Symposium S16
1 - 2 July 2020
XMM-Newton: Current scientific highlights and future prospects
Aims and scope
The 20 years of XMM-Newton observations have dramatically changed and
increased our understanding of all astronomical X-ray emitting sources,
from the solar system objects in our neighbourhood to distant AGN or
clusters of galaxies. We propose to host for the first time a symposium
at the EAS to celebrate XMM-Newton's 20th anniversary by highlighting its
current scientific achievements, with an emphasis on programs led by
European investigators.
XMM-Newton was designed to study the most violent phenomena in the
Universe with unprecedented sensitivity for X-ray imaging (FoV of 30'
and angular resolution of ~6") in the 0.2-12 keV band, and high-resolution
spectroscopy (resolving power from 150 to 800) in the 0.33-2.5 keV band.
After twenty years of operations, more than 6,000 refereed scientific
papers have been published based on scientific observations obtained via
the yearly competitive call for proposals or public archival observations.
At the mission extension review, a statement issued by ESA concluded that
"XMM-Newton has established itself as one of the most prolific astronomical
endeavours in ESA history. Based on data gathered through XMM-Newton
observations, discoveries in almost every field of astronomy have been
produced."
Programme
- Solar System Objects and exoplanets
- Stars, star formation, young, cool and hot stellar objects and diffuse Galactic Emission
- Supernovae, Gravitational Wave Events and Gamma Ray Bursts
- Compact objects and compact binaries
- Galaxies, Active Galactic Nuclei, Clusters of Galaxies and Cosmology
- Athena and other future X-ray missions
Invited speakers
- Nathalie Degenaar (University of Amsterdam, The Netherlands)
- Margherita Giustini (Centro de Astrobiología, Villanueva de la Cañada, Spain)
- Guido Risaliti & Elisabeta Lusso (University of Firenze, Italy)
- Didier Barret (Institut de Recherche en Astrophysique et Planétologie, Toulouse, France)
Scientific organisers
Maria Diaz Trigo (ESO, Munich, Germany, co-chairperson),
Norbert Schartel (ESA, Spain, chairperson),
Natalie Webb (Institut de Recherche en Astrophysique et Planétologie, Toulouse, France, co-chairperson),
Rudy Wijnands (University of Amsterdam, The Netherlands, co-chairperson)
Contact
Norbert.Schartel @ sciops.esa.int
Updated on Fri Mar 06 10:16:00 CET 2020
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