A dataset provided by the European Space Agency

Name: RGS long-wavelength sensitivity monitor
Published: 2003-12-07T00:00:00Z

Proposal ID	016336
Title	RGS long-wavelength sensitivity monitor
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0163360201
DOI	https://doi.org/10.5270/esa-i0xb4rv
Principal Investigator, PI	Mr Fred Jansen XMM-Newton PS
Abstract	Following NRCO18, as part of the long-term effort to monitor the RGSsensitivity and possible contamination, the star zeta Puppis is an idealtarget because of the exceptional strength of its NVI and NVII lines atabout 25 and 30A respectively. So far, XMM has not been able to detect anyvariability above the few percent level. It is visible for 2 months every 6months and for this programme, I propose a further 60ks observation with asmall pointing adjustment in order for the NVI and NVII lines to be clear ofchip gaps, as much as possible, in both RGS instruments.
Publications	X-ray continuum properties of GRB afterglows observed by XMM-Newton and Chandra \|Gendre, B., Corsi, A., \| A&A \| 455-803 \| 2006 \| 2006A&A...455..803G \| http://ui.adsabs.harvard.edu/#abs/2006A&A...455..803G 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 A new search strategy for microquasar candidates using NVSS/2MASS and XMM-Newton data \|Combi, J. A., Albacete-Colombo, J. F., \| A&A \| 477-125 \| 2008 \| 2008A&A...477..125C \| http://ui.adsabs.harvard.edu/#abs/2008A&A...477..125C The Discovery of an Evolving Dust-scattered X-Ray Halo around GRB 031203 \|Vaughan, S., Willingale, R., et al. \| ApJ \| 603-5 \| 2004 \| 2004ApJ...603L...5V \| http://ui.adsabs.harvard.edu/#abs/2004ApJ...603L...5V A Very Low Luminosity X-Ray Flash: XMM-Newton Observations of GRB 031203 \|Watson, D., Hjorth, J., et al. \| ApJ \| 605-101 \| 2004 \| 2004ApJ...605L.101W \| http://ui.adsabs.harvard.edu/#abs/2004ApJ...605L.101W A Search for Discrete X-Ray Spectral Features in a Sample of Bright gamma-Ray Burst Afterglows \|Sako, Masao, Harrison, Fiona A., \| ApJ \| 623-973 \| 2005 \| 2005ApJ...623..973S \| http://ui.adsabs.harvard.edu/#abs/2005ApJ...623..973S The Soft X-Ray Blast in the Apparently Subluminous GRB 031203 \|Watson, D., Vaughan, S. A., et al. \| ApJ \| 636-967 \| 2006 \| 2006ApJ...636..967W \| http://ui.adsabs.harvard.edu/#abs/2006ApJ...636..967W 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 General X-ray properties of hot, massive stars \|Naze, Yael, \| BSRSL \| 80-109 \| 2011 \| 2011BSRSL..80..109N \| http://ui.adsabs.harvard.edu/#abs/2011BSRSL..80..109N 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 Exospheric solar wind charge exchange as seen by XMM-Newton \|Carter, J. A., Semba, S., \| AN \| 333-313 \| 2012 \| 2012AN....333..313C \| http://ui.adsabs.harvard.edu/#abs/2012AN....333..313C 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 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 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 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 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 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, RGS1, RGS2
Temporal Coverage	2003-12-06T18:11:07Z/2003-12-07T09:21:17Z
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	2003-12-07T00:00:00Z
Keywords	"nvii lines", "star zeta puppis", "percent level", "XMM", "30a respectively", "rgs sensitivity", "term effort", "chip gaps", "rgs instruments", "wavelength sensitivity", "ideal target"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Mr Fred Jansen XMM-Newton PS, 2003, 'RGS long-wavelength sensitivity monitor', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-i0xb4rv