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INTREFCAT - INTEGRAL Reference Catalog

 HEASARC
Archive

Overview

The original version of the INTEGRAL Reference Catalog as published in 2003 classified previously known bright X-ray and gamma-ray sources before the launch of INTEGRAL. These sources are, or have been at least once, brighter than ~1 milliCrab above 3 keV energy, and are expected to be detected by INTEGRAL. This catalog was used in the INTEGRAL Quick Look Analysis (QLA) to discover new sources or significantly variable sources. The authors compiled several published X-ray and gamma-ray catalogs, and surveyed recent publications for new sources. Consequently, there were 1121 sources in the original INTEGRAL Reference Catalog. In addition to the source positions, an approximate spectral model and expected flux were given for each source, and the expected INTEGRAL counting rates based on these parameters was derived. Assuming the default instrument performances and at least ~10^5 seconds exposure time for any part of the sky, it is expected that INTEGRAL will detect at least ~700 sources below 10 keV and ~400 sources above 20 keV over the mission life. After the launch of INTEGRAL, a version of this catalog was placed on the ISDC website at http://isdc.unige.ch/index.cgi?Data+catalogs and has been updated periodically since then by adding, for example, new sources discovered by INTEGRAL itself (indicated by the IGR prefix in the name). Thus, as of mid-2004, the INTEGRAL Reference Catalog contained 1390 sources. This HEASARC table is based on the web version at the ISDC, and will be updated whenever the latter is updated.

Catalog Bibcode

2003A&A...411..L59E

Bulletin

The INTREFCAT database table was last updated on 7 September 2008.

References

This table is taken from the online web page maintained by the INTEGRAL Science Data Center at the URL http://isdc.unige.ch/Data/cat/latest/catalog.html Additional information pertaining to an earlier version of this catalog: High-energy sources before INTEGRAL. INTEGRAL reference catalog. Ebisawa K., Bourban G., Bodaghee A., Mowlavi N., Courvoisier T.J.-L. <Astron. Astrophys. 411, L59 (2003)> =2003A&A...411L..59E (SIMBAD/NED BibCode) 


Provenance

This database table is updated automatically in the HEASARC database system
within one week of any changes to the online web page maintained by the
INTEGRAL Science Data Center at the URL
http://isdc.unige.ch/Data/cat/latest/catalog.html


Version Comments

The INTEGRAL Science Data Center's detailed comments about the changes made to
the catalog in the latest version:


This catalog has been built by merging different ones available in the
HEASARC database. These are:
  Liu's HMXB catalog (A&AS,2000,147,25)
  Liu's LMXB catalog (A&A,2001,368,1021)
  Macomb & Gehrels Gamma ray sources catalog (ApJS,1999,120,335)
  4th Uhuru catalog (ApJS,1978,182,489)
  HEAO1 A4 catalog (ApJS,1984,54,581)
  Piccinotti's sample AGNs Batse observations (ApJ,1999,519,637)
  Tartarus reduced ASCA AGN data
  ASCA catalog of Sugizaki et al.(2001yCat..21340077S)
  ASCA catalog of Sakano et al. (ApJS,2002,138,19)

The class numbers correspond to the HEASARC classification. When no
indication was available in the catalogs, this value has been set to
'1000'. For the HEASARC class definitions, see:
http://isdc.unige.ch/Data/cat/class.html
http://heasarc.gsfc.nasa.gov/W3Browse/catalog/class.html


The spectral models are simple descriptions of the spectral energy
distribution. The normalizations have been adjusted by fitting the flux
measurements reported in the catalogs after the assignment of a default
spectral model to each type of source. The default models and their
parameters are described in:
http://isdc.unige.ch/Data/cat/models.html

ISGRI_FLAG set to:
0: sources never detected in a single science window in the 18.3-59.9 keV band
1: sources detected at least once in a single science window in the 18.3-59.9 keV band.


ISGRI_FLAG2 set to:
1: fsources detected at least once in a single scw (i.e. the same as ISGRI_FLAG)
2: sources detected only in a mosaic
3: sources with questionable detection (e.g. reported only in one particular publication and not seen in a later mosaic).

Instrument flags for JEM-X, SPI and PICsIT are set to:
0: when the source is not detected.
1: when the source is detected.
2: when the source is detected and its position should be fixed for OSA
  (i.e. the same as SouFit=1).
These flags signify a detection at the Science Window or mosaic image
level, which has been published either in an ATel or circular, a
refereed journal, or through archival analyses.


The catalog is updated regularly when new information is published in a
refereed journal or on one of the following sites:
  IAUC new sources (from #7341)
  Astronomer's Telegrams
  IGR sources page maintained by J. Rodriguez:
  (http://isdc.unige.ch/

The latest catalog is always available for download at:
http://isdc.unige.ch/Data/cat/
or viewable online at:
http://isdc.unige.ch/Data/cat/latest


If you have any questions or comments about this catalog please contact
Claudio Ricci (claudio.ricci@unige.ch).

