The Type I superluminous supernova catalogue I: light-curve properties, models, and catalogue description
We present the most comprehensive catalogue to date of Type I superluminous supernovae
(SLSNe), a class of stripped-envelope supernovae (SNe) characterized by exceptionally …
(SLSNe), a class of stripped-envelope supernovae (SNe) characterized by exceptionally …
Integral Field Spectroscopy of 13 Tidal Disruption Event Hosts from the Zwicky Transient Facility Survey
E Hammerstein, SB Cenko, S Gezari… - The Astrophysical …, 2023 - iopscience.iop.org
The host galaxies of tidal disruption events (TDEs) have been shown to possess peculiar
properties, including high central light concentrations, unusual star formation histories, and" …
properties, including high central light concentrations, unusual star formation histories, and" …
The first two years of FLEET: an active search for superluminous supernovae
In 2019 November, we began operating Finding Luminous and Exotic Extragalactic
Transients (FLEET), a machine-learning algorithm designed to photometrically identify Type …
Transients (FLEET), a machine-learning algorithm designed to photometrically identify Type …
Needle in a Haystack: Finding Supermassive Black Hole-related Flares in the Zwicky Transient Facility Public Survey
Y Dgany, I Arcavi, L Makrygianni… - The Astrophysical …, 2023 - iopscience.iop.org
Transient accretion events onto supermassive black holes (SMBHs), such as tidal disruption
events (TDEs), Bowen Fluorescence Flares (BFFs), and active galactic nuclei (AGNs), which …
events (TDEs), Bowen Fluorescence Flares (BFFs), and active galactic nuclei (AGNs), which …
Metallicity beats sSFR: the connection between superluminous supernova host galaxy environments and the importance of metallicity for their production
C Cleland, SL McGee, M Nicholl - Monthly Notices of the Royal …, 2023 - academic.oup.com
We analyse 33 Type I superluminous supernovae (SLSNe) taken from Zwicky Transient
Facility (ZTF)'s Bright Transient Survey to investigate the local environments of their host …
Facility (ZTF)'s Bright Transient Survey to investigate the local environments of their host …
Post maximum light and late time optical imaging polarimetry of type I superluminous supernova 2020znr
F Poidevin, CMB Omand… - Monthly Notices of …, 2022 - academic.oup.com
Optical imaging polarimetry was conducted on the hydrogen poor superluminous supernova
2020znr during three phases after maximum light (≈+ 34 d,+ 288 d, and+ 289 d). After …
2020znr during three phases after maximum light (≈+ 34 d,+ 288 d, and+ 289 d). After …
Quantifying the'Needle in a Haystack'Problem of Finding Supermassive Black Hole Related Flares in the ZTF Public Survey
Transient accretion events onto supermassive black holes (SMBHs), such as Tidal
Disruption Events (TDEs), Bowen Fluorescence Flares (BFFs), and active galactic nuclei …
Disruption Events (TDEs), Bowen Fluorescence Flares (BFFs), and active galactic nuclei …
Integral Field Spectroscopy of 13 Tidal Disruption Event Hosts from the ZTF Survey
The host galaxies of tidal disruption events (TDEs) have been shown to possess peculiar
properties, including high central light concentrations, unusual star-formation histories …
properties, including high central light concentrations, unusual star-formation histories …
Population Studies of Tidal Disruption Events and Their Hosts: Understanding Host Galaxy Preferences and the Origin of the Ultraviolet and Optical Emission
E Hammerstein - 2024 - search.proquest.com
It is well-established that the majority of galaxies harbor a supermassive black hole (SMBH)
in their nucleus. While some of these SMBHs are easily studied either through signatures of …
in their nucleus. While some of these SMBHs are easily studied either through signatures of …
[PDF][PDF] Post maximum light and late time optical imaging polarimetry of superluminous supernova SN2020znr
F Poidevin, CMB Omand, I Pérez-Fournon, R Clavero… - 2021 - research.iac.es
Optical imaging polarimetry was conducted on the hydrogen poor superluminous supernova
SN2020znr during 3 phases after maximum light (≈+ 34 days,+ 288 days and+ 289 days) …
SN2020znr during 3 phases after maximum light (≈+ 34 days,+ 288 days and+ 289 days) …