A dataset provided by the European Space Agency

Name: Spectral mapping of the irregular structured Supernova remnant IC443
Published: 2001-09-08T00:00:00Z

Proposal ID	011410
Title	Spectral mapping of the irregular structured Supernova remnant IC443
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0114100101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0114100201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0114100301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0114100401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0114100501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0114100601
DOI	https://doi.org/10.5270/esa-rghfjzc
Principal Investigator, PI	Dr Fred Jansen XMM-Newton PS
Abstract	PV - IC443 is called a middle-aged supernova remnant possibly not much olderthan 1000 years with a diameter of about one degree. At least the northeasternsection lies behind a molecular cloud, which gives rise to significantvariations in photoelectrical absoption across the remnant. The remnant containsat least three sub-shells of significantly different surface brightnessesindicating different evolutionary states. Four observations covering the entireremant are used to verify EPIC.s spectral and spatial capabilities over a largedynamical range for an extended source of highly complex spectral and spatialtopology.
Publications	The plerion nebula in IC 443: The XMM-Newton view \|Bocchino, F., Bykov, A. M., \| A&A \| 376-248 \| 2001 \| 2001A&A...376..248B \| http://ui.adsabs.harvard.edu/#abs/2001A&A...376..248B XMM-Newton study of hard X-ray sources in IC 443 \|Bocchino, F., Bykov, A. M., \| A&A \| 400-203 \| 2003 \| 2003A&A...400..203B \| http://ui.adsabs.harvard.edu/#abs/2003A&A...400..203B XMM-Newton Observations of the Supernova Remnant IC 443. I. Soft X-Ray Emission from Shocked Interstellar Medium \|Troja, E., Bocchino, F., \| ApJ \| 649-258 \| 2006 \| 2006ApJ...649..258T \| http://ui.adsabs.harvard.edu/#abs/2006ApJ...649..258T XMM-Newton observations of the supernova remnant IC 443. II. Evidence of stellar ejecta in the inner regions \|Troja, E., Bocchino, F., et al. \| A&A \| 485-777 \| 2008 \| 2008A&A...485..777T \| http://ui.adsabs.harvard.edu/#abs/2008A&A...485..777T On the metal abundances inside mixed-morphology supernova remnants: the case of IC 443 and G166.0+4.3 \|Bocchino, F., Miceli, M., \| A&A \| 498-139 \| 2009 \| 2009A&A...498..139B \| http://ui.adsabs.harvard.edu/#abs/2009A&A...498..139B 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 Isolated X-Ray-Infrared Sources in the Region of Interaction of the Supernova Remnant IC 443 with a Molecular Cloud \|Bykov, A. M., Krassilchtchikov, A. M., et al. \| ApJ \| 676-1050 \| 2008 \| 2008ApJ...676.1050B \| http://ui.adsabs.harvard.edu/#abs/2008ApJ...676.1050B 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 INTEGRAL observations of the SNR IC443 region \|Bocchino, F., Krassilchtchikov, A. M., et al. \| AdSpR \| 41-396 \| 2008 \| 2008AdSpR..41..396B \| http://ui.adsabs.harvard.edu/#abs/2008AdSpR..41..396B 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 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 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 2-8 keV cosmic X-ray background spectrum as observed with XMM-Newton \|De Luca, A., Molendi, S., \| A&A \| 419-837 \| 2004 \| 2004A&A...419..837D \| http://ui.adsabs.harvard.edu/#abs/2004A&A...419..837D 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 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 Ground- and Space-Based Gamma-Ray Astronomy \|Funk, Stefan, \| ARNPS \| 65-245 \| 2015 \| 2015ARNPS..65..245F \| http://ui.adsabs.harvard.edu/#abs/2015ARNPS..65..245F Discovery of a jet-like structure with overionized plasma in the SNR IC 443 \|Greco, Emanuele, Miceli, Marco, et al. \| A&A \| 615-157 \| 2018 \| 2018A&A...615A.157G \| http://ui.adsabs.harvard.edu/#abs/2018A&A...615A.157G The Spectrum of the Universe \|Hill, Ryley, Masui, Kiyoshi W., \| ApSpe \| 72-663 \| 2018 \| 2018ApSpe..72..663H \| http://ui.adsabs.harvard.edu/#abs/2018ApSpe..72..663H High Resolution X-ray Observations of Supernova Remnants \|Bocchino, F., \| ChJAS \| 3-329 \| 2003 \| 2003ChJAS...3..329B \| http://ui.adsabs.harvard.edu/#abs/2003ChJAS...3..329B Gamma-ray astrophysics \|De Angelis, A., Mallamaci, M., \| EPJP \| 133-324 \| 2018 \| 2018EPJP..133..324D \| http://ui.adsabs.harvard.edu/#abs/2018EPJP..133..324D 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 Investigation of the Physical Origin of Overionized Recombining Plasma in the Supernova Remnant IC 443 with XMM-Newton \|Okon, Hiromichi, Tanaka, Takaaki, et al. \| ApJ \| 921-99 \| 2021 \| 2021ApJ...921...99O \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...921...99O Cosmic-Ray Acceleration in Supernova Remnants \|Sinitsyna, Vera G., Sinitsyna, Vera Y., \| Univ \| 9-98 \| 2023 \| 2023Univ....9...98S \| http://ui.adsabs.harvard.edu/#abs/2023Univ....9...98S Temperature stratification in a molecular shock: Analysis of the emission of H2 pure rotational lines in IC443G \|Dell.Ova, P., Gusdorf, A., et al. \| A&A \| 685-A69 \| 2024 \| 2024A&A...685A..69D \| http://ui.adsabs.harvard.edu/#abs/2024A&A...685A..69D 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	2000-09-25T13:13:11Z/2000-09-28T08:58:05Z
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	2001-09-08T00:00:00Z
Keywords	"dynamical range", "northeastern section lies", "surface brightnesses", "molecular cloud", "spectral mapping", "sub shells", "pv ic443", "spatial topology", "EPIC", "complex spectral", "photoelectrical absoption"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Fred Jansen XMM-Newton PS, 2001, 'Spectral mapping of the irregular structured Supernova remnant IC443', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-rghfjzc