INTEGRAL observations of Swift J174540.7-290015
ATel #8684; V. Esposito (ISDC, Switzerland), E. Kuulkers (EAS/ESAC, Spain), A. Bazzano (INAF/IAPS, Italy), V. Beckmann (APC, France), T. Bird (Southampton, UK), A. Bodaghee (GCSU, USA), J. Chenevez (DTU Space, Denmark), M. Del Santo (INAF/IASF-Pa, Italy), A. Domingo (CAB/INTA-CSIC, Spain), P. Jonker (SRON, The Netherlands), P. Kretschmar (ESA/ESAC, Spain), C. Markwardt (GSFC, USA), A. Paizis (INAF/IASF-Mi, Italy), K. Pottschmidt (UMBC/NASA GSFC, USA), C. SÃ¡nchez-FernÃ¡ndez (ESA/ESAC, Spain), R. Wijnands (UvA, The Netherlands), E. Bozzo, C. Ferrigno (ISDC, Switzerland)
on 12 Feb 2016; 16:59 UT
Credential Certification: E. Bozzo (firstname.lastname@example.org)
Subjects: X-ray, Transient
The newly discovered X-ray transient Swift J174540.7-290015 (ATel #8649) was observed within the field-of-view of the IBIS/ISGRI and JEM-X instruments on-board INTEGRAL on 2016 February 11 from 14:12 to 17:22 (UTC), while the satellite was pointing toward the Galactic Bulge (ATel #438). The total exposure time was 10.8 ks.
The source was detected in the IBIS/ISGRI mosaic at a significance of 21 sigma in the 20-40 keV energy band and 15 sigma in the 40-80 keV energy range. The corresponding fluxes were 41+/-2 mCrab and 42+/-3 mCrab. The source is also detected by JEM-X at a significance of 18 sigma in the 3-10 keV energy band and 11 sigma in the 10-20 keV energy band. The corresponding fluxes were 52+/-3 mCrab and 46+/-5 mCrab.
All uncertainties given on the above fluxes are only statistical and at 1 sigma confidence level.
The combined ISGRI+JEM-X spectrum could be well fit (reduced chi^2/d.o.f.=0.9/17) by using a simple power-law model with the column density fixed at 9.1E22 cm^(-2), as measured by Swift/XRT (see ATel #8649). The measured power-law photon index is 2.7+/-0.2 and the spectral flux evaluated from the fit is of 7.5E-10 ergs/cm^2/s in the 5-20 keV energy band and 8.3E-10 ergs/cm^2/s in the 20-100 keV energy band.
We note that neither IBIS/ISGRI nor JEM-X are able to discriminate between the different X-ray emitting sources currently active in the vicinities of Swift J174540.7-290015 due to the limited angular resolution of these instruments compared to, e.g., Swift/XRT. However, we used previous INTEGRAL observations of the Galactic Bulge to verify that none of the other sources could provide a dominating contribution in the 3-20 keV and 20-100 keV energy bands. Observations carried out in the satellite revolution 1597 (from 2015-10-11 at 05:57 to 09:34 UTC) and 1603 (from 2015-10-27 at 03:57 to08:41 UTC) showed that there is no overlapping source detected by IBIS/ISGRI and only 1A 1742-289 has a position compatible with that of Swift J174540.7-290015 in JEM-X. The latter source is always detected by JEM-X in all the above mentioned revolutions at a flux of ~15 mCrab in the 3-10 keV energy band and ~10 mCrab in the 10-20 keV energy band. We are thus confident that the reported spectrum and fluxes for Swift J174540.7-290015 from IBIS/ISGRI cannot be largely contaminated by any other source currently active around the new Swift transients, while for JEM-X a contamination at a level of 20% is possible.
Further observations of the Galactic Bulge with INTEGRAL are already planned for the coming weeks.