A dataset provided by the European Space Agency

Name 086264
Title Studying the Progenitors of Our Favorite Clusters at z>1
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0862640101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0862640201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0862640301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0862640401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0862640501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0862640601
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0862640701
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0862640801
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0862640901
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0862641001
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0862641101
...
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0862641201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0862641301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0862641401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0862641501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0862641601

DOI https://doi.org/10.57780/esa-axdu4mw
Author European Space Agency
Description Surveys in the 2020s, notably the CMB-S4 program and Athena, will reveal galaxy
clusters at high redshifts, all the way back to zvirgul3, when they first formed.
Unveiling the properties (density, temperature, entropy, metallicity) and
evolution of the intracluster medium and the galaxy-halo connection in these
early-forming systems will be among the primary science goals of both Athena and
any Chandra successor. While many of the most exciting questions about the
initial formation of galaxy clusters must wait for next-generation X-ray
missions, we can lay an important foundation now by extending studies of
statistical cluster samples into the z>1 regime.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2020-05-01T18:55:00Z/2020-11-21T21:56:54Z
Version 18.02_20200221_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 2021-12-16T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2021, Studying The Progenitors Of Our Favorite Clusters At Z&Amp;Gt;1, 18.02_20200221_1200, European Space Agency, https://doi.org/10.57780/esa-axdu4mw