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INTEGRAL detection of the neutron-star X-ray transient Swift J1734.5-3027

Erik Kuulkers, D. Eckert, C. Ferrigno, J. Chenevez, J. Alfonso-Garzón, Volker Beckmann, Antony J. Bird, Søren K. Brandt, M. Del Santo, A. Domingo, Ken Ebisawa, P. G. Jonker, Peter Kretschmar, Craig B. Markwardt, T. Oosterbroek, Adamantia Paizis, K. Pottschmidt, C. Sánchez‐Fernández, Rudy A. D. Wijnands

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Abstract

INTEGRAL Galactic bulge monitoring (see ATel #438) observations performed between UT 2013 September 3 20:43 and September 4 00:25 clearly reveal the newly detected neutron star X-ray transient Swift J1734.5-3027 (ATel #5354, GCN #15157, #15172). The JEM-X and IBIS/ISGRI flux averages during the observations are 14+/-3 mCrab (3-10 keV), 19+/-6 mCrab (10-25 keV), 23+/-2 mCrab (18-40 keV), and 17+/-2 mCrab (40-100 keV).

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What this paper is about

INTEGRAL Galactic bulge monitoring (see ATel #438) observations performed between UT 2013 September 3 20:43 and September 4 00:25 clearly reveal the newly detected neutron star X-ray transient Swift J1734.5-3027 (ATel #5354, GCN #15157, #15172). The JEM-X and IBIS/ISGRI flux averages during the observations are 14+/-3 mCrab (3-10 keV), 19+/-6 mCrab (10-25 keV), 23+/-2 mCrab (18-40 keV), and 17+/-2 mCrab (40-100 keV).

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Available abstract

INTEGRAL Galactic bulge monitoring (see ATel #438) observations performed between UT 2013 September 3 20:43 and September 4 00:25 clearly reveal the newly detected neutron star X-ray transient Swift J1734.5-3027 (ATel #5354, GCN #15157, #15172). The JEM-X and IBIS/ISGRI flux averages during the observations are 14+/-3 mCrab (3-10 keV), 19+/-6 mCrab (10-25 keV), 23+/-2 mCrab (18-40 keV), and 17+/-2 mCrab (40-100 keV).

Key concepts: Physics, Astrophysics, Neutron star, Swift, Flux (metallurgy), Astronomy, Bulge, Stars

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INTEGRAL detection of the neutron-star X-ray transient Swift J1734.5-3027 — Research Paper | ScholarLens