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| TOI-1073 , the SIMBAD biblio (11 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST08:53:17 |
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More on score
| 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 |
|---|---|---|---|---|---|---|---|---|---|
2019AJ....158..122K 
|
16 | D | 1 | 290057 | 150 | Untangling the Galaxy. I. Local structure and star formation history of the Milky Way. | KOUNKEL M. and COVEY K. | ||
|
2020AJ....159..173H
|
2609 | D | X C | 63 | 18 | 7 | HATS-47b, HATS-48Ab, HATS-49b, and HATS-72b: four warm giant planets transiting K dwarfs. | HARTMAN J.D., JORDAN A., BAYLISS D., et al. | |
| 2021MNRAS.504.5788R | 17 | D | 1 | 105 | 14 | Characterization of 92 southern TESS candidate planet hosts and a new photometric [Fe/H] relation for cool dwarfs. | RAINS A.D., ZERJAL M., IRELAND M.J., 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. | ||
|
2022ApJS..259...62I
|
17 | D | 1 | 395 | 24 | TESS Transit Timing of Hundreds of Hot Jupiters. | IVSHINA E.S. and WINN J.N. | ||
|
2022AJ....163..228P
|
17 | D | 1 | 354 | 20 | Empirical Limb-darkening Coefficients and Transit Parameters of Known Exoplanets from TESS. | PATEL J.A. and ESPINOZA N. | ||
|
2022MNRAS.513..102C
|
17 | D | 1 | 961 | 6 | The TESS Triple-9 Catalog: 999 uniformly vetted exoplanet candidates. | CACCIAPUOTI L., KOSTOV V.B., KUCHNER M., et al. | ||
|
2023AJ....166..219D
|
235 | D | X | 6 | 275 | ~ | Understanding the Planetary Formation and Evolution in Star Clusters (UPiC). I. Evidence of Hot Giant Exoplanets Formation Timescales. | DAI Y.-Z., LIU H.-G., YANG J.-Y., et al. | |
|
2024A&A...689A..53B
|
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...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. | ||
| 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. |
