Catalog (523) | Long-Term (470) | Short-Term (53) | AGN (214) | HMXB (86) | LMXB (99) | CV (35) | Other (33) | NotID
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INTEGRAL All-sky survey (current version, 523 sources)
Please refer to this catalog as: Krivonos et al., 2007, A&A, 475, 775 [NASA ADS]
SourceRa
(J2000)
Dec
(J2000)
17-60 keV, Flux1,2,3
(mCrab)
Sign.Type4Notes5
IGR J02448+144241.22014.710 2.11 ± 0.44 4.80
IGR J05305-655982.636-65.984 0.81 ± 0.13 6.23 [cnfsn]
PKS 0528+13482.73913.563 0.81 ± 0.15 5.40AGN? Quasar z=2.07;
IGR J10447-6027161.196-60.454 0.62 ± 0.09 6.89 2MASSJ10445192-6025115; [1, 2]
IGR J11203+4531170.09045.530 3.68 ± 0.53 6.94 [R74:76] [1]
IGR J11321-5311173.047-53.200 34.50 ± 2.66 12.97 [R330:330] [1]
IGR J11395-6520174.858-65.406 6.40 ± 0.65 9.85RSCVn? HD 101379; [R88:90]
IGR J12134-6015183.374-60.265 0.44 ± 0.09 4.89 1RXS J121324.5-601458;
IGR J13186-6257199.650-62.947 0.81 ± 0.09 9.00HMXB? [1, 2]
IGR J13290-6323202.268-63.392 2.26 ± 0.35 6.46 [R92:92]
IGR J14488-4009222.201-40.152 0.60 ± 0.11 5.45
IGR J15360-5750234.014-57.806 0.95 ± 0.09 10.56AGN? =IGR J15359-5750; [1, 2]
IGR J15414-5030235.350-50.512 0.61 ± 0.09 6.78CV? Galactic source; =IGR J15415-5029; [1]
IGR J15529-5029238.233-50.490 0.43 ± 0.08 5.38CV? Galactic source [1]
IGR J16058-7253241.470-72.900 1.19 ± 0.16 7.44 SWIFT J1605.9-7250?; IRAS F15596-7245?;
IGR J16336-4733248.396-47.559 7.05 ± 0.08 88.12 [cnfsn]
IGR J17036+3734255.91037.570 1.09 ± 0.21 5.19
IGR J17062-6143256.556-61.715 1.20 ± 0.16 7.50=SWIFT J1706.6-6146 [1]
IGR J17098-3628257.438-36.460 19.33 ± 0.30 64.43 [R298:305] [1, 2] [cnfsn]
IGR J17197-3010259.930-30.180 0.35 ± 0.06 5.83
IGR J17233-2837260.850-28.620 0.57 ± 0.06 9.50
IGR J17285-2922262.163-29.370 3.54 ± 0.35 10.11LMXB? XTE J1728-295; [R119:122] [1, 2]
IGR J17331-2406263.291-24.142 0.41 ± 0.06 6.83 [1, 2]
IGR J17350-2045263.740-20.754 0.64 ± 0.07 9.14
IGR J17353-3257263.848-32.934 1.01 ± 0.06 16.83HMXB? =IGR J17354-3255; [1, 2]
IGR J17379-3747264.465-37.774 7.79 ± 0.95 8.20 Burster; [R165:165] [1]
IGR J17402-3656265.087-36.936 0.70 ± 0.07 10.00HMXB? =IGR J17404-3655; [1]
IGR J17419-2802265.485-28.031 4.46 ± 0.32 13.94 [R425:426] [1] [cnfsn]
6.58 ± 0.40 16.45 [R361:362] [cnfsn]
7.38 ± 0.47 15.70 [R409:409] [cnfsn]
IGR J17427-3018265.696-30.301 0.28 ± 0.05 5.60AGN? AX J1742.6-3022 [1]
IGR J17445-2747266.082-27.772 2.69 ± 0.23 11.70 [R165:173] [1]
IGR J17505-2644267.636-26.744 0.57 ± 0.05 11.40
IGR J17507-2856267.677-28.909 2.47 ± 0.34 7.26 [R236:237] [1] [cnfsn]
IGR J17585-3057269.636-30.956 0.56 ± 0.05 11.20
IGR J17586-2129269.658-21.327 0.95 ± 0.06 15.83HMXB? [1]
IGR J18134-1636273.370-16.650 0.63 ± 0.08 7.88
IGR J18175-1530274.400-15.470 0.41 ± 0.09 4.56
XTE J1818-245274.597-24.546 2.71 ± 0.06 45.17LMXB?
