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| UCAC4 671-082611 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST19:27:59 |
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 |
|---|---|---|---|---|---|---|---|---|---|
2009AcA....59..193M 
|
15 | D | 1 | 582 | 13 | Photometric study of variable stars in the open cluster NGC 6866. | MOLENDA-ZAKOWICZ J., KOPACKI G., STESLICKI M., et al. | ||
|
2010AstL...36..338F
|
15 | D | 1 | 1150 | 6 | Proper motions and CCD photometry of stars in the region of the open cluster NGC 6866. | FROLOV V.N., ANANJEVSKAJA Y.K., GORSHANOV D.L., et al. | ||
|
2015MNRAS.453.1095B
|
16 | D | 1 | 739 | 12 | A comprehensive study of the open cluster NGC 6866. | BOSTANCI Z.F., AK T., YONTAN T., et al. | ||
|
2019ApJ...872..137S
|
17 | D | 1 | 26099 | 39 | Constraining metallicity-dependent mixing and extra mixing using [C/N] in alpha-rich field giants. | SHETRONE M., TAYAR J., JOHNSON J.A., et al. | ||
|
2019ApJ...879...69T
|
17 | D | 1 | 222609 | 141 | The Payne: self-consistent ab initio fitting of stellar spectra. | TING Y.-S., CONROY C., RIX H.-W., et al. | ||
|
2019AJ....158..147H
|
17 | D | 1 | 44781 | 43 | Spectrophotometric parallaxes with linear models: accurate distances for luminous red-giant stars. | HOGG D.W., EILERS A.-C. and RIX H.-W. | ||
|
2020MNRAS.493.1388Y
|
17 | D | 1 | 3215 | 20 | Asteroseismology of luminous red giants with Kepler I: long-period variables with radial and non-radial modes. | YU J., BEDDING T.R., STELLO D., et al. | ||
|
2020AJ....160..120J
|
17 | D | 1 | 365761 | 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. | ||
|
2020ApJ...900....4S
|
17 | D | 1 | 121537 | 14 | The age distribution of stars in the Milky Way bulge. | SIT T. and NESS M.K. |
