A dataset provided by the European Space Agency

Name: X-ray Coronae Around Massive Spirals: Probing Galaxy Formation Models
Published: 2015-08-25T22:00:00Z

Proposal ID	074322
Title	X-ray Coronae Around Massive Spirals: Probing Galaxy Formation Models
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0743220101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0743220201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0743220301
DOI	https://doi.org/10.5270/esa-0haty7q
Principal Investigator, PI	Dr Akos Bogdan
Abstract	Although the presence of hot X-ray coronae around massive spiral galaxies is afundamental prediction of galaxy formation models, the study of these coronaehas just begun. We propose observations of two spirals, which are opticallyluminous, undisturbed, and have low star formation rates. We will trace thecoronae to unprecedentedly large radii, derive their luminosity and metallicity,determine surface brightness, gas density, gas temperature profiles, and computebaryon mass fractions. These observations will be confronted with galaxyformation models, which will allow us to test AGN and SN feedback models,investigate the importance of galactic winds, and constrain the metal-loading bygalactic outflows.
Publications	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 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	2014-06-07T01:18:33Z/2014-07-28T02:54:25Z
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	2015-08-25T22:00:00Z
Keywords	"optically luminous", "fundamental prediction", "galactic winds", "gas temperature profiles", "surface brightness", "metal loading", "hot xray coronae", "galaxy formation models", "gas density", "massive spiral galaxy", "galactic outflows", "x ray coronae", "massive spirals"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Akos Bogdan, 2015, 'X-ray Coronae Around Massive Spirals: Probing Galaxy Formation Models', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-0haty7q