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INTIBISASS - INTEGRAL IBIS All-Sky Survey of Hard X-Ray Sources |
HEASARC Archive |
The current INTIBISASS table is based on the data provided in Krivonos et al. (2010: Paper II below) and replaces the earlier version available at the HEASARC from February 2008 to December 2010 which was based on Krivonos et al. (2007).
INTEGRAL/IBIS 7-year all-sky hard X-ray survey. II. Catalog of sources. Krivonos R., Tsygankov S., Revnivtsev M., Grebenev S., Churazov E., Sunyaev R. <Astron. Astrophys. 523, A61 (2010)> =2010A&A...523A..61K Catalog of hard X-ray sources detected in all-sky survey performed with INTEGRAL observatory. Krivonos R., Revnivtsev M., Lutovinov A., Sazonov S., Churazov E., Sunyaev R. <Astron. Astrophys. 475, 775 (2007)> =2007A&A...475..775K
Source_Number
A running source number, in order of increasing J2000 RA,
which uniquely identifies the hard X-ray source. There are 534 entries for
521 unique sources in this table, with some variable sources having multiple
entries for different revolution ranges.
Name
The name of the hard X-ray source. For sources whose nature was known
before their detection by INTEGRAL, their common names are given. Sources
discovered by INTEGRAL or those whose nature was established thanks to
INTEGRAL are named with an "IGR" prefix.
RA
The Right Ascension of the source in the selected equinox. This was
given in J2000 decimal degrees and to a precision of 0.001 degrees in the
original table. 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 sigma are 2.1, 1.5 and <0.8 arcminutes,
respectively. (Krivonos et al.2007: Paper I).
Dec
The Declination of the source in the selected equinox. This was
given in J2000 decimal degrees and to a precision of 0.001 degrees in the
original table. 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 sigma are 2.1, 1.5 and <0.8 arcminutes,
respectively. (Krivonos et al.2007: Paper I).
LII
The Galactic Longitude of the source.
BII
The Galactic Latitude of the source.
Confusion_Flag
This flag parameter is set to 'c' to indicate spatial
confusion: the fluxes of such confused sources should be taken with caution.
Flux
The time-averaged 17 - 60 keV flux of the source in units of 10-11 erg
cm-2 s-1 = 0.7 milliCrab, given that a flux of 1 mCrab corresponds to
1.43 x 10-11 erg s-1 cm-2 for a source with a Crab-like spectrum. The
source flux was either that measured in the 7-year time averaged map
(December 2002 - July 2009), or, if the parameter revolution_range is set,
over the indicated INTEGRAL spacecraft revolution interval 'n m' where n is
the starting revolution and m is the ending revolution (the latter is usually
the source flux during an outburst). The time range corresponding to a given
INTEGRAL revolution number can be found on the
INTEGRAL Science Operations Center website
at by clicking on the 'Schedule Information' link in the left-hand menu bar.
Flux_Error
The 1-sigma error in the time-averaged 17 - 60 keV flux of the
source in units of 10-11 erg cm-2 s-1 = 0.7 milliCrab.
Revolution_Range
The revolution range (starting ending) to which the
quoted flux measurement corresponds. If blank, the quoted source flux
is that measured in the 7-year time averaged map. The time range
corresponding to a given INTEGRAL revolution number can be found on the
INTEGRAL Science Operations Center website
at by clicking on the 'Schedule Information' link in the left-hand menu bar.
Source_Type
The general astrophysical type of the object:
LMXB (HMXB) - low- (high-) mass X-ray binary, AGN - active galactic nucleus, AXP - anomalous X-ray pulsar, SNR/PWN - supernova remnant/pulsar wind nebula, CV - cataclysmic variable, PSR/PWN - isolated pulsar or pulsar wind nebula, SGR - soft gamma repeater, RS CVn - coronally active binary star, SymbStr - symbiotic star, Star - star, Cluster - cluster of galaxies, NucStrCl - The Galactic Center nuclear star cluster.A question mark indicates that the specified source type is not firmly determined, so it should be treated with caution.
Author_1
The author(s) of the first reference discussing the specified
source. These are mainly provided for new sources and are related to
their discovery and/or their nature.
Ref_Bibcode_1
The bibliographic code (bibcode) of the first reference
discussing the specified source. These are mainly provided for new sources
and are related to their discovery and/or nature.
Author_2
The author(s) of the second reference discussing the specified
source. These are mainly provided for new sources and are related to
their discovery and/or their nature.
Ref_Bibcode_2
The bibliographic code (bibcode) of the second reference
discussing the specified source. These are mainly provided for new sources
and are related to their discovery and/or nature.
Author_3
The author(s) of the third reference discussing the specified
source. These are mainly provided for new sources and are related to
their discovery and/or their nature.
Ref_Bibcode_3
The bibliographic code (bibcode) of the third reference
discussing the specified source. These are mainly provided for new sources
and are related to their discovery and/or nature.
Author_4
The author(s) of the fourth reference discussing the specified
source. These are mainly provided for new sources and are related to
their discovery and/or their nature.
Ref_Bibcode_4
The bibliographic code (bibcode) of the fourth reference
discussing the specified source. These are mainly provided for new sources
and are related to their discovery and/or nature.
Notes
For some sources, there are additional notes such as the type
subclass, redshift information, and/or alternative source designations.
Redshifts of the extragalactic sources were obtained from the SIMBAD and/or
NED databases.
Class
The HEASARC Browse object classification, based on the classification
given in the source_type parameter.