The First Near-infrared Transmission Spectrum of HIP 41378 f, A Low-mass Temperate Jovian World in a Multiplanet System

Autor: Alam, MK, Kirk, J, Dressing, CD, López-Morales, M, Ohno, K, Gao, P, Akinsanmi, B, Santerne, A, Grouffal, S, Adibekyan, V, Barros, SCC, Buchhave, LA, Crossfield, IJM, Dai, F, Deleuil, M, Giacalone, S, Lillo-Box, J, Marley, M, Mayo, AW, Mortier, A, Santos, NC, Sousa, SG, Turtelboom, EV, Wheatley, PJ, Vanderburg, AM

Publikováno v: Alam, M K, Kirk, J, Dressing, C D, López-Morales, M, Ohno, K, Gao, P, Akinsanmi, B, Santerne, A, Grouffal, S, Adibekyan, V, Barros, S C C, Buchhave, L A, Crossfield, I J M, Dai, F, Deleuil, M, Giacalone, S, Lillo-Box, J, Marley, M, Mayo, A W, Mortier, A, Santos, N C, Sousa, S G, Turtelboom, E V, Wheatley, P J & Vanderburg, A M 2022, ' The First Near-infrared Transmission Spectrum of HIP 41378 f, A Low-mass Temperate Jovian World in a Multiplanet System ', The Astrophysical Journal Letters, vol. 927, L5 . https://doi.org/10.3847/2041-8213/ac559d
Alam, M K, Kirk, J, Dressing, C D, López-Morales, M, Ohno, K, Gao, P, Akinsanmi, B, Santerne, A, Grouffal, S, Adibekyan, V, Barros, S C C, Buchhave, L A, Crossfield, I J M, Dai, F, Deleuil, M, Giacalone, S, Lillo-Box, J, Marley, M, Mayo, A W, Mortier, A, Santos, N C, Sousa, S G, Turtelboom, E V, Wheatley, P J & Vanderburg, A M 2022, ' The First Near-infrared Transmission Spectrum of HIP 41378 f, A Low-mass Temperate Jovian World in a Multiplanet System ', Astrophysical Journal Letters, vol. 927, L5 . https://doi.org/10.3847/2041-8213/ac559d
The Astrophysical Journal Letters
The Astrophysical Journal Letters, 2022, 927, ⟨10.3847/2041-8213/ac559d⟩
apjl
apjl, 2022, 927 (1), pp.L5. ⟨10.3847/2041-8213/ac559d10.48550/arXiv.2201.02686⟩

We present a near-infrared transmission spectrum of the long period (P=542 days), temperate ($T_{eq}$=294 K) giant planet HIP 41378 f obtained with the Wide-Field Camera 3 (WFC3) instrument aboard the Hubble Space Telescope (HST). With a measured mas

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c13806425a9ccc7e13529b4da18fdeaa
https://www.repository.cam.ac.uk/handle/1810/334177

CHEOPS observations of the HD 108236 planetary system: A fifth planet, improved ephemerides, and planetary radii

Autor: Bonfanti, A, Delrez, L, Hooton, MJ, Wilson, TG, Fossati, L, Alibert, Y, Hoyer, S, Mustill, AJ, Osborn, HP, Adibekyan, V, Gandolfi, D, Salmon, S, Sousa, SG, Tuson, A, Van Grootel, V, Cabrera, J, Nascimbeni, V, Maxted, PFL, Barros, SCC, Billot, N, Bonfils, X, Borsato, L, Broeg, C, Davies, MB, Deleuil, M, Demangeon, ODS, Fridlund, M, Lacedelli, G, Lendl, M, Persson, C, Santos, NC, Scandariato, G, Szabó, GM, Collier Cameron, A, Udry, S, Benz, W, Beck, M, Ehrenreich, D, Fortier, A, Isaak, KG, Queloz, D, Alonso, R, Asquier, J, Bandy, T, Bárczy, T, Barrado, D, Barragán, O, Baumjohann, W, Beck, T, Bekkelien, A, Bergomi, M, Brandeker, A, Busch, MD, Cessa, V, Charnoz, S, Chazelas, B, Corral Van Damme, C, Demory, BO, Erikson, A, Farinato, J, Futyan, D, Garcia Muñoz, A, Gillon, M, Guedel, M, Guterman, P, Hasiba, J, Heng, K, Hernandez, E, Kiss, L, Kuntzer, T, Laskar, J, Lecavelier Des Etangs, A, Lovis, C, Magrin, D, Malvasio, L, Marafatto, L, Michaelis, H, Munari, M, Olofsson, G, Ottacher, H, Ottensamer, R, Pagano, I, Pallé, E, Peter, G, Piazza, D, Piotto, G, Pollacco, D, Ragazzoni, R, Rando, N, Ratti, F, Rauer, H, Ribas, I, Rieder, M, Rohlfs, R, Safa, F, Salatti, M, Ségransan, D, Simon, AE, Smith, AMS, Sordet, M

