REBELS-IFU: Spatially Resolved Ionizing Photon Production Efficiencies of 12 Bright Galaxies in the Epoch of Reionization
Authors:
- Lena KomarovaLKLena Komarova
- Mauro StefanonMSMauro Stefanon
- Andrés Laza-RamosALAndrés Laza-Ramos
- Hiddo S.B. AlgeraHAHiddo S.B. Algera
- Manuel AravenaMAManuel Aravena
- Rychard BouwensRBRychard Bouwens
- Rebecca BowlerRBRebecca Bowler
- Elisabete da CunhaECElisabete da Cunha
- Pratika DayalPDPratika Dayal
- Andrea FerraraAFAndrea Ferrara
- Rebecca FisherRFRebecca Fisher
- Themiya NanayakkaraTNThemiya Nanayakkara
Open Access
- 25 March 2026
- journal article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 1000 (2) , 228
Abstract
Measuring the ionizing photon production efficiency ξ ion,0 —the ratio of the ionizing photon output rate Q H 0 to the UV continuum luminosity L UV —in galaxies at z > 6 is crucial for constraining their contribution to cosmic reionization. We present integrated and spatially resolved measurements of ξ ion,0 for 12 exceptionally bright ( M UV ∼ −22 mag) star-forming galaxies at z ∼ 7 from the Reionization Era Bright Emission Line Survey (REBELS). These measurements are based on JWST NIRSpec/Integral Field Unit PRISM spectroscopy, probing the rest-frame UV and optical regime. Notably, in 8 of the 12 galaxies, the spectral coverage includes H α , enabling self-consistent dust attenuation estimates in both the ionized gas and stellar continuum via the Balmer decrement and rest-UV slope, respectively. We find global log ( ξ ion,0 ) values ranging from 25.19 ± 0.11 to 25.61 ± 0.11, with a weighted mean of 25.44 ± 0.15, consistent with the canonical value of ∼25.3. Using a sample of 25 star-forming clumps within these galaxies, we explore local variations in the ionizing photon production efficiency, finding a broader range, from 24.52 ± 0.21 to 26.18 ± 0.61. We identify strong correlations between ξ ion,0 and the specific star formation rate, star formation surface density, H β equivalent width, and stellar mass. Clumps with the highest ξ ion,0 exhibit EW 0 (H β ) ≥ 150 Å, consistent with young stellar ages. From previous Ly α measurements in three galaxies, we estimate a typical Ly α escape fraction of f esc,Ly α ∼ 2%, suggesting similar or lower escape fractions for LyC photons. Combining this with our H α measurements, we infer ionized bubble sizes ∼1 pMpc, aligned with expectations from Ly α -detected systems and reionization models.Keywords
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Funding Information
- EC ∣ European Research Council (101088789)
- Generalitat Valenciana (2021/059)
- ANID ∣ Fondo Nacional de Desarrollo Científico y Tecnológico (1252054)
- Agencia Nacional de Investigación y Desarrollo (FB210003)
- Agencia Nacional de Investigación y Desarrollo (NCN2024 112)
- UKRI ∣ STFC ∣ Rutherford Appleton Laboratory (ST/T003596/1)
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