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Title: | The Lyman-continuum photon production efficiency ξ ION OF z∼ 4–5 galaxies from IRAC-based Hα measurements : implications for the escape fraction and cosmic reionization |
Authors: | Bouwens, Rychard J. Smit, R. Labbé, I. Franx, Marijn Caruana, Joseph Oesch, Pascal A. Stefanon, M. Rasappu, N. |
Keywords: | Galaxies Astrophysics Galaxies -- Evolution Galaxies -- Observations Galaxies -- Formation |
Issue Date: | 2016 |
Publisher: | The American Astronomical Society |
Citation: | Bouwens, R. J., Smit, R., Labbé, I., Franx, M., Caruana, J., Oesch, P., ... & Rasappu, N. (2016). The Lyman-continuum photon production efficiency ξ ION OF z∼ 4–5 galaxies from IRAC-based Hα measurements: implications for the escape fraction and cosmic reionization. The Astrophysical Journal, 831(2), 176. |
Abstract: | Galaxies represent one of the preferred candidate sources to drive the reionization of the universe. Even as gains are made in mapping the galaxy UV luminosity density to $z\gt 6$, significant uncertainties remain regarding the conversion to the implied ionizing emissivity. The relevant unknowns are the Lyman-continuum (LyC) photon production efficiency ${\xi }_{\mathrm{ion}}$ and the escape fraction fesc. As we show here, the first of these unknowns is directly measurable in z = 4–5 galaxies based on the impact the Hα line has on the observed IRAC fluxes. By computing a LyC photon production rate from the implied Hα luminosities for a broad selection of z = 4–5 galaxies and comparing this against the dust-corrected UV-continuum luminosities, we provide the first-ever direct estimates of the LyC photon production efficiency ${\xi }_{\mathrm{ion}}$ for the $z\geqslant 4$ galaxy population. We find $\,{\mathrm{log}}_{10}\,{\xi }_{\mathrm{ion}}/[\mathrm{Hz}\,{\mathrm{erg}}^{-1}]$ to have a mean value of ${25.27}_{-0.03}^{+0.03}$ and ${25.34}_{-0.02}^{+0.02}$ for sub-L* z = 4–5 galaxies adopting Calzetti and SMC dust laws, respectively. Reassuringly, both derived values are consistent with the standard assumed ${\xi }_{\mathrm{ion}}$'s in reionization models, with a slight preference for higher ${\xi }_{\mathrm{ion}}$'s (by ∼0.1 dex) adopting the SMC dust law. High values of ${\xi }_{\mathrm{ion}}$ (∼25.5–25.8 dex) are derived for the bluest galaxies ($\beta \lt -2.3$) in our samples, independent of dust law and consistent with results for a z = 7.045 galaxy. Such elevated values of ${\xi }_{\mathrm{ion}}$ would have important consequences, indicating that fesc cannot be in excess of 13% for standard assumptions about the faint-end cut-off to the LF and the clumping factor. |
URI: | https://www.um.edu.mt/library/oar/handle/123456789/87319 |
Appears in Collections: | Scholarly Works - FacSciPhy |
Files in This Item:
File | Description | Size | Format | |
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The Lyman-continuum photon production efficiency.pdf Restricted Access | 1.02 MB | Adobe PDF | View/Open Request a copy |
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