activity
20042024
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 · 11.4k across the 68 of their papers we have counts for

collaborators

69 papers

astro-ph.SR2024★ 17 cited

An updated modular set of synthetic spectral energy distributions for young stellar objects

Theo Richardson, Adam Ginsburg, Rémy Indebetouw +1

Measured properties of young stellar objects (YSOs) are key tools for research into pre-main-sequence stellar evolution. YSO properties are commonly measured by comparing observed…

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.SR2020★ 21 cited

A Detailed View of the Circumstellar Environment and Disk of the Forming O-star AFGL 4176

K. G. Johnston, M. G. Hoare, H. Beuther +5

We present a detailed analysis of the disk and circumstellar environment of the forming O-type star AFGL 4176 mm1, placing results from the Atacama Large Millimeter/submillimeter A…

astro-ph.GA2020★ 169 cited

A Galactic-scale gas wave in the Solar Neighborhood

João Alves, Catherine Zucker, Alyssa A. Goodman +6

For the past 150 years, the prevailing view of the local Interstellar Medium (ISM) was based on a peculiarity known as the Gould's Belt, an expanding ring of young stars, gas, and…

astro-ph.SR2019★ 53 cited

Spiral arms and instability within the AFGL 4176 mm1 disc

K. G. Johnston, M. G. Hoare, H. Beuther +7

We present high-resolution (30 mas or 130 au at 4.2 kpc) Atacama Large Millimeter/submillimeter Array observations at 1.2 mm of the disc around the forming O-type star AFGL 4176 mm…

astro-ph.SR2019★ 15 cited

The Duration of Star Formation in Galactic Giant Molecular Clouds. I. The Great Nebula in Carina

Matthew S. Povich, Jessica T. Maldonado, Evan Haze Nuñez +1

We present a novel infrared spectral energy distribution (SED) modeling methodology that uses likelihood-based weighting of the model fitting results to construct probabilistic H-R…