From time to time, the project will observe eclipsing binary stars.

The primary component is an eclipsing binary star in a triple-star grouping.

It is used to monitor eclipsing binary stars and Mira variable stars.

Zeta Tauri is an eclipsing binary star that completes an orbit every 133 days.

The star system is the prototype of a whole group of eclipsing binary stars named Algol variables.

During this period, a nearby eclipsing binary star called N1 was considered and avoided to avoid contaminating the collected light samples.

To test his speculations, he needed data on the masses of stars, potentially available from eclipsing binary stars.

TY Pyxidis is an eclipsing binary star of combined visual magnitude 6.9.

In his early astronomical career, he studied variable stars and in particular close eclipsing binary stars.

KOI-81 is an eclipsing binary star in the constellation of Cygnus.

For eclipsing binary stars - Eclipse mapping produces images and maps of spots on both stars.

Such a background "eclipsing binary star" would dim once per orbit, mimicking the dimming signature of a planet.

At the Jagiellonian University Observatory he made systematic observations of eclipsing binary stars.

Like Epsilon Aurigae, it is an eclipsing binary star that varies in magnitude by 0.1.

The star Lambda (λ) Tauri is an eclipsing binary star.

In discovering a large number of Cepheid variables and eclipsing binary stars, it will help determine distances to nearby galaxies with greater precision.

In 2006, a group of astronomers announced the discovery of an eclipsing binary star in the Triangulum Galaxy.

Delta Cassiopeiae is an eclipsing binary star system consisting of a pair of stars that orbit about each other over a period of 759 days.

Myers conducted the first theoretical study of the eclipsing binary star Beta Lyrae as part of his dissertation.

Another way the FOP weeds out eclipsing binary star is by taking a "reconnaissance" spectrum of the star.

Russell gave a lecture titled "The Royal Road of Eclipses" concerning eclipsing binary stars.

The first eclipsing binary star system to be discovered was Algol, a star system in the constellation Perseus.

Goodricke reported the first precise measurement of the period of variation of the star Algol, which is now known to be an eclipsing binary star.

NASA's Kepler mission has discovered examples of eclipsing binary stars where the secondary is the hotter component.

The aims of Project Solaris is to detect circumbinary planets around eclipsing binary stars and to characterise these binaries to improve stellar models.