734 citations · 1.5k across the 8 of their papers we have counts for
13 papers
Improving resolution and depth of astronomical observations via modern mathematical methods for image analysis
Marco Castellano, Daniele Ottaviani, Adriano Fontana +3
In the past years modern mathematical methods for image analysis have led to a revolution in many fields, from computer vision to scientific imaging. However, some recently develop…
Stellar masses from the CANDELS survey: the GOODS-South and UDS fields
P. Santini, H. C. Ferguson, A. Fontana +35
We present the public release of the stellar mass catalogs for the GOODS-S and UDS fields obtained using some of the deepest near-IR images available, achieved as part of the Cosmi…
The galaxy stellar mass function at 3.5<z<7.5 in the CANDELS/UDS, GOODS-South, and HUDF fields
A. Grazian, A. Fontana, P. Santini +38
The galaxy stellar mass function (GSMF) at high-z provides key information on star-formation history and mass assembly in the young Universe. We aimed to use the unique combination…
The Evolution of the Galaxy Rest-Frame Ultraviolet Luminosity Function Over the First Two Billion Years
Steven L. Finkelstein, Russell E. Ryan, Casey Papovich +26
We present a robust measurement and analysis of the rest-frame ultraviolet (UV) luminosity function at z=4-8. We use deep Hubble Space Telescope imaging over the CANDELS/GOODS fiel…
The Hawk-I UDS and GOODS Survey (HUGS): Survey design and deep K-band number counts
A. Fontana, J. S. Dunlop, D. Paris +40
We present the results of a new, ultra-deep, near-infrared imaging survey executed with the Hawk-I imager at the ESO VLT, of which we make all the data public. This survey, named H…
Ultra-faint high-redshift galaxies in the Frontier Fields
Bin Yue, Andrea Ferrara, Eros Vanzella +1
By combining cosmological simulations with Frontier Fields project lens models we find that, in the most optimistic case, galaxies as faint as (AB magnitude at…