| Name | 067131 |
| Title | Disclosing the gamma-ray burst circumburst ambient with XMM-Newton |
| URL | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0671310101 |
| DOI | https://doi.org/10.5270/esa-7q5fqob |
| Author | European Space Agency |
| Description | Long GRBs signal the death of massive stars. The afterglow emission can be used to probe the progenitor ambient through a detailed study of the absorption pattern. This has been done at optical wavelengths with impressive results. We propose here to carry out similar studies in the X-ray band with high resolution spectroscopy. Taking advantage of Swift observations, we propose to trigger TOOs on selected bright GRBs within 1 d from their explosions. These data will allow us to have access to an unprecedented statistics. Detailed studies of the absorption pattern imprinted in the X-ray spectrum by the circumburst material as well as the host galaxy ISM can be carried out, allowing us to shed light on the material metallicity, composition and distance. |
| Publication | No observations found associated with the current proposal |
| Instrument | EMOS1, EMOS2, EPN, OM, RGS1, RGS2 |
| Temporal Coverage | 2014-01-03T12:50:15Z/2014-01-03T21:10:15Z |
| 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 | 2015-01-27T23:00:00Z |
| Publisher And Registrant | European Space Agency |
| Credit Guidelines | European Space Agency, 2015, Disclosing The Gamma-Ray Burst Circumburst Ambient With Xmm-Newton, 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-7q5fqob |