We propose EPIC observations to survey a virgul10 square degree area of the LMC downto a limiting point source luminosity of 2 x 10^33 erg/s. Its proximity makesthe LMC the ultimate target for obtaining a complete inventory of SNRs, X-raybinaries and SSSs, and to study the diffuse emission of the hot ISM. Most im-portantly, the high throughput of XMM-Newton will allow us to perform detailedspectral and temporal analyses of a large fraction of sources. Together with theexisting EPIC data, our observations will create a unique data set to study thestar-formation history and its implications on the morphology of the ISM in theLMC. In combination with the existing surveys of the SMC, M31 and M33 this willyield important clues for the evolution of the Local Group as a whole.
Publications
Multi-frequency study of supernova remnants in the Large Magellanic Cloud. Confirmation of the supernova remnant status of DEM L205 |Maggi, P., Haberl, F., et al. | A&A | 546-109 | 2012 | 2012A&A...546A.109M | http://ui.adsabs.harvard.edu/#abs/2012A&A...546A.109M
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
New optically identified supernova remnants in the Large Magellanic Cloud |Yew, Miranda, Filipovi\\u0107, Miroslav D., et al. | MNRAS | 500-2336 | 2021 | 2021MNRAS.500.2336Y | http://ui.adsabs.harvard.edu/#abs/2021MNRAS.500.2336Y
The VLT-FLAMES survey of massive stars. NGC 2004#115: A triple system hosting a possible short period B+BH binary |Lennon, D. J., Dufton, P. L., et al. | A&A | 665-180 | 2022 | 2022A&A...665A.180L | http://ui.adsabs.harvard.edu/#abs/2022A&A...665A.180L
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
2011-12-19T20:41:35Z/2012-04-30T08:08:59Z
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.
European Space Agency, Dr Frank Haberl, 2013, 'A survey of the Large Magellanic Cloud - I', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-ndk4ega
