An X-ray chimney extending hundreds of parsecs above and below the Galactic Centre |Ponti G. Hofmann F. et al. | Natur | 567-347 | 2019 | 2019Natur.567..347P | http://ui.adsabs.harvard.edu/#abs/2019Natur.567..347P
Discovery of periodicities in two highly variable intermediate polars towards the Galactic centre |Mondal Samaresh Ponti Gabriele et al. | A&A | 671-120 | 2023 | 2023A&A...671A.120M | http://ui.adsabs.harvard.edu/#abs/2023A&A...671A.120M
Progenitor Constraint-incorporating Shell Merger: The Case of Supernova Remnant G359.0u20130.9 |Matsunaga Kai Uchida Hiroyuki et al. | ApJ | 970-4 | 2024 | 2024ApJ...970....4M | http://ui.adsabs.harvard.edu/#abs/2024ApJ...970....4M
Instrument
EPN, OM, RGS1, RGS2, EMOS1, EMOS2
Temporal Coverage
2017-09-05T15:42:57Z/2018-09-25T22:02:00Z
Version
21.51_20241115_1113
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 Gabriele Ponti, 2019, 'XMM-Newton search for the southern counterpart of the Galactic center lobe', 21.51_20241115_1113, European Space Agency, https://doi.org/10.5270/esa-9xudeh5
Rights
Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license.
