A dataset provided by the European Space Agency

Name: RGS long-term long-wavelength contamination monitor
Published: 2009-04-26T00:00:00Z

Proposal ID	015936
Title	RGS long-term long-wavelength contamination monitor
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0159360101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0159360301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0159360401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0159360501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0159360601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0159360701 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0159360801 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0159360901 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0159361001 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0159361101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0159361201 ... https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0159361301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0159361401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0159361501
DOI	https://doi.org/10.5270/esa-pw8lzwd
Principal Investigator, PI	Mr Fred Jansen XMM-Newton PM
Abstract	Although contamination monitoring was introduced and vigorously pursued afterthe RGS and MOS were cooled in 2002 November, it is important to establish along-term contamination monitor. The star zeta Puppis is an ideal target becauseof the exceptional strength of its NVI and NVII lines at about 25 and 30Arespectively. So far, XMM has not been able to detect any variability in thisstar above the few percent level. It is visible for 2 months every 6 months andfor this long-term programme, I propose a longer observation time than usedduring the immediate post-cooling period, prefering instead the 60ks used forthe PV phase.
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 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 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 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 Revealing the broad iron Kalpha line in Cygnus X-1 through simultaneous XMM-Newton, RXTE, and INTEGRAL observations \|Duro, Refiz, Dauser, Thomas, et al. \| A&A \| 589-14 \| 2016 \| 2016A&A...589A..14D \| http://ui.adsabs.harvard.edu/#abs/2016A&A...589A..14D 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 A benchmark of the He-like triplet for ions with 6 <= Z <= 14 in Maxwellian and non-Maxwellian plasmas \|Rodriguez, Y., Gatuzz, E., et al. \| MNRAS \| 461-1374 \| 2016 \| 2016MNRAS.461.1374R \| http://ui.adsabs.harvard.edu/#abs/2016MNRAS.461.1374R 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 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 \| http://ui.adsabs.harvard.edu/#abs/2017AN....338..959R A detailed X-ray investigation of zeta Puppis. IV. Further characterization of the variability \|Naze, Yael, Ramiaramanantsoa, Tahina, et al. \| A&A \| 609-81 \| 2018 \| 2018A&A...609A..81N \| http://ui.adsabs.harvard.edu/#abs/2018A&A...609A..81N 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 Analysis of the X-ray emission of OB stars: O stars \|Ryspaeva, Elizaveta, Kholtygin, Alexander, \| RAA \| 18-104 \| 2018 \| 2018RAA....18..104R \| http://ui.adsabs.harvard.edu/#abs/2018RAA....18..104R On the geometry of the X-ray emission from pulsars: the changing aspect of the Be/X-ray pulsar SXP348 \|Cappallo, R., Laycock, S. G. T., et al. \| MNRAS \| 486-3248 \| 2019 \| 2019MNRAS.486.3248C \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.486.3248C 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 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 The EXTraS project: Exploring the X-ray transient and variable sky \|De Luca, A., Salvaterra, R., et al. \| A&A \| 650-167 \| 2021 \| 2021A&A...650A.167D \| http://ui.adsabs.harvard.edu/#abs/2021A&A...650A.167D 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	2003-05-30T09:29:28Z/2013-10-23T07:24:34Z
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	2009-04-26T00:00:00Z
Keywords	"nvii lines", "star zeta puppis", "percent level", "XMM", "post cooling period", "30a respectively", "term programme", "pv phase", "term contamination", "wavelength contamination", "ideal target"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Mr Fred Jansen XMM-Newton PM, 2009, 'RGS long-term long-wavelength contamination monitor', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-pw8lzwd