PHOEBE: PHysics Of Eclipsing BinariEs

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PHOEBE: PHysics Of Eclipsing BinariEs

Post by owlice » Fri Jun 10, 2011 11:24 am

[c]PHOEBE: PHysics Of Eclipsing BinariEs[/c][/b]
Abstract: 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 paper overviews most important scientific extensions (incorporating observational spectra of eclipsing binaries into the solution-seeking process, extracting individual temperatures from observed color indices, main-sequence constraining and proper treatment of the reddening), numerical innovations (suggested improvements to WD's Differential Corrections method, the new Nelder & Mead's downhill Simplex method) and technical aspects (back-end scripter structure, graphical user interface). While PHOEBE retains 100% WD compatibility, its add-ons are a powerful way to enhance WD by encompassing even more physics and solution reliability.

Credit: Prsa, Andrej; Matijevic, Gal; Latkovic, Olivera; Vilardell, Francesc; Wils, Patrick

Site: http://phoebe-project.org/
http://adsabs.harvard.edu/abs/2005ApJ...628..426P

Bibcode: 2011ascl.soft06002P

ID: ascl:1106.002
Last edited by Ada Coda on Sun May 27, 2018 6:33 pm, edited 1 time in total.
Reason: Updated code entry.
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