A dataset provided by the European Space Agency

Name: Energy source and pre-explosion progenitor evolution of SuperLuminous Supernovae
Published: 2018-01-19T23:00:00Z

Proposal ID	078250
Title	Energy source and pre-explosion progenitor evolution of SuperLuminous Supernovae
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0782500201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0782500301
DOI	https://doi.org/10.5270/esa-y0w5hao
Principal Investigator, PI	Dr Raffaella Margutti
Abstract	With bolometric luminosities reaching Lvirgul10^45 erg/sec, the new class of SuperLuminous Supernovae (SLSNe) outshine ordinary SNe a factor 100 and represent thedeath of the most massive stars in our Universe. Their exceptional luminosityrequires exotic explosion mechanisms and/or sources of energy whose nature isunclear. Here we propose a continuation of our successful XMM program to maptheir X-ray emission down to unprecedented limits as part of ourmulti-wavelength effort through our programs on the VLA (radio), Swift (UV) andoptical/NIR facilities. The final aim is to: (i) Pin down the energy source ofSLSNe; (ii) Map the diversity of the pre-explosion evolution of theirprogenitors.
Publications	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	2016-06-08T21:26:37Z/2016-12-25T19:42:21Z
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	2018-01-19T23:00:00Z
Keywords	"vla radio", "superluminous supernova", "XMM", "swift uv", "successful xmm program", "massive stars", "exotic explosion mechanisms", "pre explosion evolution", "energy source", "bolometric luminosities", "multi wavelength effort", "xray emission", "nir facilities", "ii map"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Raffaella Margutti, 2018, 'Energy source and pre-explosion progenitor evolution of SuperLuminous Supernovae', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-y0w5hao