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| TOI-1696 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST09:39:44 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
2021AJ....161...24G |
17 | D | 1 | 412 | 63 | Vetting of 384 TESS Objects of Interest with TRICERATOPS and statistical validation of 12 planet candidates. | GIACALONE S., DRESSING C.D., JENSEN E.L.N., et al. | ||
|
2021AJ....162...75L |
17 | D | 1 | 517 | 28 | Speckle observations of TESS exoplanet host stars. II. Stellar companions at 1-1000 au and implications for small planet detection. | LESTER K.V., MATSON R.A., HOWELL S.B., et al. | ||
|
2022MNRAS.512L..60H |
17 | D | 1 | 1974 | 9 | The flaring TESS Objects of Interest: flare rates for all two-minute cadence TESS planet candidates. | HOWARD W.S. | ||
| 2022AJ....163..286B | 1762 | T | D | S X C | 39 | 18 | 3 |
TOI-1696 and TOI-2136: Constraining the Masses of Two Mini-Neptunes with the Habitable-Zone Planet Finder. |
BEARD C., ROBERTSON P., KANODIA S., et al. |
| 2022AJ....163..298M | 1830 | T A | D | X C | 42 | 19 | 7 |
TOI-1696: A Nearby M4 Dwarf with a 3 R⊕ Planet in the Neptunian Desert. |
MORI M., LIVINGSTON J.H., DE LEON J., et al. |
| 2024ApJS..271...48G | 18 | D | 3 | 117 | ~ | Metallicities and Refined Stellar Parameters for 52 Cool Dwarfs with Transiting Planets and Planet Candidates. | GORE R., GIACALONE S., DRESSING C.D., et al. | ||
|
2024A&A...689A.302G |
18 | D | 1 | 1270 | ~ | Multiplicity of stars with planets in the solar neighbourhood. | GONZALEZ-PAYO J., CABALLERO J.A., GORGAS J., et al. | ||
|
2024A&A...691A..53S |
18 | D | 1 | 4078 | ~ | SWEET-Cat: A view on the planetary mass-radius relation. | SOUSA S.G., ADIBEKYAN V., DELGADO-MENA E., et al. | ||
|
2025ApJ...993..233W |
19 | D | 1 | 391 | ~ | An Analysis of the Radius Gap in a Sample of Kepler, K2, and TESS Exoplanets Orbiting M-dwarf Stars. | WANDERLEY F., CUNHA K., SMITH V.V., et al. | ||
| 2026AJ....171..157S | 20 | D | 2 | 480 | ~ | Most Hot Jupiters Were Cool Giant Planets for More Than 1 Gyr. | SCHMIDT S.P. and SCHLAUFMAN K.C. |