A dataset provided by the European Space Agency

Name: RGS and MOS contamination monitoring
Published: 2002-12-15T00:00:00Z

Proposal ID	015716
Title	RGS and MOS contamination monitoring
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0157160301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0157160401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0157160501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0157160601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0157160801 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0157160901 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0157161001 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0157161101
DOI	https://doi.org/10.5270/esa-vqgdipn
Principal Investigator, PI	Dr Fred Jansen
Abstract	NRCO: Early-Phase Post-Cooling RGS and MOS contamination monitorwith targets Zeta Puppis and N132D. Obs 01 and 02 to be copied and scheduled in revs 535, 538, 541, 548.
Publications	The XMM-Newton serendipitous survey. V. The Second XMM-Newton serendipitous source catalogue \|Watson, M. G., Schroder, A. C., et al. \| A&A \| 493-339 \| 2009 \| 2009A&A...493..339W \| http://ui.adsabs.harvard.edu/#abs/2009A&A...493..339W Statistical evaluation of the flux cross-calibration of the XMM-Newton EPIC cameras \|Mateos, S., Saxton, R. D., et al. \| A&A \| 496-879 \| 2009 \| 2009A&A...496..879M \| http://ui.adsabs.harvard.edu/#abs/2009A&A...496..879M A detailed X-ray investigation of zeta Puppis. I. The dataset and some preliminary results \|Naze, Y., Flores, C. A., \| A&A \| 538-22 \| 2012 \| 2012A&A...538A..22N \| http://ui.adsabs.harvard.edu/#abs/2012A&A...538A..22N The XMM Cluster Survey: optical analysis methodology and the first data release \|Mehrtens, Nicola, Romer, A. Kathy, et al. \| MNRAS \| 423-1024 \| 2012 \| 2012MNRAS.423.1024M \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.423.1024M Evidence for the Importance of Resonance Scattering in X-Ray Emission Line Profiles of the O Star zeta Puppis \|Leutenegger, Maurice A., Owocki, Stanley P., et al. \| ApJ \| 659-642 \| 2007 \| 2007ApJ...659..642L \| http://ui.adsabs.harvard.edu/#abs/2007ApJ...659..642L A Search for New Galactic Magnetars in Archival Chandra and XMM-Newton Observations \|Muno, M. P., Gaensler, B. M., et al. \| ApJ \| 680-639 \| 2008 \| 2008ApJ...680..639M \| http://ui.adsabs.harvard.edu/#abs/2008ApJ...680..639M X-ray spectroscopy of early-type stars: The present and the future \|Rauw, G., Naze, Y., \| AN \| 329-222 \| 2008 \| 2008AN....329..222R \| http://ui.adsabs.harvard.edu/#abs/2008AN....329..222R X-rays, clumping and wind structures \|Oskinova, Lidia, Hamann, Wolf-Rainer, et al. \| BSRSL \| 80-54 \| 2011 \| 2011BSRSL..80...54O \| http://ui.adsabs.harvard.edu/#abs/2011BSRSL..80...54O An All-Sky Atlas of Radio/X-ray Associations \|Flesch, E., \| PASA \| 27-283 \| 2010 \| 2010PASA...27..283F \| http://ui.adsabs.harvard.edu/#abs/2010PASA...27..283F The XMM Cluster Survey: X-ray analysis methodology \|Lloyd-Davies, E. J., Romer, A. Kathy, et al. \| MNRAS \| 418-14 \| 2011 \| 2011MNRAS.418...14L \| http://ui.adsabs.harvard.edu/#abs/2011MNRAS.418...14L Classification of X-Ray Sources in the XMM-Newton Serendipitous Source Catalog \|Lin, Dacheng, Webb, Natalie A., \| ApJ \| 756-27 \| 2012 \| 2012ApJ...756...27L \| http://ui.adsabs.harvard.edu/#abs/2012ApJ...756...27L An XMM-Newton Survey of the Soft X-Ray Background. II. An All-Sky Catalog of Diffuse O VII and O VIII Emission Intensities \|Henley, David B., Shelton, Robin L., \| ApJS \| 202-14 \| 2012 \| 2012ApJS..202...14H \| http://ui.adsabs.harvard.edu/#abs/2012ApJS..202...14H The XMM-Newton serendipitous ultraviolet