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20012026
most citedGaia Data Release 2. Summary of the contents and survey properties

8.6k citations · 21.2k across the 86 of their papers we have counts for

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astro-ph2008★ 97 cited

Artificial Intelligence Approach to the Determination of Physical Properties of Eclipsing Binaries. I. The EBAI Project

A. Prsa, E. F. Guinan, E. J. Devinney +5

Achieving maximum scientific results from the overwhelming volume of astronomical data to be acquired over the next few decades will demand novel, fully automatic methods of data a…

astro-ph2007

Pipeline Reduction of Binary Light Curves from Large-Scale Surveys

Andrej Prsa, Tomaz Zwitter

One of the most important changes in observational astronomy of the 21st Century is a rapid shift from classical object-by-object observations to extensive automatic surveys. As CC…

astro-ph2006

Introducing Powell's Direction Set Method to a Fully Automated Analysis of Eclipsing Binary Stars

A. Prsa, T. Zwitter

With recent observational advancements, substantial amounts of photometric and spectroscopic eclipsing binary data have been acquired. As part of an ongoing effort to assemble a re…

astro-ph2006★ 14 cited

Disentangling effective temperatures of individual eclipsing binary components by means of color-index constraining

A. Prsa, T. Zwitter

Eclipsing binary stars are gratifying objects because of their unique geometrical properties upon which all important physical parameters such as masses, radii, temperatures, lumin…

astro-ph2005★ 898 cited

A Computational Guide to Physics of Eclipsing Binaries. Paper I. Demonstrations and Perspectives

A. Prsa, T. Zwitter

PHOEBE (PHysics Of Eclipsing BinariEs) is a modeling package for eclipsing binary stars, built on top of the widely used WD program (Wilson & Devinney 1971). This introductory pape…

astro-ph2004★ 4 cited

Introducing adapted Nelder & Mead's downhill simplex method to a fully automated analysis of eclipsing binaries

A. Prsa, T. Zwitter

Eclipsing binaries are extremely attractive objects because absolute physical parameters (masses, luminosities, radii) of both components may be determined from observations. Since…