A dataset provided by the European Space Agency

Name 002394
Title Temporal-Spectral Analysis of BHC LMC X-1, LMC X-3
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0023940101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0023940401

DOI 10.5270/esa-0w7xsub
Author Dr Demosthenes Kazanas
Description We propose XMM EPIC CCD observations in timing mode of the Black Hole Candidates (BHC) LMC X-1 and LMC X-3. Our goal is to probe the spatial structure of the X-ray emitting hot coronae by the combined temporal-spectral analysis of time lags between different energy bands in the XMM range as a function of the Fourier frequency. These lags appear to be at odds with predictions of accretion disk models. The unique properties of XMM allow the search for a transition in the lag sign from positive to negative at E < 2 keV, thus identifying the source of soft photons, whose Comptonization gives rise to the observed X-ray spectra and timing properties in these objests. This study will thus complement those carried out by RXTE at exclusively high (> 2 keV) X-ray energies.
Publication The column density towards LMC X-1 . Hanke, M., Wilms, J., et all. . A&A . 509-8 . 2010 . 2010A&A...509L...8H ,
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 ,
Probing the Environment of Accreting Compact Objects . Hanke, Manfred, . PhDT . 0-9 . 2011 . 2011PhDT.........9H ,
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 ,
Millihertz quasi-periodic oscillations and broad iron line from LMC X-1 . Alam, Md. Shah, Dewangan, G. C., et all. . MNRAS . 445-4259 . 2014 . 2014MNRAS.445.4259A ,
The population of X-ray supernova remnants in the Large Magellanic Cloud . Maggi, P., Haberl, F., et all. . A&A . 585-162 . 2016 . 2016A&A...585A.162M ,
Revealing the broad iron Kalpha line in Cygnus X-1 through simultaneous XMM-Newton, RXTE, and INTEGRAL observations . Duro, Refiz, Dauser, Thomas, et all. . A&A . 589-...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2002-04-21T14:29:13Z/2002-09-26T16:43:47Z
Version PPS_NOT_AVAILABLE
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 2005-01-01T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2005-01-01T00:00:00Z, 002394, PPS_NOT_AVAILABLE. https://doi.org/10.5270/esa-0w7xsub