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 I superluminous supernovae (SLSNe) in transient alert streams.
Sebastian Gomez +7 more
doaj +1 more source
Core-collapse supernovae: Reflections and directions [PDF]
36 pages, 20 figures (43 eps files); submitted to Progress of Theoretical and Experimental Physics (PTEP)
H.-T. Janka +5 more
openaire +3 more sources
Effects of Symmetry Energy on the Equation of State for Simulations of Core-collapse Supernovae and Neutron-star Mergers [PDF]
We construct a new equation of state (EOS) for numerical simulations of core-collapse supernovae and neutron-star mergers based on an extended relativistic mean-field model with a small symmetry energy slope L, which is compatible with both experimental ...
Hong Shen +3 more
semanticscholar +1 more source
Relativistic Jets in Core-collapse Supernovae [PDF]
Abstract After decades of extensive research the mechanism driving core-collapse supernovae (CCSNe) is still unclear. One common mechanism is a neutrino-driven outflow, but others have been proposed. Among those, a long-standing idea is that jets play an important role in supernova (SN) explosions. Gamma-ray bursts (GRBs) that accompany “
Tsvi Piran +3 more
openaire +4 more sources
The Palomar Transient Factory Core-collapse Supernova Host-galaxy Sample. I. Host-galaxy Distribution Functions and Environment Dependence of Core-collapse Supernovae [PDF]
Several thousand core-collapse supernovae (CCSNe) of different flavors have been discovered so far. However, identifying their progenitors has remained an outstanding open question in astrophysics.
S. Schulze +56 more
semanticscholar +1 more source
Possible Detection of the Progenitor of the Type II Supernova SN 2023ixf
Stellar evolution theory predicts multiple pathways to the explosive deaths of stars as supernovae. Locating and characterizing the progenitors of well-studied supernovae is important to constrain the theory and to justify and design future surveys to ...
Joanne L Pledger, Michael M Shara
doaj +1 more source
A low energy core-collapse supernova without a hydrogen envelope [PDF]
The final fate of massive stars depends on many factors, including mass, rotation rate, magnetic fields and metallicity. Theory suggests that some massive stars (initially greater than 25-30 solar masses) end up as Wolf-Rayet stars which are deficient in
A Filippenko +43 more
core +2 more sources
The Physics of Core-Collapse Supernovae: Explosion Mechanism and Explosive Nucleosynthesis [PDF]
Recent developments in multi-dimensional simulations of core-collapse supernovae have considerably improved our understanding of this complex phenomenon.
L. Boccioli, L. Roberti
semanticscholar +1 more source
The Sun and core-collapse supernovae are leading probes of the neutrino lifetime [PDF]
The large distances travelled by neutrinos emitted from the Sun and core-collapse supernovae together with the characteristic energy of such neutrinos provide ideal conditions to probe their lifetime, when the decay products evade detection.
P. Mart'inez-Mirav'e +2 more
semanticscholar +1 more source
Type Ic core-collapse supernova explosions evolved from very massive stars [PDF]
We investigate the possibility of a super-luminous Type Ic core-collapse supernovae producing a large amount of 56Ni. Very massive stars with a main-sequence mass larger than 100 Msun and a metallicity 0.001 < Z < 0.004 are expected to explode as super ...
Okita, Shinpei +2 more
core +2 more sources

