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| BD+43 3217 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST06:20:20 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 1952ApJ...116..592M | 238 | 19 | Stellar spectra and colors in Cygnus at galactic latitude +14 deg. | MacRAE D.A. | |||||
|
2012ApJS..199...24T |
15 | D | 1 | 5394 | 66 | Detection of potential transit signals in the first three quarters of Kepler mission data. | TENENBAUM P., CHRISTIANSEN J.L., JENKINS J.M., et al. | ||
|
2016A&A...594A..39F |
16 | D | 1 | 51408 | 86 | Activity indicators and stellar parameters of the Kepler targets. An application of the ROTFIT pipeline to LAMOST-Kepler stellar spectra. | FRASCA A., MOLENDA-ZAKOWICZ J., DE CAT P., et al. | ||
|
2014ASPC..485..223B |
15 | D | 1 | 465820 | 45 | The JMMC stellar diameters catalog v2 (JSDC): a new release based on SearchCal improvements | BOURGES L., LAFRASSE S., MELLA G., et al. | ||
|
2019MNRAS.490.3158C |
16 | D | 1 | 465839 | 28 | A catalogue of stellar diameters and fluxes for mid-infrared interferometry. | CRUZALEBES P., PETROV R.G., ROBBE-DUBOIS S., et al. | ||
|
2021ApJS..255...17S |
17 | D | 1 | 39591 | 57 | Surface rotation and photometric activity for Kepler targets. II. G and F main-sequence stars and cool subgiant stars. | SANTOS A.R.G., BRETON S.N., MATHUR S., et al. | ||
|
2022MNRAS.510.5623M |
17 | D | 1 | 144 | 9 | Inferring the rotation period distribution of stars from their projected rotation velocities and radii: Application to late-F/early-G Kepler stars. | MASUDA K., PETIGURA E.A. and HALL O.J. | ||
|
2023ApJS..264...17Z |
17 | D | 4 | 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. | ||
|
2024MNRAS.533.1290S |
18 | D | 1 | 7737 | ~ | The impact of stellar metallicity on rotation and activity evolution in the Kepler field using gyro-kinematic ages. | SEE V., LU Y., AMARD L., et al. |