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Parviainen, H, Wilson, TG, Lendl, M, Kitzmann, D, Palle, E, Serrano, LM, Meier Valdes, E, Benz, W, Deline, A, Ehrenreich, D, Guterman, P, Heng, K, Demangeon, ODS, Bonfanti, A, Salmon, S, Singh, V, Santos, NC, Sousa, SG, Alibert, Y, Alonso, R, Anglada, G, Barczy, T, Barrado y Navascues, D, Barros, SCC, Baumjohann, W, Beck, M, Beck, T, Billot, N, Bonfils, X, Brandeker, A, Broeg, C, Cabrera, J, Charnoz, S, Cameron, AC, Van Damme, CC, Csizmadia, S, Davies, MB, Deleuil, M, Delrez, L, Demory, B-O, Erikson, A, Farinato, J, Fortier, A, Fossati, L, Fridlund, M, Gandolfi, D, Gillon, M, Guedel, M, Hoyer, S, Isaak, KG, Kiss, LL, Kopp, E, Laskar, J, des Etangs, AL, Lovis, C, Magrin, D, Maxted, PFL ORCID: https://orcid.org/0000-0003-3794-1317, Mecina, M, Nascimbeni, V, Olofsson, G, Ottensamer, R, Pagano, I, Peter, G, Piazza, D, Piotto, G, Pollacco, D, Queloz, D, Ragazzoni, R, Rando, N, Rauer, H, Ribas, I, Scandariato, G, Segransan, D, Simon, AE, Smith, AMS, Steller, M, Szabo, GM, Thomas, N, Udry, S, Van Grootel, V and Walton, NA (2022) CHEOPS finds KELT-1b darker than expected in visible light Discrepancy between the CHEOPS and TESS eclipse depths. Astronomy and Astrophysics: a European journal, 668.

Sebastian, D, Swayne, MI, Maxted, PFL ORCID: https://orcid.org/0000-0003-3794-1317, Triaud, AHMJ, Sousa, SG, Olofsson, G, Beck, M, Billot, N, Hoyer, S, Gill, S, Heidari, N, Martin, DV, Persson, CM, Standing, MR, Alibert, Y, Alonso, R, Anglada, G, Asquier, J, Bárczy, T, Barrado, D, Barros, SCC, Battley, MP, Baumjohann, W, Beck, T, Benz, W, Bergomi, M, Boisse, I, Bonfils, X, Brandeker, A, Broeg, C, Cabrera, J, Charnoz, S, Cameron, AC, Csizmadia, S, Davies, MB, Deleuil, M, Delrez, L, Demangeon, ODS, Demory, B-O, Dransfield, G, Ehrenreich, D, Erikson, A, Fortier, A, Fossati, L, Fridlund, M, Gandolfi, D, Gillon, M, Güdel, M, Hasiba, J, Hébrard, G, Heng, K, Isaak, KG, Kiss, LL, Kopp, E, Kunovac, V, Laskar, J, des Etangs, AL, Lendl, M, Lovis, C, Magrin, D, McCormac, J, Miller, NJ, Nascimbeni, V, Ottensamer, R, Pagano, I, Pallé, E, Pepe, FA, Peter, G, Piotto, G, Pollacco, D, Queloz, D, Ragazzoni, R, Rando, N, Rauer, H, Ribas, I, Lalitha, S, Santerne, A, Santos, NC, Scandariato, G, Ségransan, D, Simon, AE, Smith, AMS, Steller, M, Szabó, GM, Thomas, N, Udry, S, Van Grootel, V and Walton, NA (2022) The EBLM project – IX. Five fully convective M-dwarfs, precisely measured with CHEOPS and TESS light curves. Monthly Notices of the Royal Astronomical Society.

Borsato, L, Piotto, G, Gandolfi, D, Nascimbeni, V, Lacedelli, G, Marzari, F, Billot, N, Maxted, PFL ORCID: https://orcid.org/0000-0003-3794-1317, Sousa, S, Cameron, AC, Bonfanti, A, Wilson, TG, Serrano, LM, Garai, Z, Alibert, Y, Alonso, R, Asquier, J, Bárczy, T, Bandy, T, Barrado, D, Barros, SCC, Baumjohann, W, Beck, M, Beck, T, Benz, W, Bonfils, X, Brandeker, A, Broeg, C, Cabrera, J, Charnoz, S, Csizmadia, S, Davies, MB, Deleuil, M, Delrez, L, Demangeon, O, Demory, B-O, des Etangs, AL, Ehrenreich, D, Erikson, A, Escudé, GA, Fortier, A, Fossati, L, Fridlund, M, Gillon, M, Guedel, M, Hasiba, J, Heng, K, Hoyer, S, Isaak, KG, Kiss, L, Kopp, E, Laskar, J, Lendl, M, Lovis, C, Magrin, D, Munari, M, Olofsson, G, Ottensamer, R, Pagano, I, Pallé, E, Peter, G, Pollacco, D, Queloz, D, Ragazzoni, R, Rando, N, Rauer, H, Ribas, I, Ségransan, D, Santos, NC, Scandariato, G, Simon, A, Smith, AMS, Steller, M, Szabó, G, Thomas, N, Udry, S, Van Grootel, V and Walton, N (2021) Exploiting timing capabilities of the CHEOPS mission with warm-Jupiter planets. Monthly Notices of the Royal Astronomical Society, 506 (3). 3810 - 3830.