activity
20052018
most citedA catalog of visual-like morphologies in the 5 CANDELS fields using deep-learning

284 citations · 597 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2018★ 9 cited

Evolution of the anti-truncated stellar profiles of S0 galaxies since in the SHARDS survey: II - Structural and photometric evolution

Alejandro Borlaff, M. Carmen Eliche-Moral, John E. Beckman +7

Type-III S0 galaxies present tight scaling relations between their surface brightness photometric and structural parameters. Several evolutionary models have been proposed for the…

astro-ph.GA2015★ 284 cited

A catalog of visual-like morphologies in the 5 CANDELS fields using deep-learning

M. Huertas-Company, R. Gravet, G. Cabrera-Vives +12

We present a catalog of visual like H-band morphologies of galaxies () in the 5 CANDELS fields (GOODS-N, GOODS-S, UDS, EGS and COSMOS). Morphologies ar…

astro-ph.CO2010★ 35 cited

Improving the identification of high-z Herschel sources with position priors and optical/NIR and FIR/mm photometric redshifts

P. G. Pérez-González, E. Egami, M. Rex +36

We present preliminary results about the detection of high redshift (U)LIRGs in the Bullet cluster field by the PACS and SPIRE instruments within the Herschel Lensing Survey (HLS)…

astro-ph2006★ 100 cited

Why X-ray--Selected AGN Appear Optically Dull

J. R. Rigby, G. H. Rieke, J. L. Donley +2

We investigate why half of X-ray--selected active galactic nuclei (AGN) in deep surveys lack signs of accretion in their optical spectra. The majority of these ``optically--dull''…

astro-ph2005★ 145 cited

Unveiling a Population of X-ray Non-Detected AGN

J. L. Donley, G. H. Rieke, J. R. Rigby +1

We define a sample of 27 radio-excess AGN in the Chandra Deep Field North by selecting galaxies that do not obey the radio/infrared correlation for radio-quiet AGN and star-forming…

astro-ph2005★ 24 cited

Why Optically--Faint AGN Are Faint: The Spitzer Perspective

J. R. Rigby, G. H. Rieke, P. G. Perez-Gonzalez +5

Optically--faint X-ray sources (those with f_X/f_R > 10) constitute about 20% of X-ray sources in deep surveys, and are potentially highly obscured and/or at high redshift. Their f…