This paper introduces C olossus, a public, open-source python package for calculations
related to cosmology, the large-scale structure (LSS) of matter in the universe, and the …

We present simulations from the new" Figuring Out Gas & Galaxies in Enzo"(FOGGIE)
project. In contrast to most extant simulations of galaxy formation, which concentrate …

The Kepler survey provides a statistical census of planetary systems out to the habitable
zone. Because most planets are non-transiting, orbital architectures are best estimated …

This paper describes the design and implementation of stingray, a library in Python built to
perform time series analysis and related tasks on astronomical light curves. Its core …

With the release of Gaia DR2, it is now possible to measure the proper motions (PMs) of the
lowest-mass, ultrafaint satellite galaxies in the Milky Way's (MW) halo for the first time. Many …

We estimate the mass of the Milky Way (MW) within 21.1 kpc using the kinematics of halo
globular clusters (GCs) determined by Gaia. The second Gaia data release (DR2) contained …

We publicly release a new sample of 34 medium resolution quasar spectra at 5.77≤ z em≤
6.54 observed with the Echellette Spectrograph and Imager on the Keck telescope. This …

The second data release from the Gaia mission (DR2) provides a comprehensive and
unprecedented picture of the motions of astronomical sources in the plane of the sky …

Over the past few decades, the measurement precision of some pulsar timing experiments
has advanced from∼ 10 μs to∼ 10 ns, revealing many subtle phenomena. Such high …

We present 2–9 GHz radio observations of GW170817 covering the period 125–200 days
post-merger, taken with the Australia Telescope Compact Array (ATCA) and the Karl G …