A dataset provided by the European Space Agency

Name 021108
Title The absolute Flux calibration of OM
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0211080101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0211080201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0211080301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0211080401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0211080501
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0211080601
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0211080701

DOI 10.5270/esa-23n1q70
Author Dr Fred Jansen XMM-Newton MM
Description \t A series of non-routine calibration observations is requested in order to convert count rates to flux according to spectral type on the XMM-OM. We have observed seven targets varying in spectral type from O5V to M2V (NRCO #32) in order to calculate a count rate to flux ratio. The OM calibration team believes that it is important to observe more stars of each spectral type to reduce the statistical errors. We have checked no duplication with the AO3 observations.
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Exospheric solar wind charge exchange as seen by XMM-Newton . Carter, J. A., Semba, S., . AN . 333-313 . 2012 . 2012AN....333..313C ,
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Cross-correlation of the 2XMMi catalogue with Data Release 7 of the Sloan Digital Sky Survey . Pineau, F.-X., Motch, C., et all. . A&A . 527-126 . 2011 . 2011A&A...527A.126P ,
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Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift . Yershov, V. N., . Ap&SS . 354-97 . 2014 . 2014Ap&SS.354...97Y ,
Obscuration-dependent Evolution of Active Galactic Nuclei . Buchner, Johannes, Georgakakis, Antonis, et all. . ApJ . 802-89 . 2015 . 2015ApJ...802...89B ,
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The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
AGN spectral states from simultaneous UV and X-ray observations by XMM-Newton . Svoboda, J., Guainazzi, M., . A&A . 603-127 . 2017 . 2017A&A...603A.127S ,
Anisotropy of the galaxy cluster X-ray luminosity-temperature relation . Migkas, Konstantinos, Reiprich, Thomas H., . A&A . 611-50 . 2018 . 2018A&A...611A..50M ,
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Testing emergent gravity on galaxy cluster scales . Tamosiunas, Andrius, Bacon, David, et all. . JCAP . 5-53 . 2019 . 2019JCAP...05..053T ,
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Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2004-10-12T08:07:36Z/2005-11-05T01:59:28Z
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 2005-11-06T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2005-11-06T00:00:00Z, 021108, 17.56_20190403_1200. https://doi.org/10.5270/esa-23n1q70