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The Low-Redshift Lyman Continuum Survey II: New Insights into LyC Diagnostics

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arxiv 2203.15649 v1 pith:MHELE4VL submitted 2022-03-29 astro-ph.GA astro-ph.CO

The Low-Redshift Lyman Continuum Survey II: New Insights into LyC Diagnostics

Sophia R. Flury (1) , Anne E. Jaskot (2) , Harry C. Ferguson (3) , Gabor Worseck (4) , Kirill Makan (4) , John Chisholm (5) , Alberto Saldana-Lopez (6) , Daniel Schaerer (6)
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Stephan McCandliss (7) Bingjie Wang (7) N. M. Ford (2) M. S. Oey (8) Timothy Heckman (7) Zhiyuan Ji (1) Mauro Giavalisco (1) Ricardo Amorin (9) Hakim Atek (10) Jeremy Blaizot (11) Sanchayeeta Borthakur (12) Cody Carr (13) Marco Castellano (14) Stefano Cristiani (15) Stephane de Barros (6) Mark Dickinson (16) Steven L. Finkelstein (5) Brian Fleming (17) Fabio Fontanot (14) Thibault Garel (6) Andrea Grazian (18) Matthew Hayes (19) Alaina Henry (3) Valentin Mauerhofer (6) Genoveva Micheva (20) Goran Ostlin (19) Casey Papovich (21) Laura Pentericci (14) Swara Ravindranath (3) Joakim Rosdahl (11) Michael Rutkowski (22) Paola Santini (14) Claudia Scarlata (13) Harry Teplitz (23) Trinh Thuan (24) Maxime Trebitsch (25) Eros Vanzella (26) Anne Verhamme (6 11) Xinfeng Xu (7) ((1) University of Massachusetts Amherst (2) Williams College (3) Space Telescope Science Institute (4) Universitat Potsdam (5) University of Texas Austin (6) University of Geneva (7) Johns Hopkins University (8) University of Michigan (9) Universidad de La Serena (10) Sorbonne Universit\'e (11) Universit\'e de Lyon (12) Arizona State University (13) University of Minnesota (14) Osservatorio Astronomico di Roma (15) Osservatorio Astronomico di Trieste (16) NOIRLab (17) Laboratory for Atmospheric Space Physics (18) Osservatorio Astronomico di Padova (19) Stockholm University (20) Leibniz-Institute for Astrophysics Potsdam (21) Texas A&M (22) Minnesota State University (23) Cal Tech (24) University of Virginia (25) Kapteyn Astronomical Institute (26) Osservatoria Astronomico di Bologna)
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classification astro-ph.GA astro-ph.CO
keywords continuumdiagnosticslymanescapedensityescapingfindflux
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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The Lyman continuum (LyC) cannot be observed at the epoch of reionization (z {\gtrsim} 6) due to intergalactic H I absorption. To identify Lyman continuum emitters (LCEs) and infer the fraction of escaping LyC, astronomers have developed various indirect diagnostics of LyC escape. Using measurements of the LyC from the Low-redshift Lyman Continuum Survey (LzLCS), we present the first statistical test of these diagnostics. While optical depth indicators based on Ly{\alpha}, such as peak velocity separation and equivalent width, perform well, we also find that other diagnostics, such as the [O III]/[O II] flux ratio and star formation rate surface density, predict whether a galaxy is a LCE. The relationship between these galaxy properties and the fraction of escaping LyC flux suggests that LyC escape depends strongly on H I column density, ionization parameter, and stellar feedback. We find LCEs occupy a range of stellar masses, metallicities, star formation histories, and ionization parameters, which may indicate episodic and/or different physical causes of LyC escape.

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  1. Subaru meets JWST: A Direct Measurement of Ly$\boldsymbol{\alpha}$ Escape Fraction at $\boldsymbol{z\simeq6.2}$ with Dual Narrow-Band Imaging

    astro-ph.GA 2026-07 conditional novelty 6.5

    Completeness-weighted stacking of 56 HAEs at z≃6.2 gives median f_esc^Lyα = 0.106^{+0.066}_{-0.044} with no strong Hα-luminosity dependence and UV-linked galaxy-to-galaxy trends.