ASAS J185846+4109.9 , the SIMBAD biblio

ASAS J185846+4109.9 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.20CEST04:29:08


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Title First 3 Authors
2009AcA....59...33P viz 15       D               1 952 71 The All Sky Automated Survey. The Catalog of Variable Stars in the Kepler field of view. PIGULSKI A., POJMANSKI G., PILECKI B., et al.
2011A&A...534A.125U viz 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.
2014AJ....148..125P 16       D               1 75 3 The EB Factory project. II. Validation with the Kepler field in preparation for K2 and TESS. PARVIZI M., PAEGERT M. and STASSUN K.G.
2016MNRAS.459.1097B 16       D               1 30 12 Combination frequencies in high-amplitude δ Scuti stars. BALONA L.A.
2016ApJ...829...23D viz 16       D               1 4044 212 The Kepler catalog of stellar flares. DAVENPORT J.R.A.
2016A&A...594A..39F viz 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.
2018MNRAS.474.4322M viz 99       D       C       5 390 89 Finding binaries from phase modulation of pulsating stars with Kepler: V. Orbital parameters, with eccentricity and mass-ratio distributions of 341 new binaries. MURPHY S.J., MOE M., KURTZ D.W., et al.
2018MNRAS.479..183B viz 16       D               1 2598 17 Gaia luminosities of pulsating A-F stars in the Kepler field. BALONA L.A.
2019MNRAS.485.2380M viz 17       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.
2020A&A...638A..59B viz 17       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.

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