|Title||New Candidates for Supernova Remnants in the Large Magellanic Cloud|
|Author||Dr Patrick Kavanagh|
|Description||We propose observations of new candidates for X-ray supernova remnants (SNRs) in the Large Magellanic Cloud (LMC). Building on a successful campaign to observe candidates with ROSAT detections in past AOs (Proposal IDs 65188, 72044, 74180, 76406), we have expanded our selection criteria to include candidates with multiwavelength signatures which have yet to be detected in X-rays. Owing to the high sensitivity of XMM-Newton we will be able to confirm new SNRs that are X-ray faint because of their age or ambient medium, complete the sample of known SNRs to lower flux levels, and obtain information about abundances, densities, and supernova energies.|
|Publication||The population of X-ray supernova remnants in the Large Magellanic Cloud . Maggi, P., Haberl, F., et all. . A&A . 585-162 . 2016 . 2016A&A...585A.162M ,
Identification of high-mass X-ray binaries selected from XMM-Newton observations of the LMC* . van Jaarsveld, N., Buckley, D. A. H., et all. . MNRAS . 475-3253 . 2018 . 2018MNRAS.475.3253V ,
X-Ray Luminosity and Size Relationship of Supernova Remnants in the LMC . Ou, Po-Sheng, Chu, You-Hua, et all. . ApJ . 863-137 . 2018 . 2018ApJ...863..137O ,
New optically identified supernova remnants in the Large Magellanic Cloud . Yew, Miranda, Filipoviu0107, Miroslav D., et all. . MNRAS . 500-2336 . 2021 . 2021MNRAS.500.2336Y ,
|Instrument||EMOS1, EMOS2, EPN, OM, RGS1, RGS2|
|Mission Description||The European Space Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's 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 Earth's 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.
|Publisher And Registrant||European Space Agency|
|Credit Guidelines||European Space Agency, 2018-11-14T23:00:00Z, 080199, 17.56_20190403_1200. https://doi.org/10.5270/esa-8grrsq2|