REsolved ALMA and SMA Observations of Nearby Stars (REASONS): A population of 74 resolved planetesimal belts at millimetre wavelengthsDOI: info:10.1051/0004-6361/202451397v. 693EDP
Matrà, L., Marino, S., Wilner, D. J., Kennedy, G. M., Booth, M., Krivov, A. V., Williams, J. P., Hughes, A. M., del Burgo, C., Carpenter, J., Davies, C. L., Ertel, S., Kral, Q., Lestrade, J. -F, Marshall, J. P., Milli, J., Öberg, K. I., Pawellek, N., Sepulveda, A. G., Wyatt, M. C., Matthews, B. C., and MacGregor, M. 2025. "REsolved ALMA and SMA Observations of Nearby Stars (REASONS): A population of 74 resolved planetesimal belts at millimetre wavelengths." Astronomy and Astrophysics, 693. https://doi.org/10.1051/0004-6361/202451397.