| Proposal ID | 040480 |
| Title | Probing the Galaxy Cluster Environments of the Mysterious Short Gamma-Ray Bursts |
| Download Data Associated to the proposal | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0404800101 |
| DOI | https://doi.org/10.5270/esa-t6lqtzv |
| Principal Investigator, PI | Dr David Pooley |
| Abstract | We are currently in a period of rapid advancement in our understanding of thenature of short-duration hard-spectrum gamma-ray bursts. A handful of thisminority subclass have finally been localized, allowing for identification oftheir host galaxies. These hosts have been found to span a range of spectraltypes and star-formation rates. Particularly intriguing is the association oftwo short GRBs with galaxies that are part of clusters. We propose relativelyshort XMM observations of all well-localized short GRBs without existing XMM orChandra observations to better determine the relationship between short GRBs andgalaxy clusters as well as determine the properties (e.g., cluster mass) of thelarge-scale host environments. |
| Publications |
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| Instrument | EMOS1, EMOS2, EPN, OM, RGS1, RGS2 |
| Temporal Coverage | 2006-05-14T11:51:13Z/2006-09-10T08:53:30Z |
| 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 | 2007-10-13T00:00:00Z |
| Last Update | 2025-08-04 |
| Keywords | "XMM", " cluster mass", "rapid advancement", "galaxy cluster environments", "spectral types", "relatively short xmm", "existing xmm", "short grbs", "galaxy cluster", "minority subclass", "localized short grbs", "star formation rates", "." |
| Publisher And Registrant | European Space Agency |
| Credit Guidelines | European Space Agency, Dr David Pooley, 2007, 'Probing the Galaxy Cluster Environments of the Mysterious Short Gamma-Ray Bursts', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-t6lqtzv |