Name | 055364 |
Title | Identifying the TeV Gamma-Ray Source MGRO 1908+06 |
URL | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0553640101 |
DOI | https://doi.org/10.5270/esa-e58uhy3 |
Author | Dr DIRK PANDEL |
Description | The H.E.S.S. collaboration recently confirmed the Milagro TeV gamma-ray source MGRO 1908+06 and determined its position with sufficient accuracy to allow follow-up observations with XMM-Newton. The unusually hard TeV spectrum and the low X-ray to gamma-ray flux ratio of the source indicate that, unlike most unidentified TeV sources, it is probably not a pulsar wind nebula but may represent a new class of objects. We propose to observe MGRO 1908+06 in order to identify its X-ray counterpart, determine its location with arcsecond precision, and determine whether it is extended or a point source. The accurate source position provided by XMM-Newton will be essential to identify counterparts at other wavelengths and carry out multi-wavelength studies of the source. |
Publication | No observations found associated with the current proposal |
Instrument | EMOS1, EMOS2, EPN, OM, RGS1, RGS2 |
Temporal Coverage | 2008-09-27T00:19:25Z/2009-03-24T00:26:14Z |
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 | 2010-04-22T00:00:00Z |
Publisher And Registrant | European Space Agency |
Credit Guidelines | European Space Agency, 2010-04-22T00:00:00Z, 055364, 17.56_20190403_1200. https://doi.org/10.5270/esa-e58uhy3 |