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| BD+37 3490 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST04:38:16 |
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 |
|---|---|---|---|---|---|---|---|---|---|
2011A&A...534A.125U 
|
15 | D | O | 2 | 764 | 297 | The Kepler characterization of the variability among A- and F-type stars. I. General overview. | UYTTERHOEVEN K., MOYA A., GRIGAHCENE A., et al. | |
| 2012MNRAS.422.2960T | 15 | D | 1 | 29 | 41 | Spectrum analysis of bright Kepler γ Doradus candidate stars. | TKACHENKO A., LEHMANN H., SMALLEY B., 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. | ||
| 2017MNRAS.467.4663S | 16 | D | 1 | 47 | 11 | Search for exoplanets around pulsating stars of A-F type in Kepler short-cadence data and the case of KIC 8197761. | SOWICKA P., HANDLER G., DEBSKI B., et al. | ||
|
2018MNRAS.479..183B
|
16 | D | 1 | 2598 | 17 | Gaia luminosities of pulsating A-F stars in the Kepler field. | BALONA L.A. | ||
| 2019RAA....19....1Q | 16 | D | 1 | 172 | 1 | Physical properties of γ Doradus pulsating stars and their relationship with long-period δ Scuti variables. | QIAN S.-B., LI L.-J., HE J.-J., et al. | ||
|
2019MNRAS.485.2380M
|
16 | D | 1 | 14330 | 108 | Gaia-derived luminosities of Kepler A/F stars and the pulsator fraction across the δ Scuti instability strip. | MURPHY S.J., HEY D., VAN REETH T., 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. | ||
|
2020A&A...638A..59B
|
16 | D | 1 | 2220 | 17 | Unveiling the power spectra of δ Scuti stars with TESS. The temperature, gravity, and frequency scaling relation. | BARCELO FORTEZA S., MOYA A., BARRADO D., et al. |
