Renewed activity from the accreting millisecond X-ray pulsar MAXI J0911-655/Swift J0911.9-6452
ATel #14761; V. A. Lepingwell (Univ. of Southampton, UK), M. Fiocchi (INAF-IAPS Roma, Italy), J. Chenevez (DTU Space, Denmark), A. Bazzano (INAF-IAPS Roma, Italy), A. J. Bird, P. Charles (Univ. of Southampton, UK), E. Kuulkers (ESA/ESTEC, The Netherlands), A. Malizia, N. Masetti, M. Molina (INAF-OAS, Bologna, Italy), L. Natalucci, F. Panessa (INAF-IAPS Roma, Italy), V. Sguera (INAF-OAS, Bologna, Italy), P. Ubertini (INAF-IAPS Roma, Italy), on behalf of the INTEGRAL/GPS team.
on 7 Jul 2021; 07:03 UT
Credential Certification: Victoria Lepingwell (V.A.Lepingwell@soton.ac.uk)
Subjects: X-ray, Transient, Pulsar
During recent observations of the Galactic Plane (PI: A. Bazzano) weak hard X-ray emission was observed from the accreting millisecond X-ray pulsar MAXI J0911-655/Swift J0911.9-6452 in the globular cluster NGC 2808.
MAXI J0911-655 was detected by IBIS/ISGRI at 6.3 sigma during revolution 2381, between 2021-06-26 05:04:08 UTC and 2021-06-27 05:47:50 UTC, and during revolution 2384 between 2021-07-04 01:05:45 UTC and 2021-07-05 04:54:35 UTC with a combined effective exposure time of 6.9 ks. The 22-60 keV IBIS/ISGRI flux corresponds to (12.3 ± 2.0) mCrab.
All the data have been analysed using the Offline Software Analysis version 11.0 (OSA11). Results from the Galactic Plane Scanning are publicly available at: http://gps.iaps.inaf.it./
