UNCOVER: Significant Reddening in Cosmic Noon Quiescent Galaxies
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| Format: | Preprint |
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2024
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| author | Siegel, Jared Setton, David Greene, Jenny Suess, Katherine Whitaker, Katherine Bezanson, Rachel Leja, Joel Furtak, Lukas Cutler, Sam de Graaff, Anna Feldmann, Robert Khullar, Gourav Labbé, Ivo Marchesini, Danilo Miller, Tim Nanayakkara, Themiya Pan, Richard Price, Sedona Treiber, Helena van Dokkum, Pieter Wang, Bingjie Weaver, John |
| author_facet | Siegel, Jared Setton, David Greene, Jenny Suess, Katherine Whitaker, Katherine Bezanson, Rachel Leja, Joel Furtak, Lukas Cutler, Sam de Graaff, Anna Feldmann, Robert Khullar, Gourav Labbé, Ivo Marchesini, Danilo Miller, Tim Nanayakkara, Themiya Pan, Richard Price, Sedona Treiber, Helena van Dokkum, Pieter Wang, Bingjie Weaver, John |
| contents | We explore the physical properties of five massive quiescent galaxies at $z\sim2.5$, revealing the presence of non-negligible dust reservoirs. JWST NIRSpec observations were obtained for each target, finding no significant line emission; multiple star formation tracers independently place upper limits between $0.1-10~M_\odot / \mathrm{yr}$. Spectral energy distribution modeling with Prospector infers stellar masses between $\log_{10}[M / M_\odot] \sim 10-11$ and stellar mass-weighted ages between $1-2$ Gyr. The inferred mass-weighted effective radii ($r_{eff}\sim 0.4-1.4$ kpc) and inner $1$ kpc stellar surface densities ($\log_{10}[Σ/ M_\odot \mathrm{kpc}^2 ]\gtrsim 9$) are typical of quiescent galaxies at $z \gtrsim 2$. The galaxies display negative color gradients (redder core and bluer outskirts); for one galaxy, this effect results from a dusty core, while for the others it may be evidence of an "inside-out" growth process. Unlike local quiescent galaxies, we identify significant reddening in these typical cosmic noon passive galaxies; all but one require $A_V \gtrsim 0.4$. This finding is in qualitative agreement with previous studies but our deep 20-band NIRCam imaging is able to significantly suppress the dust-age degeneracy and confidently determine that these galaxies are reddened. We speculate about the physical effects that may drive the decline in dust content in quiescent galaxies over cosmic time. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2409_11457 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | UNCOVER: Significant Reddening in Cosmic Noon Quiescent Galaxies Siegel, Jared Setton, David Greene, Jenny Suess, Katherine Whitaker, Katherine Bezanson, Rachel Leja, Joel Furtak, Lukas Cutler, Sam de Graaff, Anna Feldmann, Robert Khullar, Gourav Labbé, Ivo Marchesini, Danilo Miller, Tim Nanayakkara, Themiya Pan, Richard Price, Sedona Treiber, Helena van Dokkum, Pieter Wang, Bingjie Weaver, John Astrophysics of Galaxies We explore the physical properties of five massive quiescent galaxies at $z\sim2.5$, revealing the presence of non-negligible dust reservoirs. JWST NIRSpec observations were obtained for each target, finding no significant line emission; multiple star formation tracers independently place upper limits between $0.1-10~M_\odot / \mathrm{yr}$. Spectral energy distribution modeling with Prospector infers stellar masses between $\log_{10}[M / M_\odot] \sim 10-11$ and stellar mass-weighted ages between $1-2$ Gyr. The inferred mass-weighted effective radii ($r_{eff}\sim 0.4-1.4$ kpc) and inner $1$ kpc stellar surface densities ($\log_{10}[Σ/ M_\odot \mathrm{kpc}^2 ]\gtrsim 9$) are typical of quiescent galaxies at $z \gtrsim 2$. The galaxies display negative color gradients (redder core and bluer outskirts); for one galaxy, this effect results from a dusty core, while for the others it may be evidence of an "inside-out" growth process. Unlike local quiescent galaxies, we identify significant reddening in these typical cosmic noon passive galaxies; all but one require $A_V \gtrsim 0.4$. This finding is in qualitative agreement with previous studies but our deep 20-band NIRCam imaging is able to significantly suppress the dust-age degeneracy and confidently determine that these galaxies are reddened. We speculate about the physical effects that may drive the decline in dust content in quiescent galaxies over cosmic time. |
| title | UNCOVER: Significant Reddening in Cosmic Noon Quiescent Galaxies |
| topic | Astrophysics of Galaxies |
| url | https://arxiv.org/abs/2409.11457 |