A dataset provided by the European Space Agency

Name 030216
Title Extending the XMM-Newton survey of AM CVn systems to longer periods
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0302160201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0302160401

DOI 10.5270/esa-3bl8p45
Author Dr Gavin Ramsay
Description We have an on-going project to survey the ultra-compact AM CVn systems using XMM-Newton. These accreting binaries have periods less than ~70 min and are hydrogen deficient. They are important astrophysically because they are expected to be strong sources of gravitational radiation in the peak sensitivity band of LISA. XMM-Newton has so far observed 7 of the 13 AM CVn systems, but this is biased towards shorter period systems. We propose to observe another 4 systems to give us a comprehensive sample of these objects. In particular, we will determine the element abundance from their X-ray spectra and characterise the X-ray and UV variability as a function of orbital period. This is essential for our understanding of their evolutionaryhistory and their energy balance.
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An Extremely Luminous Panchromatic Outburst from the Nucleus of a Distant Galaxy . Levan, A. J., Tanvir, N. R., et all. . Sci . 333-199 . 2011 . 2011Sci...333..199L ,
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 ,
XMM-Newton observations of AM CVn binaries: V396 Hya and SDSS J1240-01 . Ramsay, G., Groot, P. J., et all. . A&A . 457-623 . 2006 . 2006A&A...457..623R ,
Hard X-ray Emission Associated with White Dwarfs. III. . Bilikova, Jana, Chu, You-Hua, et all. . AJ . 140-1433 . 2010 . 2010AJ....140.1433B ,
Wavelet and R-S analysis of the X-ray flickering of cataclysmic variables . Anzolin, G., Tamburini, F., et all. . A&A . 519-69 . 2010 . 2010A&A...519A..69A ,
An All-Sky Atlas of Radio-X-ray Associations . Flesch, E., . PASA . 27-283 . 2010 . 2010PASA...27..283F ,
The XMM Cluster Survey: X-ray analysis methodology ....
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2005-07-20T13:35:39Z/2006-01-08T02:43:31Z
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 2007-01-27T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2007-01-27T00:00:00Z, 030216, 17.56_20190403_1200. https://doi.org/10.5270/esa-3bl8p45