Properties of the KISS Green Pea Galaxies
Samantha W. Brunker, John J. Salzer, Steven Janowiecki, Rose A. Finn,, George Helou

TL;DR
This paper compares properties of Green Pea galaxies identified via color and emission lines, revealing they are a rare, extreme, and likely young starburst population at intermediate redshifts, similar to high-redshift Lyα emitters.
Contribution
It demonstrates that emission-line selected galaxies from KISS overlap with color-selected Green Peas, establishing their commonality and extreme nature at intermediate redshifts.
Findings
Green Peas are extreme, young starburst systems.
They are very rare at z=0.29-0.41.
No similar extreme galaxies are found locally.
Abstract
Green Peas are a class of extreme star-forming galaxies at intermediate redshifts, originally discovered via color-selection using multi-filter, wide-field survey imaging data (Cardamone et al. 2009). They are commonly thought of as being analogs of high-redshift Ly-emitting galaxies. The defining characteristic of Green Pea galaxies is a high-excitation nebular spectrum with very large equivalent width lines, leading to the recognition that Green Pea-like galaxies can also be identified in samples of emission-line galaxies. Here we compare the properties a sample of [O III]-selected star-forming galaxies (z = 0.29-0.41) from the KPNO International Spectroscopic Survey (KISS) with the color-selected Green Peas. We find that the KISS [O III]-selected galaxies overlap with the parameter space defined by the color-selected Green Peas; the two samples appear to be drawn from the…
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