Herschel far-IR counterparts of SDSS galaxies: analysis of commonly used star formation rate estimates
We study a hundred of galaxies from the spectroscopic Sloan Digital Sky Survey (SDSS) with individual detections in the far-infrared Herschel Photodetector Array Camera and Spectrometer bands (100 or 160 μm) and in the GALEX far-ultraviolet band up to z ˜ 0.4 in the COSMOS and Lockman Hole fields. The galaxies are divided into four spectral and
Domínguez Sánchez, H. et al.
Fecha de publicación:
6
2014