A dataset provided by the European Space Agency

Name: How do the most massive BHs grow
Published: 2018-03-29T22:00:00Z

Proposal ID	079278
Title	How do the most massive BHs grow
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0792780101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0792780201
DOI	https://doi.org/10.5270/esa-l51sqgg
Principal Investigator, PI	Dr Akos Bogdan
Abstract	The BH masses of brightest cluster galaxies exhibit a steeper M BH a?? sigmarelation than their lower mass counterparts. Are these BHs different because ofthe deep gravitational potential and the rich environment they live in? How dothe most massive BHs grow? The definite test to answer these questions is tomeasure BH masses, galaxy properties, and halo properties of massive cluster andisolated ellipticals, and confront these results with cosmological simulations.However, we lack the sufficient halo mass measurements for massive isolatedellipticals. We request Chandra and XMM-Newton observations of two massiveisolated galaxies, NGC890 and NGC7052, with available BH mass measurements tocharacterize their dark matter halo properties.
Publications	Correlation between the Total Gravitating Mass of Groups and Clusters and the Supermassive Black Hole Mass of Brightest Galaxies \|Bogdan Akos Lovisari Lorenzo et al. \| ApJ \| 852-131 \| 2018 \| 2018ApJ...852..131B \| http://ui.adsabs.harvard.edu/#abs/2018ApJ...852..131B Black hole mass of central galaxies and cluster mass correlation in cosmological hydro-dynamical simulations \|Bassini L. Rasia E. et al. \| A&A \| 630-144 \| 2019 \| 2019A&A...630A.144B \| http://ui.adsabs.harvard.edu/#abs/2019A&A...630A.144B 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 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	2016-10-30T19:19:15Z/2017-01-15T06:28:48Z
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	2018-03-29T22:00:00Z
Last Update	2025-01-27
Keywords	"definite test", "deep gravitational potential", "massive cluster", "xmm newton", "cosmological simulations", "lower mass counterparts", "halo mass measurements", "galaxy properties", "massive isolated galaxy", "massive bhs grow", "massive isolated ellipticals", "XMM-Newton", "isolated ellipticals", "bh masses", "NGC890", "sigma relation", "halo properties", "XMM", "bh mass measurements"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Akos Bogdan, 2018, 'How do the most massive BHs grow', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-l51sqgg