A dataset provided by the European Space Agency

Name: The most massive IR detected galaxy cluster MOO J1142+1527 at z=1.2
Published: 2021-01-20T23:00:00Z

Proposal ID	084421
Title	The most massive IR detected galaxy cluster MOO J1142+1527 at z=1.2
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0844210101
DOI	https://doi.org/10.57780/esa-lb0x50c
Principal Investigator, PI	Dr Iacopo Bartalucci
Abstract	We propose to observe the most massive, M500 = 6x10e14 Msun, infrared selectedgalaxy cluster MOO J1142+1527 discovered in the MaDCoWS survey at z=1.2.Deep XMMobservations will allow us to determine the gas morphology at large scale andextract the radial density, temperature, pressure and hydrostatic mass profilesup to R500.X-rays will be complemented by NIKA2, an instrument which willperform Sunyaev-Zel Dovich observations with the same spatial resolution asXMM.This will allow us to explore the robustness of mass determination andestimate the non-thermal pressure support for the first time at z>1.Supportedalso by rich ancillary optical,infrared, and Chandra observations, we will beable to obtain a complete picture of the spatially resolved halo properties of this extreme cluster.
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 Unveiling the origin of XMM-Newton soft proton flares: II. Systematics in the proton spectral analysis \|Mineo T. Fioretti V. et al. \| A&A \| 691-A230 \| 2024 \| 2024A&A...691A.230M \| http://ui.adsabs.harvard.edu/#abs/2024A&A...691A.230M Search for Young Stellar Objects within 4XMM-DR13 Using CatBoost and SPE \|Ma Xiangyao Zhang Yanxia et al. \| AJ \| 168-210 \| 2024 \| 2024AJ....168..210M \| http://ui.adsabs.harvard.edu/#abs/2024AJ....168..210M
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2019-12-21T06:02:01Z/2019-12-22T13:58:41Z
Version	18.00_20191217_1110
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	2021-01-20T23:00:00Z
Last Update	2025-08-04
Keywords	"XMM", "x rays", "gas morphology", "madcows survey", "resolved halo properties", "rich ancillary optical", "radial density", "deep xmm", "M500", "spatial resolution", "hydrostatic mass profiles", "complete picture", "massive ir", "nonthermal pressure support", "6x10e14 msun"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Iacopo Bartalucci, 2021, 'The most massive IR detected galaxy cluster MOO J1142+1527 at z=1.2', 18.00_20191217_1110, European Space Agency, https://doi.org/10.57780/esa-lb0x50c