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
TYCHO SNR6.33464.150 0.64 ± 0.07 9.14SNR
Gamma Cas14.17660.712 3.32 ± 0.08 41.50Star
4U 0142+6126.63061.738 2.00 ± 0.11 18.18AXP
PERSEUS CLUSTER49.97341.509 2.64 ± 0.17 15.53Cluster Thermal emission dominates;
Crab83.63222.016 1000.00 ± 0.13 7692.31PSR
PSR 0540-6985.005-69.338 1.63 ± 0.13 12.54PSR
Vela pulsar128.835-45.182 6.98 ± 0.08 87.25PSR
eta Car161.189-59.719 0.61 ± 0.09 6.78Star
IGR J11187-5438169.580-54.660 0.52 ± 0.10 5.20XRB [1]
IGR J12349-6434188.724-64.565 3.11 ± 0.10 31.10SymbStr V* RT Cru; [1, 2]
Coma194.86527.938 1.55 ± 0.14 11.07Cluster
IGR J14003-6326210.204-63.414 0.83 ± 0.09 9.22PWN ms pulsar [1, 2, 3]
PSR 1509-58228.480-59.145 8.86 ± 0.09 98.44PSR
IGR J16175-5059244.357-50.972 0.41 ± 0.08 5.12PSR PSR J1617-5055
Triangulum A249.567-64.347 1.09 ± 0.15 7.27Cluster z=0.051;
1RXS J170849.0-400910257.214-40.142 1.09 ± 0.08 13.62AXP
RX J1713.7-3946257.991-39.862 0.40 ± 0.08 5.00SNR G347.3-0.5;
Oph cluster258.114-23.347 3.70 ± 0.08 46.25Cluster
IGR J17269-4737261.681-47.647 12.55 ± 1.40 8.96XRB XTE J1726-476; [R364:364] [1]
IGR J17448-3231266.190-32.528 0.39 ± 0.05 7.80SNR [1] [cnfsn]
IGR J17456-2901266.401-29.026 5.70 ± 0.05 114.00NucStrCl =AX J1745.6-2901; Nuclear stellar cluster; [1, 2] [cnfsn]
IGR J17475-2822266.864-28.364 2.26 ± 0.05 45.20MolCld SgrB2; [1] [cnfsn]
SGR 1806-20272.162-20.404 2.62 ± 0.07 37.43SGR
PSR J1811-1925272.862-19.423 0.74 ± 0.07 10.57PSR/PWN SNR G11.2-0.3;
IGR J18135-1751273.397-17.858 1.05 ± 0.08 13.12SNR/PWN HESS J1813-178; [1, 2]
SNR 021.5-00.9278.394-10.572 2.91 ± 0.09 32.33SNR
AX J1838.0-0655279.503-6.911 1.95 ± 0.10 19.50SNR/PWN HESS J1837-069; [1]
1E 1841-045280.329-4.938 2.64 ± 0.09 29.33PSR/PWN
PSR J1846-0258281.613-2.983 1.62 ± 0.09 18.00PSR/PWN AXP? [1]
IGR J18490-0000282.258-0.013 1.14 ± 0.08 14.25PWN [1, 2, 3, 4]
SGR 1900+14286.8399.322 0.91 ± 0.07 13.00SGR
IGR J20159+3713303.98037.230 0.86 ± 0.10 8.60SNR SNR G074.9+01.2; SWIFT J2015.9+3715
Cas A350.84658.813 3.63 ± 0.08 45.38SNR
⇑⇑⇑Selection statistics: 33 (|b|>5d: 8) 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.
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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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