Thermodynamic Limits Around M-dwarf Stars: Acknowledgements

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1 Aug 2024

(1) Samir Chitnavis, School of Biological and Behavioural Sciences, Queen Mary University of London, Mile End, London E1 4NS, UK & Digital Environment Research Institute, Queen Mary University of London, Empire House, Whitechapel E1 1HH, UK;

(2) Thomas J. Haworth, Astronomy Unit, Queen Mary University of London, Mile End Road, London E1 4NS, UK;

(3) Edward Gillen, Astronomy Unit, Queen Mary University of London, Mile End Road, London E1 4NS, UK;

(4) Conrad W. Mullineaux, School of Biological and Behavioural Sciences, Queen Mary University of London, Mile End, London E1 4NS, UK;

(5) Christopher D. P. Duffy, School of Biological and Behavioural Sciences, Queen Mary University of London, Mile End, London E1 4NS, UK & Digital Environment Research Institute, Queen Mary University of London, Empire House, Whitechapel E1 1HH, UK (Email: [email protected]).

5 Acknowledgements

CDPD and SC would like to acknowledge support from the BBSRC London Interdisciplinary Bioscience PhD Consortium (LIDo). Additionally, CDPD would like to acknowledge support from BBSRC for funding work (grant BB/T000023/1) that developed the key ideas in this work. TJH is funded by a Royal Society Dorothy Hodgkin Fellowship. EG gratefully acknowledges support from the UK Science and Technology Facilities Council (STFC; project reference ST/W001047/1).

6 Author Contribution Statement

CDPD, TJH and in discussion with EG and CWM, devised the project. TJH and EG provided stellar spectral data. Light-harvesting model development and simulations were carried out by CDPD and SC. TJH, EG and CWM provided additional interpretation of results. All authors were involved in Manuscript drafting.

7 Authors disclosure statement

There are no conflicts of interest to disclose.

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