A dataset provided by the European Space Agency

Name: Scaling Properties and the Effects of Feedback for a Complete Sample of Groups
Published: 2016-04-24T22:00:00Z

Proposal ID	074158
Title	Scaling Properties and the Effects of Feedback for a Complete Sample of Groups
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DOI	https://doi.org/10.5270/esa-yrv7jdo
Principal Investigator, PI	Dr Lorenzo Lovisari
Abstract	Upcoming X-ray surveys like eROSITA, require precise calibration between X-rayobservables and mass, down to the low-mass regime to set tight constraints onthe cosmological parameters. We propose to observe 17 galaxy groups to completeobservations for a flux limited sample consisting of 69 objectss. We will usethe sample to study the scaling properties of the low-mass systems with a viewto the eROSITA survey which is expected to detect 100,000 objects, most of themin the low mass regime. Thanks to the completeness and the size of the selectedsample we will correct for selection biases the observed scaling relations.Furthermore, we will investigate the relative importance of non-gravitationalprocesses by studying their thermodynamical properties beyond R1000.
Publications	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 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 pre-merger stage galaxy cluster: Abell 3733 \|Kaya, H. Ilker, Caglar, Turgay, \| MNRAS \| 485-4550 \| 2019 \| 2019MNRAS.485.4550K \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.485.4550K Projection effects in galaxy cluster samples: insights from X-ray redshifts \|Ramos-Ceja, M. E., Pacaud, F., et al. \| A&A \| 626-48 \| 2019 \| 2019A&A...626A..48R \| http://ui.adsabs.harvard.edu/#abs/2019A&A...626A..48R Building a cluster: shocks, cavities, and cooling filaments in the group-group merger NGC 6338 \|O.Sullivan, Ewan, Schellenberger, Gerrit, et al. \| MNRAS \| 488-2925 \| 2019 \| 2019MNRAS.488.2925O \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.488.2925O Probing cosmic isotropy with a new X-ray galaxy cluster sample through the LX-T scaling relation \|Migkas, K., Schellenberger, G., et al. \| A&A \| 636-15 \| 2020 \| 2020A&A...636A..15M \| http://ui.adsabs.harvard.edu/#abs/2020A&A...636A..15M Discrete X-Ray Sources in Galaxy Clusters \|Tugay, A. V., Zadorozhna, L. V., \| OAP \| 33-22 \| 2020 \| 2020OAP....33...22T \| http://ui.adsabs.harvard.edu/#abs/2020OAP....33...22T 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 AT 2019avd: a novel addition to the diverse population of nuclear transients \|Malyali, A., Rau, A., et al. \| A&A \| 647-9 \| 2021 \| 2021A&A...647A...9M \| http://ui.adsabs.harvard.edu/#abs/2021A&A...647A...9M 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 Cosmological implications of the anisotropy of ten galaxy cluster scaling relations \|Migkas, K., Pacaud, F., et al. \| A&A \| 649-151 \| 2021 \| 2021A&A...649A.151M \| http://ui.adsabs.harvard.edu/#abs/2021A&A...649A.151M An XMM-Newton Early-type Galaxy Atlas \|Islam, Nazma, Kim, Dong-Woo, et al. \| ApJS \| 256-22 \| 2021 \| 2021ApJS..256...22I \| http://ui.adsabs.harvard.edu/#abs/2021ApJS..256...22I The Cosmic Large-Scale Structure in X-rays (CLASSIX) Cluster Survey. IV. Superclusters in the local Universe at z \\u2264 0.03 \|B\\u00f6hringer, Hans, Chon, Gayoung, \| A&A \| 656-144 \| 2021 \| 2021A&A...656A.144B \| http://ui.adsabs.harvard.edu/#abs/2021A&A...656A.144B The Planck clusters in the LOFAR sky. I. LoTSS-DR2: New detections and sample overview \|Botteon, A., Shimwell, T. W., et al. \| A&A \| 660-78 \| 2022 \| 2022A&A...660A..78B \| http://ui.adsabs.harvard.edu/#abs/2022A&A...660A..78B Dynamical state of galaxy clusters evaluated from X-ray images \|Yuan, Z. S., Han, J. L., \| MNRAS \| 513-3013 \| 2022 \| 2022MNRAS.513.3013Y \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.513.3013Y The alignment between brightest cluster galaxies and host clusters \|Yuan, Z. S., Wen, Z. L., \| MNRAS \| 516-3159 \| 2022 \| 2022MNRAS.516.3159Y \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.516.3159Y The X-ray view of optically selected dual AGN \|De Rosa, Alessandra, Vignali, Cristian, et al. \| MNRAS \| 519-5149 \| 2023 \| 2023MNRAS.519.5149D \| http://ui.adsabs.harvard.edu/#abs/2023MNRAS.519.5149D The Planck clusters in the LOFAR sky. III. LoTSS-DR2: Dynamic states and density fluctuations of the intracluster medium \|Zhang, X., Simionescu, A., et al. \| A&A \| 672-42 \| 2023 \| 2023A&A...672A..42Z \| http://ui.adsabs.harvard.edu/#abs/2023A&A...672A..42Z The Planck clusters in the LOFAR sky. IV. LoTSS-DR2: Statistics of radio haloes and re-acceleration models \|Cassano, R., Cuciti, V., et al. \| A&A \| 672-43 \| 2023 \| 2023A&A...672A..43C \| http://ui.adsabs.harvard.edu/#abs/2023A&A...672A..43C X\\u2011HESS: A large sample of highly accreting serendipitous AGN under the XMM\\u2011Newton microscope \|Laurenti, M., Tombesi, F., et al. \| AN \| 344-20230053 \| 2023 \| 2023AN....34430053L \| http://ui.adsabs.harvard.edu/#abs/2023AN....34430053L More relaxed intracluster gas than galaxies in clusters in quasi-equilibrium \|Yuan, Z. S., Han, J. L., et al. \| MNRAS \| 523-1364 \| 2023 \| 2023MNRAS.523.1364Y \| http://ui.adsabs.harvard.edu/#abs/2023MNRAS.523.1364Y The effect of cluster dynamical state on ram-pressure stripping \|Louren\\u00e7o, Ana C. C., Jaff\\u00e9, Y. L., et al. \| MNRAS \| 526-4831 \| 2023 \| 2023MNRAS.526.4831L \| http://ui.adsabs.harvard.edu/#abs/2023MNRAS.526.4831L Distribution of Merging and Post-merger Galaxies in Nearby Galaxy Clusters \|Kim, Duho, Sheen, Yun-Kyeong, et al. \| ApJ \| 966-124 \| 2024 \| 2024ApJ...966..124K \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...966..124K 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	2014-10-10T08:17:28Z/2015-04-08T14:54:39Z
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	2016-04-24T22:00:00Z
Keywords	"require precise calibration", "thermodynamical properties", "cosmological parameters", "scaling relations", "scaling properties", "selection biases", "relative importance", "low mass systems", "000 objects", "erosita survey", "set tight constraints", "xray observables", "gravitational processes", "xray surveys", "low mass regime"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Lorenzo Lovisari, 2016, 'Scaling Properties and the Effects of Feedback for a Complete Sample of Groups', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-yrv7jdo