A dataset provided by the European Space Agency

Name 065295
Title XMM-Newton Observations of ACT SZ and X-ray-Selected Clusters


DOI https://doi.org/10.5270/esa-jhxavlo
Author Prof John P. Hughes
Description We propose to obtain sensitive XMM-Newton observations of 20 cluster candidates with significant 148-GHz SZ decrements from the Atacama Cosmology Telescope (ACT) survey that also show correlated RASS X-ray emission. The new XMM-Newton data will allow us to measure accurate X-ray luminosities and gas temperatures from which we will estimate cluster masses using established scaling relations. This data set forms a mass- and volume-limited sample of massive galaxy clusters.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2010-06-03T06:04:16Z/2010-12-26T08:06:52Z
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 2012-01-29T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2012-01-29T00:00:00Z, 065295, 17.56_20190403_1200. https://doi.org/10.5270/esa-jhxavlo