Abstract
Aims. We report on a multi-band high-energy observing campaign aimed at studying the long term spectral variability of the Anomalous X-ray Pulsar (AXP) 1RXS J170849.0-400910, one of the magnetar candidates. Methods. We observed 1RXS J170849.0-400910 in Fall 2006 and Spring 2007 simultaneously with Swift/XKT, in the 0.1-10 keV energy range, and with INTEGRAL/IBIS, in the 20-200 keV energy range. Furthermore, we also reanalyzed, using the latest calibration and software, all the publicly available INTEGRAL data since 2002, and the soft X-ray data starting from 1999 taken using BeppoSAX, Chandra, XMM-Newton and Swift/XRT, in order to study the soft and hard X-ray spectral variability of 1RXS J170849.0-400910. Results. We find a long-term variability of the hard X-ray flux, extending the hardness-intensity correlation proposed for this source over 2 orders of magnitude in energy. © ESO 2007.
Author supplied keywords
Cite
CITATION STYLE
Götz, D., Rea, N., Israel, G. L., Zane, S., Esposito, P., Gotthelf, E. V., … Turolla, R. (2007). Long term hard X-ray variability of the anomalous X-ray pulsar 1RXS J 170849.0-400910 discovered with INTEGRAL. Astronomy and Astrophysics, 475(1), 317–321. https://doi.org/10.1051/0004-6361:20078291
Register to see more suggestions
Mendeley helps you to discover research relevant for your work.