A dataset provided by the European Space Agency

Name 011689
Title Rev 31
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0116890801
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0116890901
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0116891101

DOI 10.5270/esa-h3iki1a
Author Mr Fred Jansen XMM-Newton PS
Description
Publication X-ray spectroscopic studies of stars . Gudel, M., . AdSpR . 32-2045 . 2003 . 2003AdSpR..32.2045G ,
First light measurements with the XMM-Newton reflection grating spectrometers: Evidence for an inverse first ionisation potential effect and anomalous Ne abundance in the Coronae of HR 1099 . Brinkman, A. C., Behar, E., et all. . A&A . 365-324 . 2001 . 2001A&A...365L.324B ,
The XMM-Newton view of stellar coronae: Flare heating in the coronae of HR 1099 . Audard, M., Gudel, M., . A&A . 365-318 . 2001 . 2001A&A...365L.318A ,
The first decade of science with Chandra and XMM-Newton . Santos-Lleo, Maria, Schartel, Norbert, et all. . Natur . 462-997 . 2009 . 2009Natur.462..997S ,
Calibration and in-orbit performance of the reflection grating spectrometer onboard XMM-Newton . de Vries, C. P., den Herder, J. W., et all. . A&A . 573-128 . 2015 . 2015A&A...573A.128D ,
Investigations of stellar coronae with XMM-Newton . Audard, M., . AdSpR . 32-927 . 2003 . 2003AdSpR..32..927A ,
X-ray emission from the stellar population in M 32 . Revnivtsev, M., Churazov, E., et all. . A&A . 473-783 . 2007 . 2007A&A...473..783R ,
XMM-Newton publication statistics . Ness, J.-U., Parmar, A. N., et all. . AN . 335-210 . 2014 . 2014AN....335..210N ,
The Rotation of the Hot Gas around the Milky Way . Hodges-Kluck, Edmund...
Instrument EMOS1, EMOS2, EPN, RGS1, RGS2
Temporal Coverage 2000-02-08T12:56:26Z/2000-02-10T03:44:02Z
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 2000-03-09T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2000-03-09T00:00:00Z, 011689, 17.56_20190403_1200. https://doi.org/10.5270/esa-h3iki1a