A dataset provided by the European Space Agency

Name 008134
Title An XMM Mini-survey of Ultraluminous IR Galaxies
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0081340201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0081340301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0081340401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0081340501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0081340601
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0081340801
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0081340901
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0081341001
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0081341101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0081341401

DOI https://doi.org/10.5270/esa-hlsff99
Author European Space Agency
Description We propose XMM observations of 11 ultra-luminous IRAS galaxies (ULIRG) recently
observed with ISO. The specific aim of our project is to test in hard X-ray this
well defined, well studied sample of bright ULIRGs. The observation of the hard
X-ray flux and of the FeK line properties will open a new prospective on
important questions, like the understanding of the mechanism of primary energy
production, the estimate of the X-ray emissivity of absorbed AGNs present in the
nucleus and the evaluation of their contribution to the cosmic X-ray background.
A physical knowledge of such local sources will be also crucially informative
about the nature of their distant, high-z counterparts, likely to originate the
recently discovered far-IR/sub-mm background.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2001-03-30T09:06:52Z/2002-11-19T11:43:30Z
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 2004-01-25T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2004, An Xmm Mini-Survey Of Ultraluminous Ir Galaxies, 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-hlsff99