UCAC3 265-168646 , the SIMBAD biblio

UCAC3 265-168646 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST16:15:20


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Title First 3 Authors
2012MNRAS.426.2413B 15       D               1 62 18 A search for SX Phe stars among Kepler δ Scuti stars. BALONA L.A. and NEMEC J.M.
2016MNRAS.461.4215M 214       D     X C F     4 4 16 Finding binaries from phase modulation of pulsating stars with Kepler - IV. Detection limits and radial velocity verification. MURPHY S.J., SHIBAHASHI H. and BEDDING T.R.
2017MNRAS.466.1290N viz 929       D     X C       23 66 14 Metal-rich SX Phe stars in the Kepler field. NEMEC J.M., BALONA L.A., MURPHY S.J., et al.
2018MNRAS.474.4322M viz 40           X         1 390 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.
2018A&A...614A..46B viz 16       D               1 1063 5 The envelope of the power spectra of over a thousand δ Scuti stars. The Teff - νmax scaling relation. BARCELO FORTEZA S., ROCA CORTES T. and GARCIA R.A.
2018MNRAS.479..183B viz 16       D               1 2598 17 Gaia luminosities of pulsating A-F stars in the Kepler field. BALONA L.A.
2018AcA....68..237R 40           X         1 57 ~ The Cluster AgeS Experiment (CASE). Variable Stars in the Field of the Globular Cluster M10. ROZYCZKA M., NARLOCH W., SCHWARZENBERG-CZERNY A., et al.
2019MNRAS.485.2380M viz 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.
2020AJ....159..202H 329       S   X C       6 4 ~ Forward modeling the orbits of companions to pulsating stars from their light travel time variations. HEY D.R., MURPHY S.J., FOREMAN-MACKEY D., et al.
2020A&A...638A..59B viz 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.

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