A dataset provided by the European Space Agency

Name: Testing Galaxy Formation Models with Massive Spiral Galaxies
Published: 2012-09-21T00:00:00Z

Proposal ID	067317
Title	Testing Galaxy Formation Models with Massive Spiral Galaxies
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673170101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673170201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673170301
DOI	https://doi.org/10.5270/esa-14flf3q
Principal Investigator, PI	Dr William Forman
Abstract	We propose to test galaxy formation models by characterizing the outer hotcoronae of two very massive spiral galaxies. Theoretical models predict X-rayemission (L_x>10^{40} ergs/s) at large radii around massive spiral galaxies.This emission is a fundamental prediction of current formation models thatsuccessfully predict many observed galaxy properties. We have selected twogalaxies, NGC1961 and NGC6753, that are optically luminous, undisturbed, withmoderate star formation rates, and that can be probed to sufficiently largeradii (25-50 kpc) within the large XMM FOV with 52ks and 64ks observations. Wewill derive the X-ray gas density profiles and the mean gas temperature of theextended, hot coronae for these two galaxies.
Publications	Hot X-Ray Coronae around Massive Spiral Galaxies: A Unique Probe of Structure Formation Models \|Bogdan Akos Forman William R. et al. \| ApJ \| 772-97 \| 2013 \| 2013ApJ...772...97B \| http://ui.adsabs.harvard.edu/#abs/2013ApJ...772...97B X-ray spectral variability of LINERs selected from the Palomar sample \|Hernandez-Garcia L. Gonzalez-Martin O. et al. \| A&A \| 569-26 \| 2014 \| 2014A&A...569A..26H \| http://ui.adsabs.harvard.edu/#abs/2014A&A...569A..26H Modulated X-ray emission of the magnetic O8.5V-star Tr16-22 \|Naze Yael Wade Gregg A. \| A&A \| 569-70 \| 2014 \| 2014A&A...569A..70N \| http://ui.adsabs.harvard.edu/#abs/2014A&A...569A..70N 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 Non-detection of X-ray emission from sterile neutrinos in stacked galaxy spectra \|Anderson Michael E. Churazov Eugene \| MNRAS \| 452-3905 \| 2015 \| 2015MNRAS.452.3905A \| http://ui.adsabs.harvard.edu/#abs/2015MNRAS.452.3905A A deep XMM-Newton study of the hot gaseous halo around NGC 1961 \|Anderson Michael E. Churazov Eugene \| MNRAS \| 455-227 \| 2016 \| 2016MNRAS.455..227A \| http://ui.adsabs.harvard.edu/#abs/2016MNRAS.455..227A Unveiling the Physics of Low-luminosity AGNs through X-Ray Variability: LINER versus Seyfert 2 \|Hernandez-Garcia L. Masegosa J. et al. \| ApJ \| 824-7 \| 2016 \| 2016ApJ...824....7H \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...824....7H 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 AGN spectral states from simultaneous UV and X-ray observations by XMM-Newton \|Svoboda J. Guainazzi M. \| A&A \| 603-127 \| 2017 \| 2017A&A...603A.127S \| http://ui.adsabs.harvard.edu/#abs/2017A&A...603A.127S 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 A new clean catalogue of extragalactic non-nuclear X-ray sources in nearby galaxies \|Earnshaw H. P. Roberts T. P. et al. \| MNRAS \| 483-5554 \| 2019 \| 2019MNRAS.483.5554E \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.483.5554E Hot gaseous atmospheres of rotating galaxies observed with XMM-Newton \|Juru00e1u0148ovu00e1 A. Werner N. et al. \| MNRAS \| 499-5163 \| 2020 \| 2020MNRAS.499.5163J \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.499.5163J 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 impact of precession on the observed population of ULXs \|Khan Norman Middleton Matthew J. et al. \| MNRAS \| 509-2493 \| 2022 \| 2022MNRAS.509.2493K \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.509.2493K The Redshift Evolution of Ultraluminous X-Ray Sources out to z 0.5: Comparison with X-Ray Binary Populations and Contribution to the Cosmic X-Ray Background \|Scott Barrows R. Comerford Julia M. et al. \| ApJ \| 932-27 \| 2022 \| 2022ApJ...932...27S \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...932...27S 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	2011-08-31T02:28:38Z/2012-04-22T02:49:27Z
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	2012-09-21T00:00:00Z
Last Update	2025-01-27
Keywords	"mean gas temperature", "massive spiral galaxy", "hot coronae", "successfully predict", "fundamental prediction", "galaxy properties", "outer hot coronae", "formation models", "optically luminous", "XMM", "NGC1961", "xmm fov"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr William Forman, 2012, 'Testing Galaxy Formation Models with Massive Spiral Galaxies', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-14flf3q