A dataset provided by the European Space Agency

Name 087087
Title The X-ray source population of different stellar generations in the LMC
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0870870201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0870870301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0870870401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0870870501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0870870601
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0870870701
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0870870801
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0870870901

DOI https://doi.org/10.5270/esa-[xxxxxxx]
Author Dr Vallia Antoniou
Description We propose XMM-Newton observations of 6 regions of the Large Magellanic Cloud with the strongest "clean" star-formation (SF) episodes in the virgul6-50 Myr age range. These observations will probe the X-ray source populations in regions of different stellar content down to a luminosity of virgul10^33 erg-s in our nearest star-forming galaxy thus addressing their dependence on their parent stellar populations (starburst age, metallicity etc.) The proposed observations will complement previous X-ray studies of the LMC and investigations in other galaxies where these faint XRBs cannot be observed.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2020-10-25T08:55:34Z/2021-04-29T04:36:15Z
Version 19.16_20210326_1200
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.
Creator Contact https://www.cosmos.esa.int/web/xmm-newton/xmm-newton-helpdesk
Date Published 2022-05-27T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2022-05-27T00:00:00Z, 087087, 19.16_20210326_1200. https://doi.org/10.5270/esa-[xxxxxxx]