A dataset provided by the European Space Agency

Name: Mass calibration of SPT clusters: re-observation of missing pointings
Published: 2014-10-26T00:00:00Z

Proposal ID	072477
Title	Mass calibration of SPT clusters: re-observation of missing pointings
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0724770101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0724770201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0724770301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0724770401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0724770501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0724770601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0724770701 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0724770801 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0724770901 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0724771001
DOI	https://doi.org/10.5270/esa-hqwd96q
Principal Investigator, PI	Dr Joe Mohr
Abstract	(Abridged) The South Pole Telescope (SPT) galaxy cluster survey identified viathe Sunyaev-Zeldovich (SZ) effect 158 massive clusters from its initial 720deg2 area. We are proposing to combine XMM-Newton, SPT, and weak lensingmeasurements for a sample of 20 intermediate redshift (0.3
Publications	The Million Optical - Radio/X-ray Associations (MORX) Catalogue \|Flesch Eric W. \| PASA \| 33-52 \| 2016 \| 2016PASA...33...52F \| http://ui.adsabs.harvard.edu/#abs/2016PASA...33...52F X-Ray Properties of SPT-selected Galaxy Clusters at 0.2 < z < 1.5 Observed with XMM-Newton \|Bulbul Esra Chiu I.-Non et al. \| ApJ \| 871-50 \| 2019 \| 2019ApJ...871...50B \| http://ui.adsabs.harvard.edu/#abs/2019ApJ...871...50B Mass calibration of the CODEX cluster sample using SPIDERS spectroscopy - II. The X-ray luminosity-mass relation \|Capasso R. Mohr J. J. et al. \| MNRAS \| 494-2736 \| 2020 \| 2020MNRAS.494.2736C \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.494.2736C Constraining radio mode feedback in galaxy clusters with the cluster radio AGNs properties to z u223c 1 \|Gupta N. Pannella M. et al. \| MNRAS \| 494-1705 \| 2020 \| 2020MNRAS.494.1705G \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.494.1705G A joint SZ-X-ray-optical analysis of the dynamical state of 288 massive galaxy clusters \|Zenteno A. Hernu00e1ndez-Lang D. et al. \| MNRAS \| 495-705 \| 2020 \| 2020MNRAS.495..705Z \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.495..705Z Constraints on the variation of fine structure constant from joint SPT-SZ and XMM-Newton observations \|Bora Kamal Desai Shantanu \| JCAP \| 2-12 \| 2021 \| 2021JCAP...02..012B \| http://ui.adsabs.harvard.edu/#abs/2021JCAP...02..012B A test of cosmic distance duality relation using SPT-SZ galaxy clusters Type Ia supernovae and cosmic chronometers \|Bora Kamal Desai Shantanu \| JCAP \| 6-52 \| 2021 \| 2021JCAP...06..052B \| http://ui.adsabs.harvard.edu/#abs/2021JCAP...06..052B 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	2013-05-10T08:37:21Z/2013-10-08T00:06:19Z
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	2014-10-26T00:00:00Z
Last Update	2025-01-27
Keywords	"soft proton flaring", "XMM", "combine xmm newton", "xray data", "initial 720 deg2", "XMM-Newton", "spt clusters", "mass calibration", "uniform sensitivity", "weak lensing measurements", "missing pointings", "intermediate redshift", "560 deg2 survey", "spt detection significance", "sunyaev zel", "dynamical masses"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Joe Mohr, 2014, 'Mass calibration of SPT clusters: re-observation of missing pointings', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-hqwd96q