|Title||OM Visual Grism Calibration using RT Ser|
|Author||Mr Fred Jansen XMM-Newton PS|
|Description||CAL-The primary goals of the observation of the symbiotic star RT Ser is the calibration of the wavelength scale of the visible grism. Secondary calibration goals are the grism PSF shape. Spectrophotometric calibrations are not intended, because RT Ser is known to be an eruptive nova. The OM overhead time is estimated as 5.3 ksec.|
|Publication||No observations found associated with the current proposal|
|Instrument||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, 2000-03-09T00:00:00Z, 009975, 17.56_20190403_1200. https://doi.org/10.5270/esa-y9g4pj8|