A search for extragalactic fast blue optical transients in ZTF and the rate of AT2018cow-like transients
We present a search for extragalactic fast blue optical transients (FBOTs) during Phase I of
the Zwicky Transient Facility (ZTF). We identify 38 candidates with durations above half …
the Zwicky Transient Facility (ZTF). We identify 38 candidates with durations above half …
Seven Years of Coordinated Chandra–NuSTAR Observations of SN 2014C Unfold the Extreme Mass-loss History of Its Stellar Progenitor
D Brethauer, R Margutti, D Milisavljevic… - The Astrophysical …, 2022 - iopscience.iop.org
We present the results from our 7 yr long broadband X-ray observing campaign of SN
2014C with Chandra and NuSTAR. These coordinated observations represent the first look …
2014C with Chandra and NuSTAR. These coordinated observations represent the first look …
A pre-explosion effervescent zone for the circumstellar material in SN 2023ixf
N Soker - Research in Astronomy and Astrophysics, 2023 - iopscience.iop.org
I present the effervescent zone model to account for the compact dense circumstellar
material (CSM) around the progenitor of the core collapse supernova (CCSN) SN 2023ixf …
material (CSM) around the progenitor of the core collapse supernova (CCSN) SN 2023ixf …
Oxygen and calcium nebular emission line relationships in core-collapse supernovae and Ca-rich transients
SJ Prentice, K Maguire, L Siebenaler… - Monthly Notices of the …, 2022 - academic.oup.com
This work examines the relationships between the properties (flux ratios, full width at half-
maximum velocities) of the [O i] λλ6300, 6364,[Ca ii] λλ7291, 7323, and the Ca ii near …
maximum velocities) of the [O i] λλ6300, 6364,[Ca ii] λλ7291, 7323, and the Ca ii near …
The Type II supernova SN 2020jfo in M 61, implications for progenitor system, and explosion dynamics
J Sollerman, S Yang, S Schulze… - Astronomy & …, 2021 - aanda.org
We present the discovery and extensive follow-up observations of SN 2020jfo, a Type IIP
supernova (SN) in the nearby (14.5 Mpc) galaxy M 61. Optical light curves (LCs) and spectra …
supernova (SN) in the nearby (14.5 Mpc) galaxy M 61. Optical light curves (LCs) and spectra …
Radio Analysis of SN2004C Reveals an Unusual CSM Density Profile as a Harbinger of Core Collapse
L DeMarchi, R Margutti, J Dittman… - The Astrophysical …, 2022 - iopscience.iop.org
We present extensive multifrequency Karl G. Jansky Very Large Array (VLA) and Very Long
Baseline Array (VLBA) observations of the radio-bright supernova (SN) IIb SN 2004C that …
Baseline Array (VLBA) observations of the radio-bright supernova (SN) IIb SN 2004C that …
SN 2020bio: A Double-peaked, H-poor Type IIb Supernova with Evidence of Circumstellar Interaction
We present photometric and spectroscopic observations of SN 2020bio, a double-peaked
Type IIb supernova (SN) discovered within a day of explosion, primarily obtained by Las …
Type IIb supernova (SN) discovered within a day of explosion, primarily obtained by Las …
Photometric and spectroscopic evolution of the interacting transient AT 2016jbu (Gaia16cfr)
SJ Brennan, M Fraser, J Johansson… - Monthly Notices of …, 2022 - academic.oup.com
We present the results from a high-cadence, multiwavelength observation campaign of AT
2016jbu (aka Gaia16cfr), an interacting transient. This data set complements the current …
2016jbu (aka Gaia16cfr), an interacting transient. This data set complements the current …
A Pre-explosion Extended Effervescent Zone around Core-collapse Supernova Progenitors
N Soker - The Astrophysical Journal, 2020 - iopscience.iop.org
I propose a scenario according to which the dense compact circumstellar matter (CSM) that
the ejecta of many core-collapse supernovae (CCSNe) collide with within several days after …
the ejecta of many core-collapse supernovae (CCSNe) collide with within several days after …
Modeling the remnants of core-collapse supernovae from luminous blue variable stars
S Ustamujic, S Orlando, M Miceli, F Bocchino… - Astronomy & …, 2021 - aanda.org
Context. Luminous blue variable stars (LBVs) are massive evolved stars that suffer sporadic
and violent mass-loss events. They have been proposed as the progenitors of some core …
and violent mass-loss events. They have been proposed as the progenitors of some core …