[1] The first study showing the possible escape of Lyman continuum photons was published in 2006, using data from the Far Ultraviolet Spectroscopic Explorer (FUSE).

[8] A team of astronomers at Stockholm University, Sweden, and the Geneva Observatory, Switzerland, identified 200 separate clusters of very young, massive stars, many of which are less than 10 million years old.

[12] In November 2015, a study was published in the journal Astronomy and Astrophysics by Göran Östlin et al. which examined the kinematics of H11 using observations collected at the European Southern Observatory, Paranal, Chile.

The abstract states: "In this work, we investigate the kinematics of stars and ionised gas in Haro 11, one of the most luminous blue compact galaxies in the local Universe.

"[13] In September 2003, as a result of Program 9470, Daniel Kunth and team published the first images of Haro 11 using the then newly installed ACS on the HST (specifically the Solar Blind Channel) in a study titled: "The First Deep Advanced Camera for Surveys Lyalpha Images of Local Starburst Galaxies".