A dataset provided by the European Space Agency

Name 011299
Title The Galactic Superluminal Source GRS 1915+105
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112990101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112990501

DOI 10.5270/esa-bsgrsrn
Author Dr Martin Turner
Description GT-We propose to observe the galactic black hole binary source of relativistic jets GRS 1915+105. The aim of this proposal is to search for: 1] redshifted iron lines from the ejecta, 2] asymmetric emission lines from the accretion disk, 3] QPOs at a maximum frequency of 67 Hz. Our first observation will be performed during a normal state of the source, the other one during a flaring state. The trigger of the second observation will be determined thanks to the radio monitoring of the Green Bank Interferometer. A spectral state (i.e. flat spectrum) or a high flux may trigger the observation.
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 ,
An All-Sky Atlas of Radio-X-ray Associations . Flesch, E., . PASA . 27-283 . 2010 . 2010PASA...27..283F ,
Exospheric solar wind charge exchange as seen by XMM-Newton . Carter, J. A., Semba, S., . AN . 333-313 . 2012 . 2012AN....333..313C ,
The XMM-Newton serendipitous ultraviolet source survey catalogue . Page, M. J., Brindle, C., et all. . MNRAS . 426-903 . 2012 . 2012MNRAS.426..903P ,
Ubiquitous equatorial accretion disc winds in black hole soft states . Ponti, G., Fender, R. P., et all. . MNRAS . 422-11 . 2012 . 2012MNRAS.422L..11P ,
Detection of distinct power spectra in soft and hard X-ray bands in the hard state of GRS 1915+105 . Stiele, H., Yu, W., . MNRAS . 441-1177 . 2014 . 2014MNRAS.441.1177S ,
Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift . Yershov, V. N., . Ap&SS . 354-97 . 2014 . 2014Ap&SS.354...97Y ,
Interstellar Dust Properties from a Survey of X-Ray Halos . Valencic, Lynne A., Smith, Randall K., ....
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2003-03-29T13:36:54Z/2003-10-17T04:52:33Z
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 2004-11-06T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2004-11-06T00:00:00Z, 011299, 17.56_20190403_1200. https://doi.org/10.5270/esa-bsgrsrn