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Cited article:

The Time-averaged Mass-loss Rates of Red Supergiants as Revealed by Their Luminosity Functions in M31 and M33

Philip Massey, Kathryn F. Neugent, Sylvia Ekström, Cyril Georgy and Georges Meynet
The Astrophysical Journal 942 (2) 69 (2023)
https://doi.org/10.3847/1538-4357/aca665

precision: a fast python pipeline for high-contrast imaging – application to SPHERE observations of the red supergiant VX Sagitariae

S Wolf, J A D L Blommaert, R Wesson, et al.
Monthly Notices of the Royal Astronomical Society 494 (3) 3200 (2020)
https://doi.org/10.1093/mnras/staa471

Detection of the Red Supergiant Wind from the Progenitor of Cassiopeia A

Kathryn E. Weil, Robert A. Fesen, Daniel J. Patnaude, et al.
The Astrophysical Journal 891 (2) 116 (2020)
https://doi.org/10.3847/1538-4357/ab76bf

Observing the mass-loss of nearby red supergiants through high-contrast imaging

Peter Scicluna, R. Siebenmorgen, J. A. D. L. Blommaert, et al.
Proceedings of the International Astronomical Union 14 (S343) 500 (2018)
https://doi.org/10.1017/S1743921318007421

A high-contrast imaging survey of nearby red supergiants

Peter Scicluna, Ralf Siebenmorgen, Joris Blommaert, et al.
Proceedings of the International Astronomical Union 12 (S329) 166 (2016)
https://doi.org/10.1017/S1743921317003350

The evolution of red supergiants to supernova in NGC 2100

Emma R. Beasor and Ben Davies
Monthly Notices of the Royal Astronomical Society 463 (2) 1269 (2016)
https://doi.org/10.1093/mnras/stw2054