The ALPINE-CRISTAL-JWST Survey: Stellar and Nebular Dust Attenuation of Main-sequence Galaxies at z ∼ 4–6

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Abstract
Characterizing dust attenuation is crucial for revealing the intrinsic physical properties of galaxies. We present an analysis of dust attenuation in 18 spectroscopically confirmed star-forming main-sequence galaxies at z = 4.4−5.7 observed with JWST/NIRSpec IFU and NIRCam, selected from the ALPINE and CRISTAL ALMA large programs. We fit the emission-line fluxes from NIRSpec and the broadband photometry from NIRCam with Prospector , using both spatially integrated emission and ∼0.6 kpc pixel-by-pixel measurements. We derive the stellar-to-nebular dust attenuation ratio ( f = E ( B − V ) star / E ( B − V ) neb ) from the SED fits and the Balmer decrement with H α and H β . Although individual galaxies show large scatter, the best-fit value is f = 0.5 1 − 0.03 + 0.04 , slightly higher than that measured for local starburst galaxies. We find weak correlations of f with galaxy properties, increasing with higher specific star formation rates, younger stellar ages, and more recent star formation. For the range of E ( B − V ) star = 0.009−0.15 mag for in our sample, assuming f = 1 (often adopted in high-redshift studies) instead of f = 0.51 leads to the underestimation of line luminosities and ionizing photon production efficiency ξ ion by ∼3%−36% and ∼4​​​​​​%−46%, respectively. Finally, total stellar masses estimated from spatially integrated SED fits with delayed- τ star formation histories are systematically smaller than the sums of pixel-by-pixel SED fits by a median of ∼0.26 dex, likely because the integrated fits are biased toward luminous young stellar populations.
Funding Information
  • MEXT ∣ Japan Society for the Promotion of Science (24KJ0562)
  • ANID BASAL (FB210003)
  • Agence Nationale de la Recherche (ANR-15- IDEX-01)
  • Narodowe Centrum Nauki (MO2020/38/E/ST9/00077)
  • Narodowe Centrum Nauki (UMO2020/38/E/ST9/00077)
  • ALMA-ANID (ASTRO21-0062)
  • ANID BASAL (FB210003)
  • ANID MILENIO (NCN2024_112)
  • ANID Fondecyt (1221846)
  • ANID MILENIO (NCN2024_112)
  • EC ∣ European Research Council (ERC-2019- StG-851622)
  • Belgian Federal Science Policy Office (C4000142239)
  • Fonds Wetenschappelijk Onderzoek (G0A1523N)
  • ANID MILENIO (NCN2024_112)
  • MEXT ∣ Japan Society for the Promotion of Science (JP22H04939)
  • MEXT ∣ Japan Society for the Promotion of Science (JP23K20035)
  • MEXT ∣ Japan Society for the Promotion of Science (JP24H00004)

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