Version 29, 2008-07-30
Updated by Claudio Ricci


ISGRI_flag modified, now it is 1 for sources detected in at least a single science window (in the band 18.3-59.9 keV) and 0 for sources not detected in the
 single science windows (in the band 18.3-59.9 keV).
Added a new flag, ISGRI_FLAG2, which is 0 if the source has not been detected, 1 if it has been detected in at
least a single science window (in the band 18.3-59.9 keV), 2 if it has been detected in the mosaics and 3 if the detection has not been confirmed.
Swift J2000.6+3210 = IGR J20006+3210
Swift J2127.4+5654 = IGR J21277+5656
* ISGRI flag switched to 1:
1ES 1959+650 (ATEL 1315)
GRO J1750-27 (ATEL 1385)
ESO 140-43 (ATEL 1264)
ESO 141-55 (ATEL 1264)
SAX J1750.8-2900 (ATEL 1434)
IGR J17473-2721 (ATEL 1461)
Swift J2127.4+5654
Mrk 421 (Beckmann et al. 06, ApJ 638, 642)
3C 120 (Beckmann et al. 06, ApJ 638, 642)
NGC 3081 (Beckmann et al. 06, ApJ 638, 642)
1RXS J072153.2+712031  (Beckmann et al. 06, ApJ 638, 642)
Mrk 509 (Beckmann et al. 06, ApJ 638, 642)
NGC 2110 (Ajello et al. 07, astro-ph/0712.2885 )
NGC 418 (Bird et al. 07,ApJS 170, 175)
3A 0656-072 (ATEL 1303)
AX J1754.2-2754 (ATEL 1094)
H 1426+428
SLX 1744-300 (Revnivtsev et al. 08, astro-ph/0805.2669)
1E 1742.8-2853 (Revnivtsev et al. 08, astro-ph/0805.2669)
SNR 189.1+03.0 (Hill et al. 08, MNRAS 385, 423)
HESS J1825-137 (Hill et al. 08, MNRAS 385, 423)
Mrk 421 (Sala et al. 07, A&A 473, 561)
HESS J1616-508 (Walter et al. 07, AP&SS 309, 5)
PSR B1259-63 (Shaw et al. 04, A&A 426, 33)
GRO J1655-40 (Diaz et al. 07, A&A 462, 657)
EXMS B1709-232 (Kuulkers et al. 07, A&A 466, 595)
4U 2129+12(Krivonos et al. 07, A&A 475, 775)
Swift J0519.5-3140
* SPI flag switched to 1:
Her X-1 (Bird et al. 07, ApJS 170, 175)
EXO 0331+530 (Bird et al. 07, ApJS 170, 175)
Swift J1753.5-0127 (Cadolle et al. 07, ApJ 659, 549)



* JemX flag switched to 1:
IGR J17453-2853 (ATEL 1008)
IGR J17464-2811 (Del Santo et al. 07, A&A 468L, 17)
IGR J01363+6610 (Tomsick et al. 08, astro-ph/0807.2278)
3A 0656-072 (ATEL 1303)
AX J1754.2-2754 (ATEL 1094)
IGR J17456-2901 (Belanger et al. 06, ApJ 636, 275)
H 1426+428
AX J1749.1-2733 (Grebenev et al. 07, AstL 33, 149)
Her X-1 (Klochov et al. 08, A&A 483, 151)
XTE J1817-330 (Sala et al. 07, A&A 473, 561)
H 0115+634 (Sala et al. 07, A&A 473, 561)
PSRB 1509-58 (Sala et al. 07, A&A 473, 561)
Vela pulsar (Sala et al. 07, A&A 473, 561)
Swift J1753.5-0127 (Cadolle et al. 07, ApJ 659, 549)
1A 0535+26 (Caballero et al. 07, A&A 465L, 21)
HETE J1900.1-2455 (Falanga et al. 07, A&A 464, 1069)
IGR J17497-2821 (Walter et al. 07, A&A 461, 17)



