activity
20122026
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 · 9.4k across the 72 of their papers we have counts for

collaborators
Showing 2022Show all

5 papers · 1 filter

astro-ph.GA2022★ 9 cited

Constraining quenching timescales in galaxy clusters by forward-modelling stellar ages and quiescent fractions in projected phase space

Andrew M. M. Reeves, Michael J. Hudson, Kyle A. Oman

We forward-model mass-weighted stellar ages (MWAs) and quiescent fractions in projected phase space (PPS), using data from the Sloan Digital Sky Survey, to jointly constrain an inf…

astro-ph.GA2022★ 4 cited

The north-south asymmetry of the ALFALFA HI velocity width function

Richard A. N. Brooks, Kyle A. Oman, Carlos S. Frenk

The number density of extragalactic 21-cm radio sources as a function of their spectral line-widths -- the HI width function (HIWF) -- is a sensitive tracer of the dark matter halo…

astro-ph.IM2022★ 5k cited

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

The Astropy Collaboration, Adrian M. Price-Whelan, Pey Lian Lim +133

The Astropy Project supports and fosters the development of open-source and openly-developed Python packages that provide commonly needed functionality to the astronomical communit…

astro-ph.GA2022★ 8 cited

Using EAGLE simulations to study the effect of observational constraints on the determination of HI asymmetries in galaxies

P. V. Bilimogga, K. A. Oman, M. A. W. Verheijen +1

We investigate the effect of observational constraints such as signal-to-noise, resolution and column density level on the HI morphological asymmetry () an…

astro-ph.GA2022★ 40 cited

The diversity of rotation curves of simulated galaxies with cusps and cores

Finn A. Roper, Kyle A. Oman, Carlos S. Frenk +3

We use CDM cosmological hydrodynamical simulations to explore the kinematics of gaseous discs in late-type dwarf galaxies. We create high-resolution 21-cm 'observations' of simu…