A dataset provided by the European Space Agency

Name: Circumstellar Interaction in Type Ia Supernova 2003lx
Published: 2013-07-21T00:00:00Z

Proposal ID	069479
Title	Circumstellar Interaction in Type Ia Supernova 2003lx
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0694790101
DOI	https://doi.org/10.5270/esa-5cimz8t
Principal Investigator, PI	Dr C.S.J. Pun
Abstract	Type Ia SN 2003lx was first discovered in X-ray through two serendipitous Swiftobservations in 2008 January and the corresponding merged image revealed a7-sigma source detection at 2.1+/-1.2 arcsec (0.9+/-0.5 Swift pixels) from theopticalposition of the supernova. We propose a XMM-Newton observation of Type IaSN 2003lx to study its flux and spectral properties. If confirmed, SN 2003lxwill be the first concrete X-ray SN Ia detected. The X-ray emission will thenallow us to probe the interaction between the fast moving debris of the explodedstar and the circumstellar medium (CSM). This in turns provides footprints ofthe mass-loss history of the exploded system, and may allow us to learn aboutthe nature of the progenitorand its companion.
Publications	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 A Comparison of X-Ray Photon Indices among the Narrow- and Broad-line Seyfert 1 Galaxies \|Ojha, Vineet, Chand, Hum, et al. \| ApJ \| 896-95 \| 2020 \| 2020ApJ...896...95O \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...896...95O 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 The XMM-Newton Line Emission Analysis Program (X-LEAP). I. Emission-line Survey of O VII, O VIII, and Fe L-shell Transitions \|Pan, Zeyang, Qu, Zhijie, et al. \| ApJS \| 271-62 \| 2024 \| 2024ApJS..271...62P \| http://ui.adsabs.harvard.edu/#abs/2024ApJS..271...62P 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	2012-06-28T05:14:19Z/2012-06-28T09:39:35Z
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	2013-07-21T00:00:00Z
Keywords	"type iasupernova2003lx", "circumstellar interaction", "XMM", "circumstellar medium csm", "fast moving debris", "exploded star", "merged image", "concrete xray supernovaia", "sigma source detection", "XMM-Newton", "xray emission", "spectral properties", "mass loss history", "swift pixels", "xmm newton", "exploded system"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr C.S.J. Pun, 2013, 'Circumstellar Interaction in Type Ia Supernova 2003lx', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-5cimz8t