A dataset provided by the European Space Agency

Name: The X-ray source population of different stellar generations in the LMC
Published: 2014-02-28T00:00:00Z

Proposal ID	069345
Title	The X-ray source population of different stellar generations in the LMC
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0693450201
DOI	https://doi.org/10.5270/esa-0lnsbka
Principal Investigator, PI	Dr Vallia Antoniou
Abstract	We propose XMM-Newton observations of 6 regions of the Large Magellanic Cloudwith the strongest clean star-formation (SF) episodes in the ~6-50 Myr agerange. These observations will probe the X-ray source populations in regions ofdifferent stellar content down to a luminosity of ~10^33 erg/s in our neareststar-forming galaxy thus addressing their dependence on their parent stellarpopulations (starburst age, metallicity etc.) The proposed observations willcomplement previous X-ray studies of the LMC and investigations in othergalaxies where these faint XRBs cannot be observed.
Publications	The population of X-ray supernova remnants in the Large Magellanic Cloud \|Maggi P. Haberl F. et al. \| A&A \| 585-162 \| 2016 \| 2016A&A...585A.162M \| http://ui.adsabs.harvard.edu/#abs/2016A&A...585A.162M 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 Identification of high-mass X-ray binaries selected from XMM-Newton observations of the LMC* \|van Jaarsveld N. Buckley D. A. H. et al. \| MNRAS \| 475-3253 \| 2018 \| 2018MNRAS.475.3253V \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.475.3253V X-Ray Luminosity and Size Relationship of Supernova Remnants in the LMC \|Ou Po-Sheng Chu You-Hua et al. \| ApJ \| 863-137 \| 2018 \| 2018ApJ...863..137O \| http://ui.adsabs.harvard.edu/#abs/2018ApJ...863..137O Discovery of an u223c30-yr-duration post-nova pulsating supersoft source in the Large Magellanic Cloud \|Vasilopoulos G. Koliopanos F. et al. \| MNRAS \| 499-2007 \| 2020 \| 2020MNRAS.499.2007V \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.499.2007V New optically identified supernova remnants in the Large Magellanic Cloud \|Yew Miranda Filipoviu0107 Miroslav D. et al. \| MNRAS \| 500-2336 \| 2021 \| 2021MNRAS.500.2336Y \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.500.2336Y 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 Discovery of four super-soft X-ray sources in XMM-Newton observations of the Large Magellanic Cloud \|Maitra C. Haberl F. \| A&A \| 657-26 \| 2022 \| 2022A&A...657A..26M \| http://ui.adsabs.harvard.edu/#abs/2022A&A...657A..26M 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 New 511 keV Line Data Provide Strongest sub-GeV Dark Matter Constraints \|De la Torre Luque Pedro Balaji Shyam \| ApJ \| 973-L6 \| 2024 \| 2024ApJ...973L...6D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...973L...6D
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2013-02-09T12:51:12Z/2013-02-10T00:41:29Z
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	2014-02-28T00:00:00Z
Last Update	2025-08-04
Keywords	"XMM", "XMM-Newton", "stellar content", "magellanic cloud", "xmm newton", "stellar generations", "faint xrbs", "myr age range", "star forming galaxy", "xray source population", "xray source populations", "metallicity etc"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Vallia Antoniou, 2014, 'The X-ray source population of different stellar generations in the LMC', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-0lnsbka