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Ciardullo, R.Guaita, Lucía.Padilla, NelsonFrancke Henríquez, Harold Johanns Phillippe.Treister, Ezequiel.Gronwall, CarylWolf, ChristopherMcCathran, EmilyBond, N.Gawiser, Eric.Feldmeier, John J.[The Evolution of Lyα-emitting Galaxies between z = 2.1 and z = 3.1]The Evolution of Lyα-emitting Galaxies between z = 2.1 and z = 3.1
Awan, HumnaGawiser, EricKurczynski, PeterJones, R. LynneZhan, HuPadilla, NelsonMuñoz Arancibia, Alejandra M.Orsi, ÁlvaroCora, Sofía A.Yoachim, Peter[Testing LSST Dither Strategies for Survey Uniformity and Large-Scale Structure Systematics]Testing LSST Dither Strategies for Survey Uniformity and Large-Scale Structure Systematics
Díaz Tello, J.Donzelli, C.Padilla, NelsonAkiyama, M.Fujishiro, N.Yoshikawa, T.Hanami, H.[Star formation activity in Balmer break galaxies at z < 1.5]Star formation activity in Balmer break galaxies at z < 1.5
Rodríguez, SilvioPadilla, NelsonGarcía Lambas, Diego[The effects of environment on the intrinsic shape of galaxies]The effects of environment on the intrinsic shape of galaxies
Tejos, NicolásProchaska, J. XavierCrighton, Neil H.M.Morris, Simon L.Werk, Jessica K.Theuns, TomPadilla, NelsonBielby, Rich M.Finn, Charles W.[Towards the statistical detection of the warm–hot intergalactic medium in intercluster filaments of the cosmic web]Towards the statistical detection of the warm–hot intergalactic medium in intercluster filaments of the cosmic web
Contreras Hantke, Sergio AntonioPadilla, NelsonLagos, C. D. P.[Angular momentum evolution in dark matter haloes: a study of the Bolshoi and Millennium simulations]Angular momentum evolution in dark matter haloes: a study of the Bolshoi and Millennium simulations
Paillas, EnriqueLagos, Claudia D. P.Padilla, NelsonTissera, Patricia[Baryon effects on void statistics in the EAGLE simulation]Baryon effects on void statistics in the EAGLE simulation
González Reyes, RobertoPrieto, JoaquinPadilla, NelsonJimenez, Raul[Relation between halo spin and cosmic-web filaments at z similar or equal to 3]Relation between halo spin and cosmic-web filaments at z similar or equal to 3

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