A dataset provided by the European Space Agency

Name: Mind the openParLuminosityclosePar Gap: A Test of the Magnetar-SLSN Connection With SN 2015bn
Published: 2018-06-29T22:00:00Z

Proposal ID	080286
Title	Mind the (Luminosity) Gap: A Test of the Magnetar-SLSN Connection With SN 2015bn
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0802860201
DOI	https://doi.org/10.5270/esa-cht6olp
Principal Investigator, PI	Prof Ryan Chornock
Abstract	We propose a deep late-time observation with XMM-Newton of one of the nearestknown superluminous supernovae (SLSNe), 2015bn, to perform a focused test of themodel for the optical emission of hydrogen-poor SLSNe that is powered by thespindown energy of a rapidly rotating newly born magnetar. Our early-timeobservations of SN 2015bn with XMM-Newton resulted in non-detections. However,at times later than 250 days after peak, the optical light curve of this objecthas now started to decay more rapidly than the input of energy of thehypothesized magnetar. We seek to test the hypothesis that high-energy emissionfrom the magnetar has ionized the ejecta, leading to a breakout of X-rays thatshould now be observable with XMM-Newton.
Publications	Where is the Engine Hiding Its Missing Energy? Constraints from a Deep X-Ray Non-detection of the Superluminous SN 2015bn \|Bhirombhakdi, Kornpob, Chornock, Ryan, et al. \| ApJ \| 868-32 \| 2018 \| 2018ApJ...868L..32B \| http://ui.adsabs.harvard.edu/#abs/2018ApJ...868L..32B Blasts from the Past: Supernova Shock Breakouts among X-Ray Transients in the XMM-Newton Archive \|Alp, Dennis, Larsson, Josefin, \| ApJ \| 896-39 \| 2020 \| 2020ApJ...896...39A \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...896...39A 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 Luminosity Function and Event Rate Density of XMM-Newton-selected Supernova Shock Breakout Candidates \|Sun, Hui, Liu, He-Yang, et al. \| ApJ \| 927-224 \| 2022 \| 2022ApJ...927..224S \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...927..224S XMM-Newton-discovered Fast X-ray Transients: host galaxies and limits on contemporaneous detections of optical counterparts \|Eappachen, D., Jonker, P. G., et al. \| MNRAS \| 527-11823 \| 2024 \| 2024MNRAS.52711823E \| http://ui.adsabs.harvard.edu/#abs/2024MNRAS.52711823E 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	2017-06-05T16:17:41Z/2017-06-06T03:04:21Z
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	2018-06-29T22:00:00Z
Keywords	"optical light curve", "focused test", "energy emission", "XMM", "optical emission", "hypothesized magnetar", "born magnetar", "superluminous supernova slsne", "XMM-Newton", "xmm newton resulted", "deep late time", "spindown energy", "luminosity gap", "xmm newton"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Prof Ryan Chornock, 2018, 'Mind the openParLuminosityclosePar Gap: A Test of the Magnetar-SLSN Connection With SN 2015bn', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-cht6olp