@article {498696,
	title = {Clustering properties of g-selected galaxies at z \~{} 0.8},
	journal = {Monthly Notices of the Royal Astronomical Society},
	volume = {461},
	year = {2016},
	month = {October 1, 2016},
	pages = {3421-3431},
	abstract = {Current and future large redshift surveys, as the Sloan Digital SkySurvey IV extended Baryon Oscillation Spectroscopic Survey(SDSS-IV/eBOSS) or the Dark Energy Spectroscopic Instrument (DESI), willuse emission-line galaxies (ELGs) to probe cosmological models bymapping the large-scale structure of the Universe in the redshift range0.6 < z < 1.7. With current data, we explore the halo-galaxyconnection by measuring three clustering properties of g-selected ELGsas matter tracers in the redshift range 0.6 < z < 1: (i) theredshift-space two-point correlation function using spectroscopicredshifts from the BOSS ELG sample and VIPERS; (ii) the angulartwo-point correlation function on the footprint of the CFHT-LS; (iii)the galaxy-galaxy lensing signal around the ELGs using the CFHTLenS. Weinterpret these observations by mapping them on to the latesthigh-resolution MultiDark Planck N-body simulation, using a novel(Sub)Halo-Abundance Matching technique that accounts for the ELGincompleteness. ELGs at z \~{} 0.8 live in haloes of (1 {\textpm} 0.5){\texttimes} 1012 h-1M⊙ and 22.5{\textpm} 2.5 per cent of them are satellites belonging to a larger halo.The halo occupation distribution of ELGs indicates that we are samplingthe galaxies in which stars form in the most efficient way, according totheir stellar-to-halo mass ratio.},
	keywords = {galaxies: distances and redshifts;  galaxies: haloes;  galaxies: statistics;  cosmology: observations;  cosmology: theory;  large-scale structure of Universe},
	isbn = {0035-8711},
	url = {http://adsabs.harvard.edu/abs/2016MNRAS.461.3421F},
	author = {Favole, Ginevra and Comparat, Johan and Prada, Francisco and Yepes, Gustavo and Jullo, Eric and Niemiec, Anna and Kneib, Jean-Paul and Rodr{\'\i}guez-Torres, Sergio A. and Klypin, Anatoly and Skibba, Ramin A. and Cameron K. McBride and Daniel J. Eisenstein and Schlegel, David J. and Nuza, Sebasti{\'a}n E. and Chuang, Chia-Hsun and Delubac, Timoth{\'e}e and Y{\`e}che, Christophe and Schneider, Donald P.}
}
