Extensive Lensing Survey of Optical and Near-Infrared Dark Objects (El Sonido): HST H-Faint Galaxies behind 101 Lensing Clusters
arXiv:2109.01751 · doi:10.3847/1538-4357/ac2578
Abstract
We present a Spitzer/IRAC survey of H-faint (, ) sources in 101 lensing cluster fields. Across a CANDELS/Wide-like survey area of 648 arcmin (effectively 221 arcmin in the source plane), we have securely discovered 53 sources in the IRAC Channel-2 band (CH2, 4.5 ; median CH2 AB mag) that lack robust HST/WFC3-IR F160W counterparts. The most remarkable source in our sample, namely ES-009 in the field of Abell 2813, is the brightest H-faint galaxy at 4.5 known so far ( AB mag). We show that the H-faint sources in our sample are massive (median ), star-forming (median star formation rate yr) and dust-obscured () galaxies around a median photometric redshift of . The stellar continua of 14 H-faint galaxies can be resolved in the CH2 band, suggesting a median circularized effective radius (; lensing corrected) of kpc and kpc for the resolved and whole samples, respectively. This is consistent with the sizes of massive unobscured galaxies at , indicating that H-faint galaxies represent the dusty tail of the distribution of a wider galaxy population. Comparing with the ALMA dust continuum sizes of similar galaxies reported previously, we conclude that the heavy dust obscuration in H-faint galaxies is related to the compactness of both stellar and dust continua ( kpc). These H-faint galaxies make up % of the galaxies in the stellar mass range of at , contributing to % of the cosmic star formation rate density in this epoch and likely tracing the early phase of massive galaxy formation.
arXiv comment26 pages, 10 figures, 3 tables. Accepted for publication in ApJ
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