Zusammenfassung
We present a measurement of the baryon acoustic oscillation (BAO) scale at
redshift $z=2.35$ from the three-dimensional correlation of Lyman-$\alpha$
(Ly$\alpha$) forest absorption and quasars. The study uses 266,590 quasars in
the redshift range $1.77<z<3.5$ from the Sloan Digital Sky Survey (SDSS) Data
Release 14 (DR14). The sample includes the first two years of observations by
the SDSS-IV extended Baryon Oscillation Spectroscopic Survey (eBOSS), providing
new quasars and re-observations of BOSS quasars for improved statistical
precision. Statistics are further improved by including Ly$\alpha$ absorption
occurring in the Ly$\beta$ wavelength band of the spectra. From the measured
BAO peak position along and across the line of sight, we determine the Hubble
distance $D_H$ and the comoving angular diameter distance $D_M$ relative to
the sound horizon at the drag epoch $r_d$: $D_H(z=2.35)/r_d=9.200.36$
and $D_M(z=2.35)/r_d=36.31.8$. These results are consistent at
$1.5\sigma$ with the prediction of the best-fit flat $Łambda$CDM cosmological
model reported for the Planck (2016) analysis of CMB anisotropies. Combined
with the Ly$\alpha$ auto-correlation measurement presented in a companion paper
(de Sainte Agathe et al. 2019) the BAO measurements at $z=2.34$ are within
$1.7\sigma$ of the predictions of this model.
Nutzer