The Preparation of the GTC for the Scientific Operation of CanariCam
CanariCam is a mid-IR camera and spectrograph with coronographic and polarimetric capabilities, built by the University of Florida to operate at the GTC...
The prevalence of neutral gas in massive post-main-sequence nebulae
Results are reported from a CO (J = 2-1) survey of nine type I nebulae using the 12-m NRAO antenna at KPNO; the data are presented in tables, graphs, and...
The Prevalence of the α-bimodality: First JWST α-abundance Results in M31
We present initial results from our JWST NIRSpec program to study the α-abundances in the M31 disk. The Milky Way has two chemically-defined disks, the low-α...
The primary role of the SW Sextantis stars in the evolution of cataclysmic variables
SW Sextantis stars are a relatively large group of cataclysmic variables (CVs) which plays a fundamental role in our understanding of CV structure and evolution...
The PRIMitive Asteroids Spectroscopic Survey Library, PRIMASS-L, is ready for you to dive in!!!
PRIMASS-L is a spectral library that contains the results of the PRIMitive Asteroids Spectroscopic Survey (PRIMASS). As of August 2022 this library contains...
The PRIMitive Asteroids Spectroscopic Survey Library: PRIMASS-L
The study of primitive asteroids is relevant to understanding the origin and evolution of our Solar System. These asteroids contain valuable information about...
The primordial abundance of 4He, YP, is one of the hottest themes in present-day astronomy, mostly due to its cosmological relevance. The disagreement between...
The Pristine Inner Galaxy Survey (PIGS) V: a chemo-dynamical investigation of the early assembly of the Milky Way with the most metal-poor stars in the bulge
The investigation of the metal-poor tail in the Galactic bulge provides unique information on the early Milky Way assembly and evolution. A chemo-dynamical...