Astronomers nowadays have a wealth of sophisticated publishing software at their fingertips, but are they achieving acceptable standards of presentation?
Making the Most of Transmission Spectra in Light of Stellar Activity: Needs Identified by ExoPAG's Study Analysis Group 21
Transmission spectroscopy, a method for studying exoplanetary atmospheres by measuring the wavelength-dependent radius of a planet as it transits its star...
Manufacturing, integration, and testing of ELMER structure and mechanisms
ELMER is an optical instrument for the GTC designed to observe between 3650 and 10000 Armstrong. The observing modes for the instrument at Day One shall be...
We present the science case for mapping several thousand galaxy (proto)clusters at z=1-10 with a large aperture single dish sub-mm facility, producing a high...
Mapping magnetic activity indicators across the M dwarf domain
Stellar activity poses one of the main obstacles for the detection and characterisation of exoplanets around cool stars, as it can induce radial velocity (RV)...
Mapping Magnetic Fields in Star Forming Regions with BLASTPol
A key outstanding question in our understanding of star formation is whether magnetic fields provide support against the gravitational collapse of their parent...
Mapping of Solar Magnetic Fields from the Photosphere to the Top of the Chromosphere with CLASP2
Coronal heating, chromospheric heating, and the heating & acceleration of the solar wind, are well-known problems in solar physics. Additionally, knowledge of...