OCEANS of Absorption: High-resolution NIRSpec Spectroscopy Reveals Diverse Balmer-line Absorption in Little Red Dots
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arXiv
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| Format: | Preprint |
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2026
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| author | Davis, Kelcey Brooks, Madisyn Simons, Raymond C. Trump, Jonathan R. Barro, Guillermo Haro, Pablo Arrabal Backhaus, Bren E. Cleri, Nikko J. de la Vega, Alexander Finkelstein, Steven L. Giavalisco, Mauro Grogin, Norman A. Hirschmann, Michaela Hutchison, Taylor A. Kocevski, Dale Koekemoer, Anton M. Lambrides, Erini Llerena, Mario Lucas, Ray A. Marshall, Madeline A. McGrath, Elizabeth J. Papovich, Casey Starrs, Aidan Taylor, Anthony J. Sanderbeck, Phoebe R. Upton Wang, Xin Wuyts, Stijn |
| author_facet | Davis, Kelcey Brooks, Madisyn Simons, Raymond C. Trump, Jonathan R. Barro, Guillermo Haro, Pablo Arrabal Backhaus, Bren E. Cleri, Nikko J. de la Vega, Alexander Finkelstein, Steven L. Giavalisco, Mauro Grogin, Norman A. Hirschmann, Michaela Hutchison, Taylor A. Kocevski, Dale Koekemoer, Anton M. Lambrides, Erini Llerena, Mario Lucas, Ray A. Marshall, Madeline A. McGrath, Elizabeth J. Papovich, Casey Starrs, Aidan Taylor, Anthony J. Sanderbeck, Phoebe R. Upton Wang, Xin Wuyts, Stijn |
| contents | The ``Little Red Dots' (LRDs) that appeared in JWST deep field images have been the subject of significant study since their discovery. In this work, we present high-resolution follow-up spectroscopy from the OCEANS program of 10 LRDs with Ha coverage at 3<z<7 in the CEERS/EGS field. We find Balmer-line absorption in 4 of these LRDs, a detection rate higher than the fractions reported in lower-resolution NIRSpec surveys. All of the absorbers are presented in high-resolution for the first time here and two have Balmer-line absorption detected for the first time. Of the 10 LRDs, 7 are best fit by Ha profiles with exponential wings. We find that absorbers tend to be blue-shifted with a median velocity offset of (-49 km/s) and absorption equivalent width of 5.3 Angstroms. Trends are explored to compare LRD absorption properties along the sequence of LRDs. We confirm an LRD with statistically significant absorption velocity offsets between Ha and Hb. The diversity of absorption properties can be effectively explained by a model with a radial distribution of partial-covering absorbing gas that is often co-located near the broad-line emission regions, along with a radial gradient of close inflow and distant outflow velocities for the absorbing gas. We present other interesting LRDs, including an outflow-dominated LRD and an LRD with relatively blue UV-to-optical colors but clear Balmer-line absorption. This high occurrence of absorbing hydrogen in LRDs, evident by both the Balmer-line absorption features and Balmer break strengths, implies a near-ubiquitous presence of dense, excited n=2 hydrogen. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2606_00258 |
| institution | arXiv |
| publishDate | 2026 |
| record_format | arxiv |
| spellingShingle | OCEANS of Absorption: High-resolution NIRSpec Spectroscopy Reveals Diverse Balmer-line Absorption in Little Red Dots Davis, Kelcey Brooks, Madisyn Simons, Raymond C. Trump, Jonathan R. Barro, Guillermo Haro, Pablo Arrabal Backhaus, Bren E. Cleri, Nikko J. de la Vega, Alexander Finkelstein, Steven L. Giavalisco, Mauro Grogin, Norman A. Hirschmann, Michaela Hutchison, Taylor A. Kocevski, Dale Koekemoer, Anton M. Lambrides, Erini Llerena, Mario Lucas, Ray A. Marshall, Madeline A. McGrath, Elizabeth J. Papovich, Casey Starrs, Aidan Taylor, Anthony J. Sanderbeck, Phoebe R. Upton Wang, Xin Wuyts, Stijn Astrophysics of Galaxies The ``Little Red Dots' (LRDs) that appeared in JWST deep field images have been the subject of significant study since their discovery. In this work, we present high-resolution follow-up spectroscopy from the OCEANS program of 10 LRDs with Ha coverage at 3<z<7 in the CEERS/EGS field. We find Balmer-line absorption in 4 of these LRDs, a detection rate higher than the fractions reported in lower-resolution NIRSpec surveys. All of the absorbers are presented in high-resolution for the first time here and two have Balmer-line absorption detected for the first time. Of the 10 LRDs, 7 are best fit by Ha profiles with exponential wings. We find that absorbers tend to be blue-shifted with a median velocity offset of (-49 km/s) and absorption equivalent width of 5.3 Angstroms. Trends are explored to compare LRD absorption properties along the sequence of LRDs. We confirm an LRD with statistically significant absorption velocity offsets between Ha and Hb. The diversity of absorption properties can be effectively explained by a model with a radial distribution of partial-covering absorbing gas that is often co-located near the broad-line emission regions, along with a radial gradient of close inflow and distant outflow velocities for the absorbing gas. We present other interesting LRDs, including an outflow-dominated LRD and an LRD with relatively blue UV-to-optical colors but clear Balmer-line absorption. This high occurrence of absorbing hydrogen in LRDs, evident by both the Balmer-line absorption features and Balmer break strengths, implies a near-ubiquitous presence of dense, excited n=2 hydrogen. |
| title | OCEANS of Absorption: High-resolution NIRSpec Spectroscopy Reveals Diverse Balmer-line Absorption in Little Red Dots |
| topic | Astrophysics of Galaxies |
| url | https://arxiv.org/abs/2606.00258 |