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pro vyhledávání: '"Sousa SG"'
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⟩
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
https://www.repository.cam.ac.uk/handle/1810/334177
Autor:
Lacedelli, G, Wilson, TG, Malavolta, L, Hooton, MJ, Collier Cameron, A, Alibert, Y, Mortier, A, Bonfanti, A, Haywood, RD, Hoyer, S, Piotto, G, Bekkelien, A, Vanderburg, AM, Benz, W, Dumusque, X, Deline, A, Lopez-Morales, M, Borsato, L, Rice, K, Fossati, L, Latham, DW, Brandeker, A, Poretti, E, Sousa, SG, Sozzetti, A, Salmon, S, Burke, CJ, Van Grootel, V, Fausnaugh, MM, Adibekyan, V, Huang, CX, Osborn, HP, Mustill, AJ, Palle, E, Bourrier, V, Nascimbeni, V, Alonso, R, Anglada, G, Barczy, T, Barrado Y Navascues, D, Barros, SCC, Baumjohann, W, Beck, M, Beck, T, Billot, N, Bonfils, X, Broeg, C, Buchhave, LA, Cabrera, J, Charnoz, S, Cosentino, R, Csizmadia, S, Davies, MB, Deleuil, M, Delrez, L, Demangeon, O, Demory, BO, Ehrenreich, D, Erikson, A, Esparza-Borges, E, Floren, HG, Fortier, A, Fridlund, M, Futyan, D, Gandolfi, D, Ghedina, A, Gillon, M, Güdel, M, Guterman, P, Harutyunyan, A, Heng, K, Isaak, KG, Jenkins, JM, Kiss, L, Laskar, J, Lecavelier Des Etangs, A, Lendl, M, Lovis, C, Magrin, D, Marafatto, L, Martinez Fiorenzano, AF, Maxted, PFL, Mayor, M, Micela, G, Molinari, E, Murgas, F, Narita, N, Olofsson, G, Ottensamer, R, Pagano, I, Pasetti, A, Pedani, M, Pepe, FA, Peter, G, Phillips, DF, Pollacco, D, Queloz, D, Ragazzoni, R, Rando, N, Ratti, F
We present a precise characterization of the TOI-561 planetary system obtained by combining previously published data with TESS and CHEOPS photometry, and a new set of $62$ HARPS-N radial velocities (RVs). Our joint analysis confirms the presence of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::71b42fabcaf5754135d8e8c72573eeb5
https://www.repository.cam.ac.uk/handle/1810/333408
https://www.repository.cam.ac.uk/handle/1810/333408
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
https://www.repository.cam.ac.uk/handle/1810/325194
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
Autor:
Lendl, M, Csizmadia, S, Deline, A, Fossati, L, Kitzmann, D, Heng, K, Hoyer, S, Salmon, S, Benz, W, Broeg, C, Ehrenreich, D, Fortier, A, Queloz, D, Bonfanti, A, Brandeker, A, Collier Cameron, A, Delrez, L, Garcia Muñoz, A, Hooton, MJ, Maxted, PFL, Morris, BM, Van Grootel, V, Wilson, TG, Alibert, Y, Alonso, R, Asquier, J, Bandy, T, Bárczy, T, Barrado, D, Barros, SCC, Baumjohann, W, Beck, M, Beck, T, Bekkelien, A, Bergomi, M, Billot, N, Biondi, F, Bonfils, X, Bourrier, V, Busch, MD, Cabrera, J, Cessa, V, Charnoz, S, Chazelas, B, Corral Van Damme, C, Davies, MB, Deleuil, M, Demangeon, ODS, Demory, BO, Erikson, A, Farinato, J, Fridlund, M, Futyan, D, Gandolfi, D, Gillon, M, Guterman, P, Hasiba, J, Hernandez, E, Isaak, KG, Kiss, L, Kuntzer, T, Lecavelier Des Etangs, A, Lüftinger, T, Laskar, J, Lovis, C, Magrin, D, Malvasio, L, Marafatto, L, Michaelis, H, Munari, M, Nascimbeni, V, Olofsson, G, Ottacher, H, Ottensamer, R, Pagano, I, Pallé, E, Peter, G, Piazza, D, Piotto, G, Pollacco, D, Ratti, F, Rauer, H, Ragazzoni, R, Rando, N, Ribas, I, Rieder, M, Rohlfs, R, Safa, F, Santos, NC, Scandariato, G, Ségransan, D, Simon, AE, Singh, V, Smith, AMS, Sordet, M, Sousa, SG, Steller, M, Szabó, GM, Thomas, N, Tschentscher, M
The CHEOPS space mission dedicated to exoplanet follow-up was launched in December 2019, equipped with the capacity to perform photometric measurements at the 20 ppm level. As CHEOPS carries out its observations in a broad optical passband, it can pr
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9c86a503f56dad96157cbfe6ef129bc4
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
Autor:
Overbeek, JC, Friel, ED, Donati, P, Smiljanic, R, Jacobson, HR, Hatzidimitriou, D, Held, EV, Magrini, L, Bragaglia, A, Randich, S, Vallenari, A, Cantat-Gaudin, T, Tautvaišienė, G, Jiménez-Esteban, F, Frasca, A, Geisler, D, Villanova, S, Tang, B, Muñoz, C, Marconi, G, Carraro, G, San Roman, I, Drazdauskas, A, Ženovienė, R, Gilmore, G, Jeffries, RD, Flaccomio, E, Pancino, E, Bayo, A, Costado, MT, Damiani, F, Jofré, P, Monaco, L, Prisinzano, L, Sousa, SG, Zaggia, S
$\textit{Context}$. Trumpler 23 is a moderately populated, intermediate-age open cluster within the solar circle at a $R_\text{GC}$ ~ 6 kpc. It is in a crowded field very close to the Galactic plane and the color–magnitude diagram shows significant
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8cd7640c9430ae98bcc037be386093ef
https://www.repository.cam.ac.uk/handle/1810/263511
https://www.repository.cam.ac.uk/handle/1810/263511
Autor:
Pancino, E, Lardo, C, Altavilla, G, Marinoni, S, Ragaini, S, Cocozza, G, Bellazzini, M, Sabbi, E, Zoccali, M, Donati, P, Heiter, U, Koposov, SE, Blomme, R, Morel, T, Símon-Díaz, S, Lobel, A, Soubiran, C, Montalban, J, Valentini, M, Casey, AR, Blanco-Cuaresma, S, Jofré, P, Worley, CC, Magrini, L, Hourihane, A, François, P, Feltzing, S, Gilmore, G, Randich, S, Asplund, M, Bonifacio, P, Drew, JE, Jeffries, RD, Micela, G, Vallenari, A, Alfaro, EJ, Allende Prieto, C, Babusiaux, C, Bensby, T, Bragaglia, A, Flaccomio, E, Hambly, N, Korn, AJ, Lanzafame, AC, Smiljanic, R, Van Eck, S, Walton, NA, Bayo, A, Carraro, G, Costado, MT, Damiani, F, Edvardsson, B, Franciosini, E, Frasca, A, Lewis, J, Monaco, L, Morbidelli, L, Prisinzano, L, Sacco, GG, Sbordone, L, Sousa, SG, Zaggia, S, Koch, A
The $\textit{Gaia}$-ESO survey (GES) is now in its fifth and last year of observations and has produced tens of thousands of high-quality spectra of stars in all Milky Way components. This paper presents the strategy behind the selection of astrophys
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0f5ecdf6ca8c2fb028f5663f7fcbdfc9
https://www.repository.cam.ac.uk/handle/1810/263292
https://www.repository.cam.ac.uk/handle/1810/263292
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