Proposal ID | 085298 |
Title | XMM+eROSITA cross calibration |
Download Data Associated to the proposal | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0852980101 |
DOI | https://doi.org/10.5270/esa-rdn6mtd |
Principal Investigator, PI | Dr NORBERT SCHARTEL (PS) |
Abstract | XMM+eROSITA cross calibration observations1) SN 1987A2) RX J0720.4-31253) PG 1634+7064) PG 1634+7065) PG 1634+7066) Clump structure |
Publications |
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Instrument | EMOS1, EMOS2, EPN, OM, RGS1, RGS2 |
Temporal Coverage | 2019-09-06T19:29:57Z/2020-03-09T05:16:13Z |
Version | 18.02_20200221_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. |
Creator Contact | https://www.cosmos.esa.int/web/xmm-newton/xmm-newton-helpdesk |
Date Published | 2020-12-31T23:00:00Z |
Keywords | "J0720.4", "clump structure", "rx j0720", "pg 1634", "XMM", "erosita cross calibration" |
Publisher And Registrant | European Space Agency |
Credit Guidelines | European Space Agency, Dr NORBERT SCHARTEL (PS), 2020, 'XMM+eROSITA cross calibration', 18.02_20200221_1200, European Space Agency, https://doi.org/10.5270/esa-rdn6mtd |