IGR J18219-1347275.500-13.790 0.50 ± 0.09 5.56
XTE J1824-141276.110-14.440 0.68 ± 0.09 7.56HMXB? X-Ray Pulsar; =IGR J18246-1425; [1]
IGR J18256-1035276.434-10.585 0.58 ± 0.09 6.44
IGR J18293-1213277.340-12.220 0.52 ± 0.09 5.78
AX J183039-1002277.660-10.049 0.68 ± 0.09 7.56AGN? [1]
IGR J18325-0756278.112-7.938 6.40 ± 0.27 23.70 [R62:66] [1]
7.99 ± 0.26 30.73 [R429:432]
IGR J18354-2417278.850-24.290 0.41 ± 0.08 5.12 1WGA J1835.4-2418
IGR J18462-0223281.567-2.387 23.89 ± 2.04 11.71HMXB? [R610:610] [1, 2]
IGR J18486-0047282.104-0.787 0.95 ± 0.08 11.88AGN? strong radio source, high X-ray abs.; [1]
IGR J18539+0727283.5007.488 17.58 ± 0.60 29.30LMXB? [R62:62] [1, 2]
IGR J18578-3405284.469-34.096 4.12 ± 0.56 7.36AGN? [R408:408]
XTE J1901+014285.4151.447 2.28 ± 0.08 28.50HMXB? [1]
IGR J19108+0917287.6419.312 0.35 ± 0.07 5.00
IGR J19193+0754289.8207.908 0.36 ± 0.07 5.14 high systematic noise from GRS 1915+105;
SWIFT J1922.7-1716290.615-17.300 4.78 ± 0.58 8.24 [R371:371] [1]
IGR J19443+2117296.00021.310 0.75 ± 0.12 6.25AGN? =SWIFTJ194353.0+212119; =RX J1943.9+2118; [1, 2]
IGR J19583+1941299.60019.690 0.66 ± 0.14 4.71
SWIFT J2037.2+4151309.30041.850 0.53 ± 0.09 5.89
IGR J20569+4940314.21549.679 0.70 ± 0.10 7.00 3A 2056+493; Blazar or microQSO; [1]
⇑⇑⇑Selection statistics: 56 (|b|>5d: 14, S/N<5σ: 5, &2, 20?) Last updated: May 27 2011
  1. Time-averaged source flux in mCrab units. A flux of 1 mCrab corresponds to 1.43e-11 erg/s/cm2 for a source with a Crab-like spectrum.
  2. Source flux was measured on the map averaged over the indicated spacecraft revolution.
  3. General astrophysical type of the object. LMXB (HMXB) - low- (high-) mass X-ray binary, AGN - active galactic nucleus, SNR/PWN - supernova remnant/pulsar wind nebula CV - cataclysmic variable, PSR - isolated pulsar or pulsar wind nebula, SGR - soft gamma repeater, RS CVn - coronally active binary star, SymbStr - symbiotic star, MolCld - Molecular cloud, Cluster - cluster of galaxies.
  4. Additional notes and/or alternative source names. References are mainly provided for new sources and are related to their discovery and/or nature.
Notes on catalog
  • The positional accuracy of sources detected by IBIS/ISGRI depends on the source significance. The estimated 68% confidence intervals for sources detected at 5-6, 10, and > 20 standart deviations are 2.1, 1.5, and < 0.8 arcmin, respectively.
WEB Links
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This page is maintained by Roman Krivonos (krivonos [re-move] iki.rssi.ru)
(c) 2017 Russian Science Data Center // Space Research Institute // Russian Academy of Sciences // Moscow, Russia
(c) Max Planck Institut für Astrophysik // Garching, Germany

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