BD-14 1137b , the SIMBAD biblio

BD-14 1137b , the SIMBAD biblio (39 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST11:57:28


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Title First 3 Authors
2020ApJ...897....7M 140       D     X C       3 36 18 Tidal inflation reconciles low-density sub-Saturns with core accretion. MILLHOLLAND S., PETIGURA E. and BATYGIN K.
2020AJ....160..114C viz 1153     A D S   X C       27 17 19 The multiplanet system TOI-421: a warm Neptune and a super puffy mini-Neptune transiting a G9 V star in a visual binary. CARLEO I., GANDOLFI D., BARRAGAN O., et al.
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.
2021A&A...652A.110L 17       D               1 82 7 Why do more massive stars host larger planets? LOZOVSKY M., HELLED R., PASCUCCI I., et al.
2021ApJ...921...24S viz 17       D               1 328 1 The occurrence-weighted median planets discovered by transit surveys orbiting solar-type stars and their implications for planet formation and evolution. SCHLAUFMAN K.C. and HALPERN N.D.
2022MNRAS.510.2111K 1039       D     X C F     23 15 6 Atmospheric mass-loss and stellar wind effects in young and old systems - I. Comparative 3D study of TOI-942 and TOI-421 systems. KUBYSHKINA D., VIDOTTO A.A., VILLARREAL D'ANGELO C., et al.
2022MNRAS.510.3039K 1234       S   X C F     26 9 3 Atmospheric mass loss and stellar wind effects in young and old systems - II. Is TOI-942 the past of TOI-421 system? KUBYSHKINA D., VIDOTTO A.A., VILLARREAL D'ANGELO C., et al.
2022AJ....164...15E viz 17       D               1 514 13 The Ariel Target List: The Impact of TESS and the Potential for Characterizing Multiple Planets within a System. EDWARDS B. and TINETTI G.
2022MNRAS.515..706B 2086           X C F     47 9 ~ On the transit spectroscopy features of warm Neptunes in the TOI-421 system, revealed with their 3D aeronomy simulations. BEREZUTSKY A.G., SHAIKHISLAMOV I.F., RUMENSKIKH M.S., et al.
2023AJ....165...14B 44           X         1 26 3 Importance of Sample Selection in Exoplanet-atmosphere Population Studies. BATALHA N.E., WOLFGANG A., TESKE J., et al.
2023RAA....23f5005B 17       D               1 60 ~ Relation between Mass and Radius of Exoplanets Distinguished by their Density. BETZLER A.S. and MIRANDA J.G.V.
2023A&A...676A.106B viz 17       D               1 76 ~ ExoMDN: Rapid characterization of exoplanet interior structures with mixture density networks. BAUMEISTER P. and TOSI N.
2024AJ....167..203M viz 45           X         1 805 ~ DIAmante TESS AutoRegressive Planet Search (DTARPS). II. Hundreds of New TESS Candidate Exoplanets. MELTON E.J., FEIGELSON E.D., MONTALTO M., et al.
2024MNRAS.530.2166B 18       D               1 79 ~ Cool Gaseous Exoplanets: surveying the new frontier with Twinkle. BOOTH L., SARKAR S., GRIFFIN M., et al.
2024A&A...685A.143M viz 18       D               1 535 ~ Planets similar in size are often dissimilar in interior. MAMONOVA E., SHAN Y., HATALOVA P., 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...686A.301K viz 1523     A D     X C       34 5 ~ Characterisation of the TOI-421 planetary system using CHEOPS, TESS, and archival radial velocity data. KRENN A.F., KUBYSHKINA D., FOSSATI L., 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.
2024MNRAS.533..374B 134           X         3 11 ~ 3D aeronomy of two mini-neptunes in the HD 63433 system and their in-transit absorption in Ly α and metastable He I lines. BEREZUTSKY A.G., SHAIKHISLAMOV I.F., RUMENSKIKH M.S., et al.
2024AJ....168..115B viz 18       D               1 224 ~ Different Planetary Eccentricity-period (PEP) Distributions of Small and Giant Planets. BASHI D., MAZEH T. and FAIGLER S.
