TY - GEN
T1 - Early type galaxies and structural parameters from ESO public survey KiDS
AU - Kids Collaboration
AU - Roy, N.
AU - Napolitano, N. R.
AU - La Barbera, F.
AU - Tortora, C.
AU - Getman, F.
AU - Radovich, M.
AU - Capaccioli, M.
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 - Cavuoti, Stefano
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
AU - Irisarri, Nancy
AU - Jakobs, Arthur
N1 - Publisher Copyright:
© Springer International Publishing Switzerland 2016.
PY - 2016
Y1 - 2016
N2 - The Kilo Degree survey (KiDS) is a large-scale optical imaging survey carried out with the VLT Survey Telescope (VST), which is the ideal tool for galaxy evolution studies.We expect to observemillions of galaxies for which we extract the structural parameters in four wavebands (u, g, r and i). This sample will represent the largest dataset with measured structural parameters up to a redshift z D 0:5. In this paper we will introduce the sample, and describe the 2D fitting procedure using the 2DPHOT environment and the validation of the parameters with an external catalog.
AB - The Kilo Degree survey (KiDS) is a large-scale optical imaging survey carried out with the VLT Survey Telescope (VST), which is the ideal tool for galaxy evolution studies.We expect to observemillions of galaxies for which we extract the structural parameters in four wavebands (u, g, r and i). This sample will represent the largest dataset with measured structural parameters up to a redshift z D 0:5. In this paper we will introduce the sample, and describe the 2D fitting procedure using the 2DPHOT environment and the validation of the parameters with an external catalog.
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U2 - 10.1007/978-3-319-19330-4_21
DO - 10.1007/978-3-319-19330-4_21
M3 - Conference contribution
AN - SCOPUS:84978983172
SN - 9783319193298
T3 - Astrophysics and Space Science Proceedings
SP - 135
EP - 138
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 -