activity
20142022
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 · 5.2k across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.IM20225k 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.GA20218 cited

Measuring the alpha-abundance of subsolar-metallicity stars in the Milky Way's central half-parsec: testing globular cluster and dwarf galaxy infall scenarios

Rory O. Bentley, Tuan Do, Wolfgang Kerzendorf +4

While the Milky Way Nuclear star cluster has been studied extensively, how it formed is uncertain. Studies have shown it contains a solar and supersolar metallicity population that…

astro-ph.GA20162 cited

Observational constraints on the formation and evolution of the Milky Way nuclear star cluster with Keck and Gemini

Tuan Do, Andrea Ghez, Mark Morris +7

Due to its proximity, the Milky Way nuclear star cluster provides us with a wealth of data not available in other galactic nuclei. In particular, with adaptive optics, we can obser…

astro-ph.GA201696 cited

KMOS view of the Galactic Centre - II. Metallicity distribution of late-type stars

A. Feldmeier-Krause, W. Kerzendorf, N. Neumayer +5

Knowing the metallicity distribution of stars in the Galactic Centre has important implications for the formation history of the Milky Way nuclear star cluster. However, this distr…

astro-ph.SR201440 cited

Spectroscopy of the Type Ia supernova 2011fe past 1000 days

S. Taubenberger, N. Elias-Rosa, W. E. Kerzendorf +11

In this letter we present an optical spectrum of SN 2011fe taken 1034 d after the explosion, several hundred days later than any other spectrum of a Type Ia supernova (disregarding…

astro-ph.SR201414 cited

Radial velocity measurements of the pulsating zirconium star: LS IV -14 116

C. Simon Jeffery, Amir Ahmad, Naslim Neelamkodan +1

The helium-rich hot subdwarf LS IV -14 116 shows remarkably high surface abundances of zirconium, yttrium, strontium, and germanium, indicative of strong chemical stratification in…