2017ApJ...843..139A


C.D.S. - SIMBAD4 rel 1.7 - 2020.12.02CET14:54:47

2017ApJ...843..139A - Astrophys. J., 843, 139-139 (2017/July-2)

Search for extended sources in the galactic plane using six years of Fermi-Large Area Telescope Pass 8 data above 10 GeV.

ACKERMANN M., AJELLO M., BALDINI L., BALLET J., BARBIELLINI G., BASTIERI D., BELLAZZINI R., BISSALDI E., BLOOM E.D., BONINO R., BOTTACINI E., BRANDT T.J., BREGEON J., BRUEL P., BUEHLER R., CAMERON R.A., CARAGIULO M., CARAVEO P.A., CASTRO D., CAVAZZUTI E., CECCHI C., CHARLES E., CHEKHTMAN A., CHEUNG C.C., CHIARO G., CIPRINI S., COHEN J.M., COSTANTIN D., COSTANZA F., CUTINI S., D'AMMANDO F., DE PALMA F., DESIANTE R., DIGEL S.W., DI LALLA N., DI MAURO M., DI VENERE L., FAVUZZI C., FEGAN S.J., FERRARA E.C., FRANCKOWIAK A., FUKAZAWA Y., FUNK S., FUSCO P., GARGANO F., GASPARRINI D., GIGLIETTO N., GIORDANO F., GIROLETTI M., GREEN D., GRENIER I.A., GRONDIN M.-H., GUILLEMOT L., GUIRIEC S., HARDING A.K., HAYS E., HEWITT J.W., HORAN D., HOU X., JOHANNESSON G., KAMAE T., KUSS M., LA MURA G., LARSSON S., LEMOINE-GOUMARD M., LI J., LONGO F., LOPARCO F., LUBRANO P., MAGILL J.D., MALDERA S., MALYSHEV D., MANFREDA A., MAZZIOTTA M.N., MICHELSON P.F., MITTHUMSIRI W., MIZUNO T., MONZANI M.E., MORSELLI A., MOSKALENKO I.V., NEGRO M., NUSS E., OHSUGI T., OMODEI N., ORIENTI M., ORLANDO E., ORMES J.F., PALIYA V.S., PANEQUE D., PERKINS J.S., PERSIC M., PESCE-ROLLINS M., PETROSIAN V., PIRON F., PORTER T.A., PRINCIPE G., RAINO S., RANDO R., RAZZANO M., RAZZAQUE S., REIMER A., REIMER O., REPOSEUR T., SGRO C., SIMONE D., SISKIND E.J., SPADA F., SPANDRE G., SPINELLI P., SUSON D.J., TAK D., THAYER J.B., THOMPSON D.J., TORRES D.F., TOSTI G., TROJA E., VIANELLO G., WOOD K.S. and WOOD M.

Abstract (from CDS):

The spatial extension of a γ-ray source is an essential ingredient to determine its spectral properties, as well as its potential multiwavelength counterpart. The capability to spatially resolve γ-ray sources is greatly improved by the newly delivered Fermi-Large Area Telescope (LAT) Pass 8 event-level analysis, which provides a greater acceptance and an improved point-spread function, two crucial factors for the detection of extended sources. Here, we present a complete search for extended sources located within 7° from the Galactic plane, using 6 yr of Fermi-LAT data above 10 GeV. We find 46 extended sources and provide their morphological and spectral characteristics. This constitutes the first catalog of hard Fermi-LAT extended sources, named the Fermi Galactic Extended Source Catalog, which allows a thorough study of the properties of the Galactic plane in the sub-TeV domain.

Abstract Copyright: © 2017. The American Astronomical Society. All rights reserved.

Journal keyword(s): catalogs - gamma rays: general - gamma rays: general

Nomenclature: Tables 1-3: FGES JHHMM.m+DDMM N=46.

Status at CDS : Large table(s) will be appraised for possible ingestion in VizieR.

