A dataset provided by the European Space Agency

Name: Probing the Energetics and Environments of Hydrogen-poor Core-Collapse SNe
Published: 2017-07-12T22:00:00Z

Proposal ID	078242
Title	Probing the Energetics and Environments of Hydrogen-poor Core-Collapse SNe
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0782420201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0782420301
DOI	https://doi.org/10.5270/esa-xn5i2up
Principal Investigator, PI	Dr Raffaella Margutti
Abstract	Envelope-stripped, core-collapse SNe (i.e. Type Ibc) have recently enjoyed asurge of interest thanks to their association with Gamma-Ray Bursts (GRBs). Thepeculiar circumstances that enable a small fraction of SNe Ibc to launch arelativistic jet are not understood. Along the same line, the progenitors of SNeIbc and their relation to those of GRBs have yet to be observationallyidentified. Here we propose a continuation of our XMM program, as part of ourmulti-wavelength effort, to enable progress. The primary goals are: (i)Constrain the pre-SN mass-loss history of the progenitor star by sampling theenvironment around H-stripped core-collapse SNe. (ii) Constrain the presence ofengines driving the explosion of the most energetic SNe Ibc that are NOT observationally associated with GRBs.
Publications	SN 2016coi (ASASSN-16fp): An Energetic H-stripped Core-collapse Supernova from a Massive Stellar Progenitor with Large Mass Loss \|Terreran, G., Margutti, R., et al. \| ApJ \| 883-147 \| 2019 \| 2019ApJ...883..147T \| http://ui.adsabs.harvard.edu/#abs/2019ApJ...883..147T 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 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	2016-06-06T05:42:57Z/2016-06-22T12:37:15Z
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	2017-07-12T22:00:00Z
Keywords	"XMM", "progenitor star", "sne ibc", "engines driving", "ii constrain", "core collapse sne", "relativistic jet", "multi wavelength effort", "envelope stripped", "xmm program", "type ibc", "energetic sne ibc"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Raffaella Margutti, 2017, 'Probing the Energetics and Environments of Hydrogen-poor Core-Collapse SNe', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-xn5i2up