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| BD+43 1836 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST15:52:07 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 1969ApJ...157..327U | 433 | 1 | A finding list of early-type stars in regions of intermediate galactic latitude. | UPGREN A.R. and STARON R.T. | |||||
|
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. | ||
|
2018A&A...609A.116R |
16 | D | 1 | 143018 | 65 | Empirical photometric calibration of the Gaia red clump: Colours, effective temperature, and absolute magnitude. | RUIZ-DERN L., BABUSIAUX C., ARENOU F., 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. | ||
|
2020MNRAS.493.5807C |
16 | D | 1 | 152 | ~ | Supersolar metallicity in G0-G3 main-sequence stars with V < 15. II. An extension of the sample. | CHAVEZ M., TAPIA-SCHIAVON C., BERTONE E., 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. | ||
|
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. | ||
|
2023AJ....165..267H |
17 | D | 1 | 64663 | 1 | Bioverse: A Comprehensive Assessment of the Capabilities of Extremely Large Telescopes to Probe Earth-like O2 Levels in Nearby Transiting Habitable-zone Exoplanets. | HARDEGREE-ULLMAN K.K., APAI D., BERGSTEN G.J., et al. | ||
|
2024MNRAS.533..395L |
18 | D | 1 | 1559 | ~ | Atmospheric parameters and chemical abundances within 100 pc: a sample of G, K, and M main-sequence stars. | LOPEZ-VALDIVIA R., ADAME L., ZAGALA LAGUNAS E., et al. |