Bibcode
Altamirano, D.; Wijnands, R.; van der Klis, M.; Patruno, A.; Watts, A.; Armas Padilla, M.; Cavecchi, Y.; Degenaar, N.; Kalamkar, M.; Kaur, R.; Yang, Y. J.; Casella, P.; Linares, M.; Soleri, P.; Rea, N.
Bibliographical reference
The Astronomer's Telegram, #2565
Advertised on:
4
2010
Citations
10
Refereed citations
9
Description
On April 10th, it was discovered (ATel #2548) using INTEGRAL that the
neutron-star X-ray binary Swift J1749.4-2807 (Wijnands et al. 2009,
MNRAS, 393, 126) was again in outburst. Using follow-up Swift and
INTEGRAL observations the source activity was confirmed (ATel #2548 and
#2561). On April 14th, 2010 (20:58:00 UT), RXTE performed a pointed
observation of Swift J1749.4-2807. The observation lasted for about
1.6 ksec, at a background-corrected count rate of ~30 cts/sec/PCU (2
PCUs were active during this observation) in the 2-16 keV range.