A dataset provided by the European Space Agency

Name 090275
Title Capturing the Missing Baryons with X-ray and Sunyaev-Zel.dovich Data
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0902750101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0902750201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0902750301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0902750401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0902750501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0902750601
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0902750701
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0902750801
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0902750901

DOI https://doi.org/10.57780/esa-ky6r3rp
Author European Space Agency
Description Stacking of SZ signals (Y) by stellar mass produces a significant signal, which
has been used to infer the halo gas mass of galaxies. Interpreting the stacked
signal assumes the Y distribution (at fixed M*) is narrow, symmetric, and for a
uniform sample of objects. These conditions are violated when stacking in
stellar mass bins, so one must understand the distribution of Y as a function of
galaxy environment (M*, gal/M*,tot). This cannot be obtained from the weak
individual SZ signals, but can be inferred from X-ray observations. We propose
to complete our X-ray studies of 15 nearby galaxies that were previously used in
a stack of SZ signals. We will measure the distribution of Y _X (X-ray analog
of SZ) to quantify the dependence of halo gas mass on galaxy environment.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2022-05-10T01:36:47Z/2023-01-23T09:43:19Z
Version 20.09_20221024_1724
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 2024-03-02T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2024, Capturing The Missing Baryons With X-Ray And Sunyaev-Zel.Dovich Data, 20.09_20221024_1724, European Space Agency, https://doi.org/10.57780/esa-ky6r3rp