New Light-Time Curve of Eclipsing Binary AM Leo

Light Curve Changes in the Eclipsing Binary V719 Her

The Spitzer 24μm Photometric Light Curve of the Eclipsing M-dwarf Binary GU Boötis

We present a carefully controlled set of Spitzer 24 μm MIPS time series observations of the low mass eclipsing binary star GU Boötis (GU Boo). Our data cover three secondary eclipses of the system: two consecutive events and an additional eclipse six weeks later. The study’s main purpose is the long wavelength characterization of GU Boo’s light curve, independent of limb darkening and less sens...

The Spitzer 24 μ m Photometric Light Curve of the Eclipsing M - dwarf Binary

We present a carefully controlled set of Spitzer 24 μm MIPS time series observations of the low mass eclipsing binary star GU Boötis (GU Boo). Our data cover three secondary eclipses of the system: two consecutive events and an additional eclipse six weeks later. The study’s main purpose is the long wavelength characterization of GU Boo’s light curve, independent of limb darkening and less sens...

Automated analysis of eclipsing binary lightcurves. I. EBAS — a new Eclipsing Binary Automated Solver with EBOP

We present a new algorithm— Eclipsing Binary Automated Solver (EBAS), to analyse lightcurves of eclipsing binaries. The algorithm is designed to analyse large numbers of lightcurves, and is therefore based on the relatively fast EBOP code. To facilitate the search for the best solution, EBAS uses two parameter transformations. Instead of the radii of the two stellar components, EBAS uses the su...

Eclipsing Binary Pulsars

The first eclipsing binary pulsar, PSR B1957+20, was discovered in 1987. Since then, 13 other eclipsing low-mass binary pulsars have been found; 12 of these are in globular clusters. In this paper we list the known eclipsing binary pulsars and their properties, with special attention to the eclipsing systems in 47 Tuc. We find that there are two fundamentally different groups of eclipsing binar...