BD+29 2654b , the SIMBAD biblio

BD+29 2654b , the SIMBAD biblio (13 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST05:02:27


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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.
2023AJ....166...49D viz 1480     A D     X C       34 5 ~ A Mini-Neptune Orbiting the Metal-poor K Dwarf BD+29 2654. DAI F., SCHLAUFMAN K.C., REGGIANI H., et al.
2024MNRAS.531.3698H 206 ~ Shallower radius valley around low-mass hosts: evidence for icy planets, collisions, or high-energy radiation scatter. HO C.S.K., ROGERS J.G., VAN EYLEN V., et al.
2024A&A...687L...1L viz 18       D               1 140 ~ Resonant sub-Neptunes are puffier. LELEU A., DELISLE J.-B., BURN R., et al.
2024A&A...689A..53B viz 18       D               1 194 ~ The TROY project III. Exploring co-orbitals around low-mass stars. BALSALOBRE-RUZA O., LILLO-BOX J., BARRADO D., et al.
2024A&A...689A.179O 1030     A D S   X C       22 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.
2025A&A...693A.285S viz 65       D     X         2 221 ~ Connection between planetary He I λ10 830 Å absorption and extreme-ultraviolet emission of planet-host stars. SANZ-FORCADA J., LOPEZ-PUERTAS M., LAMPON M., et al.
2025ApJ...979..120H 47           X         1 15 ~ On the Formation of Planets in the Milky Way's Thick Disk. HALLATT T. and LEE E.J.
2025ApJ...980...34R 47           X         1 17 ~ Detectability of Emission from Exoplanet Outflows Calculated by pyTPCI, a New 1D Radiation-hydrodynamic Code. ROSENER R., ZHANG M. and BEAN J.L.
2025AJ....169..204Z 233           X C F     3 35 ~ Constraining Atmospheric Composition from the Outflow: Helium Observations Reveal the Fundamental Properties of Two Planets Straddling the Radius Gap. ZHANG M., BEAN J.L., WILSON D., et al.
2025MNRAS.539.2144A 205       D       C F     21 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.
2025A&A...698A.112L 93             C       1 84 ~ sunset: A database of synthetic atmospheric-escape transmission spectra for nearly every transiting planet. LINSSEN D., OKLOPCIC A. and MacLEOD M.
2025A&A...700A.222C viz 47           X         1 11 ~ Characterizing planetary systems with SPIRou: Detection of a sub-Neptune in a 6-day period orbit around the M dwarf Gl 410. CARMONA A., DELFOSSE X., OULD-ELHKIM M., et al.

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