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| BD-19 4173c , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.24CEST18:08:06 |
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.484.3522H | 938 | D | X C F | 21 | 6 | 17 | K2-290: a warm Jupiter and a mini-Neptune in a triple-star system. | HJORTH M., JUSTESEN A.B., HIRANO T., et al. | |
2019ApJ...874L..31T 
|
17 | D | 1 | 403 | 62 | Connecting giant planet atmosphere and interior modeling: constraints on atmospheric metal enrichment. | THORNGREN D. and FORTNEY J.J. | ||
|
2019A&A...630A.135U
|
17 | D | 1 | 501 | 16 | Beyond the exoplanet mass-radius relation. | ULMER-MOLL S., SANTOS N.C., FIGUEIRA P., et al. | ||
| 2022ApJ...925L...5B | 45 | X | 1 | 7 | 4 | The Chaotic History of the Retrograde Multi-planet System in K2-290A Driven by Distant Stars. | BEST S. and PETROVICH C. | ||
|
2022AJ....164..104R
|
45 | X | 1 | 105 | 10 | A Tendency Toward Alignment in Single-star Warm-Jupiter Systems. | RICE M., WANG S., WANG X.-Y., et al. | ||
|
2022PASP..134h2001A
|
108 | D | X | 3 | 366 | 39 | Stellar Obliquities in Exoplanetary Systems. | ALBRECHT S.H., DAWSON R.I. and WINN J.N. | |
| 2022ApJS..263...33C | 18 | D | 1 | 85 | 2 | An Early Catalog of Planet-hosting Multiple-star Systems of Order Three and Higher. | CUNTZ M., LUKE G.E., MILLARD M.J., et al. | ||
| 2023ApJ...944L..41F | 47 | X | 1 | 19 | 2 | NEID Reveals That the Young Warm Neptune TOI-2076 b Has a Low Obliquity. | FRAZIER R.C., STEFANSSON G., MAHADEVAN S., et al. | ||
| 2023A&A...674A.120A | 19 | 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. | ||
| 2023MNRAS.524.1113S | 19 | D | 1 | 85 | ~ | TESS spots a mini- interior to a hot saturn in the TOI-2000 system. | SHA L., VANDERBURG A.M., HUANG C.X., et al. |
