TY  - JOUR
AU  - Catalán Torrecilla, Cristina
AU  - Gil De Paz, Armando
AU  - Castillo Morales, María África
AU  - Pérez González, Pablo Guillermo
AU  - Marino, Raffaella Anna
PY  - 2015
DO  - 10.1051/0004-6361/201526023
SN  - 1432-0746
UR  - https://hdl.handle.net/20.500.14352/24349
T2  - Astronomy & Astrophysics
AB  - Context. The star formation rate (SFR) is one of the main parameters used to analyze the evolution of galaxies through time. The need for recovering the light reprocessed by dust commonly requires the use of low spatial resolution far-infrared data....
LA  - eng
PB  - EDP Sciencies
KW  - Integral field spectroscopy
KW  - Luminous infrared galaxies
KW  - Potsdam multiaperture spectrophotometer
KW  - Formation rate indicators
KW  - Similar-to 2
KW  - Forming galaxies
KW  - Nearby galaxies
KW  - Formation history
KW  - Formation rates
KW  - Dust attenuation
TI  - Star formation in the local Universe from the CALIFA sample. I. Calibrating the SFR using IFS data
TY  - journal article
VL  - 584
ER  -