Simbad objects: 78

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Number of rows : 78

N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2021
#notes
1 SNR G132.6+01.5 SNR 02 17 40 +62 45.0           ~ 158 0
2 W 3 MoC 02 27 04.10 +61 52 27.1           ~ 969 3
3 SNR G150.3+04.5 SNR 04 31 16.8 +55 53 24           ~ 14 0
4 SNR G160.8+02.6 SNR 05 01 00.000 +46 40 00.00           ~ 192 0
5 M 1 SNR 05 34 31.94 +22 00 52.2           ~ 5673 4
6 SNR G180.0-01.7 SNR 05 39 00.000 +27 50 00.00           ~ 217 2
7 NAME Gal Anticenter reg 05 46 +28.9           ~ 738 0
8 IC 443 SNR 06 18 02.7 +22 39 36           ~ 1112 1
9 SNR G189.6+03.3 SNR 06 19 +22.2           ~ 26 0
10 LBN 188.69+04.25 HII 06 22 32 +22 58.5           ~ 43 1
11 NAME Pup A SNR 08 24 07 -42 59.8           ~ 527 1
12 NAME Vela X Psr 08 33 08.880 -45 11 24.36           ~ 249 1
13 NAME Vela Jr SN SNR 08 52.0 -46 20           ~ 409 2
14 QSO B0903-573 BLL 09 04 53.17928113 -57 35 05.7821238           ~ 67 1
15 HESS J1023-575 gam 10 23 -57.5           ~ 53 0
16 Cl Westerlund 2 OpC 10 23 58.1 -57 45 49   11.59 10.5     ~ 288 0
17 SNR G298.5-00.3 SNR 12 12.7 -62 52           ~ 29 0
18 SNR G298.6-00.0 SNR 12 13 41.000 -62 37 00.00           ~ 35 0
19 PSR J1301-6305 Psr 13 01 45.76 -63 05 33.9           ~ 102 2
20 PSR J1357-6429 Psr 13 57 02.525 -64 29 29.89           ~ 121 1
21 AX J1418.7-6058 X 14 18 38.6 -60 57 49           ~ 44 0
22 PSR J1418-6058 Psr 14 18 42.725 -60 58 01.89           ~ 105 0
23 2EGS J1418-6049 gam 14 18 46 -60 58.7           ~ 73 0
24 NAME Kookaburra reg 14 19 -60.9           ~ 48 1
25 AX J1420.1-6049 Rad 14 20 07.8 -60 48 56           ~ 21 0
26 PSR J1420-6048 Psr 14 20 08.190 -60 48 14.85           ~ 127 0
27 ESO 134-11 HII 14 40 29 -62 38.7           ~ 510 1
28 HESS J1507-622 gam 15 07 30 -62 25.0           ~ 33 0
29 PSR J1614-5048 Psr 16 14 11.29 -50 48 03.5           ~ 98 0
30 1FHL J1615.3-5146 gam 16 15 12.62 -51 34 53.3           ~ 52 0
31 SNR G332.4+00.1 SNR 16 15 20 -50 42.0           ~ 82 0
32 PSR J1616-5109 Psr 16 16 30.9 -51 09 17           ~ 7 0
33 PSR J1617-5055 Psr 16 17 29.35 -50 55 12.8           ~ 101 1
34 PKS 1613-50 Rad 16 17 33.000 -51 02 00.00           ~ 460 3
35 3FGL J1620.0-5101 gam 16 20 02 -51 01.7           ~ 6 0
36 3FHL J1633.0-4746e HXB 16 32 01.87 -47 52 28.3           O8I 150 3
37 HESS J1634-472 gam 16 34 -47.2           ~ 25 0
38 CTB 33 Rad 16 35 06.9 -47 47 25           ~ 108 1
39 SNR G338.3-00.0 Rad 16 40 30.0 -46 33 00           ~ 133 2
