A dataset provided by the European Space Agency

Name 076280
Title The Planck Cluster Cosmological Sample


DOI 10.5270/esa-g1668pp
Author Dr William Forman
Description The Planck Cosmological Reference Sample of 189 SZ-selected provides the opportunity to define the low redshift benchmark for cluster evolution studies. To completely characterize the sample requires 12 XMM-Newton observations, each sufficient to measure the key mass proxy M_{YX} to an accuracy of 5% or better. In addition, the observations will enable detailed studies of cluster scaling relations, measurement of the scatter around these relations, and enable improvements in the Planck SZ measurements using accurate X-ray determined positions and sizes. The ultimate goal is to compare high z and low z cluster samples to constrain cosmological parameters as well as to understand any differences between X-ray and SZ cluster selection functions.
Publication The population of X-ray supernova remnants in the Large Magellanic Cloud . Maggi, P., Haberl, F., et all. . A&A . 585-162 . 2016 . 2016A&A...585A.162M ,
Identification of high-mass X-ray binaries selected from XMM-Newton observations of the LMC* . van Jaarsveld, N., Buckley, D. A. H., et all. . MNRAS . 475-3253 . 2018 . 2018MNRAS.475.3253V ,
X-Ray Luminosity and Size Relationship of Supernova Remnants in the LMC . Ou, Po-Sheng, Chu, You-Hua, et all. . ApJ . 863-137 . 2018 . 2018ApJ...863..137O ,
The cool-core state of Planck SZ-selected clusters versus X-ray-selected samples: evidence for cool-core bias . Rossetti, M., Gastaldello, F., et all. . MNRAS . 468-1917 . 2017 . 2017MNRAS.468.1917R ,
Probing cosmic isotropy with a new X-ray galaxy cluster sample through the LX-T scaling relation . Migkas, K., Schellenberger, G., et all. . A&A . 636-15 . 2020 . 2020A&A...636A..15M ,
New optically identified supernova remnants in the Large Magellanic Cloud . Yew, Miranda, Filipoviu0107, Miroslav D., et all. . MNRAS . 500-2336 . 2021 . 2021MNRAS.500.2336Y ,
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2015-04-18T01:29:55Z/2016-02-17T06:28:32Z
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 2017-03-18T23:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2017-03-18T23:00:00Z, 076280, 17.56_20190403_1200. https://doi.org/10.5270/esa-g1668pp