2008UvA-DARE (University of Amsterdam)Requires access

RXTE confirms persistent activity of burster IGR J17473-2721

Craig B. Markwardt, D. Altamirano, Jean H. Swank, J. J. M. in ’t Zand

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Abstract

Following reports of bursting activity of IGR J17473-2721 (= XTE J1747-274) by the AGILE team (Del Monte et al., ATEL #1445) and from Swift (Altamirano et al., ATEL #1459), we note that RXTE PCA monitoring scans of the source also reveal persistent activity. Scans on 2008-03-28 at 18:50 UT and 2008-03-31 at 15:10 UT found 2-10 keV fluxes of about 13 and 18 mCrab, respectively. Previous scans are consistent with quiescent level (with 2-sigma upper limits ~6 mCrab).

About this research paper

What this paper is about

Following reports of bursting activity of IGR J17473-2721 (= XTE J1747-274) by the AGILE team (Del Monte et al., ATEL #1445) and from Swift (Altamirano et al., ATEL #1459), we note that RXTE PCA monitoring scans of the source also reveal persistent activity. Scans on 2008-03-28 at 18:50 UT and 2008-03-31 at 15:10 UT found 2-10 keV fluxes of about 13 and 18 mCrab, respectively. Previous scans are consistent with quiescent level (with 2-sigma upper limits ~6 mCrab).

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Available abstract

Following reports of bursting activity of IGR J17473-2721 (= XTE J1747-274) by the AGILE team (Del Monte et al., ATEL #1445) and from Swift (Altamirano et al., ATEL #1459), we note that RXTE PCA monitoring scans of the source also reveal persistent activity. Scans on 2008-03-28 at 18:50 UT and 2008-03-31 at 15:10 UT found 2-10 keV fluxes of about 13 and 18 mCrab, respectively. Previous scans are consistent with quiescent level (with 2-sigma upper limits ~6 mCrab).

Key concepts: Bursting, Astrophysics, Physics, Sigma, Astronomy, Psychology, Neuroscience

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