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LF 8 +14 341 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST08:25:18 |
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 |
---|---|---|---|---|---|---|---|---|---|
1959ApJS....4...23M | 1574 | 1 | Stellar spectra in Milky Way regions. VIII. A region in Orion. | McCUSKEY S.W. | |||||
2015A&A...579A..19A | 16 | D | 1 | 8376 | 75 | K2 Variable Catalogue: Variable stars and eclipsing binaries in K2 campaigns 1 and 0. | ARMSTRONG D.J., KIRK J., LAM K.W.F., et al. | ||
2016ApJS..222...14V | 16 | D | 1 | 209 | 177 | Planetary candidates from the first year of the K2 mission. | VANDERBURG A., LATHAM D.W., BUCHHAVE L.A., et al. | ||
2016ApJS..225...32B | 16 | D | 1 | 1473 | 266 | Spectral properties of cool stars: extended abundance analysis of 1,617 planet-search stars. | BREWER J.M., FISCHER D.A., VALENTI J.A., et al. | ||
2016ApJS..226....7C | 16 | D | 7 | 400 | 165 | 197 candidates and 104 validated planets in K2's first five fields. | CROSSFIELD I.J.M., CIARDI D.R., PETIGURA E.A., et al. | ||
2019AJ....158...87D | 17 | D | 2 | 179 | ~ | Characterizing K2 candidate planetary systems orbiting low-mass stars. IV. Updated properties for 86 cool dwarfs observed during Campaigns 1-17. | DRESSING C.D., HARDEGREE-ULLMAN K., SCHLIEDER J.E., et al. | ||
2019ApJS..244...11K | 17 | D | 1 | 2120 | 48 | Detection of hundreds of new planet candidates and eclipsing binaries in K2 campaigns 0-8. | KRUSE E., AGOL E., LUGER R., et al. | ||
2022ApJS..258...16P | 18 | D | 1 | 4579 | 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. | ||
2022MNRAS.514.4300B | 18 | D | 1 | 954 | 7 | Linking chromospheric activity and magnetic field properties for late-type dwarf stars. | BROWN E.L., JEFFERS S.V., MARSDEN S.C., et al. | ||
2023A&A...670A..75C | 65 | D | X | 2 | 53 | 4 | New compact hierarchical triple system candidates identified using Gaia DR3. | CZAVALINGA D.R., MITNYAN T., RAPPAPORT S.A., et al. |