A dataset provided by the European Space Agency

Name 015716
Title RGS and MOS contamination monitoring
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0157160301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0157160401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0157160501
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0157160601
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0157160801
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0157160901
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0157161001
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0157161101

DOI 10.5270/esa-vqgdipn
Author Dr Fred Jansen
Description NRCO: Early-Phase Post-Cooling RGS and MOS contamination monitor with targets Zeta Puppis and N132D. Obs 01 and 02 to be copied and scheduled in revs 535, 538, 541, 548.
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A systematic cross-search for radio-infrared counterparts of XMM- Newton sources . Combi, J. A., Albacete Colombo, J. F., et all. . Ap&SS . 331-53 . 2011 . 2011Ap&SS.331...53C ,
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Constraints on the Ubiquity of Coronal X-Ray Cycles . Hoffman, John, Gunther, Hans M., . ApJ . 759-145 . 2012 . 2012ApJ...759..145H ,
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Constraints on Porosity and Mass Loss in O-star Winds from the Modeling of X-Ray Emission Line Profile Shapes . Leutenegger, Maurice A., Cohen, David H., et all. . ApJ . 770-80 . 2013 . 2013ApJ...770...80L ,
Automatic Classification of Time-variable X-Ray Sources . Lo, Kitty K., Farrell, Sean, et all. . ApJ . 786-20 . 2014 . 2014ApJ...786...20L ,
The diversity of quasars unified by accretion and orientation . Shen, Yue, Ho, Luis C., . Natur . 513-210 . 2014 . 2014Natur.513..210S ,
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 ,
Global Modeling of X-Ray Spectra Produced in O-type Star Winds . Herve, A., Rauw, G., et all. . ApJ . 748-89 . 2012 . 2012ApJ...748...89H ,
Sunyaev-Zel.dovich effect or not? Detecting the main foreground effect of most galaxy clusters . Xiao, Weike, Chen, Chen, et all. . MNRAS . 432-41 . 2013 . 2013MNRAS.432L..41X ,
The population of X-ray supernova remnants in the Large Magellanic Cloud . Maggi, P., Haberl, F., et all. . A&A . 585-162 . 2016 . 2016A&A...585A.162M ,
The Interaction of the Fermi Bubbles with the Milky Way.s Hot Gas Halo . Miller, Matthew J., Bregman, Joel N., . ApJ . 829-9 . 2016 . 2016ApJ...829....9M ,
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 ,
Identification of high-mass X-ray binaries selected from XMM-Newton observations of the LMC* . van Jaarsveld, N., Buckley, D. A. H., et all. . MNRAS . 475-3253 . 2018 . 2018MNRAS.475.3253V ,
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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X-Ray Luminosity and Size Relationship of Supernova Remnants in the LMC . Ou, Po-Sheng, Chu, You-Hua, et all. . ApJ . 863-137 . 2018 . 2018ApJ...863..137O ,
Testing emergent gravity on galaxy cluster scales . Tamosiunas, Andrius, Bacon, David, et all. . JCAP . 5-53 . 2019 . 2019JCAP...05..053T ,
An Observational Link between AGN Eddington Ratio and [N II]u03bb6583-Hu03b1 at 0.6 < z < 1.7 . Oh, Kyuseok, Ueda, Yoshihiro, et all. . ApJ . 880-112 . 2019 . 2019ApJ...880..112O ,
Chandra Follow-up of the SDSS DR8 Redmapper Catalog Using the MATCha Pipeline . Hollowood, Devon L., Jeltema, Tesla, et all. . ApJS . 244-22 . 2019 . 2019ApJS..244...22H ,
Stellar mass as a galaxy cluster mass proxy: application to the Dark Energy Survey redMaPPer clusters . Palmese, A., Annis, J., et all. . MNRAS . 493-4591 . 2020 . 2020MNRAS.493.4591P ,
Spatially Resolved Chandra Spectroscopy of the Large Magellanic Cloud Supernova Remnant N132D . Sharda, Piyush, Gaetz, Terrance J., et all. . ApJ . 894-145 . 2020 . 2020ApJ...894..145S ,
Plasma Diagnostics of the Supernova Remnant N132D using Deep XMM-Newton Observations with the Reflection Grating Spectrometer . Suzuki, Hitomi, Yamaguchi, Hiroya, et all. . ApJ . 900-39 . 2020 . 2020ApJ...900...39S ,
New optically identified supernova remnants in the Large Magellanic Cloud . Yew, Miranda, Filipoviu0107, Miroslav D., et all. . MNRAS . 500-2336 . 2021 . 2021MNRAS.500.2336Y ,
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2002-11-10T07:58:24Z/2002-12-15T11:18:26Z
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 2002-12-15T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2002-12-15T00:00:00Z, 015716, 17.56_20190403_1200. https://doi.org/10.5270/esa-vqgdipn