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arXiv · 2502.00743

Green peas in the southern sky: Broad-band color selection and spectroscopic follow up

Yejin Jeong·Hyunjin Shim·Eunchong Kim·Jeong Hwan Lee
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Abstract

We present a systematic search for 1696 Green Pea (GP) galaxy candidates in the southern hemisphere selected from the Dark Energy Survey Data Release 2 (DES DR2) and provide preliminary results from spectroscopic follow-up observations of 26 targets chosen among them. Our selection criteria include the colors in $gri$-bands and compact morphology in the color composite images. The multi-wavelength spectral energy distribution fitting shows that the selected GP candidates exhibit star formation rates up to several tens $\mathrm{M}_\odot\,\mathrm{yr}^{-1}$. With the mean stellar mass of $\mathrm{log}\,M_*/\mathrm{M}_\odot=8.6$, GP candidates are located at roughly 1 dex above the main sequence of star-forming galaxies at $z\sim0.3$. Spectroscopic follow-up observations of the GP candidates with Gemini/GMOS are underway. All 26 targets are spectroscopically confirmed to be at $z=0.3-0.41$ and have [OIII] equivalent width larger than 85$\r{A}$, classified to be starbursts with low to moderate dust attenuation. These confirmed GPs show a lower metallicity offset from the mass-metallicity relation of local star-forming galaxies, indicating that GPs are less chemically evolved systems at their early stage of evolution.

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Yejin Jeong, Hyunjin Shim, Eunchong Kim, Jeong Hwan Lee. 2025-02-02. Green peas in the southern sky: Broad-band color selection and spectroscopic follow up. https://arxiv.org/abs/2502.00743

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