A dataset provided by the European Space Agency

Name 030321
Title Simultaneous XMM-Newton - RXTE observations of 1E1740.7-2942
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0303210201

DOI 10.5270/esa-t2n6lwq
Author Dr Emrah Kalemci
Description It has been known that sources that have high absorption column density (NH) also have high dust column density along the line of sight. The differential delays caused by small angle scattering from dust may have important effects on the power spectra of Galactic black holes (GBHs) at low energies, and impact studies that use the relation between the rms amplitude of variability and energy to determine the origin of QPOs from these sources. We propose to observe high NH (1E23 cm-2) GBH 1E1740.7-2942 for 20 ks simultaneously with XMM-Newton and RXTE. By comparing the power spectra from the PSF in XMM-Newton (using imaging and excluding the scattering halo) and the RXTE data, we will investigate the effects of small angle scattering on the timing properties of GBHs.
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 ,
A Search for New Galactic Magnetars in Archival Chandra and XMM-Newton Observations . Muno, M. P., Gaensler, B. M., et all. . ApJ . 680-639 . 2008 . 2008ApJ...680..639M ,
Two Rapidly Variable Galactic X-ray Transients Observed with Chandra, XMM-Newton, and Suzaku . Heinke, C. O., Tomsick, J. A., et all. . ApJ . 701-1627 . 2009 . 2009ApJ...701.1627H ,
An All-Sky Atlas of Radio-X-ray Associations . Flesch, E., . PASA . 27-283 . 2010 . 2010PASA...27..283F ,
Suzaku Detection of an Intense X-Ray Flare from an A-Type Star, HD161084 . Miura, Junichiro, Tsujimoto, Masahiro, et all. . PASJ . 60-49 . 2008 . 2008PASJ...60S..49M ,
Classification of X-Ray Sources in the XMM-Newton Serendipitous Source Catalog . Lin, Dacheng, Webb, Natalie A., . ApJ . 756-27 . 2012 . 2012ApJ...756...27L ,
The XMM-Newton serendipitous ultraviolet source survey catalogue . Page, M. J., Brindle, C., et all. . MNRAS . 426-903 . 2012 . 2012MNRAS.426..903P ,
Automatic Classific...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2005-10-02T01:15:14Z/2005-10-02T07:53:47Z
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 2006-10-21T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2006-10-21T00:00:00Z, 030321, 17.56_20190403_1200. https://doi.org/10.5270/esa-t2n6lwq