A dataset provided by the European Space Agency

Name: XMM Observations of Black-Hole X-Ray Binaries in Outburst
Published: 2003-09-21T00:00:00Z

Proposal ID	009356
Title	XMM Observations of Black-Hole X-Ray Binaries in Outburst
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0093562701
DOI	https://doi.org/10.5270/esa-djnsdte
Principal Investigator, PI	Prof Walter Lewin
Abstract	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 aseries of high time-resolution X-ray spectral observations with the XMMReflection Grating Spectrometer. High-resolution X-ray spectra will likelyexhibit emission lines and absorption edges characteristic of the accretion diskgeometry, temperatures, and abundances. We expect that they will also show thegeneral-relativistic effects of the extreme gravitational environment near theblack hole. Whenever possible we will make (near) simultaneous radio, optical,X-ray timing (RXTE) and gamma-ray observations.
Publications	The XMM-Newton serendipitous survey. V. The Second XMM-Newton serendipitous source catalogue \|Watson, M. G., Schroder, A. C., et al. \| A&A \| 493-339 \| 2009 \| 2009A&A...493..339W \| http://ui.adsabs.harvard.edu/#abs/2009A&A...493..339W Statistical evaluation of the flux cross-calibration of the XMM-Newton EPIC cameras \|Mateos, S., Saxton, R. D., et al. \| A&A \| 496-879 \| 2009 \| 2009A&A...496..879M \| http://ui.adsabs.harvard.edu/#abs/2009A&A...496..879M Modeling the Accretion Disk X-Ray Continuum of Black Hole Candidates \|Pszota, Gabor, Cui, Wei, \| ApJ \| 663-1201 \| 2007 \| 2007ApJ...663.1201P \| http://ui.adsabs.harvard.edu/#abs/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 \| http://ui.adsabs.harvard.edu/#abs/2009ApJ...700.1831T 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 \| http://ui.adsabs.harvard.edu/#abs/2007NewA...12..471Y Modelling the high-mass accretion rate spectra of GX 339-4: black hole spin from reflection? \|Kolehmainen, Mari, Done, Chris, \| MNRAS \| 416-311 \| 2011 \| 2011MNRAS.416..311K \| http://ui.adsabs.harvard.edu/#abs/2011MNRAS.416..311K Ubiquitous equatorial accretion disc winds in black hole soft states \|Ponti, G., Fender, R. P., et al. \| MNRAS \| 422-11 \| 2012 \| 2012MNRAS.422L..11P \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.422L..11P Looking into the inner black hole accretion disc with relativistic models of iron line \|Svoboda, Jiri, \| PhDT \| 0-467 \| 2010 \| 2010PhDT.......467S \| http://ui.adsabs.harvard.edu/#abs/2010PhDT.......467S 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 \| http://ui.adsabs.harvard.edu/#abs/2014MNRAS.437..316K Tracing the Reverberation Lag in the Hard State of Black Hole X-Ray Binaries \|De Marco, B., Ponti, G., et al. \| ApJ \| 814-50 \| 2015 \| 2015ApJ...814...50D \| http://ui.adsabs.harvard.edu/#abs/2015ApJ...814...50D High ionisation absorption in low mass X-ray binaries \|Ponti, G., Bianchi, S., et al. \| AN \| 337-512 \| 2016 \| 2016AN....337..512P \| http://ui.adsabs.harvard.edu/#abs/2016AN....337..512P The Million Optical - Radio/X-ray Associations (MORX) Catalogue \|Flesch, Eric W., \| PASA \| 33-52 \| 2016 \| 2016PASA...33...52F \| http://ui.adsabs.harvard.edu/#abs/2016PASA...33...52F Crossing the Eddington Limit: Examining Disk Spectra at High Accretion Rates \|Sutton, Andrew D., Swartz, Douglas A., et al. \| ApJ \| 836-48 \| 2017 \| 2017ApJ...836...48S \| http://ui.adsabs.harvard.edu/#abs/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 al. \| ApJ \| 855-61 \| 2018 \| 2018ApJ...855...61W \| http://ui.adsabs.harvard.edu/#abs/2018ApJ...855...61W Classification of 4XMM-DR9 sources by machine learning \|Zhang, Yanxia, Zhao, Yongheng, \| MNRAS \| 503-5263 \| 2021 \| 2021MNRAS.503.5263Z \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.503.5263Z High-density Reflection Spectroscopy of Black Hole X-Ray Binaries in the Hard State \|Liu, Honghui, Jiang, Jiachen, et al. \| ApJ \| 951-145 \| 2023 \| 2023ApJ...951..145L \| http://ui.adsabs.harvard.edu/#abs/2023ApJ...951..145L The current state of disk wind observations in BHLMXBs through X-ray absorption lines in the iron band \|Parra, M., Petrucci, P. -O., et al. \| A&A \| 681-49 \| 2024 \| 2024A&A...681A..49P \| http://ui.adsabs.harvard.edu/#abs/2024A&A...681A..49P Robust constraints on feebly interacting particles using XMM-Newton \|Luque, Pedro De la Torre, Balaji, Shyam, \| PhRvD \| 109-L101305 \| 2024 \| 2024PhRvD.109j1305L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j1305L Multimessenger search for electrophilic feebly interacting particles from supernovae \|Luque, Pedro De la Torre, Balaji, Shyam, \| PhRvD \| 109-103028 \| 2024 \| 2024PhRvD.109j3028L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j3028L Importance of Cosmic-Ray Propagation on Sub-GeV Dark Matter Constraints \|De la Torre Luque, Pedro, Balaji, Shyam, \| ApJ \| 968-46 \| 2024 \| 2024ApJ...968...46D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...968...46D
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 Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs 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 Earths 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
Keywords	"relativistic effects", "XMM", "outburst throughout", "exhibit emission lines", "accretion disk geometry", "absorption edges characteristic", "black hole", "resolution xray spectra", "gamma ray", "wide range", "blackhole xray binary"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Prof Walter Lewin, 2003, 'XMM Observations of Black-Hole X-Ray Binaries in Outburst', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-djnsdte