Finding New Debris Discs at Sub-millimetre Wavelengths
Authors
Mark Booth
Patricia Luppe
Sebastian Marino
Joshua B. Lovell
Jonathan P. Marshall
Gaspard Duchêne
Isabel Rebollido
Mark C. Wyatt
Riouhei Nakatani
Aya E. Higuchi
Miguel Chavez-Dagostino
Hiroshi Kobayashi
Abstract
Debris discs reveal the architectures and dynamical histories of planetary systems. Sub-millimetre observations trace large dust grains within debris discs, revealing their bulk properties. Debris discs have so far only been detected around ~20% of stars, representing the bright end of the population. A new facility is required to reach fainter discs, overcoming the confusion limit, with multiwavelength capabilities for characterisation, sensitivity to large-scale emission for nearby targets and a large field of view for surveying distant populations. All of this is made possible with the Atacama Large Aperture Submillimetre Telescope (AtLAST).
