TOI-905 , the SIMBAD biblio

TOI-905 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST03:51:52


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Title First 3 Authors
2020AJ....159...19Z viz 17       D               1 125 132 SOAR TESS Survey. I. Sculpting of TESS planetary systems by stellar companions. ZIEGLER C., TOKOVININ A., BRICENO C., et al.
2020A&A...639A..35H viz 16       D               1 448 18 The correlation between photometric variability and radial velocity jitter. Based on TESS and HARPS observations. HOJJATPANAH S., OSHAGH M., FIGUEIRA P., et al.
2020AJ....160..229D 2980       D     X C       72 31 11 TOI 564 b and TOI 905 b: grazing and fully Transiting hot Jupiters discovered by TESS. DAVIS A.B., WANG S., JONES M., et al.
2021AJ....162...75L viz 17       D               1 517 28 Speckle observations of TESS exoplanet host stars. II. Stellar companions at 1-1000 au and implications for small planet detection. LESTER K.V., MATSON R.A., HOWELL S.B., et al.
2022MNRAS.512L..60H viz 17       D               1 1974 9 The flaring TESS Objects of Interest: flare rates for all two-minute cadence TESS planet candidates. HOWARD W.S.
2022AJ....163..228P viz 17       D               4 354 20 Empirical Limb-darkening Coefficients and Transit Parameters of Known Exoplanets from TESS. PATEL J.A. and ESPINOZA N.
2024A&A...683A.125P viz 18       D               1 3561 ~ Analysis of the public HARPS/ESO spectroscopic archive Ca II H&K time series for the HARPS radial velocity database. PERDELWITZ V., TRIFONOV T., TEKLU J.T., et al.
2024A&A...691A..53S viz 18       D               1 4078 ~ SWEET-Cat: A view on the planetary mass-radius relation. SOUSA S.G., ADIBEKYAN V., DELGADO-MENA E., et al.
2025ApJ...988L...4H 19       D               1 301 ~ Hundreds of TESS Exoplanets Might Be Larger than We Thought. HAN T., ROBERTSON P., BRANDT T.D., et al.
2025A&A...699A.100D viz 19       D               1 2580 ~ The Gaia spectroscopic catalogue of exoplanets and host stars. DE LAVERNY P., LIGI R., CRIDA A., et al.
2026AJ....171..157S 20       D               2 480 ~ Most Hot Jupiters Were Cool Giant Planets for More Than 1 Gyr. SCHMIDT S.P. and SCHLAUFMAN K.C.

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