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
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
Keywords	"xray source populations", "stellar content", "XMM", "xray source population", "myr age range", "xmm newton", "magellanic cloud", "stellar generations", "star forming galaxy", "metallicity etc", "XMM-Newton", "faint xrbs"
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