Proposal ID | 030087 |
Title | Magnetic CVs from SDSS |
Download Data Associated to the proposal | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0300870201 |
DOI | https://doi.org/10.5270/esa-zc9psz5 |
Principal Investigator, PI | Prof Paula Szkody |
Abstract | We propose to continue our XMM-Newton observations of new magnetic CVs found inthe Sloan Digital Sky Survey. Our results from the first 2 yrs include theidentification of the base level of X-ray flux from objects in the lowest statesof mass transfer as well as discovery of X-ray eclipses and flares. We proposecontinuing this work on 7 new systems found in the latest SDSS data, including 3confirmed Polars and 4 likely Polars/Intermediate Polars. We exploit the highsensitivity and large energy coverage of XMM-Newton to delineate the shock vsblob heating in the typical low accretion regimes encountered in the SDSS datacompared to previous X-ray surveys. Our results indicate that low accretion ratesystems may represent a large fraction of the magnetic CV population. |
Publications |
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Instrument | EMOS1, EMOS2, EPN, OM, RGS1, RGS2 |
Temporal Coverage | 2005-04-21T11:58:25Z/2006-02-07T23:32:25Z |
Version | 17.56_20190403_1200 |
Mission Description | The European Space Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs 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 Earths 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 | 2007-07-11T00:00:00Z |
Last Update | 2025-01-27 |
Keywords | "mass transfer", "sdss data", "SDSS", "magnetic cvs", "xmm newton", "blob heating", "base level", "XMM-Newton", "xray flux", "xray eclipses", "intermediate polars", "energy coverage", "XMM", "xray surveys", "magnetic cv population" |
Publisher And Registrant | European Space Agency |
Credit Guidelines | European Space Agency, Prof Paula Szkody, 2007, 'Magnetic CVs from SDSS', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-zc9psz5 |