Instruct: Identify the main and secondary category of Arxiv papers based on the titles and abstracts
Query: The Giant Gemini GMOS survey of z>4.4 quasars - I. Measuring the mean
  free path across cosmic time   We have obtained spectra of 163 quasars at $z_\mathrm{em}>4.4$ with the
Gemini Multi Object Spectrometers on the Gemini North and South telescopes, the
largest publicly available sample of high-quality, low-resolution spectra at
these redshifts. From this homogeneous data set, we generated stacked quasar
spectra in three redshift intervals at $z\sim 5$. We have modelled the flux
below the rest-frame Lyman limit ($\lambda_\mathrm{r}<912$\AA) to assess the
mean free path $\lambda_\mathrm{mfp}^{912}$ of the intergalactic medium to
HI-ionizing radiation. At mean redshifts $z_\mathrm{q}=4.56$, 4.86 and 5.16, we
measure $\lambda_\mathrm{mfp}^{912}=(22.2\pm 2.3, 15.1\pm 1.8, 10.3\pm
1.6)h_{70}^{-1}$ proper Mpc with uncertainties dominated by sample variance.
Combining our results with $\lambda_\mathrm{mfp}^{912}$ measurements from lower
redshifts, the data are well modelled by a simple power-law
$\lambda_\mathrm{mfp}^{912}=A[(1+z)/5]^\eta$ with $A=(37\pm 2)h_{70}^{-1}$ Mpc
and $\eta = -5.4\pm 0.4$ between $z=2.3$ and $z=5.5$. This rapid evolution
requires a physical mechanism -- beyond cosmological expansion -- which reduces
the cosmic effective Lyman limit opacity. We speculate that the majority of HI
Lyman limit opacity manifests in gas outside galactic dark matter haloes,
tracing large-scale structures (e.g. filaments) whose average density (and
consequently neutral fraction) decreases with cosmic time. Our measurements of
the strongly redshift-dependent mean free path shortly after the completion of
HI reionization serve as a valuable boundary condition for numerical models
thereof. Having measured $\lambda_\mathrm{mfp}^{912}\approx 10$ Mpc at $z=5.2$,
we confirm that the intergalactic medium is highly ionized by that epoch and
that the redshift evolution of the mean free path does not show a break that
would indicate a recent end to HI reionization.

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The categories of this paper are: hep-ex
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The categories of this paper are: ao-sci
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The categories of this paper are: hep-th
29
The categories of this paper are: funct-an
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The categories of this paper are: mtrl-th
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The categories of this paper are: cmp-lg
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The categories of this paper are: solv-int
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The categories of this paper are: hep-ph
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The categories of this paper are: nucl-ex
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The categories of this paper are: quant-ph
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The categories of this paper are: adap-org
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The categories of this paper are: math
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The categories of this paper are: nlin
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The categories of this paper are: dg-ga
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The categories of this paper are: plasm-ph
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The categories of this paper are: nucl-th