Cecil G. Davis

VizieR Online Data Catalog: Spectroscopic analysis of Tuc III stream (Li+, 2018)

T. S. Li, Joshua D. Simon, Kyler Kuehn, Andrew B. Pace et autres

VizieR Online Data Catalog: R-band light curves of DES J0408-5359 (Courbin+ 2018)

F. Courbin, V. Bonvin, E. Buckley‐Geer, Christopher D. Fassnacht et autres

Spectroscopic Classification of AT2016cvv as a normal Type Ia Supernova

D. C. Leonard, Patrick Sheehan, Darragh N. McCarthy, Katherine B. Follette et autres

Spectroscopic Classification of AT2016cvw as a normal Type Ia Supernova

D. C. Leonard, Patrick Sheehan, Darragh N. McCarthy, Katherine B. Follette et autres

NOT and LT spectroscopic classification of supernovae Gaia15acz and Gaia15aek

Seppo Mattila, J. Harmanen, T. Kangas, Andrzej S. Piascik et autres

Time-dependent fourier analysis, application to nonlinear pulsations of stellar models

Cecil G. Davis, G. Kovácks, J. R. Buchler

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Polarimetric Standard Stars Observed with FORS1 at ESO-VLT

Elena Mason, S. Bagnulo, T. Szeifert, R Cabanac et autres

A Paranal Observatory project aims to analyze all the polarimetric standard stars in use at FORS1 to both check they have a constant polarization signal and measure the instrumental polarization. Preliminary results for 3 standards in the FORS1 calibration plans are presented.

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Photometry of Gliese 372

Tod F. Ramseyer, C. Lasley, Cecil G. Davis, C. Leonard et autres

Photometry of Gliese 372 was obtained during the 1996–1997 and 1997–1998 observing seasons. Our 3 σ limit on the presence of night-to-night variations, such as those due to eclipses or starspots, is ±0.024 mag. Over a single night, our limit on the …

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Colors of RR Lyrae Stars

Cecil G. Davis

The methods of Davis & Cox are applied to a series of models described by Bono & Stellingwerf to determine the colors of RR Lyrae stars. Convection is ignored, and the radiation flow is treated by a complete variable Eddington, multifrequency‐dependent radiative …

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Radiative Transfer Effects on the Colors of RR Lyrae Stars

Cecil G. Davis

The methods of Davis and Cox (1980), are applied to a series of models described by Bono and Stellingwerf (1994) to deter-mine the colors of RR Lyrae stars. Convection is ignored and the radiation flow is treated by a complete variable Eddington, …

The importance of radiative transfer in stellar pulsation models

Cecil G. Davis

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Computational astrophysics: Pulsating stars

Cecil G. Davis

The field of computational astrophysics in pulsating star studies has grown considerably since the advent of the computer. Initially calculations were done on the IBM 704 with 32K of memory and now we use the CRAY YMP computers with considerably more memory. …