A dataset provided by the European Space Agency

Name: Most of the Baryons in Galaxies
Published: 2010-01-17T00:00:00Z

Proposal ID	055387
Title	Most of the Baryons in Galaxies
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0553870101
DOI	https://doi.org/10.5270/esa-312e3zk
Principal Investigator, PI	Prof JOEL BREGMAN
Abstract	Galaxies are missing most of their baryons when compared to the cosmologicalbaryon to dark matter ratio. The Milky Way is missing 2/3 of its baryons andless massive galaxies have retained less than 10% of their baryons. Theorysuggests that these baryons were expelled by intense galactic winds during theprimary star formation period. These galactic winds carry gas far beyond thevirial radius of small and modest galaxies, but the most massive galaxies shouldretain much of this material. e propose to test this picture by searching forthe missing baryons surrounding the most massive spiral galaxy, UGC 12591, afairly isolated galaxy with a rotational velocity of almost 500 km/sec. Ifsuccessful, we will detect a significant fraction of the 5E11 Msun of its missing baryons.
Publications	Exospheric solar wind charge exchange as seen by XMM-Newton \|Carter J. A. Semba S. \| AN \| 333-313 \| 2012 \| 2012AN....333..313C \| http://ui.adsabs.harvard.edu/#abs/2012AN....333..313C The cosmological analysis of X-ray cluster surveys - II. Application of the CR-HR method to the XMM archive \|Clerc N. Sadibekova T. et al. \| MNRAS \| 423-3561 \| 2012 \| 2012MNRAS.423.3561C \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.423.3561C XMM-Newton Detects a Hot Gaseous Halo in the Fastest Rotating Spiral Galaxy UGC 12591 \|Dai Xinyu Anderson Michael E. et al. \| ApJ \| 755-107 \| 2012 \| 2012ApJ...755..107D \| http://ui.adsabs.harvard.edu/#abs/2012ApJ...755..107D An XMM-Newton Survey of the Soft X-Ray Background. II. An All-Sky Catalog of Diffuse O VII and O VIII Emission Intensities \|Henley David B. Shelton Robin L. \| ApJS \| 202-14 \| 2012 \| 2012ApJS..202...14H \| http://ui.adsabs.harvard.edu/#abs/2012ApJS..202...14H 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 Statistical properties of dwarf novae-type cataclysmic variables: the outburst catalogue \|Coppejans Deanne L. Kording Elmar G. et al. \| MNRAS \| 456-4441 \| 2016 \| 2016MNRAS.456.4441C \| http://ui.adsabs.harvard.edu/#abs/2016MNRAS.456.4441C The Interaction of the Fermi Bubbles with the Milky Ways Hot Gas Halo \|Miller Matthew J. Bregman Joel N. \| ApJ \| 829-9 \| 2016 \| 2016ApJ...829....9M \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...829....9M SPIDERS: the spectroscopic follow-up of X-ray selected clusters of galaxies in SDSS-IV \|Clerc N. Merloni A. et al. \| MNRAS \| 463-4490 \| 2016 \| 2016MNRAS.463.4490C \| http://ui.adsabs.harvard.edu/#abs/2016MNRAS.463.4490C 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 The Circum-Galactic Medium of Massive Spirals. II. Probing the Nature of Hot Gaseous Halo around the Most Massive Isolated Spiral Galaxies \|Li Jiang-Tao Bregman Joel N. et al. \| ApJS \| 233-20 \| 2017 \| 2017ApJS..233...20L \| http://ui.adsabs.harvard.edu/#abs/2017ApJS..233...20L Baryon Budget of the Hot Circumgalactic Medium of Massive Spiral Galaxies \|Li Jiang-Tao Bregman Joel N. et al. \| ApJ \| 855-24 \| 2018 \| 2018ApJ...855L..24L \| http://ui.adsabs.harvard.edu/#abs/2018ApJ...855L..24L A Study of X-Ray Emission of Galaxies Hosting Molecular Outflows (MOX Sample) \|Laha Sibasish Guainazzi Matteo et al. \| ApJ \| 868-10 \| 2018 \| 2018ApJ...868...10L \| http://ui.adsabs.harvard.edu/#abs/2018ApJ...868...10L X-ray properties of the X-CLASS-redMaPPer galaxy cluster sample: the luminosity-temperature relation \|Molham Mona Clerc Nicolas et al. \| MNRAS \| 494-161 \| 2020 \| 2020MNRAS.494..161M \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.494..161M X-ray signatures of black hole feedback: hot galactic atmospheres in IllustrisTNG and X-ray observations \|Truong Nhut Pillepich Annalisa et al. \| MNRAS \| 494-549 \| 2020 \| 2020MNRAS.494..549T \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.494..549T Multiwavelength classification of X-ray selected galaxy cluster candidates using convolutional neural networks \|Kosiba Matej Lieu Maggie et al. \| MNRAS \| 496-4141 \| 2020 \| 2020MNRAS.496.4141K \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.496.4141K SPIDERS: overview of the X-ray galaxy cluster follow-up and the final spectroscopic data release \|Clerc N. Kirkpatrick C. C. et al. \| MNRAS \| 497-3976 \| 2020 \| 2020MNRAS.497.3976C \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.497.3976C An X-Ray- and SZ-bright Diffuse Source toward M31: A Local Hot Bridge \|Qu Zhijie Huang Rui et al. \| ApJ \| 907-14 \| 2021 \| 2021ApJ...907...14Q \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...907...14Q 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 Solar Cycle Temporal Variation of the Solar Wind Charge Exchange X-Ray Lines \|Qu Zhijie Koutroumpa Dimitra et al. \| ApJ \| 930-21 \| 2022 \| 2022ApJ...930...21Q \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...930...21Q 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	2008-12-15T19:26:50Z/2008-12-16T17:36:19Z
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	2010-01-17T00:00:00Z
Last Update	2025-01-27
Keywords	"virial radius", "ugc 12591", "massive spiral galaxy", "fairly isolated galaxy", "massive galaxy", "intense galactic winds", "modest galaxy", "dark matter ratio", "rotational velocity", "cosmological baryon", "5e11 msun"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Prof JOEL BREGMAN, 2010, 'Most of the Baryons in Galaxies', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-312e3zk