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Illuminating the Dark Side of Cosmic Star Formation. III. Building the Largest Homogeneous Sample of Radio-selected Dusty Star-forming Galaxies in COSMOS with PhoEBO
The Astrophysical Journal, 962 (2024); 26. https://doi.org/10.3847/1538-4357/ad1519
Gentile, Fabrizio; Talia, Margherita; Behiri, Meriem; Zamorani, Giovanni; Barchiesi, Luigi; Vignali, Cristian; Pozzi, Francesca; Bethermin, Matthieu; Enia, Andrea; Faisst, Andreas L.; Giulietti, Marika; Gruppioni, Carlotta; Lapi, Andrea; Massardi, Marcella; Smolčić, Vernesa; Vaccari, Mattia; Cimatti, Andrea Više autora...

Institucijski repozitorij: Repozitorij Prirodoslovno-matematičkog fakulteta

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Gentile, F., Talia, M., Behiri, M., Zamorani, G., Barchiesi, L., Vignali, C. ... Cimatti, A. (2024). Illuminating the Dark Side of Cosmic Star Formation. III. Building the Largest Homogeneous Sample of Radio-selected Dusty Star-forming Galaxies in COSMOS with PhoEBO. The Astrophysical Journal, 962.. doi: 10.3847/1538-4357/ad1519

Gentile, Fabrizio, et al. "Illuminating the Dark Side of Cosmic Star Formation. III. Building the Largest Homogeneous Sample of Radio-selected Dusty Star-forming Galaxies in COSMOS with PhoEBO." The Astrophysical Journal, vol. 962, 2024. https://doi.org/10.3847/1538-4357/ad1519

Gentile, Fabrizio, Margherita Talia, Meriem Behiri, Giovanni Zamorani, Luigi Barchiesi, Cristian Vignali, Francesca Pozzi, et al. "Illuminating the Dark Side of Cosmic Star Formation. III. Building the Largest Homogeneous Sample of Radio-selected Dusty Star-forming Galaxies in COSMOS with PhoEBO." The Astrophysical Journal 962 (2024). https://doi.org/10.3847/1538-4357/ad1519

Gentile, F., et al. (2024) 'Illuminating the Dark Side of Cosmic Star Formation. III. Building the Largest Homogeneous Sample of Radio-selected Dusty Star-forming Galaxies in COSMOS with PhoEBO', The Astrophysical Journal, 962. doi: 10.3847/1538-4357/ad1519

Gentile F, Talia M, Behiri M, Zamorani G, Barchiesi L, Vignali C, i sur.. Illuminating the Dark Side of Cosmic Star Formation. III. Building the Largest Homogeneous Sample of Radio-selected Dusty Star-forming Galaxies in COSMOS with PhoEBO. The Astrophysical Journal [Internet]. 02.02.2024. [pristupljeno 25.11.2024.];962. doi: 10.3847/1538-4357/ad1519

F. Gentile, et al., "Illuminating the Dark Side of Cosmic Star Formation. III. Building the Largest Homogeneous Sample of Radio-selected Dusty Star-forming Galaxies in COSMOS with PhoEBO", The Astrophysical Journal, vol. 962, Veljača 2024. [Online]. Dostupno na: https://urn.nsk.hr/urn:nbn:hr:217:425331. [Citirano: 25.11.2024.]

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Naslov (engleski)Illuminating the Dark Side of Cosmic Star Formation. III. Building the Largest Homogeneous Sample of Radio-selected Dusty Star-forming Galaxies in COSMOS with PhoEBO
AutorFabrizio Gentile
AutorMargherita Talia
AutorMeriem Behiri
AutorGiovanni Zamorani
AutorLuigi Barchiesi
AutorCristian Vignali
AutorFrancesca Pozzi
AutorMatthieu Bethermin
AutorAndrea Enia
AutorAndreas L. Faisst
AutorMarika Giulietti
AutorCarlotta Gruppioni
AutorAndrea Lapi
AutorMarcella Massardi
AutorVernesa Smolčić
AutorMattia Vaccari
AutorAndrea Cimatti
Autorova ustanovaSveučilište u Zagrebu
Prirodoslovno-matematički fakultet
(Fizički odsjek)
Znanstveno / umjetničko
područje, polje i grana		PRIRODNE ZNANOSTI
Fizika
Sažetak (engleski)
In the last decades, an increasing scientific interest has been growing in the elusive population of dark (i.e., lacking an optical/near-IR, hereafter NIR, counterpart) dusty star-forming galaxies (DSFGs). Although extremely promising for their likely contribution to the cosmic star formation rate density (SFRD) and for their possible role in the evolution of the first massive and passive galaxies around z ∼ 3, the difficulty in selecting statistically significant samples of dark DSFGs is limiting their scientific potentialities. This work presents the first panchromatic study of a sample of 263 radio-selected NIR-dark (RS-NIRdark) galaxies discovered in the COSMOS field following the procedure by Talia et al. These sources are selected as radio-bright galaxies (S 3 GHz > 12.65 μJy) with no counterpart in the NIR-selected COSMOS2020 catalog (Ks ≳ 25.5 mag). For these sources, we build a new photometric catalog including accurate photometry from the optical to the radio obtained with a new deblending pipeline (Photometry Extractor for Blended Objects, or PHOEBO). We employ this catalog to estimate the photo-zs and the physical properties of the galaxies through an spectral energy distribution-fitting procedure performed with two different codes (MAGPHYS and CIGALE). Finally, we estimate the active galactic nucleus contamination in our sample by performing a series of complementary tests. The high values of the median extinction (A v ∼ 4) and star formation rate (SFR ∼ 500 M ⊙ yr‑1) confirm the likely DSFG nature of the RS-NIRdark galaxies. The median photo-z (z ∼ 3) and the presence of a significant tail of high-z candidates (z > 4.5) suggest that these sources are important contributors to the cosmic SFRD and the evolutionary path of galaxies at high redshifts.
Ključne riječi (engleski)
Jezikengleski
Vrsta publikacijeZnanstveni rad - Izvorni znanstveni rad
Status objaveObjavljen
Vrsta recenzijeRecenziran - međunarodna recenzija
Verzija publikacijeObjavljena verzija rada (izdavačev PDF)
Naslov časopisaThe Astrophysical Journal
Brojčani podacivol. 962, 26
p-ISSN0004-637X
e-ISSN1538-4357
DOIhttps://doi.org/10.3847/1538-4357/ad1519
URN:NBNurn:nbn:hr:217:425331
Datum objave publikacije2024-02-02
URL dokumentahttps://iopscience.iop.org/article/10.3847/1538-4357/ad1519
Vrsta resursaTekst
Prava pristupaOtvoreni pristup
Uvjeti korištenjaIkona licence Imenovanje 4.0 međunarodna (CC BY 4.0)
Javna napomena© 2024. The Author(s). Published by the American Astronomical Society. Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.. Received 2023 March 27; revised 2023 December 4; accepted 2023 December 7; published 2024 February 2.
Datum i vrijeme pohrane2024-06-10 12:37:50