1
26 PSR J0751+1807 Psr 07 51 09.1539 +18 07 38.335           ~ 252 1
27 NAME Vela X Psr 08 33 08.880 -45 11 24.36           ~ 241 1
28 NAME Vela XYZ Rad 08 34.0 -45 50           ~ 1107 2
29 NAME Vela Pulsar Psr 08 35 20.65525 -45 10 35.1545           ~ 2044 1
30 NAME Car Arm PoG 10 00 -60.0           ~ 377 1
31 SNR G284.3-01.8 Rad 10 18.3 -59 00           ~ 101 2
32 PSR J1028-5819 Psr 10 28 27.888 -58 19 06.14           ~ 86 1
33 PSR B1046-58 Psr 10 48 12.391 -58 32 02.68           ~ 228 0
34 PSR B1055-52 Psr 10 57 58.970 -52 26 56.52           ~ 680 0
35 PSR J1124-5916 Psr 11 24 39.1 -59 16 20           ~ 132 1
36 SNR G292.0+01.8 SNR 11 24 59 -59 19.1           ~ 289 1
37 CPD-63 2495 HXB 13 02 47.6541729595 -63 50 08.625922862 10.34 10.72 9.98 10.03   O9.5Ve 670 1
38 PSR J1357-6429 Psr 13 57 02.525 -64 29 29.89           ~ 117 1
39 SNR G312.4-00.4 SNR 14 09.9 -61 29           ~ 88 1
40 PSR J1418-6058 Psr 14 18 42.725 -60 58 01.89           ~ 103 0
41 2EGS J1418-6049 gam 14 18 46 -60 58.7           ~ 73 0
42 NAME Kookaburra reg 14 19 -60.9           ~ 47 1
43 PSR J1420-6048 Psr 14 20 08.190 -60 48 14.85           ~ 124 0
44 PSR J1459-60 Psr 14 59 30.222 -60 53 19.87           ~ 43 0
45 PSR J1509-5850 Psr 15 09 27.153 -58 50 56.05           ~ 90 0
46 PSR B1509-58 Psr 15 13 55.52 -59 08 08.8           ~ 792 1
47 PSR J1614-2230 Psr 16 14 36.5070 -22 30 31.207           ~ 275 1
48 PSR B1706-44 Psr 17 09 42.62 -44 29 05.8           ~ 571 1
49 HESS J1718-385 gam 17 18 07 -38 33.0           ~ 29 0
50 PSR J1718-3825 Psr 17 18 13.576 -38 25 18.56           ~ 74 0
51 PSR J1732-31 Psr 17 32 33.551 -31 31 20.85           ~ 60 0
52 PSR J1740+1000 Psr 17 40 25.91 +10 00 06.0           ~ 54 0
53 PSR J1741-2054 Psr 17 41 57.282 -20 54 04.11           ~ 93 1
54 PSR J1744-1134 Psr 17 44 29.4103 -11 34 54.727           ~ 205 1
55 NAME Gal Center reg 17 45 40.04 -29 00 28.1           ~ 11450 0
56 NAME Mouse Rad 17 47 15.78 -29 58 01.0           ~ 90 1
57 PSR J1747-2958 Psr 17 47 15.869 -29 58 00.93           ~ 105 1
58 PSR J1809-2332 Psr 18 09 50.250 -23 32 22.68     21.47 19.61 17.48 M5 78 0
59 PSR J1813-1246 Psr 18 13 23.768 -12 46 00.63           ~ 72 0
60 PSR J1826-1256 Psr 18 26 08.570 -12 56 33.53           ~ 98 1
61 PSR B1823-13 Psr 18 26 13.06 -13 34 48.1           ~ 349 1
62 V* V479 Sct HXB 18 26 15.0561532140 -14 50 54.249464136 12.02 12.23 11.27 11.04   ON6V((f))z 491 2
63 HD 170061 Be* 18 28 00.7384916673 -14 42 24.620334247 9.17 9.85 9.53 9.74   OBe 35 0
64 PSR J1833-1034 Psr 18 33 33.612 -10 34 07.69           ~ 388 1
65 PSR J1836+5925 Psr 18 36 13.661 +59 25 29.77           ~ 122 1
66 PSR J1907+06 Psr 19 07 54.751 +06 02 15.79           ~ 88 0
67 PSR J1930+1852 Psr 19 30 30.13 +18 52 14.1           ~ 78 1
68 SNR G068.8+02.6 SNR 19 52 55 +32 54.2           ~ 328 1
69 PSR B1951+32 Psr 19 52 58.181 +32 52 40.98           ~ 550 2
70 PSR J1958+2846 Psr 19 58 40.1020152614 +28 45 54.090901230           ~ 53 0
71 MGRO J2019+37 gam 20 20.1 +36 43           ~ 53 0
72 NAME gam Cyg SNR SNR 20 20 17.100 +40 26 09.00           ~ 199 2
73 PSR J2021+3651 Psr 20 21 05.40 +36 51 04.5           ~ 148 1
74 GRO J2021+37 gam 20 21 19.9 +37 15 12           ~ 92 2
75 GRO J2019+40 gam 20 21.5 +40 26           ~ 126 1
76 PSR J2021+4026 Psr 20 21 30.496 +40 26 53.56           ~ 207 2
77 Cl Berkeley 87 OpC 20 21 43.01 +37 22 13.8           ~ 107 0
78 * gam Cyg V* 20 22 13.7018357 +40 15 24.044963 3.44 2.90 2.23 1.74 1.40 F8Ib 550 0
79 TeV J2032+4130 gam 20 32.1 +41 34           ~ 118 0
80 [MT91] 213 Be* 20 32 13.1248987067 +41 27 24.343749507 13.12 13.08 11.266     B0Vp 208 0
81 V* V1521 Cyg HXB 20 32 25.78 +40 57 27.9           WN4/5-6/7 1762 2
82 1AGL J2032+4102 gam 20 32 27.70 +41 02 00.0           ~ 8 1
83 Ass Cyg OB 2 As* 20 33.2 +41 19           ~ 785 0
84 PSR J2043+2740 Psr 20 43 43.5 +27 40 56           ~ 96 0
85 PSR J2124-3358 Psr 21 24 43.8464 -33 58 44.961           ~ 247 1
86 NAME Boomerang PWN G106.6+2.9 SNR 22 29 +61.2           ~ 30 1
87 PSR J2229+6114 Psr 22 29 05.262 +61 14 08.48           ~ 173 2
88 PSR J2238+59 Psr 22 38 14.6 +59 04 48           ~ 13 0
89 [ME95] CLUST 3 As* ~ ~           ~ 3 0
90 SNR G203.0+12.0 SNR ~ ~           ~ 6 1

    Equat.    Gal    SGal    Ecl

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2020.06.02-05:06:08

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