A dataset provided by the European Space Agency

Name 069075
Title A survey of the Large Magellanic Cloud - II
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0690750101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0690750201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0690750301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0690750401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0690750501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0690750601
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0690750701
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0690750801
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0690750901
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0690751001
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0690751101
...
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0690751201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0690751301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0690751401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0690751501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0690751601
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0690751701
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0690751801
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0690751901
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0690752001
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0690752101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0690752201

DOI https://doi.org/10.5270/esa-7o928p8
Author Dr Frank Haberl
Description We propose EPIC observations to survey a virgul10 square degree area of the LMC down
to a limiting point source luminosity of 2 x 10^33 erg/s. Its proximity makes
the LMC the ultimate target for obtaining a complete inventory of SNRs, X-ray
binaries 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 detailed
spectral and temporal analyses of a large fraction of sources. Together with the
existing EPIC data, our observations will create a unique data set to study the
star-formation history and its implications on the morphology of the ISM in the
LMC. In combination with the existing surveys of the SMC, M31 and M33 this will
yield important clues for the evolution of the Local Group as a whole.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2012-09-22T02:06:30Z/2013-03-05T10:39:29Z
Version 17.56_20190403_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 2014-03-15T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Dr Frank Haberl, 2014, 069075, 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-7o928p8