A dataset provided by the European Space Agency

Name: EPIC Gain comma contamination and CTI monitoring-1ES0102
Published: 2017-11-09T23:00:00Z

Proposal ID	041298
Title	EPIC Gain, contamination and CTI monitoring-1ES0102
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412980101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412980201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412980301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412980501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412980701 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412980801 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412980901 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412981001 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412981201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412981301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412981401 ... https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412981501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412981601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412981701 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412982001 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412982101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412982201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412982301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412982401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412982501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412983201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412983301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412983401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412983501
DOI	https://doi.org/10.5270/esa-fxne1uz
Principal Investigator, PI	Dr Fred Jansen XMM-Newton MM
Abstract	EPIC ROUTINE CAL - The AXAF standard candle source, 1ES0102-72 in the SMC regionwill be observed periodically. The strong emission lines at low energies will bemeasured to determine the CCD gain and CTI at the boresight location. In addition, apparent secular changes in various emission line strengths may be used to track contamination build-up. (was proposal 13572)
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 new super-soft X-ray source in the Small Magellanic Cloud: Discovery of the first Be/white dwarf system in the SMC? \|Sturm, R., Haberl, F., et al. \| A&A \| 537-76 \| 2012 \| 2012A&A...537A..76S \| http://ui.adsabs.harvard.edu/#abs/2012A&A...537A..76S 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 XMM-Newton observations of the Small Magellanic Cloud: RX J0105.9-7203, a 726 s Be/X-ray binary pulsar \|Eger, P., Haberl, F., \| A&A \| 485-807 \| 2008 \| 2008A&A...485..807E \| http://ui.adsabs.harvard.edu/#abs/2008A&A...485..807E XMM-Newton observations of the Small Magellanic Cloud: Long term evolution of frequently observed Be/X-ray binaries \|Eger, P., Haberl, F., \| A&A \| 491-841 \| 2008 \| 2008A&A...491..841E \| http://ui.adsabs.harvard.edu/#abs/2008A&A...491..841E 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 The XMM-Newton survey of the Small Magellanic Cloud \|Haberl, F., Sturm, R., et al. \| A&A \| 545-128 \| 2012 \| 2012A&A...545A.128H \| http://ui.adsabs.harvard.edu/#abs/2012A&A...545A.128H Supernova remnants: the X-ray perspective \|Vink, Jacco, \| A&ARv \| 20-49 \| 2012 \| 2012A&ARv..20...49V \| http://ui.adsabs.harvard.edu/#abs/2012A&ARv..20...49V 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 The XMM-Newton survey of the Small Magellanic Cloud: The X-ray point-source catalogue \|Sturm, R., Haberl, F., et al. \| A&A \| 558-3 \| 2013 \| 2013A&A...558A...3S \| http://ui.adsabs.harvard.edu/#abs/2013A&A...558A...3S Active galactic nuclei behind the SMC selected from radio and X-ray surveys \|Sturm, R., Draskovic, D., et al. \| A&A \| 558-101 \| 2013 \| 2013A&A...558A.101S \| http://ui.adsabs.harvard.edu/#abs/2013A&A...558A.101S 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 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 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 SNR 1E 0102.2-7219 as an X-ray calibration standard in the 0.5-1.0 keV bandpass and its application to the CCD instruments aboard Chandra, Suzaku, Swift and XMM-Newton \|Plucinsky, Paul P., Beardmore, Andrew P., et al. \| A&A \| 597-35 \| 2016 \| 2016A&A...597A..35P \| http://ui.adsabs.harvard.edu/#abs/2016A&A...597A..35P SNR 1E 0102.2-7219 as an X-ray calibration standard in the 0.5-1.0 keV bandpass and its application to the CCD instruments aboard Chandra, Suzaku, Swift and XMM-Newton \|Plucinsky, Paul P., Beardmore, Andrew P., et al. \| A&A \| 597-35 \| 2017 \| 2017A&A...597A..35P \| http://ui.adsabs.harvard.edu/#abs/2017A&A...597A..35P Discovery of a 26.2 day period in the long-term X-ray light curve of SXP 1323: a very short orbital period for a long spin period pulsar \|Carpano, S., Haberl, F., \| A&A \| 602-81 \| 2017 \| 2017A&A...602A..81C \| http://ui.adsabs.harvard.edu/#abs/2017A&A...602A..81C A Comprehensive Library of X-Ray Pulsars in the Small Magellanic Cloud: Time Evolution of Their Luminosities and Spin Periods \|Yang, J., Laycock, S. G. T., et al. \| ApJ \| 839-119 \| 2017 \| 2017ApJ...839..119Y \| http://ui.adsabs.harvard.edu/#abs/2017ApJ...839..119Y 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 Identification of AGN in the XMM-Newton X-ray survey of the SMC \|Maitra, Chandreyee, Haberl, Frank, et al. \| A&A \| 622-29 \| 2019 \| 2019A&A...622A..29M \| http://ui.adsabs.harvard.edu/#abs/2019A&A...622A..29M 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 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 Anticorrelation between X-ray luminosity and pulsed fraction in the Small Magellanic Cloud pulsar SXP 1323 \|Yang, Jun, Zezas, Andreas, et al. \| MNRAS \| 479-1 \| 2018 \| 2018MNRAS.479L...1Y \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.479L...1Y The supernova remnant population of the Small Magellanic Cloud \|Maggi, Pierre, Filipovi\\u0107, Miroslav D., et al. \| A&A \| 631-127 \| 2019 \| 2019A&A...631A.127M \| http://ui.adsabs.harvard.edu/#abs/2019A&A...631A.127M 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 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 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 eROSITA calibration and performance verification phase: High-mass X-ray binaries in the Magellanic Clouds \|Haberl, F., Maitra, C., et al. \| A&A \| 661-25 \| 2022 \| 2022A&A...661A..25H \| http://ui.adsabs.harvard.edu/#abs/2022A&A...661A..25H Losing a minute every two years: SRG X-ray view of the rapidly accelerating X-ray pulsar SXP 1323 \|Mereminskiy, I. A., Mushtukov, A. A., et al. \| A&A \| 661-33 \| 2022 \| 2022A&A...661A..33M \| http://ui.adsabs.harvard.edu/#abs/2022A&A...661A..33M Spitzer and Herschel studies of dust in supernova remnants in the Small Magellanic Cloud \|Matsuura, Mikako, Ayley, Victoria, et al. \| MNRAS \| 513-1154 \| 2022 \| 2022MNRAS.513.1154M \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.513.1154M The MeerKAT 1.3 GHz Survey of the Small Magellanic Cloud \|Cotton, W. D., Filipovi\\u0107, M. D., et al. \| MNRAS \| 529-2443 \| 2024 \| 2024MNRAS.529.2443C \| http://ui.adsabs.harvard.edu/#abs/2024MNRAS.529.2443C 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	2006-11-05T00:54:41Z/2017-11-05T00:35:34Z
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	2017-11-09T23:00:00Z
Keywords	"epic gain", "apparent secular", "emission lines", "epic routine cal", "1es0102 72", "smc region", "low energies", "ccd gain", "boresight location", "emission line strengths", "EPIC", "track contamination build"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Fred Jansen XMM-Newton MM, 2017, 'EPIC Gain comma contamination and CTI monitoring-1ES0102', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-fxne1uz