TY - JOUR
T1 - The one-dimensional power spectrum from the SDSS DR14 Lyα forests
AU - Chabanier, S.
AU - Palanque-Delabrouille, Nathalie
AU - Yeche, Christophe
AU - Le Goff, Jean-Marc
AU - Armengaud, Eric
AU - Bautista, Julian Ernesto
AU - Blomqvist, Michael
AU - Busca, Nicolas G.
AU - Dawson, Kyle S.
AU - Etourneau, Thomas
AU - Font-Ribera, Andreu
AU - Lee, Yonghae
AU - des Bourboux, Helion du Mas
AU - Pieri, Matthew
AU - Rich, J.
AU - Rossi, Graziano
AU - Schneider, Donald P.
AU - Slosar, Anže
PY - 2019/7/10
Y1 - 2019/7/10
N2 - We present a measurement of the 1D Lyα forest flux power spectrum, using the
complete Baryon Oscillation Spectroscopic Survey (BOSS) and first extended-BOSS (eBOSS) quasars at zqso > 2.1, corresponding to the fourteenth data release (DR14) of the Sloan Digital Sky Survey (SDSS). Our results cover thirteen bins in redshift from zLyα = 2.2 to 4.6, and scales up to k = 0.02 (km/s)−1. From a parent sample of 180,413 visually inspected spectra, we selected the 43,751 quasars with the best quality; this data set improves the previous result from the ninth data release (DR9), both in statistical precision (achieving a reduction by a factor of two) and in redshift coverage. We also present a thorough investigation of identified sources of systematic uncertainties that affect the measurement. The resulting 1D power spectrum of this work is in excellent agreement with the one from the BOSS DR9 data.
AB - We present a measurement of the 1D Lyα forest flux power spectrum, using the
complete Baryon Oscillation Spectroscopic Survey (BOSS) and first extended-BOSS (eBOSS) quasars at zqso > 2.1, corresponding to the fourteenth data release (DR14) of the Sloan Digital Sky Survey (SDSS). Our results cover thirteen bins in redshift from zLyα = 2.2 to 4.6, and scales up to k = 0.02 (km/s)−1. From a parent sample of 180,413 visually inspected spectra, we selected the 43,751 quasars with the best quality; this data set improves the previous result from the ninth data release (DR9), both in statistical precision (achieving a reduction by a factor of two) and in redshift coverage. We also present a thorough investigation of identified sources of systematic uncertainties that affect the measurement. The resulting 1D power spectrum of this work is in excellent agreement with the one from the BOSS DR9 data.
U2 - 10.1088/1475-7516/2019/07/017
DO - 10.1088/1475-7516/2019/07/017
M3 - Article
SN - 1475-7516
VL - 2019
JO - Journal of Cosmology and Astroparticle Physics
JF - Journal of Cosmology and Astroparticle Physics
IS - 7
M1 - 017
ER -