* Refined positions for:
H1553-54 (ATEL 1371, Swift/UVOT)
IGR J09522-6231 (Sazonov et al. 08, A&A 487, 509, Chandra)
IGR J08390-4833 (Sazonov et al. 08, A&A 487, 509, Chandra)
IGR J14493-5534 (Sazonov et al. 08, A&A 487, 509, Chandra)
IGR J14561-3738 (Sazonov et al. 08, A&A 487, 509, Chandra)
IGR J21343+4738 (Sazonov et al. 08, A&A 487, 509, Chandra)
IGR J23523+5844 (Sazonov et al. 08, A&A 487, 509, Chandra)
IGR J02466-4222 (Sazonov et al. 08, A&A 487, 509, Chandra)
IGR J16562-3301 (ATEL 1270, Swift/XRT)
IGR J06117-6625 (ATEL 1033, Optical)
IGR J12131+0700 (Masetti et al. 08, A&A 482, 113, Swift/XRT)
IGR J14175-4641 (ATEL 990, Swift/XRT)
IGR J14552-5133 (ATEL 990, Swift/XRT)
IGR J16351-5806 (ATEL 990, Swift/XRT)
IGR J18483-0311 (Sguera et al. 07, A&A 467, 249, Swift/XRT)
GRS 1741.9-2853 (ATEL 1013, Chandra)
IGR J09026-4812 (ATEL 1018, Chandra)
IGR J08408-4503 (Leyder et al. 07, A&A 465L, 35, Swift/XRT)
IGR J11215-5952 (Romano et al. 07, A&A 469L, 5, Swift/XRT)
IGR J11321-5311 (Sguera et al. 07, A&A 468L, 21, Swift/XRT)
IGR J17254-3257 (Chevenez et al. 07, A&A 469L, 27, Swift/XRT)
IGR J16194-2810 (Masetti et al. 07, A&A 470, 331, Swift/XRT)
IGR J00234+6141 (Bonnet-Bidaud et al. 07, A&A 473, 185,Swift/XRT)
IGR J18135-1751 (Funk et al. 07, A&A 470, 249)
IGR J17464-2811 (ATEL 1136)
IGR J17091-3624 (ATEL 1140)
IGR J17098-3628 (ATEL 1140)
IGR J18135-1751 (Helfond et al. 07, ApJ 665, 1297)
IGR J21247+5058 (Molina et al. 2007, MNRAS 382, 937, XMM)
IGR J11435-6109 (ATEL 1231)
IGR J06239-6052 (ATEL 1253)
IGR J02097+5222 (Malizia et al. 07, ApJ 668, 81, Chandra)
Swift J0216.3+5128 (Malizia et al. 07, ApJ 668, 81, Chandra)
IGR J10404-4625 (Malizia et al. 07, ApJ 668, 81, Chandra)
IGR J13109-5552 (Malizia et al. 07, ApJ 668, 81, Chandra)
IGR J14003-6326 (Malizia et al. 07, ApJ 668, 81, Chandra)
IGR J14175-4641 (Malizia et al. 07, ApJ 668, 81, Chandra)
IGR J14552-5133 (Malizia et al. 07, ApJ 668, 81, Chandra)
IGR J15539-6142 (Malizia et al. 07, ApJ 668, 81, Chandra)
IGR J16482-3036 (Malizia et al. 07, ApJ 668, 81, Chandra)
IGR J16562-3301 (Malizia et al. 07, ApJ 668, 81, Chandra)
IGR J18244-5622 (Malizia et al. 07, ApJ 668, 81, Chandra)
IGR J18259-0706 (Malizia et al. 07, ApJ 668, 81, Chandra)
IGR J19443+2117 (Malizia et al. 07, ApJ 668, 81, Chandra)
IGR J21178+5139 (Malizia et al. 07, ApJ 668, 81, Chandra)
IGR J14298-6715 (ATEL 1273, Swift/XRT)
IGR J14331-6112 (ATEL 1273, Swift/XRT)
IGR J14471-6414 (ATEL 1273, Swift/XRT)
IGR J17445-2747 (ATEL 1273, Swift/XRT)
IGR J18256-1035 (ATEL 1273, Swift/XRT)
IGR J00040+7020 (ATEL 1274, Swift/XRT)
IGR J00256+6821 (ATEL 1274, Swift/XRT)
IGR J01528-0326 (ATEL 1274, Swift/XRT)
IGR J02501+5440 (ATEL 1274, Swift/XRT)
IGR J16056-6110 (ATEL 1274, Swift/XRT)
IGR J11366-6002 (ATEL 1288, Swift/XRT)
IGR J16024-6107 (ATEL 1288, Swift/XRT)
IGR J19405-3016 (ATEL 1288, Swift/XRT)
IGR J22292+6647 (ATEL 1288, Swift/XRT)
IGR J23308+7120 (ATEL 1288, Swift/XRT)
IGR J02343+3229 (Rodriguez et al. 08, A&A 482, 731, Swift/XRT)
IGR J10147-6354 (Rodriguez et al. 08, A&A 482, 731, Swift/XRT)
IGR J11187-5438 (Rodriguez et al. 08, A&A 482, 731, Swift/XRT)
IGR J16385-2057 (Rodriguez et al. 08, A&A 482, 731, Swift/XRT)
IGR J18490-0000 (Rodriguez et al. 08, A&A 482, 731, Swift/XRT)
IGR J19308+0530 (Rodriguez et al. 08, A&A 482, 731, Swift/XRT)
IGR J19378-0617 (Rodriguez et al. 08, A&A 482, 731, Swift/XRT)
IGR J00333+6122 (ATEL 1322, Swift/XRT)
IGR J18485-0047 (ATEL 1322, Swift/XRT)
IGR J21272+4241 (ATEL 1322, Swift/XRT)
IGR J18173-2509 (ATEL 1397, XMM)
IGR J16426+6536 (ATEL 1397, XMM)
IGR J18325-0756 (ATEL 1423, Swift/XRT)
IGR J18173-2509 (ATEL 1437, Swift/XRT)
IGR J13186-6257 (ATEL 1539, Swift/XRT)
IGR J15529-5029 (ATEL 1539, Swift/XRT)
IGR J17404-3655 (ATEL 1539, Swift/XRT)
IGR J09253+6929 (ATEL 1538, Swift/XRT)
IGR J11098-6457 (ATEL 1538, Swift/XRT)
IGR J00234+6141 (Tomsick et al. 08, astro-ph/0807.2278, Chandra)
IGR J06074+2205 (Tomsick et al. 08, astro-ph/0807.2278, Chandra)
IGR J10101-5654 (Tomsick et al. 08, astro-ph/0807.2278, Chandra)
IGR J11305-6256 (Tomsick et al. 08, astro-ph/0807.2278, Chandra)
IGR J17200-3116 (Tomsick et al. 08, astro-ph/0807.2278, Chandra)
IGR J09026-4812 (Tomsick et al. 08, astro-ph/0807.2278, Chandra)
IGR J18214-1318 (Tomsick et al. 08, astro-ph/0807.2278, Chandra)
IGR J18256-1035 (Tomsick et al. 08, astro-ph/0807.2278, Chandra)
IGR J18259-0706 (Tomsick et al. 08, astro-ph/0807.2278, Chandra)
IGR J18325-0756 (Tomsick et al. 08, astro-ph/0807.2278, Chandra)
IGR J20187+4041 (ATEL 1595, XMM)
IGR J02466-4222 (Sazonov et al. 08, A&A 487, 509, Chandra)
IGR J08390-4833 (Sazonov et al. 08, A&A 487, 509, Chandra)
IGR J09523-6231 (Sazonov et al. 08, A&A 487, 509, Chandra)
IGR J14492-5535 (Sazonov et al. 08, A&A 487, 509, Chandra)
IGR J14561-3738 (Sazonov et al. 08, A&A 487, 509, Chandra)
IGR J21347+4737 (Sazonov et al. 08, A&A 487, 509, Chandra)
IGR J23523+5844 (Sazonov et al. 08, A&A 487, 509, Chandra)
AX J1754.2-2754 (ATEL 1143, SWIFT/XRT)



