A dataset provided by the European Space Agency

Name 065720
Title Zeta Orionis: EPIC Detector Response
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0657200101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0657200201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0657200301

DOI 10.5270/esa-z4zss65
Author Dr Arvind Parmar XMM-Newton MM
Description For monitorization of the detector distribution through the prominent and separated Carbon and Oxygen lines. It shall be observed once per year for 90 ks in Small Window mode with the THICK filter.
Publication X-Ray Emission from Magnetic Massive Stars . Naze, Yael, Petit, Veronique, et all. . ApJS . 215-10 . 2014 . 2014ApJS..215...10N ,
The Rotation of the Hot Gas around the Milky Way . Hodges-Kluck, Edmund J., Miller, Matthew J., . ApJ . 822-21 . 2016 . 2016ApJ...822...21H ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
Perspectives for observing hot massive stars with XMM-Newton in the years 2017-2027 . Rauw, G., . AN . 338-207 . 2017 . 2017AN....338..207R ,
Is the Pollock.s paradigm of X-ray emission for O stars correct? . Ryspaeva, E. B., Kholtygin, A. F., . AN . 338-959 . 2017 . 2017AN....338..959R ,
Analysis of the X-ray emission of OB stars: O stars . Ryspaeva, Elizaveta, Kholtygin, Alexander, . RAA . 18-104 . 2018 . 2018RAA....18..104R ,
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2010-09-03T01:11:17Z/2012-08-29T16:33:20Z
Version 17.56_20190403_1200
Mission Description The European Space Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's 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 Earth's 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 2011-09-04T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2011-09-04T00:00:00Z, 065720, 17.56_20190403_1200. https://doi.org/10.5270/esa-z4zss65