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• W4387494664 startingPage "72" @default.
• W4387494664 abstract "Abstract A growing number of far-infrared (FIR) bright sources completely invisible in deep extragalactic optical surveys hint at an elusive population of z > 4 dusty, star-forming galaxies. Cycle 1 JWST surveys are now detecting their rest-frame optical light, which provides key insight into their stellar properties and statistical constraints on the population as a whole. This work presents the JWST Near Infrared Camera (NIRCam) counterpart from the COSMOS-Web survey to an FIR SCUBA-2 and Atacama Large Millimeter/submillimeter Array (ALMA) source, AzTECC71, which was previously undetected at wavelengths shorter than 850 μ m. AzTECC71, among the reddest galaxies in COSMOS-Web with F277W − F444W ∼ 0.9, is undetected in NIRCam/F150W and F115W and fainter in F444W than other submillimeter galaxies identified in COSMOS-Web by 2–4 magnitudes. This is consistent with the system having both a lower stellar mass and higher redshift than the median dusty, star-forming galaxy. With deep ground- and space-based upper limits combined with detections in F277W, F444W, and the FIR including ALMA Band 6, we find a high probability (99%) that AzTECC71 is at z > 4 with <?CDATA ${z}_{mathrm{phot}}={5.7}_{-0.7}^{+0.8}$?> <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML overflow=scroll> <mml:msub> <mml:mrow> <mml:mi>z</mml:mi> </mml:mrow> <mml:mrow> <mml:mi>phot</mml:mi> </mml:mrow> </mml:msub> <mml:mo>=</mml:mo> <mml:msubsup> <mml:mrow> <mml:mn>5.7</mml:mn> </mml:mrow> <mml:mrow> <mml:mo>−</mml:mo> <mml:mn>0.7</mml:mn> </mml:mrow> <mml:mrow> <mml:mo>+</mml:mo> <mml:mn>0.8</mml:mn> </mml:mrow> </mml:msubsup> </mml:math> . This galaxy is massive ( <?CDATA $mathrm{log},{M}_{* }/{M}_{odot }sim 10.7$?> <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML overflow=scroll> <mml:mi>log</mml:mi> <mml:mspace width=0.25em /> <mml:msub> <mml:mrow> <mml:mi>M</mml:mi> </mml:mrow> <mml:mrow> <mml:mo>*</mml:mo> </mml:mrow> </mml:msub> <mml:mrow> <mml:mo stretchy=true>/</mml:mo> </mml:mrow> <mml:msub> <mml:mrow> <mml:mi>M</mml:mi> </mml:mrow> <mml:mrow> <mml:mo>⊙</mml:mo> </mml:mrow> </mml:msub> <mml:mo>∼</mml:mo> <mml:mn>10.7</mml:mn> </mml:math> ) and infrared-luminous ( <?CDATA $mathrm{log},{L}_{mathrm{IR}}/{L}_{odot }sim 12.7$?> <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML overflow=scroll> <mml:mi>log</mml:mi> <mml:mspace width=0.25em /> <mml:msub> <mml:mrow> <mml:mi>L</mml:mi> </mml:mrow> <mml:mrow> <mml:mi>IR</mml:mi> </mml:mrow> </mml:msub> <mml:mrow> <mml:mo stretchy=true>/</mml:mo> </mml:mrow> <mml:msub> <mml:mrow> <mml:mi>L</mml:mi> </mml:mrow> <mml:mrow> <mml:mo>⊙</mml:mo> </mml:mrow> </mml:msub> <mml:mo>∼</mml:mo> <mml:mn>12.7</mml:mn> </mml:math> ), comparable to other optically undetected but FIR-bright dusty, star-forming galaxies at z > 4. This population of luminous, infrared galaxies at z > 4 is largely unconstrained but comprises an important bridge between the most extreme dust-obscured galaxies and more typical high-redshift star-forming galaxies. If further FIR-selected galaxies that drop out of the F150W filter in COSMOS-Web have redshifts z > 4 like AzTECC71, then the volume density of such sources may be ∼3–10 × greater than previously estimated." @default.
• W4387494664 created "2023-10-11" @default.
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• W4387494664 date "2023-10-01" @default.
• W4387494664 modified "2023-10-12" @default.
• W4387494664 title "A Near-infrared-faint, Far-infrared-luminous Dusty Galaxy at z ∼ 5 in COSMOS-Web" @default.
• W4387494664 cites W1634409775 @default.
• W4387494664 cites W1681063222 @default.
• W4387494664 cites W1748091613 @default.
• W4387494664 cites W1851451509 @default.
• W4387494664 cites W1912798299 @default.
• W4387494664 cites W1973986763 @default.
• W4387494664 cites W1987470578 @default.
• W4387494664 cites W1993202096 @default.
• W4387494664 cites W1996990154 @default.
• W4387494664 cites W2006676156 @default.
• W4387494664 cites W2019615555 @default.
• W4387494664 cites W2019866699 @default.
• W4387494664 cites W2025105301 @default.
• W4387494664 cites W2030954280 @default.
• W4387494664 cites W2034608771 @default.
• W4387494664 cites W2051510431 @default.
• W4387494664 cites W2052262351 @default.
• W4387494664 cites W2060753691 @default.
• W4387494664 cites W2079304679 @default.
• W4387494664 cites W2093697839 @default.
• W4387494664 cites W2095044009 @default.
• W4387494664 cites W2099344750 @default.
• W4387494664 cites W2100336040 @default.
• W4387494664 cites W2110830624 @default.
• W4387494664 cites W2123628940 @default.
• W4387494664 cites W2132759038 @default.
• W4387494664 cites W2144632906 @default.
• W4387494664 cites W2146573890 @default.
• W4387494664 cites W2158528198 @default.
• W4387494664 cites W2162596494 @default.
• W4387494664 cites W2198891478 @default.
• W4387494664 cites W2491291961 @default.
• W4387494664 cites W2526143871 @default.
• W4387494664 cites W2530734350 @default.
• W4387494664 cites W2530964153 @default.
• W4387494664 cites W2531087724 @default.
• W4387494664 cites W2581974067 @default.
• W4387494664 cites W2596029414 @default.
• W4387494664 cites W2613683462 @default.
• W4387494664 cites W2615022007 @default.
• W4387494664 cites W2620847899 @default.
• W4387494664 cites W2785179448 @default.
• W4387494664 cites W2785840027 @default.
• W4387494664 cites W2814038463 @default.
• W4387494664 cites W2899552690 @default.
• W4387494664 cites W2918016348 @default.
• W4387494664 cites W2949614108 @default.
• W4387494664 cites W2949874561 @default.
• W4387494664 cites W2963186413 @default.
• W4387494664 cites W2964363227 @default.
• W4387494664 cites W2973849959 @default.
• W4387494664 cites W2974547947 @default.
• W4387494664 cites W3014142888 @default.
• W4387494664 cites W3014882801 @default.
• W4387494664 cites W3025083636 @default.
• W4387494664 cites W3036357039 @default.
• W4387494664 cites W3081840799 @default.
• W4387494664 cites W3092289729 @default.

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