A dataset provided by the European Space Agency

Name 072120
Title XMM-Newton observations of the enigmatic black hole candidate IGR J17091-3624


DOI 10.5270/esa-294xo7c
Author Dr Diego Altamirano
Description For nearly 20 years, the microquasar GRS 1915+105 was unique in the Galaxy for its powerful jets, massive winds, and exotic X-ray variability. In February 2011, IGR J17091-3624 went into outburst and began to mimic GRS 1915+105, opening a complete new window to understand accretion disk physics at Eddington rates. To progress further, GRS 1915+105 and IGR J17091--3624 need to be studied and compared in their different spectral states. We therefore propose a maximum of two ToO 40 ksec observations of IGR J17091-3624 with XMM-Newton in case the source is still active during AO12. These observations will sample spectral states not yet observed with high-resolution spectroscopy and at energies <2 keV.
Publication The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
An atlas of exotic variability in IGR J17091-3624: a comparison with GRS 1915+105 . Court, J. M. C., Altamirano, D., et all. . MNRAS . 468-4748 . 2017 . 2017MNRAS.468.4748C ,
Modelling the effect of absorption from the interstellar medium on transient black hole X-ray binaries . Eckersall, A. J., Vaughan, S., . MNRAS . 471-1468 . 2017 . 2017MNRAS.471.1468E ,
Swift-XRT, Chandra, and XMM-Newton observations of IGR J17091-3624 as it returns into quiescence . Pereyra, M., Altamirano, D., et all. . MNRAS . 497-1115 . 2020 . 2020MNRAS.497.1115P ,
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2013-09-12T21:27:37Z/2013-09-13T10:10:57Z
Version 17.56_20190403_1200
Mission Description The European Space Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's second cornerstone of the Horizon 2000 Science Programme. It carries 3 high throughput X-ray telescopes with an unprecedented effective area, and an optical monitor, the first flown on a X-ray observatory. The large collecting area and ability to make long uninterrupted exposures provide highly sensitive observations.
Since Earth's atmosphere blocks out all X-rays, only a telescope in space can detect and study celestial X-ray sources. The XMM-Newton mission is helping scientists to solve a number of cosmic mysteries, ranging from the enigmatic black holes to the origins of the Universe itself. Observing time on XMM-Newton is being made available to the scientific community, applying for observational periods on a competitive basis.
Creator Contact https://www.cosmos.esa.int/web/xmm-newton/xmm-newton-helpdesk
Date Published 2014-10-01T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2014-10-01T00:00:00Z, 072120, 17.56_20190403_1200. https://doi.org/10.5270/esa-294xo7c