source survey catalogue \|Page, M. J., Brindle, C., et al. \| MNRAS \| 426-903 \| 2012 \| 2012MNRAS.426..903P \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.426..903P Hot stars observed by XMM-Newton. I. The catalog and the properties of OB stars \|Naze, Y., \| A&A \| 506-1055 \| 2009 \| 2009A&A...506.1055N \| http://ui.adsabs.harvard.edu/#abs/2009A&A...506.1055N A systematic cross-search for radio/infrared counterparts of XMM- Newton sources \|Combi, J. A., Albacete Colombo, J. F., et al. \| Ap&SS \| 331-53 \| 2011 \| 2011Ap&SS.331...53C \| http://ui.adsabs.harvard.edu/#abs/2011Ap&SS.331...53C A Detailed X-Ray Investigation of zeta Puppis. II. The Variability on Short and Long Timescales \|Naze, Yael, Oskinova, Lidia M., \| ApJ \| 763-143 \| 2013 \| 2013ApJ...763..143N \| http://ui.adsabs.harvard.edu/#abs/2013ApJ...763..143N Constraints on the Ubiquity of Coronal X-Ray Cycles \|Hoffman, John, Gunther, Hans M., \| ApJ \| 759-145 \| 2012 \| 2012ApJ...759..145H \| http://ui.adsabs.harvard.edu/#abs/2012ApJ...759..145H A detailed X-ray investigation of zeta Puppis. III. Spectral analysis of the whole RGS spectrum \|Herve, A., Rauw, G., \| A&A \| 551-83 \| 2013 \| 2013A&A...551A..83H \| http://ui.adsabs.harvard.edu/#abs/2013A&A...551A..83H 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 al. \| ApJ \| 770-80 \| 2013 \| 2013ApJ...770...80L \| http://ui.adsabs.harvard.edu/#abs/2013ApJ...770...80L Automatic Classification of Time-variable X-Ray Sources \|Lo, Kitty K., Farrell, Sean, et al. \| ApJ \| 786-20 \| 2014 \| 2014ApJ...786...20L \| http://ui.adsabs.harvard.edu/#abs/2014ApJ...786...20L The diversity of quasars unified by accretion and orientation \|Shen, Yue, Ho, Luis C., \| Natur \| 513-210 \| 2014 \| 2014Natur.513..210S \| http://ui.adsabs.harvard.edu/#abs/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 \| http://ui.adsabs.harvard.edu/#abs/2014Ap&SS.354...97Y Global Modeling of X-Ray Spectra Produced in O-type Star Winds \|Herve, A., Rauw, G., et al. \| ApJ \| 748-89 \| 2012 \| 2012ApJ...748...89H \| http://ui.adsabs.harvard.edu/#abs/2012ApJ...748...89H Sunyaev-Zel.dovich effect or not? Detecting the main foreground effect of most galaxy clusters \|Xiao, Weike, Chen, Chen, et al. \| MNRAS \| 432-41 \| 2013 \| 2013MNRAS.432L..41X \| http://ui.adsabs.harvard.edu/#abs/2013MNRAS.432L..41X The population of X-ray supernova remnants in the Large Magellanic Cloud \|Maggi, P., Haberl, F., et al. \| A&A \| 585-162 \| 2016 \| 2016A&A...585A.162M \| http://ui.adsabs.harvard.edu/#abs/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 \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...829....9M The Million Optical - Radio/X-ray Associations (MORX) Catalogue \|Flesch, Eric W., \| PASA \| 33-52 \| 2016 \| 2016PASA...33...52F \| http://ui.adsabs.harvard.edu/#abs/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 \| http://ui.adsabs.harvard.edu/#abs/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 al. \| MNRAS \| 475-3253 \| 2018 \| 2018MNRAS.475.3253V \| http://ui.adsabs.harvard.edu/#abs/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 \| http://ui.adsabs.harvard.edu/#abs/2018A&A...611A..50M The XMM Cluster Survey: Present status and latest results \|Viana, P. T. P., Mehrtens, N., et al. \| AN \| 334-462 \| 2013 \| 2013AN....334..462V \| http://ui.adsabs.harvard.edu/#abs/2013AN....334..462V X-Ray Luminosity and Size Relationship of Supernova Remnants in the LMC \|Ou, Po-Sheng, Chu, You-Hua, et al. \| ApJ \| 863-137 \| 2018 \| 2018ApJ...863..137O \| http://ui.adsabs.harvard.edu/#abs/2018ApJ...863..137O Testing emergent gravity on galaxy cluster scales \|Tamosiunas, Andrius, Bacon, David, et