A dataset provided by the European Space Agency

Proposal ID 030254
Title Dark Matter in Elliptical Galaxies
Download Data Associated to the proposal

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0302540201

DOI https://doi.org/10.5270/esa-x4io6x2
Principal Investigator, PI Dr Ewan O.Sullivan
Abstract While the brightest group and cluster dominant elliptical galaxies are believedto have large dark matter halos, recent dynamical measurements suggest that somemoderate luminosity ellipticals contain little or no dark matter. However, anX-ray mass measurement for one of these galaxies produces a conflicting result.We have undertaken the first systematic survey of mass profiles in ordinaryellipticals with X-ray halos using archival data, but almost all the galaxieswith X-ray data available lie in high density environments. In order to rectifythis bias, we propose to observe four elliptical galaxies in low densityenvironments with the goal of understanding their halo properties.
Publications
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2005-05-02T09:45:32Z/2005-05-02T19:14:08Z
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 2006-08-03T00:00:00Z
Keywords "low density environments", "ordinary ellipticals", "xray halos", "mass profiles", "xray data", "halo properties", "systematic survey", "moderate luminosity ellipticals", "elliptical galaxy", "dark matter halos", "dark matter", "density environments", "archival data", "galaxy produces", "xray mass measurement", "dynamical measurements"
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Dr Ewan O.Sullivan, 2006, 'Dark Matter in Elliptical Galaxies', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-x4io6x2