A dataset provided by the European Space Agency

Name 009364
Title The X-ray Properties of Local Galaxies: Bridging the Gap to High-z
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0093640301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0093640401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0093640701
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0093640901
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0093641001
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0093641101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0093641201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0093641301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0093641401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0093641501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0093641601
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https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0093641701

DOI https://doi.org/10.5270/esa-wpwxf66
Author European Space Agency
Description We propose to observe a representive sample of local starburst
galaxies at X-ray wavelengths as part of a multi-wavelength campaign
to understand star-formation and quantify global star formation rates (SFR). The
goal of these observations is to calibrate the thermal hard X-ray emission from
high-mass binaries, an independent SFR indicator free from dust extinction,
against other indicators (e.g. radio, FIR, optical, H\alpha, and UV) and to form
a self consistent model of star-formation in the local universe. This star
formation template will provide the basis for understanding and relating the
deep surveys at X-ray, UV, and radio wavelengths that have already been
undertaken or are planned for the near future with {\it AXAF} and {\it XMM}.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2001-01-07T09:35:55Z/2003-06-18T23:29:35Z
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 2004-07-03T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2004, The X-Ray Properties Of Local Galaxies: Bridging The Gap To High-Z, 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-wpwxf66