# SONS: The JCMT legacy survey of debris discs in the submillimetre

## TL;DR

The SONS survey used the JCMT to image debris discs around nearby stars at submillimetre wavelengths, revealing their sizes, masses, and evolution, and providing a valuable target list for high-resolution follow-up observations.

## Contribution

This paper presents the first large-scale submillimetre imaging survey of debris discs, doubling the number of such discs observed at these wavelengths and characterizing their properties.

## Key findings

- Detected excess emission around 49 of 100 stars
- Discs range from 1 to 10 times the size of the Kuiper Belt
- Disc mass shows a tentative decline with stellar age

## Abstract

Debris discs are evidence of the ongoing destructive collisions between planetesimals, and their presence around stars also suggests that planets exist in these systems. In this paper, we present submillimetre images of the thermal emission from debris discs that formed the SCUBA-2 Observations of Nearby Stars (SONS) survey, one of seven legacy surveys undertaken on the James Clerk Maxwell telescope between 2012 and 2015. The overall results of the survey are presented in the form of 850 microns (and 450 microns, where possible) images and fluxes for the observed fields. Excess thermal emission, over that expected from the stellar photosphere, is detected around 49 stars out of the 100 observed fields. The discs are characterised in terms of their flux density, size (radial distribution of the dust) and derived dust properties from their spectral energy distributions. The results show discs over a range of sizes, typically 1-10 times the diameter of the Edgeworth-Kuiper Belt in our Solar System. The mass of a disc, for particles up to a few millimetres in size, is uniquely obtainable with submillimetre observations and this quantity is presented as a function of the host stars' age, showing a tentative decline in mass with age. Having doubled the number of imaged discs at submillimetre wavelengths from ground-based, single dish telescope observations, one of the key legacy products from the SONS survey is to provide a comprehensive target list to observe at high angular resolution using submillimetre/millimetre interferometers (e.g., ALMA, SMA).