CHEOPS finds KELT-1b darker than expected in visible light: discrepancy between the CHEOPS and TESS eclipse depths

H. Parviainen*, T.G. Wilson, M. Lendl, D. Kitzmann, E. Pallé, L.M. Serrano, E. Meier Valdes, W. Benz, A. Deline, D. Ehrenreich, P. Guterman, K. Heng, O.D.S. Demangeon, A. Bonfanti, S. Salmon, V. Singh, N.C. Santos, S.G. Sousa, Y. Alibert, R. AlonsoG. Anglada, T. Bárczy, D. Barrado Y Navascues, S.C.C. Barros, W. Baumjohann, M. Beck, T. Beck, N. Billot, X. Bonfils, A. Brandeker, C. Broeg, J. Cabrera, S. Charnoz, A. Collier Cameron, C. Corral Van Damme, S. Csizmadia, M.B. Davies, M. Deleuil, L. Delrez, B.-O. Demory, A. Erikson, J. Farinato, A. Fortier, L. Fossati, M. Fridlund, D. Gandolfi, M. Gillon, M. Güdel, S. Hoyer, K.G. Isaak, L.L. Kiss, E. Kopp, J. Laskar, A. Lecavelier Des Etangs, C. Lovis, D. Magrin, P.F.L. Maxted, M. Mecina, V. Nascimbeni, G. Olofsson, R. Ottensamer, I. Pagano, G. Peter, D. Piazza, G. Piotto, D. Pollacco, D. Queloz, R. Ragazzoni, N. Rando, H. Rauer, I. Ribas, G. Scandariato, D. Ségransan, A.E. Simon, A.M.S. Smith, M. Steller, G.M. Szabó, N. Thomas, S. Udry, V. Van Grootel, N.A. Walton

*Corresponding author for this work

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