Robert C. Nichol

TL;DR: In this paper, spectral indicators measured up to a month after the lightcurve peak luminosity were used to characterise the supernova properties, and examined these for potential correlations with host galaxy type, light curveve shape, color excess, and redshift.

TL;DR: In this paper, the authors identify quenching slow rotators in the MaNGA sample by selecting those which lie below the star forming sequence and identify a sample of fast rotators which were matched in stellar mass.

TL;DR: The Deep Underground Neutrino Experiment (DUNE) is a powerful tool for a variety of physics topics, as it enables opportunities not only to perform precision neutrino measurements that may uncover deviations from the present three-flavor mixing paradigm, but also to discover new particles and unveil new interactions and symmetries beyond those predicted in the Standard Model (SM).

TL;DR: In this paper, the authors investigate the properties of satellite galaxies that surround isolated hosts within the redshift range 0.01 < z < 0.15, using data taken as part of the Galaxy And Mass Assembly survey.

TL;DR: In this article, boosting and kernel density estimation techniques which have minimal astrophysical input, and compare their performance on 20,000 simulated Dark Energy Survey lightcurves, are presented.