TOI-1694b , the SIMBAD biblio

TOI-1694b , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST06:46:19


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Title First 3 Authors
2021ApJS..254...39G viz 17       D               1 2206 165 The TESS Objects of Interest Catalog from the TESS Prime Mission. GUERRERO N.M., SEAGER S., HUANG C.X., et al.
2022AJ....163..297C 17       D               1 216 18 The TESS-Keck Survey: Science Goals and Target Selection. CHONTOS A., MURPHY J.M.A., MacDOUGALL M.G., et al.
2023AJ....165...60V viz 505     A S   X C       10 53 5 TESS-Keck Survey. XIV. Two Giant Exoplanets from the Distant Giants Survey. VAN ZANDT J., PETIGURA E.A., MacDOUGALL M., et al.
2023AJ....166...33M viz 17       D               1 193 ~ The TESS-Keck Survey. XV. Precise Properties of 108 TESS Planets and Their Host Stars. MacDOUGALL M.G., PETIGURA E.A., GILBERT G.J., et al.
2023MNRAS.523.1163F 131           X   F     2 10 ~ TOI-2498 b: a hot bloated super-Neptune within the Neptune desert. FRAME G., ARMSTRONG D.J., CEGLA H.M., et al.
2024AJ....167..250V 179           X C       3 9 ~ ethraid: A Simple Method for Characterizing Long-period Companions Using Doppler, Astrometric, and Imaging Constraints. VAN ZANDT J. and PETIGURA E.A.
2024ApJS..272...32P viz 18       D               1 212 ~ The TESS-Keck Survey. XX. 15 New TESS Planets and a Uniform RV Analysis of All Survey Targets. POLANSKI A.S., LUBIN J., BEARD C., et al.
2025AJ....169..212H 2034 T   A     X C F     41 10 ~ An Obliquity Measurement of the Hot Neptune
TOI-1694b.
HANDLEY L.B., HOWARD A.W., RUBENZAHL R.A., et al.
2025A&A...698A.112L 19       D               1 84 ~ sunset: A database of synthetic atmospheric-escape transmission spectra for nearly every transiting planet. LINSSEN D., OKLOPCIC A. and MacLEOD M.
2025PASP..137f5002M 19       D               1 21 ~ Exo-Dragonfly: Adapting the Dragonfly Telephoto Array to the Observation of Exoplanet Transits. MANN C.R., LAFRENIERE D., ARTIGAU E., et al.
2026A&A...705A.142R viz 50           X         1 55 ~ True spin-orbit obliquity distribution: Data-driven confirmation of no clustering of misaligned planets. ROSSI A.M., RAINER M., BORSA F., et al.

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