The Nature of Extremely Red H-[4.5]>4 Galaxies revealed with SEDS and CANDELS
Karina I. Caputi, James S. Dunlop, Ross J. McLure, Jiasheng Huang,, Giovanni G. Fazio, Matthew L. N. Ashby, Marco Castellano, Adriano Fontana,, Michele Cirasuolo, Omar Almaini, Eric F. Bell, Mark Dickinson, Jennifer L., Donley, Sandra M. Faber, Henry C. Ferguson

TL;DR
This study analyzes 25 extremely red mid-infrared galaxies to understand their nature, revealing a diverse population mainly consisting of dust-obscured, high-redshift galaxies, some hosting active galactic nuclei, and discussing implications for future JWST discoveries.
Contribution
It provides a detailed characterization of extremely red H-[4.5]>4 galaxies using multi-band photometry, identifying their diverse nature and potential as high-redshift galaxy candidates.
Findings
Majority are dust-obscured, massive galaxies at 3<zphot<5
Some sources likely host dust-obscured AGN
Includes potential z~6 galaxy candidates
Abstract
We have analysed a sample of 25 extremely red H-[4.5]>4 galaxies, selected using 4.5 micron data from the Spitzer SEDS survey and deep H-band data from the Hubble Space Telescope (HST) CANDELS survey, over ~180 square arcmin of the UKIDSS Ultra Deep Survey (UDS) field. Our aim is to investigate the nature of this rare population of mid-infrared (mid-IR) sources that display such extreme near-to-mid-IR colours. Using up to 17-band photometry (U through 8.0 microns), we have studied in detail their spectral energy distributions, including possible degeneracies in the photometric redshift/internal extinction (zphot-Av) plane. Our sample appears to include sources of very different nature. Between 45% and 75% of them are dust-obscured, massive galaxies at 3<zphot<5. All of the 24 micron-detected sources in our sample are in this category. Two of these have S(24 micron)>300 microJy, which at…
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