A dataset provided by the European Space Agency

Proposal ID 088310
Title Casting X-rays on a blue galaxy cluster with a red spiral BCG
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https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0883100101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0883100201

DOI https://doi.org/10.57780/esa-6jwkffz
Principal Investigator, PI Prof Yuanyuan Su
Abstract SDSS-C4 3028 is a cluster of galaxies identified in the Sloan Digital SkySurvey. It stands out as a nearby cluster containing a surprisingly largefraction of star forming galaxies, which is not fully understood in the standardmodel of galaxy evolution. It is also very unusual that the brightest galaxy ofthis cluster is a passive red spiral galaxy. We propose an XMM pointing thatcovers the entire cluster to determine its dynamical state and to obtain a morerobust cluster mass measurement. We will also verify whether this passive redspiral galaxy is the brightest cluster galaxy residing at the the bottom of thegravitational potential of this cluster. SDSS-C4 3028 provides a valuableopportunity to study the evolutionary link between galaxies and clusters.
Publications
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2021-11-10T07:23:35Z/2021-11-11T02:06:55Z
Version 19.16_20210326_1200
Mission Description The European Space Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs 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 Earths 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 2022-12-01T00:00:00Z
Keywords "standard model", "brightest galaxy", "SDSS", "gravitational potential", "XMM", "casting xray", "galaxy evolution", "evolutionary link", "blue galaxy cluster", "star forming galaxy", "red spiral bcg", "sdss c4 3028", "nearby cluster"
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Prof Yuanyuan Su, 2022, 'Casting X-rays on a blue galaxy cluster with a red spiral BCG', 19.16_20210326_1200, European Space Agency, https://doi.org/10.57780/esa-6jwkffz