* Added new sources (ISGRI flag set to 1)
IGR J16558-4150 (ATEL 987)
IGR J17191-2821 (ATEL 1022)
IGR J17464-2811 (ATEL 970)
IGR J08390-4833 (ATEL 1488)
IGR J14561-3738 (Sazonov et al. 07, A&A 462, 57)
IGR J02466-4222 (Sazonov et al. 08, A&A 487, 509
IGR J16562-3301 (ATEL 799)
IGR J06117-6625 (ATEL 1033)
IGR J12131+0700 (ATEL 1310)
XTE J1810-189 (ATEL 1430)
IGR J17453-2853 (Kuulkers et al. 07, A&A 466, 595)
IGR J17454-2703 (Kuulkers et al. 07, A&A 466, 595)
IGR J17456-2901b (Kuulkers et al. 07, A&A 466, 595)
IGR J22517+2217 (Bassani et al. 07, ApJ 669L, 1)
IGR J18175-1530 (ATEL 1248)
IGR J18462-0223 (ATEL 1319)
IGR J10447-6027 (Leyder et al. 08, A&A 477, 29)
IGR J23206+6431 (ATEL 1363)
IGR J19112+1358 (ATEL 1489)
Swift J2037.2+4151 (ATEL 967)
CXOU J164710.2-455216 (ATEL 953)
V1062 Tau (Revnivtsev et al. 08, astro-ph/0805.2669)
RX J0137.7+5814 (Krivonos et al. 07, A&A 475, 775)
IGR J05305-6559 (Krivonos et al. 07, A&A 475, 775)
IGR J13290-6323 (Krivonos et al. 07, A&A 475, 775)
RX J1713.7-3946 (Krivonos et al. 07, A&A 475, 775)
IGR J17353-3539 (Krivonos et al. 07, A&A 475, 775)
IGR J18578-3405 (Krivonos et al. 07, A&A 475, 775)
IGR J20569-4940 (Krivonos et al. 07, A&A 475, 775)
IGR J17585-3057 (Krivonos et al. 07, A&A 475, 775)



