A dataset provided by the European Space Agency

Name: Unlocking the Mysteries of Hot Gaseous Coronae: A Legacy Study of NGC 6753
Published: 2017-04-27T22:00:00Z

Proposal ID	078243
Title	Unlocking the Mysteries of Hot Gaseous Coronae: A Legacy Study of NGC 6753
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0782430101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0782430201
DOI	https://doi.org/10.5270/esa-epgxicy
Principal Investigator, PI	Dr Akos Bogdan
Abstract	Hot gaseous coronae in the dark matter halos of present day massive galaxies arethe fundamental prediction of galaxy formation models. Although the firstcoronae around massive spirals have recently been detected, these data onlyallow us to measure their basic properties and carry notable systematicuncertainties. We propose a deep XMM-Newton observation of NGC6753. We will (1)establish the temperature and metallicity structure of the gas, (2) utilizecomplex spectral models, thereby removing the systematic uncertainties, and (3)constrain the baryon mass fraction. Thus, we will place robust constraints onstate-of-the-art galaxy formation models, and probe the physical processes thatplay a crucial role in galaxy evolution.
Publications	Probing the Hot X-Ray Corona around the Massive Spiral Galaxy NGC 6753 Using Deep XMM-Newton Observations \|Bogdan Akos Bourdin Herve et al. \| ApJ \| 850-98 \| 2017 \| 2017ApJ...850...98B \| http://ui.adsabs.harvard.edu/#abs/2017ApJ...850...98B 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	2016-04-12T04:41:58Z/2016-04-15T11:08:27Z
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	2017-04-27T22:00:00Z
Last Update	2025-01-27
Keywords	"basic properties", "massive spirals", "fundamental prediction", "galaxy evolution", "NGC 6753", "galaxy formation models", "hot gaseous coronae", "thereby removing", "dark matter halos", "complex spectral models", "XMM-Newton", "baryon mass fraction", "ngc 6753", "robust constraints", "systematic uncertainties", "physical processes", "massive galaxy", "XMM", "deep xmm newton", "metallicity structure"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Akos Bogdan, 2017, 'Unlocking the Mysteries of Hot Gaseous Coronae: A Legacy Study of NGC 6753', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-epgxicy