Only a small fraction of the SDSS objects were detected in the last two surveys. Among the results is a list of twenty galaxies with the highest magnitudes which have hot dust of several hundred degrees. Of these twenty, all could be classified as GPs and/or LCGs. Also among the results, the luminosity is obtained in the sample galaxies in a wide wavelength range. At the highest luminosities, the sample galaxies had luminosites approaching those of high-redshift Lyman-break galaxy. In January 2014, authors A. Jaskot, M. Oey, J. Salzer, A. Van Sistine and M. Haynes gave a presentation titled "Neutral Gas and Low-Redshift Starbursts: From Infall to Ionization" to the American Astronomical Society at their meeting #223. The presentation included data from The Arecibo Observatory Legacy Fast ALFA Survey (ALFALFA). The authors analyzed the optical spectra of the GPs and concluded "While the ALFALFA survey demonstrates the role of external processes in triggering starbursts, the Green Peas show that starbursts' radiation can escape to affect their external environment", finding "that the Peas are likely optically thin to Lyman continuum (LyC) radiation." In June 2014, authors A. Jaskot and M. Oey published a conference report titled "The Origin and Optical Depth of Ionizing Photons in the Green Pea Galaxies". This appears in "Massive Young Star Clusters Near and Far: From the Milky Way to Reionization", based on the 2013 Guillermo Haro Conference. More details here:Two papers by Jaskot and Oey  In May 2015, authors A. Henry, C. Scarlata, C. L. Martin and D. Erb published a paper in the Astrophysical Journal entitled, "Lyα Emission from Green Peas: The Role of Circumgalactic Gas Density, Covering, and Kinematics". In this paper, ten Green Peas were studied in the ultraviolet, using high resolution spectroscopy with the Hubble Space Telescope using the Cosmic Origins Spectrograph. This study showed, for the first time, that Green Peas have strong Lyα emission much like distant, high-redshift galaxies observed in a younger universe. Henry et al. explored the physical mechanisms that determine how Lyα escapes from the Green Peas, and concluded that variations in the neutral hydrogen column density were the most important factor.