* Identification changed
IGR J09522-6231 (Sazonov et al. 08, A&A 487, 509)
IGR J14561-3738 (Sazonov et al. 08, A&A 487, 509)
IGR J21343+4738 (Sazonov et al. 08, A&A 487, 509)
IGR J23523+5844 (Sazonov et al. 08, A&A 487, 509)
IGR J16562-3301 (ATEL 1270)
IGR J16500-3307 (Masetti et al. 08, A&A 482, 113)
1RXS J174607.8-213333 (Masetti et al. 08, A&A 482, 113)
IGR J14331-6112 (Masetti et al. 08, A&A 482, 113)
IGR J18483-0311 (Masetti et al. 08, A&A 482, 113)
IGR J18027-2016 (Masetti et al. 08, A&A 482, 113)
SAX J1818.6-1703 (Masetti et al. 08, A&A 482, 113)
Swift J2000.6+3210 (Masetti et al. 08, A&A 482, 113)
IGR J14298-6715 (Masetti et al. 08, A&A 482, 113)
IGR J18048-1455 (Masetti et al. 08, A&A 482, 113)
IGR J03334+3718 (Masetti et al. 08, A&A 482, 113)
IGR J06117-6625 (ATEL 1033)
IGR J09446-2636 (Masetti et al. 08, A&A 482, 113)
IGR J09523-6231 (Masetti et al. 08, A&A 482, 113)
IGR J12131+0700 (Masetti et al. 08, A&A 482, 113)
IGR J13038+5348 (Masetti et al. 08, A&A 482, 113)
IGR J13109-5552 (Masetti et al. 08, A&A 482, 113)
IGR J14471-6414 (Masetti et al. 08, A&A 482, 113)
IGR J16056-6110 (Masetti et al. 08, A&A 482, 113)
IGR J16385-2057 (Masetti et al. 08, A&A 482, 113)
IGR J17418-1212 (Masetti et al. 08, A&A 482, 113)
IGR J19405-3016 (Masetti et al. 08, A&A 482, 113)
IGR J21272+4241 (Masetti et al. 08, A&A 482, 113)
IGR J00040+7020 (Masetti et al. 08, A&A 482, 113)
IGR J00256+6821 (Masetti et al. 08, A&A 482, 113)
IGR J01528-0326 (Masetti et al. 08, A&A 482, 113)
IGR J02343+3229 (Masetti et al. 08, A&A 482, 113)
IGR J02504+5443 (Masetti et al. 08, A&A 482, 113)
IGR J07437-5137 (Masetti et al. 08, A&A 482, 113)
IGR J11366-6002 (Masetti et al. 08, A&A 482, 113)
IGR J15161-3827 (Masetti et al. 08, A&A 482, 113)
IGR J15539-6142 (Masetti et al. 08, A&A 482, 113)
IGR J16024-6107 (Masetti et al. 08, A&A 482, 113)
IGR J23308+7120 (Masetti et al. 08, A&A 482, 113)
IGR J23524+5842 (Masetti et al. 08, A&A 482, 113)
IGR J06292+4858 (Masetti et al. 08, A&A 482, 113)
IGR J08023-6954 (Masetti et al. 08, A&A 482, 113)
IGR J16358-4726 (ATEL 1450)
IGR J17453-2853 (Kuulkers et al. 07, A&A 466, 595)
IGR J09026-4812 (ATEL 1018)
IGR J08408-4503 (Leyder et al. 07, A&A 465L, 35)
IGR J16194-2810 (Masetti et al. 07, A&A 470, 331)
IGR J06239-6052 (ATEL 1253)
IGR J19308+0530 (Rodriguez et al. 08, A&A 482, 731)
IGR J19378-0617 (Rodriguez et al. 08, A&A 482, 731)
IGR J00333+6122 (ATEL 1363)
IGR J18027-2016 (Chaty et al. 08, A&A 484, 783)
IGR J16479-4514 (Rahoui et al. 08, A&A 484, 801)
IGR J16493-4348 (ATEL 1396)
IGR J17473-2721 (ATEL 1445)
IGR J08390-4833 (ATEL 1488)
IGR J17464-2811 (ATEL 1496)
IGR J09253+6929 (ATEL 1540)
IGR J11098-6457 (ATEL 1540)
IGR J10147-6354 (Rodriguez et al. 08, A&A 482, 731)
IGR J05346-5759 (Gotz et al. 06, A&A 448, 873)
IGR J11321-5311 (Sguera et al. 07, A&A 468, L21)
IGR J17191-2881 (ATEL 1065)
IGR J17364-2711 (Chelovekov et al. 06, Astron. Letters 32, 456)
IGR J17407-2808 (Sguera et al. 06, ApJ 646, 452)
IGR J17473-2721 (ATEL 1445)
IGR J20187+4041 (ATEL 1623)
IGR J17404-3655 (ATEL 1620)
IGR J18173-2509 (ATEL 1620)
IGR J18259-0706 (Tomsick et al. 08, astro-ph/0807.2278)
IGR J08390-4833 (Sazonov et al. 08, A&A 487, 509)
IGR J16194-2810 (Sala et al. 07, A&A 473, 561)
IGR J19267+1325 (ATEL 1653)
* Counterparts added
IGR J09522-6231 (Sazonov et al. 08, A&A 487, 509)
IGR J21343+4738 (Sazonov et al. 08, A&A 487, 509)
IGR J23523+5844 (Sazonov et al. 08, A&A 487, 509)
IGR J18027-2016 (Masetti et al. 08, A&A 482, 113)
IGR J06117-6625 (ATEL 1033)
IGR J12131+0700 (Masetti et al. 08, A&A 482, 113)
IGR J17418-1212 (Masetti et al. 08, A&A 482, 113)
IGR J00256+6821 (Masetti et al. 08, A&A 482, 113)
IGR J02504+5443 (Masetti et al. 08, A&A 482, 113)
