A dataset provided by the European Space Agency

Name: The Evolution of Galaxies in Groups
Published: 2010-06-24T00:00:00Z

Proposal ID	060359
Title	The Evolution of Galaxies in Groups
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0603590101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0603590201
DOI	https://doi.org/10.5270/esa-3fnc2cx
Principal Investigator, PI	Dr John Mulchaey
Abstract	We propose to observe two fields from the CNOC2 redshift survey to study theevolution of galaxies in groups. The proposed observations will allow typicalX-ray groups to be discovered out to z=0.8. The unique aspect of our program isthat we have already identified a large sample of optically-selected groups inthese fields over the same redshift interval. The combination of the X-ray andoptically-selected samples will allow the construction of a sample spanning thefull range of dynamical states of groups.
Publications	Exploring the Diversity of Groups at 0.1 < z < 0.8 with X-Ray and Optically Selected Samples \|Connelly J. L. Wilman David J. et al. \| ApJ \| 756-139 \| 2012 \| 2012ApJ...756..139C \| http://ui.adsabs.harvard.edu/#abs/2012ApJ...756..139C An XMM-Newton Survey of the Soft X-Ray Background. II. An All-Sky Catalog of Diffuse O VII and O VIII Emission Intensities \|Henley David B. Shelton Robin L. \| ApJS \| 202-14 \| 2012 \| 2012ApJS..202...14H \| http://ui.adsabs.harvard.edu/#abs/2012ApJS..202...14H 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 The Interaction of the Fermi Bubbles with the Milky Ways Hot Gas Halo \|Miller Matthew J. Bregman Joel N. \| ApJ \| 829-9 \| 2016 \| 2016ApJ...829....9M \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...829....9M 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 A sensitive search for unknown spectral emission lines in the diffuse X-ray background with XMM-Newton \|Gewering-Peine A. Horns D. \| JCAP \| 6-36 \| 2017 \| 2017JCAP...06..036G \| http://ui.adsabs.harvard.edu/#abs/2017JCAP...06..036G AGN spectral states from simultaneous UV and X-ray observations by XMM-Newton \|Svoboda J. Guainazzi M. \| A&A \| 603-127 \| 2017 \| 2017A&A...603A.127S \| http://ui.adsabs.harvard.edu/#abs/2017A&A...603A.127S A luminous X-ray outburst from an intermediate-mass black hole in an off-centre star cluster \|Lin Dacheng Strader Jay et al. \| NatAs \| 2-656 \| 2018 \| 2018NatAs...2..656L \| http://ui.adsabs.harvard.edu/#abs/2018NatAs...2..656L Tidal Disruption of a Main-sequence Star by an Intermediate-mass Black Hole: A Bright Decade \|Chen Jin-Hong Shen Rong-Feng \| ApJ \| 867-20 \| 2018 \| 2018ApJ...867...20C \| http://ui.adsabs.harvard.edu/#abs/2018ApJ...867...20C Multiwavelength Follow-up of the Hyperluminous Intermediate-mass Black Hole Candidate 3XMM J215022.4-055108 \|Lin Dacheng Strader Jay et al. \| ApJ \| 892-25 \| 2020 \| 2020ApJ...892L..25L \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...892L..25L Elusive middle-weight black hole is caught shredding a star \|No authors \| Natur \| 580-307 \| 2020 \| 2020Natur.580Q.307. \| http://ui.adsabs.harvard.edu/#abs/2020Natur.580Q.307. An X-Ray- and SZ-bright Diffuse Source toward M31: A Local Hot Bridge \|Qu Zhijie Huang Rui et al. \| ApJ \| 907-14 \| 2021 \| 2021ApJ...907...14Q \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...907...14Q 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 Mass Spin and Ultralight Boson Constraints from the Intermediate-mass Black Hole in the Tidal Disruption Event 3XMM J215022.4-055108 \|Wen Sixiang Jonker Peter G. et al. \| ApJ \| 918-46 \| 2021 \| 2021ApJ...918...46W \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...918...46W The Solar Cycle Temporal Variation of the Solar Wind Charge Exchange X-Ray Lines \|Qu Zhijie Koutroumpa Dimitra et al. \| ApJ \| 930-21 \| 2022 \| 2022ApJ...930...21Q \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...930...21Q Strong constraints on decay and annihilation of dark matter from heating of gas-rich dwarf galaxies \|Wadekar Digvijay Wang Zihui \| PhRvD \| 106-75007 \| 2022 \| 2022PhRvD.106g5007W \| http://ui.adsabs.harvard.edu/#abs/2022PhRvD.106g5007W The XMM-Newton Line Emission Analysis Program (X-LEAP). I. Emission-line Survey of O VII O VIII and Fe L-shell Transitions \|Pan Zeyang Qu Zhijie et al. \| ApJS \| 271-62 \| 2024 \| 2024ApJS..271...62P \| http://ui.adsabs.harvard.edu/#abs/2024ApJS..271...62P From Active Stars to Black Holes: A Discovery Tool for Galactic X-Ray Sources \|Rodriguez Antonio C. \| PASP \| 136-054201 \| 2024 \| 2024PASP..136e4201R \| http://ui.adsabs.harvard.edu/#abs/2024PASP..136e4201R 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	2009-06-01T07:54:25Z/2009-06-08T06:22:24Z
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	2010-06-24T00:00:00Z
Keywords	"typical xray", "sample spanning", "cnoc2 redshift survey", "redshift interval"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr John Mulchaey, 2010, 'The Evolution of Galaxies in Groups', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-3fnc2cx