A dataset provided by the European Space Agency

Name: EPIC energy routine calibration
Published: 2004-07-04T00:00:00Z

Proposal ID	016556
Title	EPIC energy routine calibration
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0165560101
DOI	https://doi.org/10.5270/esa-2pz3hfn
Principal Investigator, PI	Dr Fred Jansen XMM-Newton PS
Abstract	obs 01: Cas A placed such that it is distributed over all four inner pn CCDs
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 Modelling the spectral response of the Swift-XRT CCD camera: experience learnt from in-flight calibration \|Godet O. Beardmore A. P. et al. \| A&A \| 494-775 \| 2009 \| 2009A&A...494..775G \| http://ui.adsabs.harvard.edu/#abs/2009A&A...494..775G 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 Recovering Swift-XRT energy resolution through CCD charge trap mapping \|Pagani C. Beardmore A. P. et al. \| A&A \| 534-20 \| 2011 \| 2011A&A...534A..20P \| http://ui.adsabs.harvard.edu/#abs/2011A&A...534A..20P 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 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 Formation pathway for lonely stripped-envelope supernova progenitors: implications for Cassiopeia A \|Hirai Ryosuke Sato Toshiki et al. \| MNRAS \| 499-1154 \| 2020 \| 2020MNRAS.499.1154H \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.499.1154H 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 In-flight calibration of the Insight-Hard X-ray Modulation Telescope \|Li Xiaobo Li Xufang et al. \| JHEAp \| 27-64 \| 2020 \| 2020JHEAp..27...64L \| http://ui.adsabs.harvard.edu/#abs/2020JHEAp..27...64L 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	2004-07-03T10:05:43Z/2004-07-03T21:08:45Z
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	2004-07-04T00:00:00Z
Keywords	"obs 01", "EPIC", "inner pn ccds"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Fred Jansen XMM-Newton PS, 2004, 'EPIC energy routine calibration', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-2pz3hfn