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Luminosity Functions beyond the spectroscopic limit. I. Method and near-infrared LFs in the HDF-N and HDF-S
Micol Bolzonella, Roser Pello', Dario Maccagni
We have developed a Monte Carlo method to compute the luminosity function of galaxies, based on photometric redshifts, which takes into account the non-gaussianity of the probabili…
Physical Properties of Low-Luminosity Galaxies at z ~ 2
M. Lemoine-Busserolle, T. Contini, R. Pello +3
We report the results obtained from ISAAC/VLT near-IR spectroscopy of two low-luminosity z ~ 1.9 galaxies located in the core of the lensing cluster AC114. The amplification factor…
Looking for the First Galaxies with EMIR/GTC
Roser Pello, Daniel Schaerer
The new Pop III models by Schaerer (2002) have been used to derive the observed properties of the first galaxies in terms of the expected magnitudes and colors. The dependence of t…