TY - GEN
T1 - Galaxy evolutionwithin the kilo-degree survey
AU - Kids Collaboration
AU - Tortora, C.
AU - Napolitano, N. R.
AU - La Barbera, F.
AU - Roy, N.
AU - Radovich, M.
AU - Getman, F.
AU - Brescia, M.
AU - Cavuoti, Stefano
AU - Capaccioli, M.
AU - Longo, G.
AU - Amaro, Valeria
AU - Amon, Alexandra
AU - Applegate, Douglas
AU - Asgari, Marika
AU - Begeman, Kor
AU - Belikov, Andrey
AU - Bilicki, Maciej
AU - Blake, Chris
AU - Eriksen, Martin Borstad
AU - Boxhoorn, Danny
AU - Brescia, Massimo
AU - Brouwer, Margot
AU - Buddelmeijer, Hugo
AU - Buddendiek, Axel
AU - Cacciato, Marcello
AU - Cai, Yanchuan
AU - Capaccioli, Massimo
AU - Chisari, Elisa
AU - Choi, Ami
AU - Cordes, Oliver Mark
AU - Covone, Giovanni
AU - Dall’Ora, Massimo
AU - de Jong, Jelte
AU - Dvornik, Andrej
AU - Edge, Alastair
AU - Erben, Thomas
AU - Conti, Ian Fenech
AU - Franse, Jeroen
AU - Georgiou, Christos
AU - Getman, Fedor
AU - Giblin, Benjamin
AU - Grado, Aniello
AU - Harnois-Déraps, Joachim
AU - Helmich, Ewout
AU - Herbonnet, Ricardo
AU - Heymans, Catherine
AU - Hildebrandt, Hendrik
AU - Hoekstra, Henk
AU - Hojjati, Alireza
AU - Huang, Zhuoyi
N1 - Publisher Copyright:
© Springer International Publishing Switzerland 2016.
PY - 2016/1/1
Y1 - 2016/1/1
N2 - The ESO Public Kilo-Degree Survey (KiDS) is an optical wide-field imaging survey carried out with the VLT Survey Telescope and the OmegaCAM camera. KiDS will scan 1,500 deg2in four optical filters (u, g, r, i). Designed to be a weak lensing survey, it is ideal for galaxy evolution studies, thanks to the high spatial resolution of VST, the excellent seeing and the photometric depth. The surface photometry has provided with structural parameters (e.g. size and Sérsic index), aperture and total magnitudes have been used to obtain photometric redshifts from Machine Learning methods and stellar masses/luminositites from stellar population synthesis. Our project aimed at investigating the evolution of the colour and structural properties of galaxies with mass and environment up to redshift z ~ 0:5 and more, to put constraints on galaxy evolution processes, as galaxy mergers.
AB - The ESO Public Kilo-Degree Survey (KiDS) is an optical wide-field imaging survey carried out with the VLT Survey Telescope and the OmegaCAM camera. KiDS will scan 1,500 deg2in four optical filters (u, g, r, i). Designed to be a weak lensing survey, it is ideal for galaxy evolution studies, thanks to the high spatial resolution of VST, the excellent seeing and the photometric depth. The surface photometry has provided with structural parameters (e.g. size and Sérsic index), aperture and total magnitudes have been used to obtain photometric redshifts from Machine Learning methods and stellar masses/luminositites from stellar population synthesis. Our project aimed at investigating the evolution of the colour and structural properties of galaxies with mass and environment up to redshift z ~ 0:5 and more, to put constraints on galaxy evolution processes, as galaxy mergers.
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U2 - 10.1007/978-3-319-19330-4_19
DO - 10.1007/978-3-319-19330-4_19
M3 - Conference contribution
AN - SCOPUS:84978945733
SN - 9783319193298
T3 - Astrophysics and Space Science Proceedings
SP - 123
EP - 128
BT - The Universe of Digital Sky Surveys - A Meeting to Honour the 70th Birthday of Massimo Capaccioli
A2 - Napolitano, Nicola R.
A2 - Marconi, Marcella
A2 - Iodice, Enrichetta
A2 - Longo, Giuseppe
A2 - Paolillo, Maurizio
PB - Springer Science and Business Media B.V.
T2 - Conference on Universe of Digital Sky Surveys, 2014
Y2 - 25 November 2014 through 28 November 2014
ER -