A dataset provided by the European Space Agency

Name 014463
Title XMM- Newton observations of the microquasars 1E 1740.7-2942 and GRS 1758-258
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0144630101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0144630201

DOI 10.5270/esa-wd2tct7
Author Dr Paolo Goldoni
Description We propose to observe the Galactic Microquasars 1E1740.7-2942 and GRS 1758-258 in their standard low-hard state. The aim of this proposal is to search for the ultrasoft component recently detected in GRS 1758-258. Its presence could argue in favor of the two component accretion flow models recently invoked for accretion in Black Hole binary systems. We plan to use these data in conjunction with the data obtained from the INTEGRAL Galacic Plane and Galactic Center Deep Exposure Core program observation in order to measure the high energy Comptonised spectrum in the gamma-ray domain. We will have access to these data as members of this team are IBIS-INTEGRAL CoIs. A total of 20 ksec is requested for this project. A total of 20 ksec is requested for this project.
Publication The XMM-Newton serendipitous survey. V. The Second XMM-Newton serendipitous source catalogue . Watson, M. G., Schroder, A. C., et all. . A&A . 493-339 . 2009 . 2009A&A...493..339W ,
Statistical evaluation of the flux cross-calibration of the XMM-Newton EPIC cameras . Mateos, S., Saxton, R. D., et all. . A&A . 496-879 . 2009 . 2009A&A...496..879M ,
The XMM Cluster Survey: optical analysis methodology and the first data release . Mehrtens, Nicola, Romer, A. Kathy, et all. . MNRAS . 423-1024 . 2012 . 2012MNRAS.423.1024M ,
Two Rapidly Variable Galactic X-ray Transients Observed with Chandra, XMM-Newton, and Suzaku . Heinke, C. O., Tomsick, J. A., et all. . ApJ . 701-1627 . 2009 . 2009ApJ...701.1627H ,
Accretion states of the Galactic microquasar GRS 1758-258 . Soria, Roberto, Broderick, Jess W., et all. . MNRAS . 415-410 . 2011 . 2011MNRAS.415..410S ,
An All-Sky Atlas of Radio-X-ray Associations . Flesch, E., . PASA . 27-283 . 2010 . 2010PASA...27..283F ,
The XMM Cluster Survey: X-ray analysis methodology . Lloyd-Davies, E. J., Romer, A. Kathy, et all. . MNRAS . 418-14 . 2011 . 2011MNRAS.418...14L ,
Classification of X-Ray Sources in the XMM-Newton Serendipitous Source Catalog . Lin, Dacheng, Webb, Natalie A., . ApJ . 756-27 . 2012 . 2012ApJ...756...27L ,
The XMM-Newton serendipitous ultr...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2002-09-28T03:51:31Z/2003-09-12T01:28:45Z
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 2004-10-12T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2004-10-12T00:00:00Z, 014463, 17.56_20190403_1200. https://doi.org/10.5270/esa-wd2tct7