A dataset provided by the European Space Agency

Name: Energy resolved timing of SS433: the supercritical disk and the jets
Published: 2013-10-26T00:00:00Z

Proposal ID	069487
Title	Energy resolved timing of SS433: the supercritical disk and the jets
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0694870201
DOI	https://doi.org/10.5270/esa-0jmkxku
Principal Investigator, PI	Dr Aleksei Medvedev
Abstract	We propose EPIC observations of the microquasar SS 433, the only knownpersistent superaccretor in the Galaxy. Previous studies of the XMM data showedthat different parts of SS 433 spectrum are dominated by different sources ofradiation. Preliminary results of the cross-correlation analysis of low-resolution RXTE spectra and existing short-duration XMM data, revealedcorrelations in variability between different energy ranges with time lags of 20s. We request a longer (115 ks) observations in the timing mode to obtain high-resolution data, sufficient for the cross-correlation and variability analysis.These new data will give us the unique opportunity to investigate directly thenon-stationary processes and spatial structure of the most inner parts of the supercritical accretion disk.
Publications	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 \| http://ui.adsabs.harvard.edu/#abs/2014Ap&SS.354...97Y 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 An Upper Limit on Nickel Overabundance in the Supercritical Accretion Disk Wind of SS 433 from X-ray Spectroscopy \|Medvedev, P. S., Khabibullin, I. I., et al. \| AstL \| 44-390 \| 2018 \| 2018AstL...44..390M \| http://ui.adsabs.harvard.edu/#abs/2018AstL...44..390M 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 Ultraluminous X-Ray Sources \|Fabrika, S. N., Atapin, K. E., et al. \| AstBu \| 76-6 \| 2021 \| 2021AstBu..76....6F \| http://ui.adsabs.harvard.edu/#abs/2021AstBu..76....6F The EXTraS project: Exploring the X-ray transient and variable sky \|De Luca, A., Salvaterra, R., et al. \| A&A \| 650-167 \| 2021 \| 2021A&A...650A.167D \| http://ui.adsabs.harvard.edu/#abs/2021A&A...650A.167D XMM-Newton campaign on the ultraluminous X-ray source NGC 247 ULX-1: outflows \|Pinto, C., Soria, R., et al. \| MNRAS \| 505-5058 \| 2021 \| 2021MNRAS.505.5058P \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.505.5058P From Active Stars to Black Holes: A Discovery Tool for Galactic X-Ray Sources \|Rodriguez, Antonio C., \| PASP \| 136-054201 \| 2024 \| 2024PASP..136e4201R \| http://ui.adsabs.harvard.edu/#abs/2024PASP..136e4201R Discovering the Mass-Scaled Damping Timescale from Microquasars to Blazars \|Zhang, Haoyang, Yang, Shenbang, \| ApJ \| 967-L18 \| 2024 \| 2024ApJ...967L..18Z \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...967L..18Z 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, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2012-10-03T19:13:37Z/2012-10-05T08:38:54Z
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	2013-10-26T00:00:00Z
Keywords	"resolution data", "supercritical disk", "persistent superaccretor", "supercritical accretion disk", "microquasar ss 433", "stationary processes", "XMM", "energy ranges", "spatial structure", "cross correlation", "variability analysis", "energy resolved", "cross correlation analysis", "EPIC", "time lags", "ss 433 spectrum", "xmm data"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Aleksei Medvedev, 2013, 'Energy resolved timing of SS433: the supercritical disk and the jets', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-0jmkxku