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: 2020-01-21T23:00:00Z

Proposal ID	082172
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=0821721101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0821721301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0821722001 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0821722101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0821722201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0821722401
DOI	https://doi.org/10.5270/esa-sy4vj66
Principal Investigator, PI	Dr Gabriel Pratt
Abstract	We propose to observe 15 galaxy clusters from the low-mass part of arepresentative SZ-selected sample of 45 objects at 0.5
Publications	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	2018-11-12T13:46:48Z/2018-12-24T02:55:28Z
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	2020-01-21T23:00:00Z
Last Update	2025-01-27
Keywords	"archival xray data", "gt programme", "probe icm physics", "mass profiles", "sample doubles", "M500", "gravitational processes", "low mass", "mass range", "log mass range", "precision individual pressure", "galaxy cluster", "XMM", "gas density"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Gabriel Pratt, 2020, '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-sy4vj66