Extensive Lensing Survey of Optical and Near-infrared Dark Objects (El Sonido): HST H-faint Galaxies behind 101 Lensing Clusters

We present a Spitzer/IRAC survey of H-faint (H-160 greater than or similar to 26.4, < 5 sigma) sources in 101 lensing cluster fields. Across a CANDELS/Wide-like survey area of similar to 648 arcmin(2) (effectively similar to 221 arcmin(2) in the source plane), we have securely discovered 53 sourc...

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Veröffentlicht in:The Astrophysical journal 2021-12, Vol.922 (2), p.114, Article 114
Hauptverfasser: Sun, Fengwu, Egami, Eiichi, Pérez-González, Pablo G., Smail, Ian, Caputi, Karina I., Bauer, Franz E., Rawle, Timothy D., Fujimoto, Seiji, Kohno, Kotaro, Dudzevičiūtė, Ugnė, Atek, Hakim, Bianconi, Matteo, Chapman, Scott C., Combes, Francoise, Jauzac, Mathilde, Jolly, Jean-Baptiste, Koekemoer, Anton M., Magdis, Georgios E., Rodighiero, Giulia, Rujopakarn, Wiphu, Schaerer, Daniel, Steinhardt, Charles L., Van der Werf, Paul, Walth, Gregory L., Weaver, John R.
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Sprache:eng
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Zusammenfassung:We present a Spitzer/IRAC survey of H-faint (H-160 greater than or similar to 26.4, < 5 sigma) sources in 101 lensing cluster fields. Across a CANDELS/Wide-like survey area of similar to 648 arcmin(2) (effectively similar to 221 arcmin(2) in the source plane), we have securely discovered 53 sources in the IRAC Channel-2 band (CH2, 4.5 mu m; median CH2 = 22.46 +/- 0.11 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 mu m known so far (CH2 = 20.48 +/- 0.03 AB mag). We show that the H-faint sources in our sample are massive (median M-star = 10 10.3 +/- 0.3 M-circle dot, star-forming (median star formation rate =1001 M-circle dot yr(-1)), and dust-obscured (A(v) = 2.6 +/- 0.3) galaxies around a median photometric redshift of z = 3.9 +/- 0.4. The stellar continua of 14 H-faint galaxies can be resolved in the CH2 band, suggesting a median circularized effective radius (R-e,R-circ; lensing corrected) of 1.9 +/- 0.2 kpc and
ISSN:0004-637X
1538-4357
1538-4357
DOI:10.3847/1538-4357/ac2578