The second IBIS/ISGRI soft gamma-ray survey catalog

被引:129
作者
Bird, AJ [1 ]
Barlow, EJ
Bassani, L
Bazzano, A
Bélanger, G
Bodaghee, A
Capitanio, F
Dean, AJ
Fiocchi, M
Hill, AB
Lebrun, F
Malizia, A
Mas-Hesse, JM
Molina, M
Moran, L
Renaud, M
Sguera, V
Shaw, SE
Stephen, JB
Terrier, R
Ubertini, P
Walter, R
Willis, DR
Winkler, C
机构
[1] Univ Southampton, Sch Phys & Astron, Southampton SO17 1BJ, Hants, England
[2] INAF, IASF, Bologna, Italy
[3] INAF, IASF, Rome, Italy
[4] CEA Saclay, DAPNIA, Serv Astrophys, F-91191 Gif Sur Yvette, France
[5] Coll France, APC, Federat Rech, F-75231 Paris, France
[6] Observ Geneva, INTEGRAL Sci Data Ctr, CH-1291 Versoix, Switzerland
[7] CSIC, Ctr Astrobiol, INTA, E-28850 Madrid, Spain
[8] Estec, ESA, Res & Sci Support Dept, NL-2201 AZ Noordwijk, Netherlands
关键词
Galaxy : general; gamma rays : observations; surveys;
D O I
10.1086/498090
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In this paper we report the second soft gamma-ray source catalog obtained with the IBIS/ISGRI gamma-ray imager on board the INTEGRAL satellite. The scientific data set is based on more than 10 Ms of high-quality observations performed during the first 2 years of Core Program and public IBIS/ISGRI observations, and covers similar to 50% of the whole sky. The main aim of the first survey was to scan systematically, for the first time at energies above 20 keV, the whole Galactic plane to achieve a limiting sensitivity of similar to 1 mcrab in the central radian. The target of the second year of the INTEGRAL mission lifetime was to expand as much as possible our knowledge of the soft gamma- ray sky, with the same limiting sensitivity, to at least 50% of the whole sky, mainly by including a substantial coverage of extragalactic fields. This catalog comprises more than 200 high-energy sources detected in the energy range 20-100 keV, including new transients not active during the first year of operation, faint persistent objects revealed with longer exposure time, and several Galactic and extragalactic sources in sky regions not observed in the first survey. The mean position error for all the sources detected with significance above 10 sigma is similar to 40 '', enough to identify most of them with a known X-ray counterpart and to unveil the nature of most of the strongly absorbed ones, even though they are very difficult to detect in X-rays.
引用
收藏
页码:765 / 776
页数:12
相关论文
共 80 条
  • [1] Discovery of extended VHE gamma-ray emission from the asymmetric pulsar wind nebula in MSH 15-52 with HESS
    Aharonian, F
    Akhperjanian, AG
    Aye, KM
    Bazer-Bachi, AR
    Beilicke, M
    Benbow, W
    Berge, D
    Berghaus, P
    Bernlöhr, K
    Boisson, C
    Bolz, O
    Braun, I
    Breitling, F
    Brown, AM
    Gordo, JB
    Chadwick, PM
    Chounet, LM
    Cornils, R
    Costamante, L
    Degrange, B
    Djannati-Ataï, A
    Drury, LO
    Dubus, G
    Emmanoulopoulos, D
    Espigat, P
    Feinstein, F
    Fleury, P
    Fontaine, G
    Fuchs, Y
    Funk, S
    Gallant, YA
    Giebels, B
    Gillessen, S
    Glicenstein, JF
    Goret, P
    Hadjichristidis, C
    Hauser, M
    Heinzelmann, G
    Henri, G
    Hermann, G
    Hinton, JA
    Hofmann, W
    Holleran, M
    Horns, D
    de Jager, OC
    Khélifi, B
    Komin, N
    Konopelko, A
    Latham, IJ
    Le Gallou, R
    [J]. ASTRONOMY & ASTROPHYSICS, 2005, 435 (01): : L17 - L20
  • [2] [Anonymous], 2003, IAU CIRC
  • [3] X-RAY OBSERVATIONS OF THE OPHIUCHUS, PKS 0745-191 AND CYGNUS-A CLUSTERS OF GALAXIES
    ARNAUD, KA
    JOHNSTONE, RM
    FABIAN, AC
    CRAWFORD, CS
    NULSEN, PEJ
    SHAFER, RA
    MUSHOTZKY, RF
    [J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1987, 227 (01) : 241 - &
  • [4] LOCALIZATION, TIME HISTORIES, AND ENERGY-SPECTRA OF A NEW TYPE OF RECURRENT HIGH-ENERGY TRANSIENT SOURCE
    ATTEIA, JL
    BOER, M
    HURLEY, K
    NIEL, M
    VEDRENNE, G
    FENIMORE, EE
    KLEBESADEL, RW
    LAROS, JG
    KUZNETSOV, AV
    SUNYAEV, RA
    TEREKHOV, OV
    KOUVELIOTOU, C
    CLINE, T
    DENNIS, B
    DESAI, U
    ORWIG, L
    [J]. ASTROPHYSICAL JOURNAL, 1987, 320 (02) : L105 - L110
  • [5] BeppoSAX serendipitous discovery of the X-ray pulsar SAX J1802.7-2017
    Augello, G
    Iaria, R
    Robba, NR
    Di Salvo, T
    Burderi, L
    Lavagetto, G
    Stella, L
    [J]. ASTROPHYSICAL JOURNAL, 2003, 596 (01) : L63 - L66
  • [6] Discovery of a transient X-ray pulsar, AX J1841.0-0536, in the Scutum arm region with ASCA
    Bamba, A
    Yokogawa, J
    Ueno, M
    Koyama, K
    Yamauchi, S
    [J]. PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, 2001, 53 (06) : 1179 - 1183
  • [7] Detection and analysis of a new INTEGRAL hard X-ray transient, IGR J17285-2922
    Barlow, EJ
    Bird, AJ
    Clark, DJ
    Cornelisse, R
    Dean, AJ
    Hill, AB
    Moran, L
    Sguera, V
    Shaw, SE
    Willis, DR
    Capitanio, F
    Del Santo, M
    Bassani, L
    [J]. ASTRONOMY & ASTROPHYSICS, 2005, 437 (02) : L27 - L30
  • [8] The Burst Alert telescope (BAT) on the swift MIDEX mission
    Barthelmy, SD
    [J]. X-RAY AND GAMMA-RAY INSTRUMENTATION FOR ASTRONOMY XIII, 2004, 5165 : 175 - 189
  • [9] BASSANI L, 2005, ASTRON TEL, V537
  • [10] Bélanger G, 2004, ASTROPHYS J, V601, pL163, DOI 10.1086/381738