|
other query modes : |
Identifier query |
Coordinate query |
Criteria query |
Reference query |
Basic query |
Script submission |
TAP |
Output options |
Object types |
Help |
| CD-26 2288d , the SIMBAD biblio (20 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST10:16:35 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
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. | ||
| 2021MNRAS.507.2782O | 1380 | A | D | X C | 33 | 11 | 16 | TOI-431/HIP 26013: a super-Earth and a sub-Neptune transiting a bright, early K dwarf, with a third RV planet. | OSBORN A., ARMSTRONG D.J., CALE B., et al. |
|
2021ApJS..256...33T |
518 | D | X C | 12 | 56 | 23 | The Magellan-TESS Survey. I. Survey description and midsurvey results. | TESKE J., WANG S.X., WOLFGANG A., et al. | |
|
2022AJ....164...15E |
17 | D | 2 | 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. | ||
| 2022A&A...662A..19J | 85 | F | 1 | 12 | 9 | Nucleation and growth of iron pebbles explains the formation of iron-rich planets akin to Mercury. | JOHANSEN A. and DORN C. | ||
| 2023MNRAS.519.6028R | 17 | D | 1 | 86 | 7 | Exoplanet atmosphere evolution: emulation with neural networks. | ROGERS J.G., JANO MUNOZ C., OWEN J.E., et al. | ||
|
2023ApJS..265....4K |
17 | D | 1 | 454 | 2 | ExoClock Project. III. 450 New Exoplanet Ephemerides from Ground and Space Observations. | KOKORI A., TSIARAS A., EDWARDS B., et al. | ||
|
2023A&A...676A.106B |
17 | D | 1 | 76 | ~ | ExoMDN: Rapid characterization of exoplanet interior structures with mixture density networks. | BAUMEISTER P. and TOSI N. | ||
| 2024MNRAS.527.4467F | 18 | D | 1 | 72 | ~ | NIGHT: A compact, near-infrared, high-resolution spectrograph to survey helium in exoplanet systems. | FARRET JENTINK C., BOURRIER V., LOVIS C., et al. | ||
| 2024MNRAS.530.3500K | 735 | D | S X C | 15 | 9 | ~ | The XUV-driven escape of the planets around TOI-431 and ν2 Lupi. | KING G.W., CORRALES L.R., FERNANDEZ FERNANDEZ J., 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...687L...1L |
18 | D | 2 | 140 | ~ | Resonant sub-Neptunes are puffier. | LELEU A., DELISLE J.-B., BURN R., et al. | ||
| 2025ApJ...980..175J | 1166 | A | D | X C | 25 | 14 | ~ | Estimating the Mass Escaping Rates of Radius-valley-spanning Planets in the TOI-431 System via X-Ray and Ultraviolet Evaporation. | JIANG X., JIANG J.H., BURN R., et al. |
| 2025MNRAS.537.3175A | 19 | D | 1 | 68 | ~ | The NCORES programme: precise planetary masses, null results, and insight into the planet mass distribution near the radius gap. | ARMSTRONG D.J., OSBORN A., BURN R., et al. | ||
| 2025AJ....169..239M | 93 | X | 2 | 23 | ~ | Low 4.5 μm Dayside Emission Disfavors a Dark Bare-rock Scenario for the Hot Super-Earth TOI-431 b. | MONAGHAN C., ROY P.-A., BENNEKE B., 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. | ||
| 2025ApJ...987...85R | 19 | D | 1 | 241 | ~ | Characterizing Exoplanets for Assessing Their Potential Habitability. | RODRIGUEZ-MOZOS J.M. and MOYA A. | ||
| 2025AJ....170..108H | 47 | X | 1 | 14 | ~ | HD 35843: A Sun-like Star Hosting a Long-period Sub-Neptune and Inner Super-Earth. | HESSE K., MIRELES I., BOUCHY F., et al. | ||
| 2025A&A...701A.184K | 93 | C | 1 | 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. |