A dataset provided by the European Space Agency

Name: Overionization in supernova remnants: a deep look at the SNR IC 443
Published: 2011-03-31T00:00:00Z

Proposal ID	060011
Title	Overionization in supernova remnants: a deep look at the SNR IC 443
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0600110101
DOI	https://doi.org/10.5270/esa-xt4125i
Principal Investigator, PI	Ms Eleonora Troja
Abstract	IC 443 is a Galactic supernova remnant with a peculiar morphology: acenter-filled thermal X-ray emission within a radio/optical shell. The presenceof overionized plasma, addressed in previous works, would be a robust clue tothe nature of the center-bright X-rays, which is not yet understood. Our studiesshow significant spectral variations across the remnant, which may lead to thefictitious detection of overionization. We propose a deep observation of thenortheast region in order to obtain a high-quality dataset, and perform aspatially resolved spectroscopy of the brightest X-ray emission of IC 443. Weaim to decisively address the issue of overionization, and to constrain themechanisms of X-ray production from the center of this remnant.
Publications	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 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 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 Gamma-ray astrophysics \|De Angelis, A., Mallamaci, M., \| EPJP \| 133-324 \| 2018 \| 2018EPJP..133..324D \| http://ui.adsabs.harvard.edu/#abs/2018EPJP..133..324D On the in-flight calibration plans of modern x-ray observatories \|Guainazzi, Matteo, David, Laurence, et al. \| JATIS \| 1-47001 \| 2015 \| 2015JATIS...1d7001G \| http://ui.adsabs.harvard.edu/#abs/2015JATIS...1d7001G 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 Modeling the mixed-morphology supernova remnant IC 443. Origins of its complex morphology and X-ray emission \|Ustamujic, S., Orlando, S., et al. \| A&A \| 649-14 \| 2021 \| 2021A&A...649A..14U \| http://ui.adsabs.harvard.edu/#abs/2021A&A...649A..14U The EXTraS project: Exploring the X-ray transient and variable sky \|De Luca, A., Salvaterra, R., et al. \| A&A \| 650-167 \| 2021 \| 2021A&A...650A.167D \| http://ui.adsabs.harvard.edu/#abs/2021A&A...650A.167D 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 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 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	2010-03-07T23:11:04Z/2010-03-09T01:05:21Z
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	2011-03-31T00:00:00Z
Keywords	"center bright xray", "overionized plasma", "fictitious detection", "supernova remnant", "spectral variations", "optical shell", "galactic supernova remnant", "northeast region", "deep look", "quality dataset", "ic 443", "robust clue", "resolved spectroscopy", "xray production", "brightest xray emission"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Ms Eleonora Troja, 2011, 'Overionization in supernova remnants: a deep look at the SNR IC 443', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-xt4125i