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We present a Bayesian surrogate model for the analysis of periodic or quasi-periodic time series data. We describe a computationally efficient implementation that enables Bayesian model comparison. We...
We present 4 model series of the CODEX dynamical opacity-sampling models of Mira variables with solar abundances, designed to have parameters similar to $o$ Cet, R Leo and R Cas. We demonstrate that t...
Cosmological observations indicate that our universe is flat and dark energy (DE) dominated at present. The luminosity distance plays an important role in the investigation of the evolution and stru...
Quasi-periodic oscillations and dwarf nova oscillations occur in dwarf novae and nova-like variables during outburst and occasionally during quiescence, and have analogues in high-mass X-ray binaries ...
Time-series photometry of wz sge after the 2001 outburst。
In this work we present an adaptive parallel methodology to optimize the identification of time series through parametric models, applying it to the case of sunspot series. We employ high precision ...
We designed a prime focus CCD photometer, Argos, optimized for high speed time-series measurements of blue variables (Nather &Mukadam 2004) for the 2.1mtelescope at McDonald Observatory. Lack of an...
DISCRETE FOURIER TRANSFORMS OF THE SERIES WITH RANDOMLY MISSED DATA:EXPERIMENTAL TESTS。
INFLUENCE OF DIFFERENT COLLISIONAL PROCESSES ON THE STARK BROADENING WITHIN SPECTRAL SERIES: THE O VI CASE
MICROMETRIC MEASUREMENTS OF DOUBLE STARS - POP PAIRS (SERIES 47)。
MICROMETER MEASUREMENTS OF DOUBLE STARS (SERIES 48)。
MICROMETER MEASUREMENTS OF DOUBLE STARS (SERIES 50)。
A set of 71 measurements of double and multiple stars, carried out with the Large Zeiss Refractor 65/1055 cm of the Belgrade Observatory, is communicated. The bulk of these measurements, 41 in all, ...
A set of 38 mesurements of double stars, carried out with the Zeiss Refractor 65/1055 cm of the Belgrade Observatory, is communicated.
The equivalent width and central depth data of Mn 539.4 nm solar spectral line, observed in the period from 1979 to 1992 at Kitt Peak Observatory, was analyzed in pursuit for periodic changes. As th...

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