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| BD-14 1137b , the SIMBAD biblio (39 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST11:57:28 |
| Bibcode/DOI | Score |
in Title|Abstract| Keywords |
in a table | in teXt, Caption, ... | Nb occurence | Nb objects in ref |
Citations (from ADS) |
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 |
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 |
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 |
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 |
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 |
17 | D | 1 | 76 | ~ | ExoMDN: Rapid characterization of exoplanet interior structures with mixture density networks. | BAUMEISTER P. and TOSI N. | ||
|
2024AJ....167..203M |
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 |
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 |
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 |
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 |
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. |