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| TOI-1333 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST13:27:16 |
Sort references on where and how often the object is cited
trying to find the most relevant references on this object.
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 |
|---|---|---|---|---|---|---|---|---|---|
2021AJ....161..194R 
|
2342 | A | D | S X C | 55 | 22 | 24 | TESS delivers five new hot giant planets orbiting bright stars from the full-frame images. | RODRIGUEZ J.E., QUINN S.N., ZHOU G., et al. |
|
2022AJ....163..160B
|
17 | D | 2 | 240 | 9 | Stellar Companions to TESS Objects of Interest: A Test of Planet-Companion Alignment. | BEHMARD A., DAI F. and HOWARD A.W. | ||
|
2022PASP..134h2001A
|
60 | D | X | 2 | 366 | 39 | Stellar Obliquities in Exoplanetary Systems. | ALBRECHT S.H., DAWSON R.I. and WINN J.N. | |
| 2022MNRAS.516...75B | 102 | D | C | 3 | 115 | 9 | Exploring the dependence of hot Jupiter occurrence rates on stellar mass with TESS. | BELEZNAY M. and KUNIMOTO M. | |
|
2024AJ....167...74L
|
18 | D | 1 | 318 | ~ | High-resolution Imaging of a TESS Control Sample: Verifying a Deficit of Close-in Stellar Companions to Exoplanet Host Stars. | LITTLEFIELD C., HOWELL S.B., CIARDI D.R., 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. | ||
|
2025A&A...697A.102T
|
65 | D | X | 2 | 176 | ~ | Ariel stellar characterisation III. Fast rotators and new FGK stars in the Ariel mission candidate sample. | TSANTAKI M., MAGRINI L., DANIELSKI C., et al. | |
| 2025ApJ...988L...4H | 19 | D | 1 | 301 | ~ | Hundreds of TESS Exoplanets Might Be Larger than We Thought. | HAN T., ROBERTSON P., BRANDT T.D., et al. | ||
|
2025A&A...699A.100D
|
19 | D | 1 | 2580 | ~ | The Gaia spectroscopic catalogue of exoplanets and host stars. | DE LAVERNY P., LIGI R., CRIDA A., 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. |
