A dataset provided by the European Space Agency

Proposal ID 078445
Title X-raying the X-ray under luminous clusters in the Planck SZ Catalogue
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DOI https://doi.org/10.5270/esa-1659f9k
Principal Investigator, PI Dr Mariachiara Rossetti
Abstract We propose to perform snapshot observations of a population of clusters whichemerged in the Second Planck Catalogue of SZ sources as being under luminous inX-rays with respect to the prediction based on their measured SZ flux. Thisprogram will allow us to confirm or challenge the detection of these objects byfirmly assessing their flux, to measure their gas content and to map the gasdistribution, allowing us to discriminate between different scenarios for theirorigin. The detection of this population of objects has important implicationsfor understanding selection effects in SZ and X-ray surveys, for thereconstruction of the mass function of galaxy clusters and for the calibrationof scaling relations.
Publications
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2016-05-14T07:31:29Z/2017-04-30T02:59:47Z
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 2018-05-22T22:00:00Z
Last Update 2025-01-27
Keywords "x raying", "mass function", "planck catalogue", "scaling relations", "sz flux", "firmly assessing", "planck sz catalogue", "gas distribution", "gas content", "galaxy cluster", "luminous cluster", "sz sources", "xray surveys", "selection effects", "perform snapshot"
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Dr Mariachiara Rossetti, 2018, 'X-raying the X-ray under luminous clusters in the Planck SZ Catalogue', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-1659f9k