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| TOI-4087 , the SIMBAD biblio (11 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST10:21:10 |
| 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.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. | ||
|
2023ApJS..265....1Y |
583 | D | X | 14 | 55 | 5 | The TESS Grand Unified Hot Jupiter Survey. II. Twenty New Giant Planets. | YEE S.W., WINN J.N., HARTMAN J.D., et al. | |
| 2024ApJS..274...20P | 18 | D | 1 | 223 | ~ | Statistics and Habitability of F-type Star-Planet Systems. | PATEL S.D., CUNTZ M. and WEINBERG N.N. | ||
|
2024AJ....168..177C |
18 | D | 1 | 260 | ~ | Detecting Exoplanet Transits with the Next Generation of X-Ray Telescopes. | CILLEY R., KING G.W. and CORRALES L. | ||
|
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...978...46K | 19 | D | 1 | 49 | ~ | Separating Super-puffs versus Hot Jupiters among Young Puffy Planets. | KARALIS A., LEE E.J. and THORNGREN D.P. | ||
| 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. |