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| WASP-180B , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST10:21:25 |
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 |
|---|---|---|---|---|---|---|---|---|---|
| 2019MNRAS.490.2467T | 447 | A | D | X C F | 10 | 6 | ~ | WASP-180Ab: Doppler tomography of a hot Jupiter orbiting the primary star in a visual binary. | TEMPLE L.Y., HELLIER C., ANDERSON D.R., et al. |
2020MNRAS.498.1726M 
|
16 | D | 1 | 337 | 26 | A search for transiting planets around FGKM dwarfs and subgiants in the TESS full frame images of the Southern ecliptic hemisphere. | MONTALTO M., BORSATO L., GRANATA V., et al. | ||
|
2022PASP..134h2001A
|
17 | D | 1 | 366 | 39 | Stellar Obliquities in Exoplanetary Systems. | ALBRECHT S.H., DAWSON R.I. and WINN J.N. | ||
| 2023MNRAS.521.2969B | 17 | D | 3 | 87 | 2 | Planet engulfment detections are rare according to observations and stellar modelling. | BEHMARD A., DAI F., BREWER J.M., et al. | ||
| 2023A&A...674A.120A | 17 | D | 1 | 189 | 1 | DREAM II. The spin-orbit angle distribution of close-in exoplanets under the lens of tides. | ATTIA O., BOURRIER V., DELISLE J.-B., et al. | ||
|
2024ApJS..270...14W
|
18 | D | 1 | 333 | ~ | Long-term Variations in the Orbital Period of Hot Jupiters from Transit-timing Analysis Using TESS Survey Data. | WANG W., ZHANG Z., CHEN Z., et al. | ||
| 2024AJ....167..126R | 18 | D | 2 | 141 | ~ | The Orbital Geometries and Stellar Obliquities of Exoplanet-hosting Multistar Systems. | RICE M., GERBIG K. and VANDERBURG A. | ||
|
2024AJ....168..177C
|
45 | X | 1 | 260 | ~ | Detecting Exoplanet Transits with the Next Generation of X-Ray Telescopes. | CILLEY R., KING G.W. and CORRALES L. | ||
| 2026ApJ...996L...7W | 20 | D | 1 | 48 | ~ | Unified Kraft Break at ∼6500 K: A Newly Identified Single-star Obliquity Transition Matches the Classical Rotation Break. | WANG X.-Y., WANG S. and ONG J.M.J. | ||
|
2026A&A...705A.142R
|
50 | X | 1 | 55 | ~ | True spin-orbit obliquity distribution: Data-driven confirmation of no clustering of misaligned planets. | ROSSI A.M., RAINER M., BORSA F., et al. |
