A dataset provided by the European Space Agency

Proposal ID 093499
Title ToO Proposal for AO22
Download Data Associated to the proposal

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0934990101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0934990201
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DOI https://doi.org/10.57780/esa-by4d9dg
Principal Investigator, PI Dr NORBERT SCHARTEL (PS)
Abstract XRISM COORDINATIONS#1 SS 43 50ks#2 4U1916-053 150 ks#3 NGC4151 150 ks = 3x50 ks
Publications No publications found for current proposal!
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2024-04-14T14:56:52Z/2024-06-24T04:38:37Z
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.
Creator Contact https://www.cosmos.esa.int/web/xmm-newton/xmm-newton-helpdesk
Date Published 2025-07-02T00:00:00Z
Last Update 2026-07-09
Keywords XMM-Newton, OM, RGS, EPIC, X-ray, Multi-Mirror, SAS
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Dr NORBERT SCHARTEL (PS), 2025, 'ToO Proposal for AO22', 21.51_20241115_1113, European Space Agency, https://doi.org/10.57780/esa-by4d9dg
Rights Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license.