IC 4518a (Masetti et al. 08, A&A 482, 113)
XTE J1810-189 (ATEL 1430)
IGR J14175-4641 (ATEL 990)
IGR J09026-4812 (ATEL 1018)
IGR J16056-6110 (ATEL 1033)
IGR J16500-3307 (ATEL 1034)
IGR J17453-2853 (ATEL 1058)
IGR J16194-2810 (Masetti et al. 07, A&A 470, 331)
IGR J18135-1751 (Funk et al. 07, A&A 470, 249)
IGR J11435-6109 (ATEL 1231)
IGR J06239-6052 (ATEL 1253)
IGR J00040+7020 (ATEL 1274)
IGR J00256+6821 (ATEL 1274)
IGR J02501+5440 (ATEL 1274)
IGR J11366-6002 (ATEL 1288)
IGR J16024-6107 (ATEL 1288)
IGR J19405-3016 (ATEL 1288)
IGR J22292+6647 (ATEL 1288)
IGR J23308+7120 (ATEL 1288)
IGR J02343+3229 (Rodriguez et al. 08, A&A 482, 731)
IGR J11187-5438 (Rodriguez et al. 08, A&A 482, 731)
IGR J16385-2057 (Rodriguez et al. 08, A&A 482, 731)
IGR J18490-0000 (Rodriguez et al. 08, A&A 482, 731)
IGR J19308+0530 (Rodriguez et al. 08, A&A 482, 731)
IGR J19378-0617 (Rodriguez et al. 08, A&A 482, 731)
IGR J13149+4422 (Rodriguez et al. 08, A&A 482, 731)
IGR J18559+1535 (Rodriguez et al. 08, A&A 482, 731)
IGR J23254+5842 (Rodriguez et al. 08, A&A 482, 731)
IGR J00333+6122 (ATEL 1322)
IGR J18485-0047 (ATEL 1322)
IGR J16493-4348 (Hill et al. 08, MRAS 385, 423)
IGR J02524-0829 (ATEL 1363)
IGR J16320-4751 (Chaty et al. 08, A&A 484, 783)
IGR J16393-4643 (Chaty et al. 08, A&A 484, 783)
IGR J17091-3624 (Chaty et al. 08, A&A 484, 783)
IGR J17252-3616 (Chaty et al. 08, A&A 484, 783)
IGR J17597-2201 (Chaty et al. 08, A&A 484, 783)
IGR J18483-0311 (Chaty et al. 08, A&A 484, 783)
IGR J19140+0951 (Chaty et al. 08, A&A 484, 783)
IGR J16195-4945 (Rahoui et al. 08, A&A 484, 801)
IGR J16207-5129 (Rahoui et al. 08, A&A 484, 801)
IGR J16318-4848 (Rahoui et al. 08, A&A 484, 801)
IGR J16320-4751 (Rahoui et al. 08, A&A 484, 801)
IGR J16358-4726 (Rahoui et al. 08, A&A 484, 801)
IGR J16418-4532 (Rahoui et al. 08, A&A 484, 801)
IGR J16465-4507 (Rahoui et al. 08, A&A 484, 801)
IGR J16479-4514 (Rahoui et al. 08, A&A 484, 801)
IGR J17544-2619 (Rahoui et al. 08, A&A 484, 801)
IGR J19140+0951 (Rahoui et al. 08, A&A 484, 801)
IGR J18173-2509 (ATEL 1397)
IGR J16426+6536 (ATEL 1397)
IGR J18325-0756 (ATEL 1423)
IGR J18307-1232
IGR J17404-3655 (ATEL 1539)
IGR J11098-6457 (ATEL 1538)
IGR J09253+6929 (ATEL 1538)
IGR J20187+4041 (ATEL 1623)
IGR J00234+6141 (Tomsick et al. 08, astro-ph/0807.2278)
IGR J06074+2205 (Tomsick et al. 08, astro-ph/0807.2278)
IGR J10101-5654 (Tomsick et al. 08, astro-ph/0807.2278)
IGR J11305-6256 (Tomsick et al. 08, astro-ph/0807.2278)
IGR J17200-3116 (Tomsick et al. 08, astro-ph/0807.2278)
IGR J09026-4812 (Tomsick et al. 08, astro-ph/0807.2278)
IGR J18214-1318 (Tomsick et al. 08, astro-ph/0807.2278)
IGR J18256-1035 (Tomsick et al. 08, astro-ph/0807.2278)
IGR J18259-0706 (Tomsick et al. 08, astro-ph/0807.2278)
IGR J18325-0756 (Tomsick et al. 08, astro-ph/0807.2278)
IGR J14515-5542 (Tomsick et al. 08, astro-ph/0807.2278)
IGR J11435-6109 (Tomsick et al. 08, astro-ph/0807.2278)
IGR J17456-2901 (Belanger et al. 06, ApJ 636, 275)
4U 1735-444 (ATEL 1048)
IGR J00254+6822 (ATEL 941)
IGR J18259-0706 (Simbad)
AX J1841.3-0455 (Simbad)
IGR J21277+5656 (Simbad)
H 1426+428 (Simbad)
IGR J15479-4529 (Revnivtsev et al. 08, astro-ph/0805.2669)
IGR J16493-4348 (Hill et al. 08, MNRAS 385, 423)
IGR J10109-5746 (Hill et al. 08, MNRAS 385, 423)
3A 1845-024 (Hill et al. 08, MNRAS 385, 423)
SNR 189.1+03.0 (Hill et al. 08, MNRAS 385, 423)
HESS J1825-137 (Hill et al. 08, MNRAS 385, 423)
GT 0236+610 (Simbad)
IGR J17453-2853 (ATEL 1008)
Ginga 1843+009 (Simbad)
Ginga 1826-24 (Simbad)
IGR J19267+1325 (ATEL 1653)
* ISGRI flag set to 0 (sources detected with other names)
PKS 0611-663 (ATEL 1033)
NGC 4180 (ATEL 1310)
1RXS J094439.5-263353
Swift J1656.3-3302
GX 304-1
1RXS J182557.5-07102
PSR B1841-04
Swift J2127.4+5654



