A dataset provided by the European Space Agency

Name 078469
Title Exploring the Wing of the SMC


DOI https://doi.org/10.5270/esa-dok8bgr
Author Dr Frank Haberl
Description The Magellanic Cloud provides the nearest example for tidally interacting and star-forming galaxies. The wing of the Small Magellanic Cloud is an excellent target, to study sources in a tidally disturbed environment. We propose to survey further regions of the wing of the Small Magellanic Cloud to better constrain the X-ray source population and the amount of diffuse X-ray emission in this region.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2016-04-30T17:36:42Z/2016-12-10T23:31:09Z
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 2017-12-22T23:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2017-12-22T23:00:00Z, 078469, 17.56_20190403_1200. https://doi.org/10.5270/esa-dok8bgr