2025AJ....169....8H 112       D     X         3 27 ~ The Search for the In-betweeners: How Packed Are TESS Planetary Systems? HORNER J., WITTENMYER R.A., KANE S.R., et al.
2025MNRAS.538.3263P 140           X         3 15 ~ Limits on the atmospheric metallicity and aerosols of the sub-Neptune GJ 3090 b from high-resolution CRIRES+ spectroscopy. PARKER L.T., MENDONCA J.M., DIAMOND-LOWE H., et al.
2025ApJ...984L..44D 2267 T   A     X C       47 8 ~
TOI-421 b: A Hot Sub-Neptune with a Haze-free, Low Mean Molecular Weight Atmosphere.
DAVENPORT B., KEMPTON E.M.-R., NIXON M.C., et al.
2025MNRAS.540.1144F 112       D         F     2 159 ~ The eccentricity distribution of warm sub-Saturns in TESS. FAIRNINGTON T.R., DONG J., HUANG C.X., et al.
2025ApJ...987...85R 19       D               1 241 ~ Characterizing Exoplanets for Assessing Their Potential Habitability. RODRIGUEZ-MOZOS J.M. and MOYA A.
2025A&A...700L..14S 75     A     X         2 11 ~ Volatile enrichment in low-mass planets as signatures of past planetary disruption. SUCERQUIA M., MONTESINOS M., AGUDELO A.M., et al.
2025ApJ...990..187W 47           X         1 13 ~ Formation of Organic Hazes in CO2-rich Sub-Neptune Atmospheres within the Graphite Stability Regime. WANG S., YANG Z., HE C., et al.
2025A&A...701A..79N 47           X         1 16 ~ The Hot-Neptune Initiative (HONEI) I. Two hot sub-Neptunes on a close-in eccentric orbit (TOI-5800 b) and a farther-out circular orbit (TOI-5817 b). NAPONIELLO L., VISSAPRAGADA S., BONOMO A.S., et al.
2025A&A...701A.184K 93           X         2 18 ~ The SPACE Program I. The featureless spectrum of HD 86226 c challenges sub-Neptune atmosphere trends. KAHLE K.A., BLECIC J., ASHTARI R., et al.
2025A&A...701A.190B 1008     A     X C       21 10 ~ ATREIDES I. Embarking on a trek across the exo-Neptunian landscape with the TOI-421 system. BOURRIER V., STEINER M., CASTRO-GONZALEZ A., et al.
2025A&A...701A.296F 47           X         1 7 ~ Competing chemical signatures in the atmosphere of TOI-270 d: Inference of sulfur and carbon chemistry. FELIX L., KITZMANN D., DEMORY B.-O., et al.
2025ApJ...993L..46B 159       D     X         4 10 ~ Not All Sub-Neptune Exoplanets Have Magma Oceans. BREZA B., NIXON M.C. and KEMPTON E.M.-R.
2025AJ....170..298S 47           X         1 8 ~ A Comprehensive Reanalysis of K2-18 b's JWST NIRISS+NIRSpec Transmission Spectrum. SCHMIDT S.P., MacDONALD R.J., TSAI S.-M., et al.
2025ApJ...994..184C 47           X         1 11 ~ Mapping the SO2 Shoreline in Gas Giant Exoplanets. CROSSFIELD I.J.M., AHRER E.-M., BRANDE J., et al.
2025ApJ...995...95N 47           X         1 9 ~ Magma Ocean Interactions Can Explain JWST Observations of the Sub-Neptune TOI-270 d. NIXON M.C., SOMERS R.S., SAVEL A.B., et al.
2025ApJ...995L..43B 93           X         2 12 ~ A Compact Multiplanet System of Three Transiting Giant Planets around TIC 118798035. BRAHM R., TRIFONOV T., JORDAN A., et al.
2026AJ....171..178G 500           X         10 21 ~ JWST COMPASS: Insights into the Systematic Noise Properties of NIRSpec/G395H from a Uniform Reanalysis of Seven Transmission Spectra. GORDON T.A., BATALHA N.M., BATALHA N.E., et al.
2026AJ....171..180W 300           X C       5 12 ~ JWST COMPASS: NIRSpec/G395H Transmission Observations of the Sub-Neptune HD 15337 c. WALLACK N.L., GAO P., GREKLEK-MCKEON M., et al.
2026MNRAS.545f2066O 50           X         1 9 ~ Resolving the flat-spectrum conundrum: clumpy aerosol distributions in sub-Neptune atmospheres. OWEN J.E. and KIRK J.

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