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: 2022-06-12T00:00:00Z

Proposal ID	088196
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=0881960101
DOI	https://doi.org/10.57780/esa-bukiida
Principal Investigator, PI	Dr Iacopo Bartalucci
Abstract	We propose to observe 6 SZ-selected galaxy clusters to complete the follow-up ofa large representative sample of 45 objects at 0.5 < z < 0.9. All are targets ofan ongoing 300h Guaranteed Time Programme of high-resolution (< 18 ) SZobservations with NIKA2. The sample, extracted from the Planck and ACT surveys,covers an unprecedented mass range at these redshifts. Combining measurements ofgas density from XMM-Newton imaging and pressure from NIKA2 SZ maps, we willstudy individual radial thermodynamic and mass profiles, their dispersion, andthe relations between YSZ, YX and mass for the first time in this mass andredshift range.
Publications	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	2021-05-23T23:35:40Z/2021-05-24T09:30:40Z
Version	19.16_20210326_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	2022-06-12T00:00:00Z
Keywords	"act surveys", "galaxy cluster", "gas density", "mass range", "XMM", "low mass", "nika2 sz maps", "xmm newton imaging", "probe icm physics", "XMM-Newton", "mass profiles", "individual radial thermodynamic", "redshift range"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Iacopo Bartalucci, 2022, 'A novel X-ray-SZ imaging programme to probe ICM physics at low mass and high z', 19.16_20210326_1200, European Space Agency, https://doi.org/10.57780/esa-bukiida