A dataset provided by the European Space Agency

Name 015936
Title RGS long-term long-wavelength contamination monitor
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0159360101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0159360301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0159360401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0159360501
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0159360601
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http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0159360801
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0159360901
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0159361001
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0159361101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0159361201
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http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0159361301
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http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0159361501

DOI 10.5270/esa-pw8lzwd
Author Mr Fred Jansen XMM-Newton PM
Description Although contamination monitoring was introduced and vigorously pursued after the RGS and MOS were cooled in 2002 November, it is important to establish a long-term contamination monitor. The star zeta Puppis is an ideal target because of the exceptional strength of its NVI and NVII lines at about 25 and 30A respectively. So far, XMM has not been able to detect any variability in this star above the few percent level. It is visible for 2 months every 6 months and for this long-term programme, I propose a longer observation time than used during the immediate post-cooling period, prefering instead the 60ks used for the PV phase.
Publication The XMM-Newton serendipitous survey. V. The Second XMM-Newton serendipitous source catalogue . Watson, M. G., Schroder, A. C., et all. . A&A . 493-339 . 2009 . 2009A&A...493..339W ,
Statistical evaluation of the flux cross-calibration of the XMM-Newton EPIC cameras . Mateos, S., Saxton, R. D., et all. . A&A . 496-879 . 2009 . 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 ,
The XMM Cluster Survey: optical analysis methodology and the first data release . Mehrtens, Nicola, Romer, A. Kathy, et all. . MNRAS . 423-1024 . 2012 . 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 all. . ApJ . 659-642 . 2007 . 2007ApJ...659..642L ,
A Search for New Galactic Magnetars in Archival Chandra and XMM-Newton Observations . Muno, M. P., Gaensler, B. M., et all. . ApJ . 680-639 . 2008 . 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 ,
X-rays, clumping and wind structures . Oskinova, Lidia, Hamann, Wolf-Rainer, et all. . BSRSL . 80-54 . 2011 . ...,
An All-Sky Atlas of Radio-X-ray Associations . Flesch, E., . PASA . 27-283 . 2010 . 2010PASA...27..283F ,
The XMM Cluster Survey: X-ray analysis methodology . Lloyd-Davies, E. J., Romer, A. Kathy, et all. . MNRAS . 418-14 . 2011 . 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 ,
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 ,
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 ,
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 ,
Constraints on the Ubiquity of Coronal X-Ray Cycles . Hoffman, John, Gunther, Hans M., . ApJ . 759-145 . 2012 . 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 ,
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 ,
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 ,
Revealing the broad iron Kalpha line in Cygnus X-1 through simultaneous XMM-Newton, RXTE, and INTEGRAL observations . Duro, Refiz, Dauser, Thomas, et all. . A&A . 589-14 . 2016 . 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 ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 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 all. . MNRAS . 461-1374 . 2016 . 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 ,
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 ,
A detailed X-ray investigation of zeta Puppis. IV. Further characterization of the variability . Naze, Yael, Ramiaramanantsoa, Tahina, et all. . A&A . 609-81 . 2018 . 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 ,
The XMM Cluster Survey: Present status and latest results . Viana, P. T. P., Mehrtens, N., et all. . AN . 334-462 . 2013 . 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 ,
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 all. . MNRAS . 486-3248 . 2019 . 2019MNRAS.486.3248C ,
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 ,
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 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 2009-04-26T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2009-04-26T00:00:00Z, 015936, 17.56_20190403_1200. https://doi.org/10.5270/esa-pw8lzwd