A dataset provided by the European Space Agency

Name: A Complete X-ray Selected Sample of Galaxy Groups
Published: 2013-03-27T00:00:00Z

Proposal ID	067035
Title	A Complete X-ray Selected Sample of Galaxy Groups
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0670350101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0670350201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0670350301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0670350401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0670350501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0670350701 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0670351201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0670351301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0670351401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0670351501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0670351601 ... https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0670351701
DOI	https://doi.org/10.5270/esa-g0a4wyx
Principal Investigator, PI	Dr John Mulchaey
Abstract	We propose an XMM-Newton survey of a complete X-ray selected sample of nearbygalaxy groups. The groups have been selected to overlap with the Sloan DigitalSky Survey. The XMM observations will provide a vital comparison sample to X-rayselected group samples being studied at high redshift. We will use the XMMobservations to: 1) Determine the properties of the intragroup medium in arepresentative sample of X-ray groups; 2) Study the evolution of the galaxypopulation in X-ray groups from z=1 to the present; 3) Determine the formationtimescales of brightest group galaxies and 4) Compare the AGN populations inX-ray groups to clusters.
Publications	A volume-limited sample of X-ray galaxy groups and clusters - I. Radial entropy and cooling time profiles \|Panagoulia, E. K., Fabian, A. C., \| MNRAS \| 438-2341 \| 2014 \| 2014MNRAS.438.2341P \| http://ui.adsabs.harvard.edu/#abs/2014MNRAS.438.2341P 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 The Tight Relation between X-Ray and Ultraviolet Luminosity of Quasars \|Lusso, E., Risaliti, G., \| ApJ \| 819-154 \| 2016 \| 2016ApJ...819..154L \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...819..154L A volume-limited sample of X-ray galaxy groups and clusters - II. X-ray cavity dynamics \|Panagoulia, E. K., Fabian, A. C., et al. \| MNRAS \| 444-1236 \| 2014 \| 2014MNRAS.444.1236P \| http://ui.adsabs.harvard.edu/#abs/2014MNRAS.444.1236P 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 Connecting optical and X-ray tracers of galaxy cluster relaxation \|Roberts, Ian D., Parker, Laura C., \| MNRAS \| 475-4704 \| 2018 \| 2018MNRAS.475.4704R \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.475.4704R The non-uniformity of galaxy cluster metallicity profiles \|Lovisari, L., Reiprich, T. H., \| MNRAS \| 483-540 \| 2019 \| 2019MNRAS.483..540L \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.483..540L A Comparison of X-Ray Photon Indices among the Narrow- and Broad-line Seyfert 1 Galaxies \|Ojha, Vineet, Chand, Hum, et al. \| ApJ \| 896-95 \| 2020 \| 2020ApJ...896...95O \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...896...95O A Luminous X-Ray Transient in SDSS J143359.16+400636.0: A Likely Tidal Disruption Event \|Brightman, Murray, Ward, Charlotte, et al. \| ApJ \| 909-102 \| 2021 \| 2021ApJ...909..102B \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...909..102B On the Reliability of Photometric and Spectroscopic Tracers of Halo Relaxation \|Zhoolideh Haghighi, Mohammad H., Raouf, Mojtaba, et al. \| ApJ \| 904-36 \| 2020 \| 2020ApJ...904...36Z \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...904...36Z The composite X-ray spectra of radio-loud and radio-quiet SDSS quasars \|Zhou, Min-Hua, Gu, Min-Feng, \| RAA \| 21-4 \| 2021 \| 2021RAA....21....4Z \| http://ui.adsabs.harvard.edu/#abs/2021RAA....21....4Z 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 X-ray emission from a rapidly accreting narrow-line Seyfert 1 galaxy at z = 6.56 \|Wolf, J., Nandra, K., et al. \| A&A \| 669-127 \| 2023 \| 2023A&A...669A.127W \| http://ui.adsabs.harvard.edu/#abs/2023A&A...669A.127W 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	2011-12-27T14:38:37Z/2012-02-27T15:39:57Z
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	2013-03-27T00:00:00Z
Keywords	"complete xray", "galaxy population", "XMM", "intragroup medium", "xmm newton survey", "vital comparison sample", "nearby galaxy", "agn populations", "XMM-Newton", "formation timescales"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr John Mulchaey, 2013, 'A Complete X-ray Selected Sample of Galaxy Groups', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-g0a4wyx