ROSATI, PIERO

ROSATI, PIERO  

Mostra records
Risultati 1 - 8 di 8 (tempo di esecuzione: 0.011 secondi).
Titolo Data di pubblicazione Autori Rivista Serie Titolo libro
GMASS ultradeep spectroscopy of galaxies at z ~ 2 I. the stellar metallicity 2008 Daddi, E.Berta, S.Franceschini, A.Cassata, P.Rodighiero, G.Rosati, P. + ASTRONOMY & ASTROPHYSICS - -
Candels: The cosmic assembly near-infrared deep extragalactic legacy survey - The hubble space telescope observations, imaging data products, and mosaics 2011 Cassata, PaoloDaddi, EmanueleROSATI, PIEROScarlata, Claudia + ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES - -
Candels: The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey 2011 Cassata, PaoloDaddi, EmanueleRosati, PieroScarlata, Claudia + ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES - -
Magnifying the Early Episodes of Star Formation: Super Star Clusters at Cosmological Distances 2017 Vanzella E.Castellano M.Mercurio A.Rosati P.Mignoli M.Cristiani S.Grazian A.Bergamini P. + THE ASTROPHYSICAL JOURNAL - -
Quantifying the suppression of the (un)-obscured star formation in galaxy cluster cores at 0.2≲ z ≲0.9 2019 RODRIGUEZ MUNOZ, LUCIARodighiero, GMercurio, ARosati, PPuglisi, AFranceschini, ABaronchelli, IEnia, A F MIANI, EDOARDOVulcani, B + MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY - -
Strong lensing models of eight CLASH clusters from extensive spectroscopy: accurate total mass reconstructions in the cores 2019 P. RosatiMERCURIO, AMATABERGAMINI, PIETROE. VanzellaMAIER, Charles S. + ASTRONOMY & ASTROPHYSICS - -
Enhanced cluster lensing models with measured galaxy kinematics 2019 P. BergaminiP. RosatiA. MercurioM. MeneghettiAGNELLO, ANTONELLAC. GiocoliG. RodighieroE. Vanzella + ASTRONOMY & ASTROPHYSICS - -
Inquiring into the nature of the Abell 2667 brightest cluster galaxy: physical properties from MUSE 2019 Iani E.Rodighiero G.Mancini C.Rodriguez-Munoz L.Rosati P.Berta S.Cassata P.Concas A.Enia A.Franceschini A.Mercurio A.Morselli L.SABATINI, GABRIELLA + MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY - -