A dataset provided by the European Space Agency

Name 090389
Title Galaxy groups as the ultimate probe of AGN feedback
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0903890901
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0903891701
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0903892301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0903892401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0903892701
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0903892801
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0903893001
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0903893601

DOI https://doi.org/10.57780/esa-7lagqm5
Author European Space Agency
Description Every major modern hydrodynamical simulation suite now includes a prescription
for AGN feedback to reproduce realistic populations of galaxies. However, these
simulations generally do not offer much insight into the nature of feedback. On
the other hand, the hot gas content of galaxy groups is highly sensitive to the
implemented feedback scheme: the predicted gas fraction differs by an order of
magnitude from one simulation to another. Here we propose to observe a sample of
40 galaxy groups exhibiting X-ray emission on scales >12., with the aim of
providing benchmark thermodynamic and gas fraction profiles out to R500 without
requiring any extrapolation. The proposed program will gather a well controlled
sample of systems spanning an order of magnitude in mass 1e13 < M500 < 1e14 Mo.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2022-05-05T04:24:36Z/2022-08-27T14:52:47Z
Version 20.08_20220509_1852
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 2023-09-15T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2023, Galaxy Groups As The Ultimate Probe Of Agn Feedback, 20.08_20220509_1852, European Space Agency, https://doi.org/10.57780/esa-7lagqm5