A dataset provided by the European Space Agency

Name: A novel X-ray-SZ imaging programme to probe ICM physics at low mass and high z
Published: 2019-02-16T23:00:00Z

Proposal ID	080097
Title	A novel X-ray-SZ imaging programme to probe ICM physics at low mass and high z
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0800970901 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0800971001 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0800971201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0800971501
DOI	https://doi.org/10.5270/esa-7iydqms
Principal Investigator, PI	Dr Gabriel Pratt
Abstract	We propose to observe 15 low-mass SZ selected galaxy clusters from arepresentative sample of 45 objects at 0.53x10e14 Msun, the full sample, extracted from Planck and ACT,covers an unprecedented mass range. Archival X-ray data are available at highmass. Combining the gas density from XMM and the pressure from NIKA2, we willdouble the (log) mass range of our study of the pressure, entropy and HE massprofiles, their dispersion, and the relations between Ysz, Yx and M500. Thesample adds 3 Gyr of look-back time beyond z>0.5, and will serve as an importantprobe of the impact of gravitational and non-gravitational processes on the ICM.
Publications	General relativistic orbital decay in a seven-minute-orbital-period eclipsing binary system \|Burdge Kevin B. Coughlin Michael W. et al. \| Natur \| 571-528 \| 2019 \| 2019Natur.571..528B \| http://ui.adsabs.harvard.edu/#abs/2019Natur.571..528B Classification of 4XMM-DR9 sources by machine learning \|Zhang Yanxia Zhao Yongheng \| MNRAS \| 503-5263 \| 2021 \| 2021MNRAS.503.5263Z \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.503.5263Z The Planck clusters in the LOFAR sky. I. LoTSS-DR2: New detections and sample overview \|Botteon A. Shimwell T. W. et al. \| A&A \| 660-78 \| 2022 \| 2022A&A...660A..78B \| http://ui.adsabs.harvard.edu/#abs/2022A&A...660A..78B The Planck clusters in the LOFAR sky. III. LoTSS-DR2: Dynamic states and density fluctuations of the intracluster medium \|Zhang X. Simionescu A. et al. \| A&A \| 672-42 \| 2023 \| 2023A&A...672A..42Z \| http://ui.adsabs.harvard.edu/#abs/2023A&A...672A..42Z The Planck clusters in the LOFAR sky. IV. LoTSS-DR2: Statistics of radio haloes and re-acceleration models \|Cassano R. Cuciti V. et al. \| A&A \| 672-43 \| 2023 \| 2023A&A...672A..43C \| http://ui.adsabs.harvard.edu/#abs/2023A&A...672A..43C The XMM-Newton Line Emission Analysis Program (X-LEAP). I. Emission-line Survey of O VII O VIII and Fe L-shell Transitions \|Pan Zeyang Qu Zhijie et al. \| ApJS \| 271-62 \| 2024 \| 2024ApJS..271...62P \| http://ui.adsabs.harvard.edu/#abs/2024ApJS..271...62P From Active Stars to Black Holes: A Discovery Tool for Galactic X-Ray Sources \|Rodriguez Antonio C. \| PASP \| 136-054201 \| 2024 \| 2024PASP..136e4201R \| http://ui.adsabs.harvard.edu/#abs/2024PASP..136e4201R
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2018-01-21T00:08:46Z/2018-02-03T21:59:34Z
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	2019-02-16T23:00:00Z
Last Update	2025-01-27
Keywords	"archival xray data", "gt programme", "probe icm physics", "mass profiles", "M500", "low mass sz", "gravitational processes", "low mass", "mass range", "log mass range", "galaxy cluster", "sample adds", "XMM", "gas density", "3x10e14 msun"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Gabriel Pratt, 2019, 'A novel X-ray-SZ imaging programme to probe ICM physics at low mass and high z', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-7iydqms