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| TYC 3122-289-1 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST22:05:24 |
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 |
|---|---|---|---|---|---|---|---|---|---|
2019A&A...626A.119G 
|
1584 | S X C | 37 | 23 | ~ | The EBLM project. VI. Mass and radius of five low-mass stars in F+M binaries discovered by the WASP survey. | GILL S., MAXTED P.F.L., EVANS J.A., et al. | ||
|
2019MNRAS.488.4905S
|
16 | D | 1 | 1041 | ~ | SuperWASP dispositions and false positive catalogue. | SCHANCHE N., COLLIER CAMERON A., ALMENARA J.M., et al. | ||
| 2020MNRAS.491.1548G | 41 | X | 1 | 3 | ~ | NGTS and WASP photometric recovery of a single-transit candidate from TESS. | GILL S., BAYLISS D., COOKE B.F., et al. | ||
|
2022ApJS..258...16P
|
17 | D | 1 | 4582 | 43 | TESS Eclipsing Binary stars. I. Short-cadence observations of 4584 eclipsing binaries in sectors 1-26. | PRSA A., KOCHOSKA A., CONROY K.E., et al. | ||
|
2023ApJS..264...17Z
|
17 | D | 1 | 31380 | 1 | Stellar Parameters and Spectroscopic Properties of TESS Objects Observed in the LAMOST Low- and Medium-resolution Spectral Survey. | ZHANG L.-Y., SU T., MISRA P., et al. | ||
|
2023A&A...674A..34G
|
17 | D | 1 | 307215 | 85 | Gaia Data Release 3 Stellar multiplicity, a teaser for the hidden treasure. | GAIA COLLABORATION, ARENOU F., BABUSIAUX C., et al. | ||
| 2024MNRAS.531.1765L | 18 | D | 1 | 37 | ~ | The first low-mass eclipsing binary within the fully convective zone from TMTS. | LIU C., WANG X., ZHANG X., et al. | ||
| 2025AJ....170..322E | 65 | D | X | 2 | 209 | ~ | Eclipse Timing Variations of Circumbinary Substellar Objects in TESS Data. | ESMER E.M. and DAYLAN T. | |
| 2025AJ....170..356T | 19 | D | 1 | 514 | ~ | A Sample of Eccentric Eclipsing Binaries in TESS. | TANG Y., CHEN X., GAI N., et al. |
