A.E. Jaskot; M.S. Oey (2014). "The Origin and Optical Depth of Ionizing Photons in the Green Pea Galaxies". Massive Young Star Clusters Near and Far: From the Milky Way to Reionization: 171. arXiv:1402.4429. Bibcode:2014mysc.conf..171J. ISBN978-607-8379-01-9.
J.C. Lee; J.J. Salzer; J. Melbourne (December 2004). "Metal Abundances of KISS Galaxies. III. Nebular Abundances for Fourteen Galaxies and the Luminosity-Metallicity Relationship for H II Galaxies". The Astrophysical Journal. 616 (2): 752–767. arXiv:astro-ph/0408342. Bibcode:2004ApJ...616..752L. doi:10.1086/425156. S2CID16689645.
J.C. Lee; J.J. Salzer; J. Melbourne (December 2004). "Metal Abundances of KISS Galaxies. III. Nebular Abundances for Fourteen Galaxies and the Luminosity-Metallicity Relationship for H II Galaxies". The Astrophysical Journal. 616 (2): 752–767. arXiv:astro-ph/0408342. Bibcode:2004ApJ...616..752L. doi:10.1086/425156. S2CID16689645.
A. Jaskot; M. Oey; J. Salzer; A. Van Sistine; et al. (January 2014). "Neutral Gas and Low-Redshift Starbursts: From Infall to Ionization". American Astronomical Society Meeting Abstracts #223. AAS Meeting #223: 328.03. Bibcode:2014AAS...22332803J.
A.E. Jaskot; M.S. Oey (2014). "The Origin and Optical Depth of Ionizing Photons in the Green Pea Galaxies". Massive Young Star Clusters Near and Far: From the Milky Way to Reionization: 171. arXiv:1402.4429. Bibcode:2014mysc.conf..171J. ISBN978-607-8379-01-9.
J.C. Lee; J.J. Salzer; J. Melbourne (December 2004). "Metal Abundances of KISS Galaxies. III. Nebular Abundances for Fourteen Galaxies and the Luminosity-Metallicity Relationship for H II Galaxies". The Astrophysical Journal. 616 (2): 752–767. arXiv:astro-ph/0408342. Bibcode:2004ApJ...616..752L. doi:10.1086/425156. S2CID16689645.
J.C. Lee; J.J. Salzer; J. Melbourne (December 2004). "Metal Abundances of KISS Galaxies. III. Nebular Abundances for Fourteen Galaxies and the Luminosity-Metallicity Relationship for H II Galaxies". The Astrophysical Journal. 616 (2): 752–767. arXiv:astro-ph/0408342. Bibcode:2004ApJ...616..752L. doi:10.1086/425156. S2CID16689645.