STAMP   = '2006-12-04T14:24:33 make_isdc_cat 1.8'
CHECKSUM= 'dPVIdNSFdNSFdNSF'   / HDU checksum updated 2007-09-14T07:57:44
DATASUM = '3720674799'         / data unit checksum updated 2007-09-14T07:57:44
END



HEASARC Implementation

The HEASARC has made some minor changes to this table compared to the
original version obtained from the ISDC. We have added two new parameters,
ra_precision and dec_precision (q.v.).


Parameters



Source_Number

  The INTEGRAL Reference Catalog source number, in order of increasing J2000 RA.


Name

  The INTEGRAL Reference Catalog source name. Often there are two or more names
  commonly used for the same source. The authors have taken the name which they
  consider to be the most popular in high-energy astrophysics and which is also
  used as a SIMBAD source identifier. Thus, users can directly put the source
  name into the SIMBAD query box.


RA

  The Right Ascension of the high-energy source. In most cases, positions are
  taken from SIMBAD. From time to time, however, the authors found and adopted
  a more recent position determination than SIMBAD. The accuracy depends on the
  individual sources, which was reflected in the representation of the source
  positions in the original CDS table where the J2000 RAs were given with a
  precision that varied from 0.001 seconds of time to 1 minute of time. To help
  users, the HEASARC has added a parameter called ra_precision which has the
  following values:
  
       ra_precision    meaning

         60.           position given with 1 minute of time precision
          6.           position given with 0.1 minutes of time precision
          1.           position given with 1 second of time precision
          0.1          position given with 0.1 seconds of time precision
          0.01         position given with 0.01 seconds of time precision
          0.001        position given with 0.001 seconds of time precision
  



Dec

  The Declination of the high-energy source. In most cases, positions are taken
  from SIMBAD. From time to time, however, the authors found and adopted a more
  recent position determination than SIMBAD. The accuracy depends on the
  individual sources, which was reflected in the representation of the source
  positions in the original CDS table where the J2000 Declinations were given
  with a precision that varied from 0.01 arcseconds to 1 degree. To help
  users, the HEASARC has added a parameter called dec_precision which has the
  following values:
  

       dec_precision    meaning
  


       3600.           position given with 1 degree of precision
        360.           position given with 0.1 degrees of precision
         60.           position given with 1 arcminute of precision
          6.           position given with 0.1 arcminutes of precision
          1.           position given with 1 arcsecond of precision
          0.1          position given with 0.1 arcseconds of precision
          0.01         position given with 0.01 arcseconds of precision
  

RA_Precision

  This parameter encodes the original precision of the RA in
  the CDS table on which this HEASARC Browse table is based, as follows:
  

       ra_precision    meaning
  


         60.           position given with 1 minute of time precision
          6.           position given with 0.1 minutes of time precision
          1.           position given with 1 second of time precision
          0.1          position given with 0.1 seconds of time precision
          0.01         position given with 0.01 seconds of time precision
          0.001        position given with 0.001 seconds of time precision
  

Dec_Precision

  This parameter encodes the original precision of the Dec in
  the CDS table on which this HEASARC Browse table is based, as follows:
  

       dec_precision    meaning
  


       3600.           position given with 1 degree of precision
        360.           position given with 0.1 degrees of precision
         60.           position given with 1 arcminute of precision
          6.           position given with 0.1 arcminutes of precision
          1.           position given with 1 arcsecond of precision
          0.1          position given with 0.1 arcseconds of precision
          0.01         position given with 0.01 arcseconds of precision
  

LII

  The Galactic Longitude of the high-energy source.


BII

  The Galactic Latitude of the high-energy source.


Error_Radius

  The positional uncertainty of the high-energy source, in arcseconds.


Pos_Ref_Bibcode

  The ADS Bibcode for the source position reference. This is for readers who
  need to know the position accuracy and/or position determination method.
  Often SIMBAD gives the source position reference as well as the position
  itself, in which case the authors have taken both. Otherwise, they searched
  for the proper references themselves.


Pos_Ref_Author

  The authors of the position reference specified by the pos_ref_bibcode
  parameter.


Source_ID

  This parameter is the unique identifier for the source, and, will remain the
  same even if the source position is modified at a later date.


ISGRI_Flag

  This parameter has the value of 1 if the source has been detected by ISGRI;
  otherwise, it is set to 0.


JEMX_Flag

  This parameter has the value of 1 if the source has been detected by JEMX;
  otherwise, it is set to 0.


SPI_Flag

  This parameter has the value of 1 if the source has been detected by SPI;
  otherwise, it is set to 0.


PICSIT_Flag

  This parameter has the value of 1 if the source has been detected by PICSIT;
  otherwise, it is set to 0.


Spectral_Model_Type

  The authors derived a "typical" spectral model and model parameters,
  including the model normalization. They followed the XSPEC format (Arnaud
  1996; http://xspec.gsfc.nasa.gov) for the definition of the models and the
  model parameters. See Sect. 4 of the published paper for more details.


Spectral_Model_Pars

  The authors derived a "typical" spectral model and model parameters,
  including the model normalization. They followed the XSPEC format (Arnaud
  1996; http://xspec.gsfc.nasa.gov) for the definition of the models and the
  model parameters. See Sect. 4 of the published paper for more details.


Flux_3_10keV

  The 3 - 10 keV energy flux, in ergs s^-1 cm^-2, and calculated from the
  assumed spectral models. The authors have taken typical JEMX soft and hard
  energy bands (3 - 10 keV and 10 - 30 keV) and ISGRI soft and hard bands
  (20 - 60 keV and 60 - 200 keV).


Flux_10_30keV

  The 10 - 30 keV energy flux, in ergs s^-1 cm^-2, and calculated from the
  assumed spectral models. The authors have taken typical JEMX soft and hard
  energy bands (3 - 10 keV and 10 - 30 keV) and ISGRI soft and hard bands
  (20 - 60 keV and 60 - 200 keV).


Flux_20_60keV

  The 20 - 60 keV energy flux, in ergs s^-1 cm^-2, and calculated from the
  assumed spectral models. The authors have taken typical JEMX soft and hard
  energy bands (3 - 10 keV and 10 - 30 keV) and ISGRI soft and hard bands
  (20 - 60 keV and 60 - 200 keV).


Flux_60_200keV

  The 60 - 200 keV energy flux, in ergs s^-1 cm^-2, and calculated from the
  assumed spectral models. The authors have taken typical JEMX soft and hard
  energy bands (3 - 10 keV and 10 - 30 keV) and ISGRI soft and hard bands
  (20 - 60 keV and 60 - 200 keV).


