A dataset provided by the European Space Agency

Name 067311
Title Constraining Cluster Evolution at z > 1 with the SpARCS-RCS Cluster Surveys
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673110201

DOI 10.5270/esa-157s9so
Author Dr Erica Ellingson
Description We propose XMM-EPIC observations of 3 clusters at high redshift from the SpARCS survey in order to constrain the evolution of X-ray scaling relations. An important difference between this survey and others is that by using galaxy-selected clusters, we can construct a sample which is unbiased in its gas properties. Each of these clusters has been detected by three methods: as a highly significant overdensity of red sequence galaxies, spectroscopically as a cluster with numerous confirmed members and velocity dispersions > 500 km-s, and as a faint, but extended X-ray source. Our proposed observations will yield accurate gas temperatures, enabling these clusters to be used in a study of the evolution of the cluster gas, galaxy and mass scaling relations to z>1.
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 ,
The XXL Survey. I. Scientific motivations - XMM-Newton observing plan - Follow-up observations and simulation programme . Pierre, M., Pacaud, F., et all. . A&A . 592-1 . 2016 . 2016A&A...592A...1P ,
The XXL Survey. II. The bright cluster sample: catalogue and luminosity function . Pacaud, F., Clerc, N., et all. . A&A . 592-2 . 2016 . 2016A&A...592A...2P ,
The XXL Survey. III. Luminosity-temperature relation of the bright cluster sample . Giles, P. A., Maughan, B. J., et all. . A&A . 592-3 . 2016 . 2016A&A...592A...3G ,
The XXL Survey . IV. Mass-temperature relation of the bright cluster sample . Lieu, M., Smith, G. P., et all. . A&A . 592-4 . 2016 . 2016A&A...592A...4L ,
The XXL Survey. VI. The 1000 brightest X-ray point sources . Fotopoulou, S., Pacaud, F., et all. . A&A . 592-5 . 2016 . 2016A&A...592A...5F ,
The XXL Survey. VII. A supercluster of galaxies at z = 0.43 . Pompei, E., Adami, C., et all. . A&A . 592-6 . 2016 . 2016A&A...592A...6P ,
The XXL Survey. VIII. MUSE characterisation of intracluster light in a z ~ 0.53 cluster of galaxies . Adami, C., Pompei, E., et all. . A&A . 592-7 . 2016 . 2016A&A...592A...7A ,
The XXL Survey. XIII. Ba...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2011-07-31T19:02:08Z/2011-08-01T04:10:50Z
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 2012-08-19T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2012-08-19T00:00:00Z, 067311, 17.56_20190403_1200. https://doi.org/10.5270/esa-157s9so