HARMONI is a visible and near-infrared (0.47 to 2.45 μm) integral field spectrograph, providing the ELT's core spectroscopic capability at first light. A pre...
The Precipitable Water Vapour GNSS monitors at the Canary Islands Astronomical Observatories: towards an optimization of the final accuracy
Since proposed by Bevis et al. in 1992, GNSS Meteorology has become a very competitive field, mainly because it provides a relatively cheap, extensive network...
The preliminary design of the M1 assembly for the European Solar Telescope
The European Solar Telescope (EST) is a 4-meter class solar telescope led by the Instituto Astrofísico de Canarias that will be erected in La Palma Island. The...
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...