The Zwicky Transient Facility Bright Transient Survey. II. A public statistical sample for exploring supernova demographics

DA Perley, C Fremling, J Sollerman… - The Astrophysical …, 2020 - iopscience.iop.org
We present a public catalog of transients from the Zwicky Transient Facility (ZTF) Bright
Transient Survey, a magnitude-limited (m< 19 mag in either the g or r filter) survey for …

A measurement of the Hubble constant from Type II supernovae

T De Jaeger, BE Stahl, W Zheng… - Monthly Notices of …, 2020 - academic.oup.com
Progressive increases in the precision of the Hubble-constant measurement via Cepheid-
calibrated Type Ia supernovae (SNe Ia) have shown a discrepancy of∼ 4.4 σ with the …

Type II supernovae from the Carnegie Supernova Project-I-II. Physical parameter distributions from hydrodynamical modelling

L Martinez, MC Bersten, JP Anderson… - Astronomy & …, 2022 - aanda.org
Linking supernovae to their progenitors is a powerful method for furthering our
understanding of the physical origin of their observed differences while at the same time …

Type II-P supernova progenitor star initial masses and SN 2020jfo: direct detection, light-curve properties, nebular spectroscopy, and local environment

CD Kilpatrick, L Izzo, RO Bentley… - Monthly Notices of …, 2023 - academic.oup.com
We present optical, ultraviolet, and infrared data of the type II supernova (SN II) 2020jfo at
14.5 Mpc. This wealth of multiwavelength data allows us to compare different metrics …

Weak mass loss from the red supergiant progenitor of the type II SN 2021yja

G Hosseinzadeh, CD Kilpatrick, Y Dong… - The Astrophysical …, 2022 - iopscience.iop.org
We present high-cadence optical, ultraviolet (UV), and near-infrared data of the nearby (D≈
23 Mpc) Type II supernova (SN) 2021yja. Many Type II SNe show signs of interaction with …

The early phases of supernova 2020pni: shock ionization of the nitrogen-enriched circumstellar material

G Terreran, WV Jacobson-Galán, JH Groh… - The Astrophysical …, 2022 - iopscience.iop.org
We present multiwavelength observations of the Type II SN 2020pni. Classified at∼ 1.3
days after explosion, the object showed narrow (FWHM intensity< 250 km s− 1) …

The radio luminosity-risetime function of core-collapse supernovae

MF Bietenholz, N Bartel, M Argo, R Dua… - The Astrophysical …, 2021 - iopscience.iop.org
We assemble a large set of 2–10 GHz radio flux density measurements and upper limits of
294 different supernovae (SNe), from the literature and our own and archival data. Only 31 …

The morphing of decay powered to interaction powered Type II supernova ejecta at nebular times

L Dessart, CP Gutiérrez, H Kuncarayakti… - Astronomy & …, 2023 - aanda.org
There is significant astronomical interest around the intense mass loss that appears to take
place in some massive stars immediately before core collapse. However, because it occurs …

The late time optical evolution of twelve core-collapse supernovae: detection of normal stellar winds

M Rizzo Smith, CS Kochanek… - Monthly Notices of the …, 2023 - academic.oup.com
We analyse the late time evolution of 12 supernovae (SNe) occurring over the last∼ 41 yr,
including nine Type IIP/L, two IIb, and one Ib/c, using UBVR optical data from the Large …

Inferencing Progenitor and Explosion Properties of Evolving Core-collapse Supernovae from Zwicky Transient Facility Light Curves

BM Subrayan, D Milisavljevic, TJ Moriya… - The Astrophysical …, 2023 - iopscience.iop.org
We analyze a sample of 45 Type II supernovae from the Zwicky Transient Facility public
survey using a grid of hydrodynamical models in order to assess whether theoretically …