NAME XO-2Sb , the SIMBAD biblio

NAME XO-2Sb , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.16CEST09:55:27


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Title First 3 Authors
2014A&A...567L...6D 96       D       C       3 5 20 The GAPS programme with HARPS-N at TNG. IV. A planetary system around XO-2S. DESIDERA S., BONOMO A.S., CLAUDI R.U., et al.
2015A&A...575A.111D viz 57       D     X         2 16 51 The GAPS programme with HARPS-N at TNG. V. A comprehensive analysis of the XO-2 stellar and planetary systems. DAMASSO M., BIAZZO K., BONOMO A.S., et al.
2015A&A...583A.135B viz 160           X         4 13 35 The GAPS programme with HARPS-N at TNG. X. Differential abundances in the XO-2 planet-hosting binary. BIAZZO K., GRATTON R., DESIDERA S., et al.
2018MNRAS.475.3090Y viz 16       D               1 483 ~ Forecasting the detectability of known radial velocity planets with the upcoming CHEOPS mission. YI J.S., CHEN J. and KIPPING D.
2018MNRAS.476.2542C 41           X         1 36 24 Hierarchical Bayesian calibration of tidal orbit decay rates among hot Jupiters. COLLIER CAMERON A. and JARDINE M.
2018ApJS..239...14J viz 16       D               1 1561 6 Revised exoplanet radii and habitability using Gaia data release 2. JOHNS D., MARTI C., HUFF M., et al.
2019PASP..131c4401D viz 17       D               1 688 5 Predicted yield of transits of known radial velocity exoplanets from the TESS primary and extended missions. DALBA P.A., KANE S.R., BARCLAY T., et al.
2021A&A...645A...7K viz 17       D               1 1569 17 Determining the true mass of radial-velocity exoplanets with Gaia. Nine planet candidates in the brown dwarf or stellar regime and 27 confirmed planets. KIEFER F., HEBRARD G., LECAVELIER DES ETANGS A., et al.
2021AJ....162..272S 17       D               1 142 10 Demographics of exoplanets in binaries. I. Architecture of S-type planetary systems revealed by the radial-velocity sample. SU X.-N., XIE J.-W., ZHOU J.-L., et al.
2022A&A...664A.161B 90             C       1 37 12 The GAPS Programme at TNG. XXXV. Fundamental properties of transiting exoplanet host stars. BIAZZO K., D'ORAZI V., DESIDERA S., et al.

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