A dataset provided by the European Space Agency

Name 014822
Title XMM-RXTE Observations of GX 339-4
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0148220201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0148220301

DOI 10.5270/esa-md862no
Author Dr Michael Nowak
Description We propose a set of 4, 15 ksec observations of the galactic black hole candidate, GX 339-4. These observations are to be performed simultaneously with a set of 4, 40 ksec RXTE observations, applied for in RXTE Cycle 7. Our goals are to correlate temporal and spectral properties. The specific goals of the XMM-Newton observations are to better resolve the Fe line-edge region, better resolve the soft spectrum, < 3 keV, i.e. the source of seed photons in Comptonization models, and to obtain high resolution spectra, to model interstellar absorption, intrinsic abundances, and to search for evidence of an X-ray heated atmosphere. When possible, simultaneous optical and radio observations will be performed.
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 ,
Black hole accretion discs in the canonical low-hard state . Reis, R. C., Fabian, A. C., . MNRAS . 402-836 . 2010 . 2010MNRAS.402..836R ,
Modeling the Accretion Disk X-Ray Continuum of Black Hole Candidates . Pszota, Gabor, Cui, Wei, . ApJ . 663-1201 . 2007 . 2007ApJ...663.1201P ,
On the Nonrelativistic Origin of Red-skewed Iron Lines in Cataclysmic Variable, Neutron Star, and Black Hole Sources . Titarchuk, Lev, Laurent, Philippe, . ApJ . 700-1831 . 2009 . 2009ApJ...700.1831T ,
An All-Sky Atlas of Radio-X-ray Associations . Flesch, E., . PASA . 27-283 . 2010 . 2010PASA...27..283F ,
Magnetic coupling of a rotating black hole with advection-dominated accretion flows . Ye, Yong-Chun, Wang, Ding-Xiong, . NewA . 12-471 . 2007 . 2007NewA...12..471Y ,
The XMM-Newton serendipitous ultraviolet source survey catalogue . Page, M. J., Brindle, C., et all. . MNRAS . 426-903 . 2012 . 2012MNRAS.426..903P ,
Interstellar medium composition through X-ray spectr...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2003-03-08T17:50:10Z/2003-03-20T06:07:48Z
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 2005-02-12T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2005-02-12T00:00:00Z, 014822, 17.56_20190403_1200. https://doi.org/10.5270/esa-md862no