The BoRG-JWST Survey: Program Overview and First Confirmations of Luminous Reionization-era Galaxies from Pure-parallel Observations

Abstract We present the BoRG-JWST survey, a combination of two JWST Cycle 1 programs aimed at obtaining NIRSpec spectroscopy of representative, UV-bright 7 < z < 10 galaxy candidates across 22 independent sight lines selected from Hubble/WFC3 pure-parallel observations. We confirm the high- z nature of 12 out of 21 observed primary targets through low-resolution prism observations, with the rest revealing themselves unsurprisingly to be z ∼ 1–3 interlopers, brown dwarfs, or yielding inconclusive results. From the Multi Shutter Array (MSA) observations, we confirm an additional nine filler sources at z > 5, highlighting the large abundance of high-redshift galaxies even in individual WFC3 pointings. The primary sample spans the absolute magnitude range −20.4 mag < M UV < −22.4 mag and harbors UV continuum slopes of β ≃ −2.5 to −2.0, representing some of the most luminous z > 7 sources currently known and comparable to the brightest NIRCam sources at z > 10. Prominent [O iii ]+H β lines are found across the full sample, while a stack of sources reveals a plethora of other rest-optical lines and additional rest-UV C III ] 1909 Å emission. Despite their luminosities, none of the low-resolution spectra display evidence for type 1 active galactic nucleus activity based on a search for broad-line emission. Lastly, we present a spectroscopic data release of 188 confirmed 0.5 ≲ z ≲ 5.0 sources from filler MSA observations, highlighting the legacy value of the survey and a representative benchmark for comparisons to deep field observations.

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Publication Details

Journal
The Astrophysical Journal
Published
2025-04-01
DOI
https://doi.org/10.3847/1538-4357/adba60
Citations
8
Primary Topic
Galaxies: Formation, Evolution, Phenomena
Type
article
Field-Weighted Citation Impact
9.24

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article

The BoRG-JWST Survey: Program Overview and First Confirmations of Luminous Reionization-era Galaxies from Pure-parallel Observations

Christian Soto, Guido Roberts-Borsani, Óscar A. Chávez Ortiz, Nicha Leethochawalit et al.
8 citations
The Astrophysical Journal
Galaxies: Formation, Evolution, Phenomena
9.24
article

The BoRG-JWST Survey: Program Overview and First Confirmations of Luminous Reionization-era Galaxies from Pure-parallel Observations

Christian Soto, Guido Roberts-Borsani, Óscar A. Chávez Ortiz, Nicha Leethochawalit, Charlotte Mason, Rebecca L. Larson, Tommaso Treu, Gene C. K. Leung, Rachel S. Somerville, Pablo Arrabal Haro, Katherine Chworowsky, Susan A. Kassin, Takahiro Morishita, L. Y. Aaron Yung, Eduardo Bañados, Sofía Rojas-Ruiz, Steven L. Finkelstein, M. Stiavelli, Micaela B. Bagley, Taylor A. Hutchison, Michele Trenti
article en
8 citations

Abstract

Abstract We present the BoRG-JWST survey, a combination of two JWST Cycle 1 programs aimed at obtaining NIRSpec spectroscopy of representative, UV-bright 7 < z < 10 galaxy candidates across 22 independent sight lines selected from Hubble/WFC3 pure-parallel observations. We confirm the high- z nature of 12 out of 21 observed primary targets through low-resolution prism observations, with the rest revealing themselves unsurprisingly to be z ∼ 1–3 interlopers, brown dwarfs, or yielding inconclusive results. From the Multi Shutter Array (MSA) observations, we confirm an additional nine filler sources at z > 5, highlighting the large abundance of high-redshift galaxies even in individual WFC3 pointings. The primary sample spans the absolute magnitude range −20.4 mag < M UV < −22.4 mag and harbors UV continuum slopes of β ≃ −2.5 to −2.0, representing some of the most luminous z > 7 sources currently known and comparable to the brightest NIRCam sources at z > 10. Prominent [O iii ]+H β lines are found across the full sample, while a stack of sources reveals a plethora of other rest-optical lines and additional rest-UV C III ] 1909 Å emission. Despite their luminosities, none of the low-resolution spectra display evidence for type 1 active galactic nucleus activity based on a search for broad-line emission. Lastly, we present a spectroscopic data release of 188 confirmed 0.5 ≲ z ≲ 5.0 sources from filler MSA observations, highlighting the legacy value of the survey and a representative benchmark for comparisons to deep field observations.

The Astrophysical JournalVol. 983(1)
Damien Foundation (BD)
National Science Foundation, National Aeronautics and Space Administration, Villum Fonden, Space Telescope Science Institute, Flatiron Health, National Research Foundation, Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung, Danmarks Grundforskningsfond
Openalex Percentile: Top 2%
Galaxies: Formation, Evolution, Phenomena
9.24
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