UNCOVER: Illuminating the Early Universe -- JWST/NIRSpec Confirmation of $z > 12$ Galaxies

Fuente: arXiv
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Autori principali: Wang, Bingjie, Fujimoto, Seiji, Labbe, Ivo, Furtak, Lukas J., Miller, Tim B., Setton, David J., Zitrin, Adi, Atek, Hakim, Bezanson, Rachel, Brammer, Gabriel, Leja, Joel, Oesch, Pascal A., Price, Sedona H., Chemerynska, Iryna, Cutler, Sam E., Dayal, Pratika, van Dokkum, Pieter, Goulding, Andy D., Greene, Jenny E., Fudamoto, Y., Khullar, Gourav, Kokorev, Vasily, Marchesini, Danilo, Pan, Richard, Weaver, John R., Whitaker, Katherine E., Williams, Christina C.
Natura: Preprint
Pubblicazione: 2023
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author Wang, Bingjie
Fujimoto, Seiji
Labbe, Ivo
Furtak, Lukas J.
Miller, Tim B.
Setton, David J.
Zitrin, Adi
Atek, Hakim
Bezanson, Rachel
Brammer, Gabriel
Leja, Joel
Oesch, Pascal A.
Price, Sedona H.
Chemerynska, Iryna
Cutler, Sam E.
Dayal, Pratika
van Dokkum, Pieter
Goulding, Andy D.
Greene, Jenny E.
Fudamoto, Y.
Khullar, Gourav
Kokorev, Vasily
Marchesini, Danilo
Pan, Richard
Weaver, John R.
Whitaker, Katherine E.
Williams, Christina C.
author_facet Wang, Bingjie
Fujimoto, Seiji
Labbe, Ivo
Furtak, Lukas J.
Miller, Tim B.
Setton, David J.
Zitrin, Adi
Atek, Hakim
Bezanson, Rachel
Brammer, Gabriel
Leja, Joel
Oesch, Pascal A.
Price, Sedona H.
Chemerynska, Iryna
Cutler, Sam E.
Dayal, Pratika
van Dokkum, Pieter
Goulding, Andy D.
Greene, Jenny E.
Fudamoto, Y.
Khullar, Gourav
Kokorev, Vasily
Marchesini, Danilo
Pan, Richard
Weaver, John R.
Whitaker, Katherine E.
Williams, Christina C.
contents Observations of high-redshift galaxies provide a critical direct test to the theories of early galaxy formation, yet to date, only three have been spectroscopically confirmed at $z>12$. Due to strong gravitational lensing over a wide area, the galaxy cluster field A2744 is ideal for searching for the earliest galaxies. Here we present JWST/NIRSpec observations of two galaxies: a robust detection at $z_{\rm spec} = 12.393^{+0.004}_{-0.001}$, and a plausible candidate at $z_{\rm spec} = 13.079^{+0.013}_{-0.001}$. The galaxies are discovered in JWST/NIRCam imaging and their distances are inferred with JWST/NIRSpec spectroscopy, all from the JWST Cycle 1 UNCOVER Treasury survey. Detailed stellar population modeling using JWST NIRCam and NIRSpec data corroborates the primeval characteristics of these galaxies: low mass ($\sim 10^8~{\rm M_\odot}$), young, rapidly-assembling, metal-poor, and star-forming. Interestingly, both galaxies are spatially resolved, having lensing-corrected rest-UV effective radii on the order of 300-400 pc, which are notably larger than other spectroscopically confirmed systems at similar redshifts. The observed dynamic range of $z \gtrsim 10$ sizes spans over 1 order of magnitude, implying a significant scatter in the size-mass relation at early times. Deep into the epoch of reionization, these discoveries elucidate the emergence of the first galaxies.
format Preprint
id arxiv_https___arxiv_org_abs_2308_03745
institution arXiv
publishDate 2023
record_format arxiv
spellingShingle UNCOVER: Illuminating the Early Universe -- JWST/NIRSpec Confirmation of $z > 12$ Galaxies
Wang, Bingjie
Fujimoto, Seiji
Labbe, Ivo
Furtak, Lukas J.
Miller, Tim B.
Setton, David J.
Zitrin, Adi
Atek, Hakim
Bezanson, Rachel
Brammer, Gabriel
Leja, Joel
Oesch, Pascal A.
Price, Sedona H.
Chemerynska, Iryna
Cutler, Sam E.
Dayal, Pratika
van Dokkum, Pieter
Goulding, Andy D.
Greene, Jenny E.
Fudamoto, Y.
Khullar, Gourav
Kokorev, Vasily
Marchesini, Danilo
Pan, Richard
Weaver, John R.
Whitaker, Katherine E.
Williams, Christina C.
Astrophysics of Galaxies
Observations of high-redshift galaxies provide a critical direct test to the theories of early galaxy formation, yet to date, only three have been spectroscopically confirmed at $z>12$. Due to strong gravitational lensing over a wide area, the galaxy cluster field A2744 is ideal for searching for the earliest galaxies. Here we present JWST/NIRSpec observations of two galaxies: a robust detection at $z_{\rm spec} = 12.393^{+0.004}_{-0.001}$, and a plausible candidate at $z_{\rm spec} = 13.079^{+0.013}_{-0.001}$. The galaxies are discovered in JWST/NIRCam imaging and their distances are inferred with JWST/NIRSpec spectroscopy, all from the JWST Cycle 1 UNCOVER Treasury survey. Detailed stellar population modeling using JWST NIRCam and NIRSpec data corroborates the primeval characteristics of these galaxies: low mass ($\sim 10^8~{\rm M_\odot}$), young, rapidly-assembling, metal-poor, and star-forming. Interestingly, both galaxies are spatially resolved, having lensing-corrected rest-UV effective radii on the order of 300-400 pc, which are notably larger than other spectroscopically confirmed systems at similar redshifts. The observed dynamic range of $z \gtrsim 10$ sizes spans over 1 order of magnitude, implying a significant scatter in the size-mass relation at early times. Deep into the epoch of reionization, these discoveries elucidate the emergence of the first galaxies.
title UNCOVER: Illuminating the Early Universe -- JWST/NIRSpec Confirmation of $z > 12$ Galaxies
topic Astrophysics of Galaxies
url https://arxiv.org/abs/2308.03745