Results 101 to 110 of about 5,737 (225)
Thesis dataset: Core-collapse supernovae in the Dark Energy Survey [PDF]
This data set contains the data underpinning the thesis "Core-collapse supernovae in the Dark Energy Survey"
Sullivan, Mark +4 more
core +1 more source
Discovery of a Relativistic Stripped-envelope Type Ic-BL Supernova at z = 2.83 with JWST
We present James Webb Space Telescope (JWST) NIRCam and NIRSpec observations of a Type Ic supernova (SN Ic) and its host galaxy (JADES-GS+53.13533-27.81457) at z = 2.83. This SN (named SN 2023adta) was identified in deep JWST/NIRCam imaging from the JWST
M. R. Siebert +28 more
doaj +1 more source
Diffuse neutrino background from past core collapse supernovae. [PDF]
Ando S, Ekanger N, Horiuchi S, Koshio Y.
europepmc +1 more source
Gravitational Waves due to Population III Core Collapse Supernovae [PDF]
Faculty Advisor: Professor Vuk MandicMy goal was to examine the accuracy of the claim in Sandick et al (2006) that LIGO would be able to observe Gravitational Waves emitted from the core collapse supernovae of Population III stars.This research was ...
Lovdal, Christopher
core
SN 2014C: A Metamorphic Supernova Exploded in the Intricate and Hydrogen-rich Surroundings
We present photometric and spectroscopic observations of supernova (SN) SN 2014C, primarily emphasizing the initial month after the explosion at approximately daily intervals.
Qian Zhai +8 more
doaj +1 more source
The role of the hadron-quark phase transition in core-collapse supernovae. [PDF]
Jakobus P +5 more
europepmc +1 more source
This is a pre-print of a chapter for the Encyclopedia of Astrophysics (edited by I. Mandel, section editor F.R.N.
Jerkstrand, Anders +2 more
openaire +2 more sources
Shock-cooling Constraints via Early-time Observations of the Type IIb SN 2022hnt
We report the results of a rapid follow-up campaign on the Type IIb supernova (SN) 2022hnt. We present a daily, multiband, photometric follow-up using the Las Cumbres Observatory, the Zwicky Transient Facility, the orbiting Swift observatory, and the ...
Joseph R. Farah +13 more
doaj +1 more source
We present complete spectropolarimetric coverage of the Type II supernova (SN) 2023ixf, ranging from 1 to 120 days after explosion. Polarimetry was obtained with the Kast double spectrograph on the Shane 3 m telescope at Lick Observatory.
Sergiy S. Vasylyev +17 more
doaj +1 more source
SN 2024aecx: A Double-peaked Rapidly Evolving Type IIb Supernova at 11 Mpc
We present the results of low-resolution spectroscopic and densely sampled multiband photometric follow-up of supernova (SN) 2024aecx. The SN was discovered in the spiral galaxy NGC 3521 (distance ∼ 11 Mpc) within a day after the explosion.
Xingzhu Zou +30 more
doaj +1 more source

