The redshift evolution of rest-UV spectroscopic properties to z ∼ 5
ABSTRACT We perform a comprehensive analysis of the redshift evolution of the rest-UV spectra of star-forming galaxies out to z ∼ 5. We combine new z ∼ 5 measurements of H i Ly α and low- and high-ionization interstellar metal absorption features with comparable measurements at z ∼ 2–4. We measure t...
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| Published in | Monthly notices of the Royal Astronomical Society Vol. 493; no. 3; pp. 3194 - 3211 |
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| Main Authors | , , , , , , , |
| Format | Journal Article |
| Language | English Norwegian |
| Published |
Oxford University Press
11.04.2020
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| Subjects | |
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| Abstract | ABSTRACT
We perform a comprehensive analysis of the redshift evolution of the rest-UV spectra of star-forming galaxies out to z ∼ 5. We combine new z ∼ 5 measurements of H i Ly α and low- and high-ionization interstellar metal absorption features with comparable measurements at z ∼ 2–4. We measure the equivalent widths of interstellar absorption features using stacked spectra in bins of Ly α equivalent width, performing corrections to Ly α strengths based on a model for the transmission of the intergalactic medium. We find a strong correlation between decreasing low-ionization absorption strength and increasing Ly α emission strength over the redshift range z ∼ 2–5, suggesting that both of these quantities are fundamentally linked to neutral gas covering fraction. At the highest Ly α equivalent widths, we observe evolution at z ∼ 5 towards greater Ly α emission strength at fixed low-ionization absorption strength. If we interpret the non-evolving relationship of Ly α emission strength and low-ionization line strength at z ∼ 2−4 as primarily reflecting the radiative transfer of Ly α photons, this evolution at z ∼ 5 suggests a higher intrinsic production rate of Ly α photons than at lower redshift. Our conclusion is supported by the joint evolution of the relationships among Ly α emission strength, interstellar absorption strength, and dust reddening. We perform additional analysis in bins of stellar mass, star formation rate, UV luminosity, and age, examining how the relationships between galaxy properties and Ly α emission evolve towards higher redshift. We conclude that increasing intrinsic Ly α photon production and strong detection of nebular C iv emission (signalling lower metallicity) at z ∼ 5 indicate an elevated ionized photon production efficiency (ξion). |
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| AbstractList | ABSTRACT
We perform a comprehensive analysis of the redshift evolution of the rest-UV spectra of star-forming galaxies out to z ∼ 5. We combine new z ∼ 5 measurements of H i Ly α and low- and high-ionization interstellar metal absorption features with comparable measurements at z ∼ 2–4. We measure the equivalent widths of interstellar absorption features using stacked spectra in bins of Ly α equivalent width, performing corrections to Ly α strengths based on a model for the transmission of the intergalactic medium. We find a strong correlation between decreasing low-ionization absorption strength and increasing Ly α emission strength over the redshift range z ∼ 2–5, suggesting that both of these quantities are fundamentally linked to neutral gas covering fraction. At the highest Ly α equivalent widths, we observe evolution at z ∼ 5 towards greater Ly α emission strength at fixed low-ionization absorption strength. If we interpret the non-evolving relationship of Ly α emission strength and low-ionization line strength at z ∼ 2−4 as primarily reflecting the radiative transfer of Ly α photons, this evolution at z ∼ 5 suggests a higher intrinsic production rate of Ly α photons than at lower redshift. Our conclusion is supported by the joint evolution of the relationships among Ly α emission strength, interstellar absorption strength, and dust reddening. We perform additional analysis in bins of stellar mass, star formation rate, UV luminosity, and age, examining how the relationships between galaxy properties and Ly α emission evolve towards higher redshift. We conclude that increasing intrinsic Ly α photon production and strong detection of nebular C iv emission (signalling lower metallicity) at z ∼ 5 indicate an elevated ionized photon production efficiency (ξion). |
| Author | Capak, Peter L Reddy, Naveen A Laursen, Peter Pahl, Anthony J Du, Xinnan Faisst, Andreas L Topping, Michael W Shapley, Alice |
| Author_xml | – sequence: 1 givenname: Anthony J orcidid: 0000-0003-4464-4505 surname: Pahl fullname: Pahl, Anthony J email: pahl@astro.ucla.edu organization: Department of Physics and Astronomy, University of California, Los Angeles, CA 90095, USA – sequence: 2 givenname: Alice surname: Shapley fullname: Shapley, Alice organization: Department of Physics and Astronomy, University of California, Los Angeles, CA 90095, USA – sequence: 3 givenname: Andreas L surname: Faisst fullname: Faisst, Andreas L organization: IPAC, California Institute of Technology, 1200 East California Boulevard, Pasadena, CA 91125, USA – sequence: 4 givenname: Peter L surname: Capak fullname: Capak, Peter L organization: IPAC, California Institute of Technology, 1200 East California Boulevard, Pasadena, CA 91125, USA – sequence: 5 givenname: Xinnan surname: Du fullname: Du, Xinnan email: pahl@astro.ucla.edu organization: Department of Physics and Astronomy, University of California Riverside, Riverside, CA 92521, USA – sequence: 6 givenname: Naveen A surname: Reddy fullname: Reddy, Naveen A organization: Department of Physics and Astronomy, University of California Riverside, Riverside, CA 92521, USA – sequence: 7 givenname: Peter surname: Laursen fullname: Laursen, Peter organization: Institute of Theoretical Astrophysics, University of Oslo, PO Box 1029, Blindern, 0315 Oslo, Norway – sequence: 8 givenname: Michael W surname: Topping fullname: Topping, Michael W organization: Department of Physics and Astronomy, University of California, Los Angeles, CA 90095, USA |
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| Copyright | 2020 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society 2020 info:eu-repo/semantics/openAccess |
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| Keywords | galaxies: evolution galaxies: ISM galaxies: high-redshift |
| Language | English Norwegian |
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We perform a comprehensive analysis of the redshift evolution of the rest-UV spectra of star-forming galaxies out to z ∼ 5. We combine new z ∼ 5... |
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| Title | The redshift evolution of rest-UV spectroscopic properties to z ∼ 5 |
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