The detection of a super-Earth and three mini-Neptunes transiting the bright ($V$ = 9.2 mag) star HD 108236 (also known as TOI-1233) was recently reported on the basis of TESS and ground-based light curves. We perform a first characterisation of the

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::00d765f822e2c4f8f2efae0530559097

The CHEOPS mission

Autor: Benz, W, Broeg, C, Fortier, A, Rando, N, Beck, T, Beck, M, Queloz, D, Ehrenreich, D, Maxted, PFL, Isaak, KG, Billot, N, Alibert, Y, Alonso, R, António, C, Asquier, J, Bandy, T, Bárczy, T, Barrado, D, Barros, SCC, Baumjohann, W, Bekkelien, A, Bergomi, M, Biondi, F, Bonfils, X, Borsato, L, Brandeker, A, Busch, MD, Cabrera, J, Cessa, V, Charnoz, S, Chazelas, B, Collier Cameron, A, Corral Van Damme, C, Cortes, D, Davies, MB, Deleuil, M, Deline, A, Delrez, L, Demangeon, O, Demory, BO, Erikson, A, Farinato, J, Fossati, L, Fridlund, M, Futyan, D, Gandolfi, D, Garcia Munoz, A, Gillon, M, Guterman, P, Gutierrez, A, Hasiba, J, Heng, K, Hernandez, E, Hoyer, S, Kiss, LL, Kovacs, Z, Kuntzer, T, Laskar, J, Lecavelier Des Etangs, A, Lendl, M, López, A, Lora, I, Lovis, C, Lüftinger, T, Magrin, D, Malvasio, L, Marafatto, L, Michaelis, H, De Miguel, D, Modrego, D, Munari, M, Nascimbeni, V, Olofsson, G, Ottacher, H, Ottensamer, R, Pagano, I, Palacios, R, Pallé, E, Peter, G, Piazza, D, Piotto, G, Pizarro, A, Pollaco, D, Ragazzoni, R, Ratti, F, Rauer, H, Ribas, I, Rieder, M, Rohlfs, R, Safa, F, Salatti, M, Santos, NC, Scandariato, G, Ségransan, D, Simon, AE, Smith, AMS, Sordet, M, Sousa, SG, Steller, M, Szabó, GM

The CHaracterising ExOPlanet Satellite (CHEOPS) was selected in 2012, as the first small mission in the ESA Science Programme and successfully launched in December 2019. CHEOPS is a partnership between ESA and Switzerland with important contributions

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::95d1a8741e8be0224f035258d630dd2e

The EBLM project-VIII. First results for M-dwarf mass, radius, and effective temperature measurements using CHEOPS light curves

Autor: Swayne, MI, Maxted, PFL, Triaud, AHMJ, Sousa, SG, Broeg, C, Florén, HG, Guterman, P, Simon, AE, Boisse, I, Bonfanti, A, Martin, D, Santerne, A, Salmon, S, Standing, MR, Van Grootel, V, Wilson, TG, Alibert, Y, Alonso, R, Anglada Escudé, G, Asquier, J, Bárczy, T, Barrado, D, Barros, SCC, Battley, M, Baumjohann, W, Beck, M, Beck, T, Bekkelien, A, Benz, W, Billot, N, Bonfils, X, Brandeker, A, Busch, MD, Cabrera, J, Charnoz, S, Collier Cameron, A, Csizmadia, S, Davies, MB, Deleuil, M, Deline, A, Delrez, L, Demangeon, ODS, Demory, BO, Dransfield, G, Ehrenreich, D, Erikson, A, Fortier, A, Fossati, L, Fridlund, M, Futyan, D, Gandolfi, D, Gillon, M, Guedel, M, Hébrard, G, Heidari, N, Hellier, C, Heng, K, Hobson, M, Hoyer, S, Isaak, KG, Kiss, L, Kunovac Hodžić, V, Lalitha, S, Laskar, J, Lecavelier Des Etangs, A, Lendl, M, Lovis, C, Magrin, D, Marafatto, L, McCormac, J, Miller, N, Nascimbeni, V, Olofsson, G, Ottensamer, R, Pagano, I, Pallé, E, Peter, G, Piotto, G, Pollacco, D, Queloz, D, Ragazzoni, R, Rando, N, Rauer, H, Ribas, I, Santos, NC, Scandariato, G, Ségransan, D, Smith, AMS, Steinberger, M, Steller, M, Szabó, GM, Thomas, N, Udry, S, Walter, I, Walton, NA, Willett, E

The accuracy of theoretical mass, radius and effective temperature values for M-dwarf stars is an active topic of debate. Differences between observed and theoretical values have raised the possibility that current theoretical stellar structure and e

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=od_______109::97d9540c08789342b94827a5e1944190
https://www.repository.cam.ac.uk/handle/1810/325194

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