CALIFA, the Calar Alto Legacy Integral Field Area survey

F. Sánchez, S.; C. Kennicutt, Robert; Gil de Paz, A.; van de Ven, Glenn; M. Vı́lchez, J.; Wisotzki, L.; J. Walcher, C.; Mast, D.; A. L. Aguerri, J.; Albiol-Pérez, Sergio; Alonso‐Herrero, A.; Alves, J.; Bakos, J.; Bartáková, T.; Bland‐Hawthorn, Joss; Boselli, A.; J. Bomans, D.; Castillo-Morales, Á.; Cortijo-Ferrero, C.; de Lorenzo-Cáceres, A.; del Olmo, A.; Dettmar, R.‐J.; I. Díaz, Á.; Ellis, Simon; Falcón‐Barroso, J.; Flores, H.; Gallazzi, Anna; García‐Lorenzo, B.; M. González Delgado, R.; Gruel, N.; Haines, Tim; Hao, Cai-Na; Husemann, B.; Iglésias-Páramo, J.; Jahnkę, K.; D. Johnson, Benjamin; Jungwiert, B.; Kalinova, V.; Kehrig, C.; Kupko, D.; R. López-Sánchez, Á.; Lyubenova, M.; A. Marino, R.; Mármol-Queraltó, E.; Márquez, I.; Masegosa, J.; E. Meidt, Sharon; Méndez‐Abreu, J.; Monreal‐Ibero, A.; Montijo, C.

doi:10.1051/0004-6361/201117353

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CALIFA, the Calar Alto Legacy Integral Field Area survey

Shared by NobleBlocks on Nov 10, 2011 • 12:00 AM UTC

Authors:

S. F. Sánchez

Robert C. Kennicutt

A. Gil de Paz

Abstract

The final product of galaxy evolution through cosmic time is the population of galaxies in the local universe. These galaxies are also those that can be studied in most detail, thus providing a stringent benchmark for our understanding of galaxy evolution. Through the huge success of spectroscopic s...

Subject

Physics

Astrophysics

Field (mathematics)

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