A dataset provided by the European Space Agency

Name 074311
Title Energy source and pre-explosion progenitor evolution of Super-Luminous SNe
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0743110301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0743110701

DOI 10.5270/esa-xi9sxfe
Author Dr Raffaella Margutti
Description With bolometric peak luminosities L >7x10^43 erg-sec, the new class of Super Luminous Super Novae (SLSNe) outshine ordinary SNe of more than a factor 10 and represent the death of the most massive stars in our Universe. Their exceptional luminosity requires exotic explosion mechanisms and-or sources of energy whose nature is unclear. Here we propose a focused XMM program to map their X-ray emission down to unprecedented limits as part of our multi-wavelength effort through 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 the diversity of the pre-explosion evolution of their progenitors.
Publication XMM-Newton publication statistics . Ness, J.-U., Parmar, A. N., et all. . AN . 335-210 . 2014 . 2014AN....335..210N ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
Results from a Systematic Survey of X-Ray Emission from Hydrogen-poor Superluminous SNe . Margutti, R., Chornock, R., et all. . ApJ . 864-45 . 2018 . 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 all. . PASJ . 72-1 . 2020 . 2020PASJ...72....1O ,
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 Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's 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 Earth's 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
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2015-11-28T23:00:00Z, 074311, 17.56_20190403_1200. https://doi.org/10.5270/esa-xi9sxfe