Catalog (523) | Long-Term (470) | Short-Term (53) | AGN (4) | HMXB (15) | LMXB (16) | CV (2) | Other (1) | NotID
Show regions file | Show data file
intibisass Twitter

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 J00291+59347.25459.563 21.88 ± 0.23 95.13LMXB [R261:264]
4U0115+6319.62563.746 125.50 ± 0.36 348.61HMXB [R667:675]
263.76 ± 0.39 676.31 [R238:238]
IGR J01363+661024.06066.188 15.44 ± 1.88 8.21HMXB [R185:185] [1, 2]
IGR J02466-422241.644-42.360 2.01 ± 0.36 5.58AGN XBONG z=0.0696; MCG -07-06-018; [R446:452] [1, 2]
1H 0323+34251.14034.168 1.99 ± 0.32 6.22AGN NL Sy1 z=0.0629; 2MASX J032441.19+341045.9; [R25:300] [1, 2]
V0332+5353.75153.172 393.29 ± 0.34 1156.74HMXB [R269:288]
V1062 Tau75.61724.732 3.95 ± 0.48 8.23CV [R102:102]
A 0535+26284.73526.324 223.49 ± 11.51 19.42HMXB [R831:831]
502.68 ± 0.58 866.69 [R352:352]
ESO 005- G 00492.575-86.554 2.79 ± 0.42 6.64AGN Sy2 z=0.006384; [R99:99]
GRO J1008-57152.447-58.298 13.62 ± 0.21 64.86HMXB [R200:203] [1]
30.27 ± 2.30 13.16 [R372:372]
3U 1022-55159.401-56.801 8.66 ± 0.40 21.65HMXB [R529:530]
IGR J11203+4531170.09045.530 3.68 ± 0.53 6.94 [R74:76] [1]
IGR J11215-5952170.429-59.869 3.40 ± 0.28 12.14HMXB SFXT [R197:198] [1, 2, 3]
10.54 ± 0.58 18.17 [R88:88]
55.91 ± 2.91 19.21 [R308:308]
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 J13290-6323202.268-63.392 2.26 ± 0.35 6.46 [R92:92]
XTE J1543-568236.011-56.748 10.47 ± 0.79 13.25HMXB [R468:468]
11.28 ± 0.57 19.79 [R37:38]
XTE J1550-564237.751-56.474 229.53 ± 0.32 717.28LMXB [R54:60]
SWIFT J1626.6-5156246.659-51.938 12.21 ± 0.93 13.13LMXB [R398:407] [1]
IGR J16358-4726248.992-47.407 13.69 ± 0.58 23.60HMXB [R54:57] [1, 2, 3] [cnfsn]
44.23 ± 5.50 8.04 [R185:185] [cnfsn]
IGR J16465-4507251.648-45.118 4.64 ± 0.34 13.65HMXB [R222:224] [1, 2] [cnfsn]
9.53 ± 0.52 18.33 [R232:233] [cnfsn]
XTE J1709-267257.386-26.658 13.36 ± 0.50 26.72LMXB [R171:172]
IGR J17098-3628257.438-36.460 19.33 ± 0.30 64.43 [R298:305] [1, 2] [cnfsn]
KS 1716-389259.003-38.879 1.51 ± 0.27 5.59HMXB XTE J1716-389; [R36:63] [1, 2, 3]
XTE J1720-318259.993-31.753 23.42 ± 0.34 68.88LMXB [R56:63]
IGR J17269-4737261.681-47.647 12.55 ± 1.40 8.96XRB XTE J1726-476; [R364:364] [1]
IGR J17285-2922262.163-29.370 3.54 ± 0.35 10.11LMXB? XTE J1728-295; [R119:122] [1, 2]
IGR J17379-3747264.465-37.774 7.79 ± 0.95 8.20 Burster; [R165:165] [1]
GRS 1736-297264.899-29.736 3.35 ± 0.30 11.17LMXB [R479:484] [1]
4.44 ± 0.35 12.69 [R408:409]
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 J17445-2747266.082-27.772 2.69 ± 0.23 11.70 [R165:173] [1]
IGR J17473-2721266.841-27.352 63.83 ± 0.40 159.57LMXB [R667:725] [1, 2]
A 1744-361267.052-36.133 11.88 ± 0.42 28.29LMXB [R181:185] [1]
4U 1745-203267.217-20.359 10.67 ± 0.47 22.70LMXB [R120:120]
SLX 1746-331267.477-33.201 6.39 ± 0.19 33.63LMXB BH X-ray transient [R106:112]
SAX J1750.8-2900267.600-29.038 35.64 ± 0.78 45.69LMXB [R670:674] [1] [cnfsn]
IGR J17507-2856267.677-28.909 2.47 ± 0.34 7.26 [R236:237] [1] [cnfsn]
XTE J1751-305267.816-30.616 7.38 ± 0.55 13.42LMXB ms-pulsar [R299:299] [1]
15.37 ± 0.65 23.65 [R546:546]
XTE J1807-294271.770-29.430 6.36 ± 0.28 22.71LMXB [R50:63]
XTE J1810-189272.585-19.070 30.60 ± 0.70 43.71LMXB Burster; [R660:674] [1]
V4722 Sgr272.685-26.150 25.10 ± 0.23 109.13LMXB [R594:606]
XTE J1817-330274.431-33.020 33.76 ± 0.18 187.56LMXB [R406:426]
IGR J18325-0756278.112-7.938 6.40 ± 0.27 23.70 [R62:66] [1]
7.99 ± 0.26 30.73 [R429:432]
IGR J18462-0223281.567-2.387 23.89 ± 2.04 11.71HMXB? [R610:610] [1, 2]
A 1845-024282.048-2.426 9.66 ± 0.92 10.50HMXB [R229:233]
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 J1858+034284.6733.437 52.68 ± 0.22 239.45HMXB [R186:193]
4U 1901+03285.9173.207 80.54 ± 0.17 473.76HMXB [R48:70]
SWIFT J1922.7-1716290.615-17.300 4.78 ± 0.58 8.24 [R371:371] [1]
IGR J21343+4738323.62547.614 1.40 ± 0.20 7.00HMXB 1RXS J213419.6+473810; USNO-B1.0 1376-0511904; [R25:200] [1]
FO Aqr334.402-8.301 2.47 ± 0.44 5.61CV [R25:25]
IGR J22517+2218342.93922.316 1.89 ± 0.33 5.73AGN Quasar z=3.668; =MG3 J225155+2217; [R316:337] [1]
⇑⇑⇑Selection statistics: 53 (|b|>5d: 13, 5?) 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
Mirror at Max Planck Institut für Astrophysik | CVS

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

Valid HTML 4.01 Transitional