A dataset provided by the European Space Agency

Name 070018
Title Unveiling the most massive clusters at z>0.5 with Planck and XMM-Newton.
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0700180201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0700180901
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0700182001
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0700182201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0700182401

DOI 10.5270/esa-xsgt4vz
Author Dr monique arnaud
Description We propose to gather spatially resolved spectroscopy of a sample of 33 massive (M_{500}>5e+14 solar masses) clusters detected blindly by Planck and confirmed to-day to be in the redshift range 0.5
Publication Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift . Yershov, V. N., . Ap&SS . 354-97 . 2014 . 2014Ap&SS.354...97Y ,
XMM-Newton publication statistics . Ness, J.-U., Parmar, A. N., et all. . AN . 335-210 . 2014 . 2014AN....335..210N ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
Pressure Profiles of Distant Galaxy Clusters in the Planck Catalogue . Bourdin, H., Mazzotta, P., et all. . ApJ . 843-72 . 2017 . 2017ApJ...843...72B ,
The stellar mass function of galaxies in Planck-selected clusters at 0.5 < z < 0.7: new constraints on the timescale and location of satellite quenching . van der Burg, Remco F. J., McGee, Sean, et all. . A&A . 618-140 . 2018 . 2018A&A...618A.140V ,
X-Ray Properties of SPT-selected Galaxy Clusters at 0.2 < z < 1.5 Observed with XMM-Newton . Bulbul, Esra, Chiu, I.-Non, et all. . ApJ . 871-50 . 2019 . 2019ApJ...871...50B ,
The Most Massive galaxy Clusters (M2C) across cosmic time: link between radial total mass distribution and dynamical state . Bartalucci, I., Arnaud, M., et all. . A&A . 628-86 . 2019 . 2019A&A...628A..86B ,
Mass variance from archival X-ray properties of Dark Energy Survey Year-1 galaxy clusters . Farahi, A., Chen, X., et all. . MNRAS . 490-3341 . 2019 . ...,
Mass calibration of the CODEX cluster sample using SPIDERS spectroscopy - II. The X-ray luminosity-mass relation . Capasso, R., Mohr, J. J., et all. . MNRAS . 494-2736 . 2020 . 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 all. . MNRAS . 494-1705 . 2020 . 2020MNRAS.494.1705G ,
The XMM Cluster Survey: new evidence for the 3.5-keV feature in clusters is inconsistent with a dark matter origin . Bhargava, S., Giles, P. A., et all. . MNRAS . 497-656 . 2020 . 2020MNRAS.497..656B ,
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2012-05-02T09:33:31Z/2013-01-20T17:55:43Z
Version 17.56_20190403_1200
Mission Description The European Space Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's 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 Earth's 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 2014-02-09T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2014-02-09T00:00:00Z, 070018, 17.56_20190403_1200. https://doi.org/10.5270/esa-xsgt4vz