output
20022025
most citedThe Astropy Project: Sustaining and Growing a Community-oriented Open-source Project and the Latest Major Release (v5.0) of the Core Package

5k citations

Showing 2019Show all

97 papers · 1 filter

astro-ph.HE201923 cited

LSQ13ddu: A rapidly-evolving stripped-envelope supernova with early circumstellar interaction signatures

Peter Clark, Kate Maguire, Cosimo Inserra +30

This paper describes the rapidly evolving and unusual supernova LSQ13ddu, discovered by the La Silla-QUEST survey. LSQ13ddu displayed a rapid rise of just 4.80.9 d to reach a…

physics.atom-ph201921 cited

Modeling tomographic measurements of photoelectron vortices in counter-rotating circularly polarized laser pulses

G. S. J. Armstrong, D. D. A. Clarke, J. Benda +3

Recent experiments [D. Pengel, S. Kerbstadt, L. Englert, T. Bayer, and M. Wollenhaupt, \href{https://journals.aps.org/pra/abstract/10.1103/PhysRevA.96.043426}{{\PRA} {\bf 96} 04342…

astro-ph.HE201955 cited

Determining the Ni distribution of type Ia supernovae from observations within days of explosion

M. R. Magee, K. Maguire, R. Kotak +4

Recent studies have shown how the distribution of Ni within the ejecta of type Ia supernovae can have profound consequences on the observed light curves. Observations at ear…

astro-ph.SR20193 cited

The NGC 346 massive star census: Nitrogen abundances for apparently single, narrow lined, hydrogen core burning B-type stars

P. L. Dufton, C. J. Evans, D. J. Lennon +1

Analyses of large spectroscopic surveys of early-type stars in the LMC have found an excess of nitrogen enriched B-type targets with a vsini<40 km/s compared with the predictions o…

astro-ph.SR201910 cited

First evidence of enhanced recombination in astrophysical environments and the implications for plasma diagnostics

A. Nemer, N. C. Sterling, J. Raymond +6

We report the first unambiguous observational evidence of Rydberg Enhanced Recombination (RER), a potentially important recombination mechanism that has hitherto been unexplored in…

astro-ph.HE201954 cited

Monte Carlo radiative transfer for the nebular phase of Type Ia supernovae

L. J. Shingles, S. A. Sim, M. Kromer +9

We extend the range of validity of the ARTIS 3D radiative transfer code up to hundreds of days after explosion, when Type Ia supernovae are in their nebular phase. To achieve this,…