BD+65 902d , the SIMBAD biblio

BD+65 902d , the SIMBAD biblio (15 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST09:20:19


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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...33D viz 696           X C       15 26 9 TOI-1136 is a Young, Coplanar, Aligned Planetary System in a Pristine Resonant Chain. DAI F., MASUDA K., BEARD C., et al.
2023AJ....166...33M viz 148       D     X C       3 193 ~ 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.
2023A&A...676L...8V 17       D               1 10 ~ Rocky sub-Neptunes formed by pebble accretion: Rain of rock from polluted envelopes. VAZAN A. and ORMEL C.W.
2023AJ....166..266R viz 17       D               1 54 ~ Evidence for Low-level Dynamical Excitation in Near-resonant Exoplanet Systems. RICE M., WANG X.-Y., WANG S., et al.
2024AJ....167...70B viz 152       D     X         4 15 ~ The TESS-Keck Survey. XVII. Precise Mass Measurements in a Young, High-multiplicity Transiting Planet System Using Radial Velocities and Transit Timing Variations. BEARD C., ROBERTSON P., DAI F., et al.
2024ApJ...961..203M 152       D     X   F     3 50 ~ Spin Dynamics of Planets in Resonant Chains. MILLHOLLAND S.C., LARA T. and TOOMLAID J.
2024A&A...684L..17M viz 45           X         1 25 ~ Orbital obliquity of the young planet TOI-5398 b and the evolutionary history of the system. MANTOVAN G., MALAVOLTA L., LOCCI D., et al.
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.
2024A&A...689A.179O 851     A D S   X C       18 59 ~ The MOPYS project: A survey of 70 planets in search of extended He I and H atmospheres No evidence of enhanced evaporation in young planets. ORELL-MIQUEL J., MURGAS F., PALLE E., et al.
2025MNRAS.540.1144F 205       D     X   F     4 159 ~ The eccentricity distribution of warm sub-Saturns in TESS. FAIRNINGTON T.R., DONG J., HUANG C.X., et al.
2025ApJ...988..247S 19       D               2 31 ~ Tidal Inflation is Stronger for Misaligned Neptune-sized Planets Than Aligned Ones. SETHI R. and MILLHOLLAND S.C.
2025AJ....170..182P 19       D               1 58 ~ An Aligned Sub-Neptune Revealed with MAROON-X and a Tendency Toward Alignment for Small Planets. POLANSKI A.S., CROSSFIELD I.J.M., SEIFAHRT A., 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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