Quantifying distributions of the lyman continuum escape fraction

Renyue Cen, Taysun Kimm

Research output: Contribution to journalArticle

20 Citations (Scopus)

Abstract

Simulations have indicated that most of the escaped Lyman continuum (LyC) photons escape through a minority of solid angles with near complete transparency, with the remaining majority of the solid angles largely opaque, resulting in a very broad and skewed probability distribution function (PDF) of the escape fraction when viewed at different angles. Thus, the escape fraction of LyC photons of a galaxy observed along a line of sight merely represents the properties of the interstellar medium along that line of sight, which may be an ill-representation of the true escape fraction of the galaxy averaged over its full sky. Here we study how LyC photons escape from galaxies at z = 4-6, utilizing high-resolution large-scale cosmological radiation-hydrodynamic simulations. We compute the PDF of the mean escape fraction (〈fesc,1D〉) averaged over mock observational samples, as a function of the sample size, compared to the true mean (if an infinite sample size is used). We find that, when the sample size is small, the apparent mean skews to the low end. For example, for a true mean of 6.7%, an observational sample of (2,10,50) galaxies at z = 4 would have have a 2.5% probability of obtaining the sample mean lower than 〈fesc,1D〉 = (0.007%, 1.8%, 4.1%) and a 2.5% probability of obtaining the sample mean greater than (43%, 18%, 11%). Our simulations suggest that at least ∼100 galaxies should be stacked in order to constrain the true escape fraction within 20% uncertainty.

Original languageEnglish
Article numberL25
JournalAstrophysical Journal Letters
Volume801
Issue number2
DOIs
Publication statusPublished - 2015 Mar 10

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escape
continuums
galaxies
simulation
probability distribution functions
line of sight
transparency
photons
hydrodynamics
minorities
distribution
sky
high resolution
radiation

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

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title = "Quantifying distributions of the lyman continuum escape fraction",
abstract = "Simulations have indicated that most of the escaped Lyman continuum (LyC) photons escape through a minority of solid angles with near complete transparency, with the remaining majority of the solid angles largely opaque, resulting in a very broad and skewed probability distribution function (PDF) of the escape fraction when viewed at different angles. Thus, the escape fraction of LyC photons of a galaxy observed along a line of sight merely represents the properties of the interstellar medium along that line of sight, which may be an ill-representation of the true escape fraction of the galaxy averaged over its full sky. Here we study how LyC photons escape from galaxies at z = 4-6, utilizing high-resolution large-scale cosmological radiation-hydrodynamic simulations. We compute the PDF of the mean escape fraction (〈fesc,1D〉) averaged over mock observational samples, as a function of the sample size, compared to the true mean (if an infinite sample size is used). We find that, when the sample size is small, the apparent mean skews to the low end. For example, for a true mean of 6.7{\%}, an observational sample of (2,10,50) galaxies at z = 4 would have have a 2.5{\%} probability of obtaining the sample mean lower than 〈fesc,1D〉 = (0.007{\%}, 1.8{\%}, 4.1{\%}) and a 2.5{\%} probability of obtaining the sample mean greater than (43{\%}, 18{\%}, 11{\%}). Our simulations suggest that at least ∼100 galaxies should be stacked in order to constrain the true escape fraction within 20{\%} uncertainty.",
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Quantifying distributions of the lyman continuum escape fraction. / Cen, Renyue; Kimm, Taysun.

In: Astrophysical Journal Letters, Vol. 801, No. 2, L25, 10.03.2015.

Research output: Contribution to journalArticle

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AB - Simulations have indicated that most of the escaped Lyman continuum (LyC) photons escape through a minority of solid angles with near complete transparency, with the remaining majority of the solid angles largely opaque, resulting in a very broad and skewed probability distribution function (PDF) of the escape fraction when viewed at different angles. Thus, the escape fraction of LyC photons of a galaxy observed along a line of sight merely represents the properties of the interstellar medium along that line of sight, which may be an ill-representation of the true escape fraction of the galaxy averaged over its full sky. Here we study how LyC photons escape from galaxies at z = 4-6, utilizing high-resolution large-scale cosmological radiation-hydrodynamic simulations. We compute the PDF of the mean escape fraction (〈fesc,1D〉) averaged over mock observational samples, as a function of the sample size, compared to the true mean (if an infinite sample size is used). We find that, when the sample size is small, the apparent mean skews to the low end. For example, for a true mean of 6.7%, an observational sample of (2,10,50) galaxies at z = 4 would have have a 2.5% probability of obtaining the sample mean lower than 〈fesc,1D〉 = (0.007%, 1.8%, 4.1%) and a 2.5% probability of obtaining the sample mean greater than (43%, 18%, 11%). Our simulations suggest that at least ∼100 galaxies should be stacked in order to constrain the true escape fraction within 20% uncertainty.

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