TOI-282 radial velocities and activity indicators
Barone A, F. Rodler, D. Gandolfi, A. Bonfanti et autres
at, it, cl, nl, se, us, rs, de, jp, pl, es (code pays fourni par la source)
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Barone A, F. Rodler, D. Gandolfi, A. Bonfanti et autres
at, it, cl, nl, se, us, rs, de, jp, pl, es (code pays fourni par la source)
Kevin Hoy, A. Zurlo, Pablo A. Peña R, Jana Köhler et autres
cl, de, it, us (code pays fourni par la source)
Kevin Hoy, A. Zurlo, Pablo A. Peña R, Jana Köhler et autres
Despite more than 6000 exoplanets being discovered to date, no satellite orbiting an exoplanet, an exomoon, has ever been confidently detected. While there are some candidates, they lack clear and convincing confirmation and remain controversial. Beyond the innate value of discovering new …
D. Gandolfi, A. Alnajjarine, L. M. Serrano, J.A. Egger et autres
TOI-1203 is a bright (V,=,8.6) G3,V star known to host a transiting warm sub-Neptune on a 25.5-day orbit. Here we report on an intensive high-precision radial velocity and photometric follow-up campaign carried out with the spectrograph and the ̧heops space telescope. We …
R. Pandey, Aina Palau, Javier Serna, R. Kuiper et autres
Abstract Using optical time series with Telescopi Joan Oró (TJO), Gaia, TESS, and NEOWISE archival data, we performed a variability study on the candidate bloated massive young stellar object (MYSO) IRAS 19520+2759. This is the first time that a bloated star candidate …
mx, us, de, es, in, cl (code pays fourni par la source)
R. Pandey, Aina Palau, Javier Serna, R. Kuiper et autres
Using optical time series with Telescopi Joan Oró (TJO), Gaia, TESS, and NEOWISE archival data, we performed a variability study on the candidate bloated massive young stellar object (MYSO) IRAS 19520+2759. This is the first time that a bloated star candidate has …
cl (code pays fourni par la source)
H. L. M. Osborne, Elisa Goffo, D. Gandolfi, G. Nowak et autres
ABSTRACT We report on the precise radial velocity follow-up of TOI-544 (HD 290498), a bright K star (V = 10.8), which hosts a small transiting planet recently discovered by the Transiting Exoplanet Survey Satellite (TESS). We collected 122 high-resolution High Accuracy Radial …
de, gb, it, es, pl, se, jp, us, cl, dk, nl (code pays fourni par la source)
H. L. M. Osborne, Vincent Van Eylen, Elisa Goffo, D. Gandolfi et autres
We report on the precise radial velocity follow-up of TOI-544 (HD 290498), a bright K star (V=10.8), which hosts a small transiting planet recently discovered by the Transiting Exoplanet Survey Satellite (TESS). We collected 122 high-resolution HARPS and HARPS-N spectra to spectroscopically …
Elisa Goffo, D. Gandolfi, J. A. Egger, Alexander J. Mustill et autres
Abstract GJ 367 is a bright (V ≈ 10.2) M1 V star that has been recently found to host a transiting ultra-short period sub-Earth on a 7.7 hr orbit. With the aim of improving the planetary mass and radius and unveiling the …
de, it, ch, se, dk, jp, cl, gb, us, at, fr, es (code pays fourni par la source)
Nikku Madhusudhan, Karan Molaverdikhani, Vincent Van Eylen, Joshua E. Schlieder et autres
We report the discovery and characterization of two transiting planets around the bright M1 V star LP 961-53 (TOI-776, J = 8.5 mag, M = 0.54 ± 0.03 M⊙) detected during Sector 10 observations of the Transiting Exoplanet Survey Satellite (TESS). Combining …
us (code pays fourni par la source)
F. Lesjak, L. Nortmann, F. Yan, D. Cont et autres
Accurately estimating the C/O ratio of hot Jupiter atmospheres is a promising pathway towards understanding planet formation and migration, as well as the formation of clouds and the overall atmospheric composition. The atmosphere of the hot Jupiter WASP-43b has been extensively analysed …
de, cn, se, fr, cl, es (code pays fourni par la source)
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