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...
Mapping stellar activity indicators across the M dwarf domain
Despite stellar magnetic activity being present in most cool stars, its effects on spectroscopic observations are still not well understood. Several activity...
Mapping the Bulge Metallicity Distribution Function with APOGEE
The origin and formation of the Milky Way bulge remains poorly understood, in part because high quality observations of the bulge have generally been restricted...
We observed EX Draconis in BV I colours for 40 nights, covering 3 outburst events, with the aim to study the disc evolution. Here, we present a preliminary...
Mapping the Old and Young Stellar Populations of Blue Compact Dwarf Galaxies: The case of Mrk5
We present a detailed spectrophotometric analysis of the blue compact dwarf galaxy Mrk5 (NGC353, Haro3), based on deep BVRIJHK broad-band and H α narrow-band...