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19992019
most citedThe [OII]3727 Luminosity Function of the Local Universe

54 citations · 225 across the 11 of their papers we have counts for

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astro-ph2008★ 11 cited

A maximum likelihood method for bidimensional experimental distributions, and its application to the galaxy merger fraction

C. López-Sanjuan, C. E. García-Dabó, M. Balcells

The determination of galaxy merger fraction of field galaxies using automatic morphological indices and photometric redshifts is affected by several biases if observational errors…

astro-ph2005★ 33 cited

GOYA Survey: U and B Number Counts in the Groth-Westphal Strip

M. C. Eliche-Moral, M. Balcells, M. Prieto +3

We present U and B galaxy differential number counts from a field of ~900 arcmin^2, based on GOYA Survey imaging of the HST Groth-Westphal strip. Source detection efficiency correc…

astro-ph2005★ 16 cited

The CIDA-UCM-Yale Shallow Survey for Emission Line Galaxies

A. Bongiovanni, G. Bruzual, G. Magris +4

We present the CIDA-UCM-Yale (Centro de Investigaciones de Astronomia, Universidad Complutense de Madrid and Yale University) survey for Halpha+[NII]6549,6584 emission-line galaxie…

astro-ph2002

Star Formation Rate estimators: [OII]3727 vs. Halpha for local star-forming galaxies

A. Aragon-Salamanca, A. Alonso-Herrero, J. Gallego +4

The [OII]3727 emission line is frequently used as an indicator of the star formation rate (SFR) despite its complex dependence on metallicity and excitation conditions. We have ana…

astro-ph2002★ 54 cited

The [OII]3727 Luminosity Function of the Local Universe

J. Gallego, C. E. Garcia-Dabo, J. Zamorano +2

The measurement of the Star Formation Rate density of the Universe is of prime importance in understanding the formation and evolution of galaxies. The [OII]3727 emission line flux…

astro-ph1999★ 27 cited

Survey for Emission-Line Galaxies: Universidad Complutense de Madrid List 3

O. Alonso, C. E. Garcia-Dabo, J. Zamorano +2

A new low-dispersion objective-prism search for low-redshift (z<0.045) emission-line galaxies (ELG) has been carried out by the Universidad Complutense de Madrid with the Schmidt T…