No abstract found for current proposal (This is a scientific proposal for an ESA mission. For specific information please contact ESDC Helpdesk - https://support.cosmos.esa.int/esdc)
Searching for highly obscured AGNs in the XMM-Newton serendipitous source catalog |Corral, A., Georgantopoulos, I., et al. | A&A | 569-71 | 2014 | 2014A&A...569A..71C | http://ui.adsabs.harvard.edu/#abs/2014A&A...569A..71C
Robust constraints on feebly interacting particles using XMM-Newton |Luque, Pedro De la Torre, Balaji, Shyam, | PhRvD | 109-L101305 | 2024 | 2024PhRvD.109j1305L | http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j1305L
Multimessenger search for electrophilic feebly interacting particles from supernovae |Luque, Pedro De la Torre, Balaji, Shyam, | PhRvD | 109-103028 | 2024 | 2024PhRvD.109j3028L | http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j3028L
Importance of Cosmic-Ray Propagation on Sub-GeV Dark Matter Constraints |De la Torre Luque, Pedro, Balaji, Shyam, | ApJ | 968-46 | 2024 | 2024ApJ...968...46D | http://ui.adsabs.harvard.edu/#abs/2024ApJ...968...46D
A comprehensive X-ray analysis of the massive O-type binary HD 93250 over two decades |Arora, Bharti, De Becker, Micha\\u00ebl, | A&A | 687-A34 | 2024 | 2024A&A...687A..34A | http://ui.adsabs.harvard.edu/#abs/2024A&A...687A..34A
Instrument
EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage
2009-01-05T10:22:08Z/2009-02-02T12:14:01Z
Version
17.56_20190403_1200
Mission Description
The European Space Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs 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 Earths 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.
European Space Agency, Dr Kenji Hamaguchi, 2010, 'X-ray Monitoring of Eta Car in 2009: Unveiling the Deep X-ray Minimum', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-edahrpp