A dataset provided by the European Space Agency

Name: Energy source and pre-explosion progenitor evolution of Super-Luminous SNe
Published: 2015-11-28T23:00:00Z

Proposal ID	074311
Title	Energy source and pre-explosion progenitor evolution of Super-Luminous SNe
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0743110301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0743110701
DOI	https://doi.org/10.5270/esa-xi9sxfe
Principal Investigator, PI	Dr Raffaella Margutti
Abstract	With bolometric peak luminosities L >7x10^43 erg/sec, the new class of SuperLuminous Super Novae (SLSNe) outshine ordinary SNe of more than a factor 10 andrepresent the death of the most massive stars in our Universe. Their exceptionalluminosity requires exotic explosion mechanisms and/or sources of energy whosenature is unclear. Here we propose a focused XMM program to map their X-rayemission down to unprecedented limits as part of our multi-wavelength effortthrough our programs on the EVLA (radio), Swift (UV) and optical/NIR facilities.The final aim is to: (i) Pin down the energy source of SLSNe; (ii) Map thediversity of the pre-explosion evolution of their progenitors.
Publications	XMM-Newton publication statistics \|Ness J.-U. Parmar A. N. et al. \| AN \| 335-210 \| 2014 \| 2014AN....335..210N \| http://ui.adsabs.harvard.edu/#abs/2014AN....335..210N 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 Results from a Systematic Survey of X-Ray Emission from Hydrogen-poor Superluminous SNe \|Margutti R. Chornock R. et al. \| ApJ \| 864-45 \| 2018 \| 2018ApJ...864...45M \| http://ui.adsabs.harvard.edu/#abs/2018ApJ...864...45M X-ray properties of high-richness CAMIRA clusters in the Hyper Suprime-Cam Subaru Strategic Program field \|Ota Naomi Mitsuishi Ikuyuki et al. \| PASJ \| 72-1 \| 2020 \| 2020PASJ...72....1O \| http://ui.adsabs.harvard.edu/#abs/2020PASJ...72....1O The composite X-ray spectra of radio-loud and radio-quiet SDSS quasars \|Zhou Min-Hua Gu Min-Feng \| RAA \| 21-4 \| 2021 \| 2021RAA....21....4Z \| http://ui.adsabs.harvard.edu/#abs/2021RAA....21....4Z 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 X-ray view of optically selected dual AGN \|De Rosa Alessandra Vignali Cristian et al. \| MNRAS \| 519-5149 \| 2023 \| 2023MNRAS.519.5149D \| http://ui.adsabs.harvard.edu/#abs/2023MNRAS.519.5149D 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	2014-06-09T02:47:36Z/2014-11-07T15:03:21Z
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	2015-11-28T23:00:00Z
Last Update	2025-01-27
Keywords	"multi wavelength effort", "ii map", "evla radio", "pre explosion evolution", "energy source", "focused xmm program", "nir facilities", "xray emission", "massive stars", "XMM", "bolometric peak luminosities", "super luminous sne", "swift uv", "exotic explosion mechanisms"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Raffaella Margutti, 2015, 'Energy source and pre-explosion progenitor evolution of Super-Luminous SNe', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-xi9sxfe