A dataset provided by the European Space Agency

Name 012650
Title LMC X-3 High S:N Point Spread Functions in EPIC
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0126500101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0126500201

DOI 10.5270/esa-nz4itfl
Author Dr Fred Jansen XMM-Newton PS
Description CAL- The bright LMC X-3 binary will be observed with the EPIC cameras to trace the PSF out into the wings. By use of different modes some correction for pile-up may be achieved. The target ideally should be measured in its lowest flux state to minimise pile-up effects. The Full window modes will capture the wings of the PSF to high S:N with minimnal confusion from background and serendipitous sources, but significant pile-up will occur in the PSF core. A small window mode in each case will be used measure the PSF core. (Assumed 2x 2.7ksec overhead for EPIC in defining RGS and OM exposures). Tho observation may be repeated at a lower flux state of the source, by rescheduling ca. 45 days after the first observation.
Publication XMM-Newton EPIC and RGS observations of LMC X-3 . Wu, K., Soria, R., et all. . A&A . 365-267 . 2001 . 2001A&A...365L.267W ,
XMM-Newton RGS spectroscopy of LMC X-3 . Page, M. J., Soria, R., et all. . MNRAS . 345-639 . 2003 . 2003MNRAS.345..639P ,
High mass X-ray binaries in the LMC: Dependence on the stellar population age and the ''propeller.. effect . Shtykovskiy, P., Gilfanov, M., . A&A . 431-597 . 2005 . 2005A&A...431..597S ,
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 ,
The XMM Cluster Survey: optical analysis methodology and the first data release . Mehrtens, Nicola, Romer, A. Kathy, et all. . MNRAS . 423-1024 . 2012 . 2012MNRAS.423.1024M ,
X-Ray Absorption from the Milky Way Halo and the Local Group . Bregman, Joel N., Lloyd-Davies, Edward J., . ApJ . 669-990 . 2007 . 2007ApJ...669..990B ,
First science results from XMM and Chandra . Charles, P. A., . Obs . 122-77 . 2002 . 2002Obs...122...77C ,
An All-Sky Atlas of Radio-X-ray Associations . Flesch, E., . PASA . 27-283 . 2010 . ...
Instrument EMOS1, EMOS2, EPN, RGS1, RGS2
Temporal Coverage 2000-06-09T06:54:19Z/2000-06-10T07:00:09Z
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 2001-10-31T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2001-10-31T00:00:00Z, 012650, 17.56_20190403_1200. https://doi.org/10.5270/esa-nz4itfl