Search Results - "Sapio, Feliciana"

AMICO galaxy clusters in KiDS-DR3: measurement of the halo bias and power spectrum normalization from a stacked weak lensing analysis by Ingoglia, Lorenzo, Covone, Giovanni, Sereno, Mauro, Giocoli, Carlo, Bardelli, Sandro, Bellagamba, Fabio, Castignani, Gianluca, Farrens, Samuel, Hildebrandt, Hendrik, Joudaki, Shahab, Jullo, Eric, Lanzieri, Denise, Lesci, Giorgio F, Marulli, Federico, Maturi, Matteo, Moscardini, Lauro, Nanni, Lorenza, Puddu, Emanuela, Radovich, Mario, Roncarelli, Mauro, Sapio, Feliciana, Schimd, Carlo

“…Galaxy clusters are biased tracers of the underlying matter density field. At very large radii beyond about 10 Mpc h−1, the shear profile shows evidence of a…”
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AMICO galaxy clusters in KiDS-DR3: Measurement of the halo bias and power spectrum normalization from a stacked weak lensing analysis by Ingoglia, Lorenzo, Covone, Giovanni, Sereno, Mauro, Giocoli, Carlo, Bardelli, Sandro, Bellagamba, Fabio, Castignani, Gianluca, Farrens, Samuel, Hildebrandt, Hendrik, Joudaki, Shahab, Jullo, Eric, Lanzieri, Denise, Lesci, Giorgio F, Marulli, Federico, Maturi, Matteo, Moscardini, Lauro, Nanni, Lorenza, Puddu, Emanuela, Radovich, Mario, Roncarelli, Mauro, Sapio, Feliciana, Schimd, Carlo

“…Galaxy clusters are biased tracers of the underlying matter density field. At very large radii beyond about 10 Mpc/\textit{h}, the shear profile shows evidence…”
Get full text