Favole, GinevraComparat, JohanPrada, FranciscoYepes, GustavoJullo, EricNiemiec, AnnaKneib, Jean-PaulRodriguez-Torres, Sergio A.Klypin, AnatolySkibba, Ramin A.Mcbride, Cameron K.Eisenstein, Daniel J.Schlegel, David J.Nuza, Sebastian E.Chuang, Chia-HsunDelubac, TimotheeYeche, ChristopheSchneider, Donald P.2016-10-182016-10-182016-10-18201610.1093/mnras/stw1483https://infoscience.epfl.ch/handle/20.500.14299/130173WOS:000383514900003Current and future large redshift surveys, as the Sloan Digital Sky Survey IV extended Baryon Oscillation Spectroscopic Survey (SDSS-IV/eBOSS) or the Dark Energy Spectroscopic Instrument (DESI), will use emission-line galaxies (ELGs) to probe cosmological models by mapping the large-scale structure of the Universe in the redshift range 0.6 < z < 1.7. With current data, we explore the halo-galaxy connection by measuring three clustering properties of g-selected ELGs as matter tracers in the redshift range 0.6 < z < 1: (i) the redshift-space two-point correlation function using spectroscopic redshifts from the BOSS ELG sample and VIPERS; (ii) the angular two-point correlation function on the footprint of the CFHT-LS; (iii) the galaxy-galaxy lensing signal around the ELGs using the CFHTLenS. We interpret these observations by mapping them on to the latest high-resolution MultiDark Planck N-body simulation, using a novel (Sub) Halo-Abundance Matching technique that accounts for the ELG incompleteness. ELGs at z similar to 0.8 live in haloes of (1 +/- 0.5) x 10(12) h(-1)M(circle dot) and 22.5 +/- 2.5 per cent of them are satellites belonging to a larger halo. The halo occupation distribution of ELGs indicates that we are sampling the galaxies in which stars form in the most efficient way, according to their stellar-to-halo mass ratio.galaxies: distances and redshiftsgalaxies: haloesgalaxies: statisticscosmology: observationscosmology: theorylarge-scale structure of UniverseClustering properties of g-selected galaxies at z similar to 0.8text::journal::journal article::research article