al. \| JCAP \| 5-53 \| 2019 \| 2019JCAP...05..053T \| http://ui.adsabs.harvard.edu/#abs/2019JCAP...05..053T An Observational Link between AGN Eddington Ratio and N II\\u03bb6583/H\\u03b1 at 0.6 &lt; z &lt; 1.7 \|Oh, Kyuseok, Ueda, Yoshihiro, et al. \| ApJ \| 880-112 \| 2019 \| 2019ApJ...880..112O \| http://ui.adsabs.harvard.edu/#abs/2019ApJ...880..112O Chandra Follow-up of the SDSS DR8 Redmapper Catalog Using the MATCha Pipeline \|Hollowood, Devon L., Jeltema, Tesla, et al. \| ApJS \| 244-22 \| 2019 \| 2019ApJS..244...22H \| http://ui.adsabs.harvard.edu/#abs/2019ApJS..244...22H Stellar mass as a galaxy cluster mass proxy: application to the Dark Energy Survey redMaPPer clusters \|Palmese, A., Annis, J., et al. \| MNRAS \| 493-4591 \| 2020 \| 2020MNRAS.493.4591P \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.493.4591P Spatially Resolved Chandra Spectroscopy of the Large Magellanic Cloud Supernova Remnant N132D \|Sharda, Piyush, Gaetz, Terrance J., et al. \| ApJ \| 894-145 \| 2020 \| 2020ApJ...894..145S \| http://ui.adsabs.harvard.edu/#abs/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 al. \| ApJ \| 900-39 \| 2020 \| 2020ApJ...900...39S \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...900...39S New optically identified supernova remnants in the Large Magellanic Cloud \|Yew, Miranda, Filipovi\\u0107, Miroslav D., et al. \| MNRAS \| 500-2336 \| 2021 \| 2021MNRAS.500.2336Y \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.500.2336Y An X-Ray- and SZ-bright Diffuse Source toward M31: A Local Hot Bridge \|Qu, Zhijie, Huang, Rui, et al. \| ApJ \| 907-14 \| 2021 \| 2021ApJ...907...14Q \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...907...14Q Classification of 4XMM-DR9 sources by machine learning \|Zhang, Yanxia, Zhao, Yongheng, \| MNRAS \| 503-5263 \| 2021 \| 2021MNRAS.503.5263Z \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.503.5263Z Fe XVII 2p-3s Line Ratio Diagnostic of Shock Formation Radius in O Stars \|Grell, Gabriel J., Leutenegger, Maurice A., \| ApJ \| 917-105 \| 2021 \| 2021ApJ...917..105G \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...917..105G The Solar Cycle Temporal Variation of the Solar Wind Charge Exchange X-Ray Lines \|Qu, Zhijie, Koutroumpa, Dimitra, et al. \| ApJ \| 930-21 \| 2022 \| 2022ApJ...930...21Q \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...930...21Q From Active Stars to Black Holes: A Discovery Tool for Galactic X-Ray Sources \|Rodriguez, Antonio C., \| PASP \| 136-054201 \| 2024 \| 2024PASP..136e4201R \| http://ui.adsabs.harvard.edu/#abs/2024PASP..136e4201R Robust constraints on feebly interacting particles using XMM-Newton \|Luque, Pedro De la Torre, Balaji, Shyam, \| PhRvD \| 109-L101305 \| 2024 \| 2024PhRvD.109j1305L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j1305L Multimessenger search for electrophilic feebly interacting particles from supernovae \|Luque, Pedro De la Torre, Balaji, Shyam, \| PhRvD \| 109-103028 \| 2024 \| 2024PhRvD.109j3028L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j3028L Importance of Cosmic-Ray Propagation on Sub-GeV Dark Matter Constraints \|De la Torre Luque, Pedro, Balaji, Shyam, \| ApJ \| 968-46 \| 2024 \| 2024ApJ...968...46D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...968...46D
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 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	2002-12-15T00:00:00Z
Keywords	"mos contamination", "obs 01", "revs 535", "targets zeta puppis"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Fred Jansen, 2002, 'RGS and MOS contamination monitoring', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-vqgdipn