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| UCAC4 524-007892 , the SIMBAD biblio (8 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST05:08:10 |
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 |
|---|---|---|---|---|---|---|---|---|---|
2019ApJS..244...11K 
|
16 | D | 1 | 2119 | 48 | Detection of hundreds of new planet candidates and eclipsing binaries in K2 campaigns 0-8. | KRUSE E., AGOL E., LUGER R., et al. | ||
|
2020AJ....160..120J
|
16 | D | 1 | 365763 | 238 | APOGEE data and spectral analysis from SDSS Data Release 16: seven years of observations including first results from APOGEE-South. | JONSSON H., HOLTZMAN J.A., ALLENDE PRIETO C., et al. | ||
|
2022AJ....163..152S
|
17 | D | 1 | 583193 | 11 | APOGEE Net: An Expanded Spectral Model of Both Low-mass and High-mass Stars. | SPRAGUE D., CULHANE C., KOUNKEL M., 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...35A
|
17 | D | 1 | 611005 | 320 | The Seventeenth Data Release of the Sloan Digital Sky Surveys: Complete Release of MaNGA, MaStar, and APOGEE-2 Data. | ABDURRO'UF, ACCETTA K., AERTS C., et al. | ||
|
2022MNRAS.514.4781X
|
17 | D | 2 | 801 | ~ | Investigation of stellar magnetic activity using variational autoencoder based on low-resolution spectroscopic survey. | XIANG Y., GU S. and CAO D. | ||
|
2023ApJS..264...17Z
|
17 | D | 3 | 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. | ||
|
2026A&A...707A..73F
|
400 | S X C F | 5 | 16 | ~ | TOI-3288 b and TOI-4666 b: Two gas giants transiting low-mass stars characterised by NIRPS. | FRENSCH Y.G.C., BOUCHY F., LO CURTO G., et al. |