40 SNR G347.3-00.5 SNR 17 12 27 -39 41.2           ~ 620 1
41 HESS J1713-381 gam 17 13 -38.1           ~ 29 1
42 SNR G348.7+00.3 SNR 17 13 43.0 -38 10 12           ~ 109 2
43 NAME CTB 37 Complex ? 17 14.1 -38 32           ~ 4 0
44 SNR G348.5+00.1 SNR 17 14 31.780 -38 28 34.50           ~ 199 3
45 NAME Gal Center reg 17 45 40.04 -29 00 28.1           ~ 11840 0
46 HESS J1800-240 gam 18 00 37 -23 59.8           ~ 24 0
47 SNR G006.4-00.1 SNR 18 01 22.7 -23 17 20           ~ 660 1
48 HESS J1800-240A gam 18 01 47.0 -23 58 39           ~ 22 0
49 PSR B1800-21 Psr 18 03 51.45 -21 37 08.1           ~ 233 1
50 1AGLR J1807-2103 gam 18 04 29.70 -21 43 57.2           ~ 59 0
51 CXOU J180432.4-214009 X 18 04 32.47 -21 40 09.8           ~ 5 0
52 W 30 SNR 18 05 38 -21 36.7           ~ 159 1
53 PSR B1823-13 Psr 18 26 13.06 -13 34 48.1           ~ 357 1
54 SNR G024.7+00.6 SNR 18 34 46 -07 05.8           ~ 79 0
55 SNR G023.3-00.3 SNR 18 34 51.80 -08 44 38.2           ~ 192 0
56 GAL 025.18+00.26 As* 18 36.3 -06 47           ~ 5 0
57 PSR J1838-0655 Psr 18 38 03.13 -06 55 33.4           ~ 82 1
58 [GH2008] 14 SNR 18 38 03.13 -06 55 33.4           ~ 70 2
59 PSR J1838-0549 Psr 18 38 38.1 -05 49 12           ~ 21 0
60 PSR J1838-0537 Psr 18 38 56.02 -05 37 09.0           ~ 29 0
61 2FHL J1839.5-0705 gam 18 39 30.2 -07 05 03           ~ 2 0
62 HESS J1841-055 gam 18 40 55.0 -05 33 00           ~ 47 1
63 [KRL2007b] 332 HXB 18 41 00.43 -05 35 46.5           B1Ib 117 1
64 Fermi J1841.1-0458 gam 18 41.1 -04 58           ~ 3 0
65 PSR J1841-0524 Psr 18 41 49.3551255320 -05 24 30.537633506           ~ 27 0
66 SNR G034.6-00.5 SNR 18 56 10.650 +01 13 21.30           ~ 834 2
67 PSR J1856+0245 Psr 18 56 50.80 +02 45 50.2           ~ 26 0
68 HESS J1857+026 gam 18 57 11.0 +02 40 00           ~ 36 0
69 HESS J1858+020 gam 18 58 20.0 +02 05 24           ~ 35 0
70 SNR G049.1-00.1 SNR 19 23 19.300 +14 09 21.00           ~ 243 0
71 ARGO J2021+4038 gam 20 19 00.0 +40 42 00           ~ 26 1
72 NAME gam Cyg SNR SNR 20 20 17.100 +40 26 09.00           ~ 200 2
73 NAME Cyg X Cld 20 28 41 +41 10.2           ~ 635 1
74 Ass Cyg OB 2 As* 20 33.2 +41 19           ~ 810 0
75 SNR G089.0+04.7 SNR 20 45.0 +50 35           ~ 197 0
76 NAME Cyg Loop SNR 20 51.0 +30 40           ~ 830 0
77 LBN 091.00-06.39 HII 21 42.3 +44 32           ~ 7 0
78 SNR G109.1-01.0 SNR 23 01 35 +58 53.0           ~ 317 0

    Equat.    Gal    SGal    Ecl

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2020.12.02-14:54:47

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