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Data reduction and astrometry strategies for wide-field images: an application to the Capodimonte Deep Field
Free accessArXiv | 2002| -
THE STELLAR MASS FUNCTION OF GALAXIES TO z ∼ 5 IN THE FORS DEEP AND GOODS-SOUTH FIELDS
British Library Online Contents | 2005| -
Predicting emission line fluxes and number counts of distant galaxies for cosmological surveys
Free accessArXiv | 2017| -
The supermassive black hole in NGC 4486a detected with SINFONI at the Very Large Telescope
British Library Online Contents | 2007| -
Predicting emission line fluxes and number counts of distant galaxies for cosmological surveys
Free accessBASE | 2017|Contributors: Pannella, M. -
The main sequence of star forming galaxies I. The local relation and its bending
Free accessArXiv | 2018| -
GOODS-Herschel:dust attenuation properties of UV selected high redshift galaxies
Free accessArXiv | 2012| -
GOODS-Herschel: dust attenuation properties of UV selected high redshift galaxies⋆
Free accessEDP Sciences | 2012| -
GOODS-Herschel: dust attenuation properties of UV selected high redshift galaxies
British Library Online Contents | 2012| -
The main sequence of star-forming galaxies – I. The local relation and its bending
Free accessBASE | 2019| -
Dust and gas in luminous proto-cluster galaxies at z = 4.05: the case for different cosmic dust evolution in normal and starburst galaxies
British Library Online Contents | 2014| -
Dark matter content and internal dynamics of NGC 4697:nmagic particle models from slit data and planetary nebula velocities
British Library Online Contents | 2008| -
Satellite content and quenching of star formation in galaxy groups at z ~ 1.8
British Library Online Contents | 2015| -
The main sequence of star forming galaxies II. A non evolving slope at the high mass end
Free accessArXiv | 2019|
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