TOI-1268 , the SIMBAD biblio

TOI-1268 , the SIMBAD biblio (24 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST06:30:24


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Title First 3 Authors
2018A&A...609A.116R viz 16       D               1 143018 65 Empirical photometric calibration of the Gaia red clump: Colours, effective temperature, and absolute magnitude. RUIZ-DERN L., BABUSIAUX C., ARENOU F., et al.
2022ApJ...926L...7D 2367     A     X C       55 12 11 NEID Rossiter-McLaughlin Measurement of
TOI-1268b: A Young Warm Saturn Aligned with Its Cool Host Star.
DONG J., HUANG C.X., ZHOU G., 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.
2022MNRAS.513..102C viz 17       D               1 961 6 The TESS Triple-9 Catalog: 999 uniformly vetted exoplanet candidates. CACCIAPUOTI L., KOSTOV V.B., KUCHNER M., et al.
2022AJ....163..289Z 85             C       1 63 7 A Mini-Neptune from TESS and CHEOPS Around the 120 Myr Old AB Dor Member HIP 94235. ZHOU G., WIRTH C.P., HUANG C.X., et al.
2022A&A...662A.107S 3107     A D     X C F     72 29 6
TOI-1268b: The youngest hot Saturn-mass transiting exoplanet.
SUBJAK J., ENDL M., CHATURVEDI P., et al.
2022AJ....164..104R viz 17       D               1 105 10 A Tendency Toward Alignment in Single-star Warm-Jupiter Systems. RICE M., WANG S., WANG X.-Y., et al.
2022PASP..134h2001A viz 60       D     X         2 366 39 Stellar Obliquities in Exoplanetary Systems. ALBRECHT S.H., DAWSON R.I. and WINN J.N.
2022MNRAS.516...75B 102       D       C       3 115 9 Exploring the dependence of hot Jupiter occurrence rates on stellar mass with TESS. BELEZNAY M. and KUNIMOTO M.
2023AJ....165..121H 87             C       1 24 1 TOI-4562b: A Highly Eccentric Temperate Jupiter Analog Orbiting a Young Field Star. HEITZMANN A., ZHOU G., QUINN S.N., et al.
2023MNRAS.519.3723M 17       D               2 48 1 Limb darkening measurements from TESS and Kepler light curves of transiting exoplanets. MAXTED P.F.L.
2023AJ....166...72S viz 17       D               1 275 ~ Variability of Known Exoplanet Host Stars Observed by TESS. SIMPSON E.R., FETHEROLF T., KANE S.R., et al.
2024MNRAS.528.4092B 90               F     1 27 ~ The variable magnetic field of V889 Her and the challenge of detecting exoplanets around young Suns using Gaussian process regression. BROWN E.L., MARSDEN S.C., JEFFERS S.V., et al.
2024AJ....167..214P 90           X         2 12 ~ Detection of an Atmospheric Outflow from the Young Hot Saturn TOI-1268b. PEREZ-GONZALEZ J., GREKLEK-MCKEON M., VISSAPRAGADA S., et al.
2024AJ....168..177C viz 18       D               1 260 ~ Detecting Exoplanet Transits with the Next Generation of X-Ray Telescopes. CILLEY R., KING G.W. and CORRALES L.
2024MNRAS.534.3893V 18       D               1 43 ~ A regularization technique to precisely infer limb darkening using transit measurements: can we estimate stellar surface magnetic fields? VERMA K., MAXTED P.F.L., SINGH A., 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...978...46K 19       D               1 49 ~ Separating Super-puffs versus Hot Jupiters among Young Puffy Planets. KARALIS A., LEE E.J. and THORNGREN D.P.
2025MNRAS.539.2144A 19       D               1 27 ~ Helium escape signatures are generally strongest during younger ages but this age dependence is lost in the diversity of observed exoplanets. ALLAN A.P. and VIDOTTO A.A.
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.
2025RNAAS...9..275M 19       D               1 365 ~ An In-depth Study of Brown Dwarfs with TESS. MARCADON F. and PRSA A.
2025A&A...704A.102H 373     A D S   X         8 111 ~ Homogeneous search for spot transits in Kepler and TESS photometry of K - M-type main-sequence stars. HARIS A., TUOMI M. and HACKMAN T.
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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