A dataset provided by the European Space Agency

Name: Energy and Environment of Hydrogen-poor Core-Collapse SNe
Published: 2017-06-14T22:00:00Z

Proposal ID	076261
Title	Energy and Environment of Hydrogen-poor Core-Collapse SNe
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0762610401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0762610501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0762610701 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0762610801
DOI	https://doi.org/10.5270/esa-o59gq9f
Principal Investigator, PI	Dr Raffaella Margutti
Abstract	Envelope-stripped, core-collapse SNe (i.e. Type Ibc SNe) were recognized as adistinct flavor of core-collapse explosions 25 years ago. SNe Ibc have onlyrecently enjoyed a surge of interest thanks to their association with Gamma-RayBursts (GRBs). The peculiar circumstances that enable a small fraction of SNeIbc to launch a relativistic jet are not understood. Along the same line, theprogenitors of SNe Ibc and their relation to those of GRBs have yet to beobservationally identified. Here we propose a focused XMM program to enableprogress. The primary goals are to (i) populate the gap between ordinary typeIbc SNe and GRBs and (ii) to probe the diversity of the environment of ordinarySNe arising from envelope-stripped progenitors.
Publications	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 Digging a little deeper: characterizing three new extreme ULX candidates \|Roberts T. P. Walton D. J. et al. \| MNRAS \| 525-3330 \| 2023 \| 2023MNRAS.525.3330R \| http://ui.adsabs.harvard.edu/#abs/2023MNRAS.525.3330R 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	2016-04-18T04:53:06Z/2016-05-16T05:58:53Z
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	2017-06-14T22:00:00Z
Last Update	2025-01-27
Keywords	"core collapse sne", "envelope stripped", "core collapse explosions", "sne ibc", "focused xmm program", "type ibc sne", "distinct flavor", "envelope stripped progenitors", "relativistic jet", "XMM", "ordinary sne"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Raffaella Margutti, 2017, 'Energy and Environment of Hydrogen-poor Core-Collapse SNe', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-o59gq9f