|
other query modes : |
Identifier query |
Coordinate query |
Criteria query |
Reference query |
Basic query |
Script submission |
TAP |
Output options |
Object types |
Help |
| TOI-4138 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST12:08:51 |
| 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..273O |
17 | D | 1 | 185 | 13 | Identifying planetary transit candidates in TESS full-frame image light curves via convolutional neural networks. | OLMSCHENK G., ISHITANI SILVA S., RAU G., et al. | ||
| 2022MNRAS.509.2908M | 1149 | A | D | X C F | 26 | 5 | 3 |
TIC 257060897b: An inflated, low-density, hot-Jupiter transiting a rapidly evolving subgiant star. |
MONTALTO M., MALAVOLTA L., GREGORIO 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...33K |
17 | D | 1 | 3171 | 19 | The TESS Faint-star Search: 1617 TOIs from the TESS Primary Mission. | KUNIMOTO M., DAYLAN T., GUERRERO N., et al. | ||
|
2024A&A...691A..53S |
18 | D | 2 | 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 |
19 | D | 1 | 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. | ||
| 2025RNAAS...9..275M | 19 | D | 1 | 365 | ~ | An In-depth Study of Brown Dwarfs with TESS. | MARCADON F. and PRSA A. | ||
| 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. |