A dataset provided by the European Space Agency

Name 020305
Title MAGNETIC CVS FROM SDSS
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0203050101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0203050201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0203050301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0203050401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0203050501
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0203050601
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0203050701
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0203050801

DOI 10.5270/esa-k1c7n69
Author Prof PAULA SZKODY
Description We propose to obtain X-ray fluxes and spectra of 8 new magnetic CVs identified during the first 2 yrs of the Sloan Digital Sky Survey. The Polars in this group represent the lowest end of mass transfer in magnetic systems. We will exploit the high sensitivity and large energy coverage of XMM to delineate the shock vs blob heating in these low accretion regimes as compared to the high accretion rate systems that have previously been found in X-ray surveys. Our findings from SDSS indicate these low accretion systems may represent a large contribution to the magnetic CV population. Thus, determining their accretion characteristics provides an important test of accretion scenarios at high magnetic fields.
Publication XMM-Newton Observations of the Extremely Low Accretion Rate Polars SDSS J155331.12+551614.5 and SDSS J132411.57+032050.5 . Szkody, Paula, Homer, Lee, et all. . AJ . 128-2443 . 2004 . 2004AJ....128.2443S ,
XMM-Newton and Optical Follow-up Observations of SDSS J093249.57+472523.0 and SDSS J102347.67+003841.2 . Homer, Lee, Szkody, Paula, et all. . AJ . 131-562 . 2006 . 2006AJ....131..562H ,
Characterizing three candidate magnetic cataclysmic variables from SDSS: XMM-Newton and optical follow-up observations. . Homer, L., Szkody, P., et all. . AJ . 132-2743 . 2006 . 2006AJ....132.2743H ,
A revision of the X-ray absorption nature of BALQSOs . Streblyanska, A., Barcons, X., et all. . A&A . 515-2 . 2010 . 2010A&A...515A...2S ,
X-ray Variability and Evidence for Pulsations from the Unique Radio Pulsar-X-ray Binary Transition Object FIRST J102347.6+003841 . Archibald, Anne M., Kaspi, Victoria M., et all. . ApJ . 722-88 . 2010 . 2010ApJ...722...88A ,
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 ,
The X-ray Energy Dependence of the Relation Between Optical and X-ray Emission in Quasars . Young, M., Elvis, M., . ApJ . 708-1388 . 2010 . 2010ApJ...708.1388Y ,
An Extremely Luminous Panchromatic Outburst from the Nucleus of a Distant Galaxy . L...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2004-01-25T02:27:02Z/2005-01-12T08:17:37Z
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 2006-02-10T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2006-02-10T00:00:00Z, 020305, 17.56_20190403_1200. https://doi.org/10.5270/esa-k1c7n69