Abstract The DESI survey will observe more than 8 million candidate luminous red galaxies (LRGs) in the redshift range 0.3 < z < 1.0. Here we present a preliminary version of the DESI LRG target section developed using Legacy Surveys Data Release 8 g, r, z and W1 photometry. This selection yields a sample with a uniform surface density of ∼600 deg−2 and very low predicted stellar contamination and redshift failure rates. During DESI Survey Validation, updated versions of this selection will be tested and optimized
The Dark Energy Spectroscopic Instrument (DESI) survey will measure large-scale structures using qua...
We evaluate the impact of imaging systematics on the clustering of luminous red galaxies (LRG), emis...
We evaluate the impact of imaging systematics on the clustering of luminous red galaxies (LRG), emis...
Abstract The DESI survey will observe more than 8 million candidate luminous red gala...
The Dark Energy Spectroscopic Instrument (DESI) is carrying out a five-year survey that aims to meas...
Abstract DESI will precisely constrain cosmic expansion and the growth of structure b...
The Dark Energy Spectroscopic Instrument (DESI) will precisely constrain cosmic expansion and the gr...
International audienceWe present two galaxy samples, selected from DESI Legacy Imaging Surveys (LS) ...
International audienceAbstract The Dark Energy Spectroscopic Instrument (DESI) will ex...
The Dark Energy Spectroscopic Instrument (DESI) Survey has obtained a set of spectroscopic measureme...
The Dark Energy Spectroscopic Instrument (DESI) survey will measure large-scale structures using qua...
We evaluate the impact of imaging systematics on the clustering of luminous red galaxies (LRG), emis...
We evaluate the impact of imaging systematics on the clustering of luminous red galaxies (LRG), emis...
Abstract The DESI survey will observe more than 8 million candidate luminous red gala...
The Dark Energy Spectroscopic Instrument (DESI) is carrying out a five-year survey that aims to meas...
Abstract DESI will precisely constrain cosmic expansion and the growth of structure b...
The Dark Energy Spectroscopic Instrument (DESI) will precisely constrain cosmic expansion and the gr...
International audienceWe present two galaxy samples, selected from DESI Legacy Imaging Surveys (LS) ...
International audienceAbstract The Dark Energy Spectroscopic Instrument (DESI) will ex...
The Dark Energy Spectroscopic Instrument (DESI) Survey has obtained a set of spectroscopic measureme...
The Dark Energy Spectroscopic Instrument (DESI) survey will measure large-scale structures using qua...
We evaluate the impact of imaging systematics on the clustering of luminous red galaxies (LRG), emis...
We evaluate the impact of imaging systematics on the clustering of luminous red galaxies (LRG), emis...