A dataset provided by the European Space Agency

Name 009356
Title XMM Observations of Black-Hole X-Ray Binaries in Outburst
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0093562701

DOI 10.5270/esa-djnsdte
Author Prof Walter Lewin
Description We propose to study the time-resolved X-ray spectra of black-hole (candidate) X-ray binaries (BHXBs) in outburst. We will be following the outburst(s) throughout their evolution over a wide range of wavelengths, and will conduct a series of high time-resolution X-ray spectral observations with the XMM Reflection Grating Spectrometer. High-resolution X-ray spectra will likely exhibit emission lines and absorption edges characteristic of the accretion disk geometry, temperatures, and abundances. We expect that they will also show the general-relativistic effects of the extreme gravitational environment near the black hole. Whenever possible we will make (near) simultaneous radio, optical, X-ray timing (RXTE) and gamma-ray observations.
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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 ,
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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 ,
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Ubiquitous equatorial accretion disc winds in black hole soft states . Ponti, G., Fender, R. P., et all. . MNRAS . 422-11 . 2012 . 2012MNRAS.422L..11P ,
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The soft component and the iron line as signatures of the disc inner radius in Galactic black hole binaries . Kolehmainen, Mari, Done, Chris, . MNRAS . 437-316 . 2014 . 2014MNRAS.437..316K ,
Tracing the Reverberation Lag in the Hard State of Black Hole X-Ray Binaries . De Marco, B., Ponti, G., et all. . ApJ . 814-50 . 2015 . 2015ApJ...814...50D ,
High ionisation absorption in low mass X-ray binaries . Ponti, G., Bianchi, S., et all. . AN . 337-512 . 2016 . 2016AN....337..512P ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
Crossing the Eddington Limit: Examining Disk Spectra at High Accretion Rates . Sutton, Andrew D., Swartz, Douglas A., et all. . ApJ . 836-48 . 2017 . 2017ApJ...836...48S ,
The Evolution of GX 339-4 in the Low-hard State as Seen by NuSTAR and Swift . Wang-Ji, Jingyi, Garcia, Javier A., et all. . ApJ . 855-61 . 2018 . 2018ApJ...855...61W ,
Instrument EMOS1, EPN, RGS1, RGS2
Temporal Coverage 2002-08-24T10:30:16Z/2002-08-25T03:32:49Z
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 2003-09-21T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2003-09-21T00:00:00Z, 009356, 17.56_20190403_1200. https://doi.org/10.5270/esa-djnsdte