|Title||A Deep XMM-Newton Legacy Survey of M33|
|Author||Dr Benjamin Williams|
|Description||We propose a deep XMM-Newton legacy survey of M33 covering the entire D25 isophote with a total of 700 ks of exposure. These data will allow us to determine how the temperature and energetics of the hot interstellar medium are affected by star formation, constrain the nature and dynamical masses of new pulsating and eclipsing X-ray binaries, and perform detailed statistical and spectral studies on the largest extragalactic population of X-ray supernova remnants. As the deepest and most complete X-ray census of an entire spiral galaxy possible with current technology, our survey will test the physics of diffuse hot gas and the evolution of X-ray source populations at luminosities never before available for such a sample.|
|Publication||No observations found associated with the current proposal|
|Instrument||EMOS1, EMOS2, EPN, OM, RGS1, RGS2|
|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.
|Publisher And Registrant||European Space Agency|
|Credit Guidelines||European Space Agency, 2011-09-11T00:00:00Z, 065051, 17.56_20190403_1200. https://doi.org/10.5270/esa-r6nli1b|