A dataset provided by the European Space Agency

Name: XMM-Newton Observations of the ACT Cosmological Sample of Clusters
Published: 2017-02-05T23:00:00Z

Proposal ID	076229
Title	XMM-Newton Observations of the ACT Cosmological Sample of Clusters
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0762290101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0762290201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0762290301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0762290401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0762290501
DOI	https://doi.org/10.5270/esa-raj9qqr
Principal Investigator, PI	Prof John P. Hughes
Abstract	We propose to complete our X-ray follow-up program aimed at observing the ACTCosmological Sample of Clusters, which is a well-defined sample of 22 massivegalaxy clusters detected by the Atacama Cosmology Telescope using theSunyaev-Zel.dovich effect (SZE). There remain five newly-discovered SZE clustersin this sample without any X-ray data. The proposed XMM-Newton EPIC observationswill provide accurate gas masses and temperatures to be used for a precisioncalibration of the SZE signal versus mass scaling law out to redshifts of 1.This effort is an essential part of our intensive multi-wavelength campaign toobtain mass measurements for the ACT Cosmological Sample of Clusters.
Publications	A Comparison of X-Ray Photon Indices among the Narrow- and Broad-line Seyfert 1 Galaxies \|Ojha, Vineet, Chand, Hum, et al. \| ApJ \| 896-95 \| 2020 \| 2020ApJ...896...95O \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...896...95O Exploiting NIKA2/XMM-Newton imaging synergy for intermediate-mass high-z galaxy clusters within the NIKA2 SZ large program. Observations of ACT-CL J0215.4+0030 at z \\u223c 0.9 \|K\\u00e9ruzor\\u00e9, F., Mayet, F., et al. \| A&A \| 644-93 \| 2020 \| 2020A&A...644A..93K \| http://ui.adsabs.harvard.edu/#abs/2020A&A...644A..93K The composite X-ray spectra of radio-loud and radio-quiet SDSS quasars \|Zhou, Min-Hua, Gu, Min-Feng, \| RAA \| 21-4 \| 2021 \| 2021RAA....21....4Z \| http://ui.adsabs.harvard.edu/#abs/2021RAA....21....4Z 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 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 Robust constraints on feebly interacting particles using XMM-Newton \|Luque, Pedro De la Torre, Balaji, Shyam, \| PhRvD \| 109-L101305 \| 2024 \| 2024PhRvD.109j1305L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j1305L Multimessenger search for electrophilic feebly interacting particles from supernovae \|Luque, Pedro De la Torre, Balaji, Shyam, \| PhRvD \| 109-103028 \| 2024 \| 2024PhRvD.109j3028L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j3028L Importance of Cosmic-Ray Propagation on Sub-GeV Dark Matter Constraints \|De la Torre Luque, Pedro, Balaji, Shyam, \| ApJ \| 968-46 \| 2024 \| 2024ApJ...968...46D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...968...46D
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2015-07-15T04:29:58Z/2016-01-24T22:25:45Z
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	2017-02-05T23:00:00Z
Keywords	"xmm newton epic", "act cosmological sample", "XMM-Newton", "atacama cosmology telescope", "xmm newton", "program aimed", "xray data", "defined sample", "gas masses", "precision calibration", "XMM", "mass scaling law", "sze cluster", "EPIC", "sze signal", "massive galaxy cluster", "dovich effect sze", "sunyaev zel", "mass measurements"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Prof John P. Hughes, 2017, 'XMM-Newton Observations of the ACT Cosmological Sample of Clusters', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-raj9qqr