The Palomar Transient Factory core-collapse supernova host-galaxy sample. I. Host-galaxy distribution functions and environment dependence of core-collapse …

S Schulze, O Yaron, J Sollerman… - The Astrophysical …, 2021 - iopscience.iop.org
Several thousand core-collapse supernovae (CCSNe) of different flavors have been
discovered so far. However, identifying their progenitors has remained an outstanding open …

Investigating the properties of stripped-envelope supernovae; what are the implications for their progenitors?

SJ Prentice, C Ashall, PA James, L Short… - Monthly Notices of …, 2019 - academic.oup.com
We present observations and analysis of 18 stripped-envelope supernovae observed during
2013–2018. This sample consists of five H/He-rich SNe, six H-poor/He-rich SNe, three …

The effect of environment on Type Ia supernovae in the Dark Energy Survey three-year cosmological sample

L Kelsey, M Sullivan, M Smith… - Monthly Notices of …, 2021 - academic.oup.com
ABSTRACT Analyses of Type Ia supernovae (SNe Ia) have found puzzling correlations
between their standardized luminosities and host galaxy properties: SNe Ia in high-mass …

Galaxies hosting an active galactic nucleus: a view from the CALIFA survey

EAD Lacerda, SF Sánchez… - Monthly Notices of …, 2020 - academic.oup.com
We study the presence of optically-selected active galactic nuclei (AGNs) within a sample of
867 galaxies extracted from the extended Calar-Alto Legacy Integral Field spectroscopy …

Concerning colour: The effect of environment on type Ia supernova colour in the dark energy survey

L Kelsey, M Sullivan, P Wiseman… - Monthly Notices of …, 2023 - academic.oup.com
Recent analyses have found intriguing correlations between the colour (c) of type Ia
supernovae (SNe Ia) and the size of their 'mass-step', the relationship between SN Ia host …

A meta-analysis of core-collapse supernova 56Ni masses

JP Anderson - Astronomy & Astrophysics, 2019 - aanda.org
Context. A fundamental property determining the transient behaviour of core-collapse
supernovae (CC SNe) is the amount of radioactive 56 Ni synthesised in the explosion. Using …

pyFIT3D and pyPipe3D—The new version of the integral field spectroscopy data analysis pipeline

EAD Lacerda, SF Sánchez, A Mejía-Narváez… - New Astronomy, 2022 - Elsevier
We present a new version of the FIT3D and Pipe3D codes, two packages to derive
properties of the stellar populations and the ionized emission lines from optical spectroscopy …

The Carnegie Supernova Project-I: Correlation between Type Ia Supernovae and Their Host Galaxies from Optical to Near-infrared Bands

SA Uddin, CR Burns, MM Phillips… - The Astrophysical …, 2020 - iopscience.iop.org
We present optical and near-infrared (NIR)(ugriYJH) photometry of host galaxies of Type Ia
supernovae (SN Ia) observed by the Carnegie Supernova Project-I. We determine host …

A galaxy-driven model of type Ia supernova luminosity variations

P Wiseman, M Vincenzi, M Sullivan… - Monthly Notices of …, 2022 - academic.oup.com
ABSTRACT Type Ia supernovae (SNe Ia) are used as standardizable candles to measure
cosmological distances, but differences remain in their corrected luminosities which display …

The Diverse Properties of Type Icn Supernovae Point to Multiple Progenitor Channels

C Pellegrino, DA Howell, G Terreran… - The Astrophysical …, 2022 - iopscience.iop.org
We present a sample of Type Icn supernovae (SNe Icn), a newly discovered class of
transients characterized by their interaction with H-and He-poor circumstellar material …