| Proposal ID | 009984 |
| Title | Shadowing by the Magellanic Bridge: the origin of the 3/4 keV background |
| Download Data Associated to the proposal | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0099840101 |
| DOI | https://doi.org/10.5270/esa-f8gmxey |
| Principal Investigator, PI | Dr Richard Mushotzky |
| Abstract | GT-The high Galactic latitude 3/4 keV background consists of both extragalactic and Galactic emission with uncertain relative contributions. The spectrum at3/4 keV shows an excess over the extrapolation of the extragalactic power lawobserved at higher energies, and this excess has been attributed to emissionfrom sources as varied as a Galactic halo, the Local Group, diffuse cosmological emission, and a bump in the spectra of discrete cosmological sources. By studying the shadow of an NH enhancement in the Magellanic Bridge, the observed flux can be separated into foreground and background components, which will place clear constraints on a number of models both Galactic and cosmological. |
| Publications |
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| Instrument | EMOS1, EMOS2, EPN, RGS1, RGS2 |
| Temporal Coverage | 2000-07-05T15:05:01Z/2000-07-05T19:01:53Z |
| Version | 17.56_20190403_1200 |
| Mission Description | The European Space Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs 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 Earths 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 | 2002-08-15T00:00:00Z |
| Last Update | 2025-01-27 |
| Keywords | "galactic halo", "kev background consists", "background components", "uncertain relative contributions", "nh enhancement", "discrete cosmological sources", "diffuse cosmological emission", "kev background", "magellanic bridge", "extragalactic power law", "galactic emission", "galactic latitude" |
| Publisher And Registrant | European Space Agency |
| Credit Guidelines | European Space Agency, Dr Richard Mushotzky, 2002, 'Shadowing by the Magellanic Bridge: the origin of the 3/4 keV background', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-f8gmxey |