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2011ATel.3551....1G - The Astronomer's Telegram, 3551, 1 (2011/August-0)
A new hard X-ray transient discovered by INTEGRAL: IGR J17498-2921.
GIBAUD L., BAZZANO A., BOZZO E., CADOLLE-BEL M., CHENEVEZ J., DRAVE S.P., FERRIGNO C., GOTZ D., KADLER M., KREYKENBOHM I., PUEHLHOFER G., RODRIGUEZ J., SANCHEZ-FERNANDEZ C. and WATANABE K.
Abstract (from CDS):
The source is detected in the IBIS/ISGRI mosaic at a preliminary significance level of 11 and 9 sigma in the 20-40 keV and 40-80 keV energy
bands, respectively. The corresponding fluxes are 19±2 and 23±3 mCrab (68% c.l., only statistical).
The best determined source position is at RA=17:49:49; DEC=-29:21:14 (J2000) with a 90% confinement radius of 2.3 arcmin.
The IBIS/ISGRI spectrum (exposure time 15.9 ks) can be well described by a a power-law with photon index 1.9±0.4 (90% c.l.). The estimated 20-100 keV flux from the spectral fit is ∼3.4e-10 erg/s/cm2.
Unfortunately, IGR J17498-2921 was located at the border of the JEM-X field of view (FOV) and thus we can not report yet on its detection at low energy (2-25 keV).
Further INTEGRAL observations of the FOV around IGR J17498-2921 are planned for the next days.
Abstract Copyright: ∼
Journal keyword(s): Gamma Ray - Binary - Black Hole - Neutron Star - Transient
Simbad objects: 1
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