A dataset provided by the European Space Agency

Name: Galaxy evolution in the large scale structure around a PISCES galaxy cluster
Published: 2011-05-15T00:00:00Z

Proposal ID	060206
Title	Galaxy evolution in the large scale structure around a PISCES galaxy cluster
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0602060101
DOI	https://doi.org/10.5270/esa-qk5ximt
Principal Investigator, PI	Dr Ben Maughan
Abstract	The effect of environment is an essential, but poorly understood ingredient ingalaxy formation. We propose to measure the gas and dark matter in the clumpsand filaments around two massive distant galaxy clusters. By combining highquality XMM data with our existing wide-field optical-NIR imaging andspectroscopy we will perform a census of the baryons in the large scalestructure around these clusters and measure the effects of environment on thefundamental physical properties of the member galaxies. Combined with a stackedweak lensing analysis, the X-ray data will be used to perform the first test ofthe galaxy group mass-observable scaling relations in an LSS environment,thereby probing the role of environment on preheating in groups.
Publications	The dark matter distribution in z ~ 0.5 clusters of galaxies. I. Determining scaling relations with weak lensing masses \|Foex G. Soucail G. et al. \| A&A \| 546-106 \| 2012 \| 2012A&A...546A.106F \| http://ui.adsabs.harvard.edu/#abs/2012A&A...546A.106F 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 \| http://ui.adsabs.harvard.edu/#abs/2014Ap&SS.354...97Y XMM-Newton publication statistics \|Ness J.-U. Parmar A. N. et al. \| AN \| 335-210 \| 2014 \| 2014AN....335..210N \| http://ui.adsabs.harvard.edu/#abs/2014AN....335..210N Ensemble X-ray variability of active galactic nuclei. II. Excess variance and updated structure function \|Vagnetti F. Middei R. et al. \| A&A \| 593-55 \| 2016 \| 2016A&A...593A..55V \| http://ui.adsabs.harvard.edu/#abs/2016A&A...593A..55V The Million Optical - Radio/X-ray Associations (MORX) Catalogue \|Flesch Eric W. \| PASA \| 33-52 \| 2016 \| 2016PASA...33...52F \| http://ui.adsabs.harvard.edu/#abs/2016PASA...33...52F Comparison of hydrostatic and dynamical masses of distant X-ray luminous galaxy clusters \|Foex G. Bohringer H. \| A&A \| 606-122 \| 2017 \| 2017A&A...606A.122F \| http://ui.adsabs.harvard.edu/#abs/2017A&A...606A.122F Classification of 4XMM-DR9 sources by machine learning \|Zhang Yanxia Zhao Yongheng \| MNRAS \| 503-5263 \| 2021 \| 2021MNRAS.503.5263Z \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.503.5263Z A study of the Sunyaev-Zeldovich increment using archival SCUBA data \|Zemcov Michael Borys Colin et al. \| MNRAS \| 376-1073 \| 2007 \| 2007MNRAS.376.1073Z \| http://ui.adsabs.harvard.edu/#abs/2007MNRAS.376.1073Z Robust constraints on feebly interacting particles using XMM-Newton \|Luque Pedro De la Torre Balaji Shyam \| PhRvD \| 109-L101305 \| 2024 \| 2024PhRvD.109j1305L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j1305L Multimessenger search for electrophilic feebly interacting particles from supernovae \|Luque Pedro De la Torre Balaji Shyam \| PhRvD \| 109-103028 \| 2024 \| 2024PhRvD.109j3028L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j3028L Importance of Cosmic-Ray Propagation on Sub-GeV Dark Matter Constraints \|De la Torre Luque Pedro Balaji Shyam \| ApJ \| 968-46 \| 2024 \| 2024ApJ...968...46D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...968...46D
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2010-04-17T08:00:59Z/2010-04-17T20:53:39Z
Version	17.56_20190403_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	2011-05-15T00:00:00Z
Keywords	"thereby probing", "galaxy evolution", "xray data", "dark matter", "quality xmm data", "XMM", "scale structure", "galaxy formation", "pisces galaxy cluster", "fundamental physical properties"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Ben Maughan, 2011, 'Galaxy evolution in the large scale structure around a PISCES galaxy cluster', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-qk5ximt