JEMX_Soft_Count_Rate

  Using the nominal INTEGRAL detector responses, the expected count rate in the
  Joint European X-Ray Monitor (JEMX), calculated for the soft JEMX energy band
  (3 - 10 keV). In the actual QLA operation, JEMX and ISGRI source count rates
  are measured in these energy bands so as to compare with the catalog. The
  following calibration files, most recent ones in July 2003 (but still based
  on pre-launch calibration), are used in this calculation:
  jmx2_rmf_grp_0003.fits for JEMX and isgr_rmf_grp_0005.fits and
  isgr_arf_rsp_0002.fits for ISGRI.
  


  After the launch of INTEGRAL, the pre-launch estimate of the JEMX effective
  area was revealed to be overestimated by a factor of 2 (P. Kretschmar, private
  communication). Therefore, the authors divided the JEMX count rates calculated
  using the aforementioned responses by a factor of two. This prescription has
  been confirmed to be valid from simultaneous INTEGRAL-RXTE observations of the
  source 3C 273 (Courvoisier et al. 2003, A&A, 411, L343) and Cyg X-1
  (Pottschmidt et al. 2003, A&A, 411, L383).


JEMX_Hard_Count_Rate

  Using the nominal INTEGRAL detector responses, the expected count rate in the
  Joint European X-Ray Monitor (JEMX), calculated for the hard JEMX energy band
  (10 - 30 keV). In the actual QLA operation, JEMX and ISGRI source count rates
  are measured in these energy bands so as to compare with the catalog. The
  following calibration files, most recent ones in July 2003 (but still based
  on pre-launch calibration), are used in this calculation:
  jmx2_rmf_grp_0003.fits for JEMX and isgr_rmf_grp_0005.fits and
  isgr_arf_rsp_0002.fits for ISGRI.
  


  After the launch of INTEGRAL, the pre-launch estimate of the JEMX effective
  area was revealed to be overestimated by a factor of 2 (P. Kretschmar, private
  communication). Therefore, the authors divided the JEMX count rates calculated
  using the aforementioned responses by a factor of two. This prescription has
  been confirmed to be valid from simultaneous INTEGRAL-RXTE observations of the
  source 3C 273 (Courvoisier et al. 2003, A&A, 411, L343) and Cyg X-1
  (Pottschmidt et al. 2003, A&A, 411, L383).


ISGRI_Soft_Count_Rate

  Using the nominal INTEGRAL detector responses, the expected count rate in the
  ISGRI CdTe array of the Imager on Board the INTEGRAL Satellite (IBIS)
  instrument, calculated for the soft ISGRI energy band (20 - 60 keV). In the
  actual QLA operation, JEMX and ISGRI source count rates are measured in these
  energy bands so as to compare with the catalog. The following calibration
  files, most recent ones in July 2003 (but still based on pre-launch
  calibration), are used in this calculation: jmx2_rmf_grp_0003.fits for JEMX
  and isgr_rmf_grp_0005.fits and isgr_arf_rsp_0002.fits for ISGRI.

  For ISGRI, actual observations of the Crab pulsar and other sources confirmed
  that the pre-launch estimate of the effective area was more or less correct
  (within 20 % or so).


ISGRI_Hard_Count_Rate

  Using the nominal INTEGRAL detector responses, the expected count rate in the
  ISGRI CdTe array of the Imager on Board the INTEGRAL Satellite (IBIS)
  instrument, calculated for the hard ISGRI energy band (60 - 200 keV). In the
  actual QLA operation, JEMX and ISGRI source count rates are measured in these
  energy bands so as to compare with the catalog. The following calibration
  files, most recent ones in July 2003 (but still based on pre-launch
  calibration), are used in this calculation: jmx2_rmf_grp_0003.fits for JEMX
  and isgr_rmf_grp_0005.fits and isgr_arf_rsp_0002.fits for ISGRI.
  


  For ISGRI, actual observations of the Crab pulsar and other sources confirmed
  that the pre-launch estimate of the effective area was more or less correct
  (within 20 % or so).


Source_Type

  A characterization of the source type, such as low-mass X-ray binary,
  high-mass X-ray binary, Seyfert-1 galaxy, etc.


Alt_Names

  Various alternate names for the high-energy source. Since there are
  many varieties of sources, the authors did not have a consistent rule to
  decide which aliases to choose. However, they did try to put at least one
  alias directly related to high-energy satellites and/or catalogs. For example,
  "4U" for the 4th Uhuru catalog (Forman et al. 1978, ApJS, 182, 489), and
  "2EG" for the 2nd EGRET source catalog (Thompson et al. 1995, ApJS, 101, 259).


Class

  The HEASARC Browse object classification, based on the value of the
  source_type parameter.


Contact Person

Questions regarding the INTREFCAT database table can be addressed to the
HEASARC User Hotline.















Science Mission Directorate Universe Division

Beyond Einstein | Origins













A service of the 

Astrophysics Science Division
at 
NASA/
GSFC

and the High Energy
Astrophysics Division 
of the 
Smithsonian Astrophysical Observatory (SAO)




HEASARC Director: 
Dr. Alan P. Smale
 

HEASARC Associate Director: Dr. Roger Brissenden


Responsible NASA Official: 


Phil Newman


Web Curator:

Karen Smale











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Page Author: Browse Software Development Team

Last Modified: Friday, 12-Sep-2008 00:55:28 EDT