In the last seven years the TESS space telescope has observed thousands of fast transients that have gone undetected, until now. With the TESSELLATE pipeline we are now searching all of the high-cadence Full Frame Images (FFIs) recorded by TESS for transient and variable phenomena. From processing less than 10% of the data from TESS, we have generated millions of detections which include...
The enormous spectroscopic datasets from current astronomical surveys provide an unprecedented opportunity to explore the stellar populations of the Milky Way and its surroundings. The largest surveys range from several million stars (e.g., LAMOST) to the roughly quarter-billion stars observed with Gaia XP spectra. These survey data are generally at low or moderate spectroscopic resolutions,...
The Aperture Array Verification Systems (AAVS), developed between 2014 and 2024 by a large international collaboration between the SKA Organization/SKAO and partner institutes and Universities, were a critical steppingstone in the path to SKA-Low. Originating from the need to validate novel antenna designs, signal processing systems, and station-level infrastructure for SKA-Low, they...
