activity
20172020
most citedMajor Merging History in CANDELS. I. Evolution of the Incidence of Massive Galaxy-Galaxy Pairs from z=3 to z~0

88 citations · 152 across the 2 of their papers we have counts for

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8 papers · 1 filter

astro-ph.GA2020

The emergence of passive galaxies in the early Universe

P. Santini, M. Castellano, E. Merlin +10

The emergence of passive galaxies in the early Universe results from the interplay among the processes responsible for their rapid assembly and for the abrupt shut-down of their SF…

astro-ph.GA201964 cited

Large Scale Structures in the CANDELS Fields: The Role of the Environment in Star Formation Activity

Nima Chartab, Bahram Mobasher, Behnam Darvish +14

We present a robust method, weighted von Mises kernel density estimation, along with boundary correction to reconstruct the underlying number density field of galaxies. We apply th…

astro-ph.GA2019

The space densities and emissivities of AGNs at

E. Giallongo, A. Grazian, F. Fiore +11

The study of the space density of bright AGNs at has been subject to extensive effort given its importance for the estimate of the cosmological ionizing emissivity and growth…

astro-ph.GA2019

The CANDELS/SHARDS multi-wavelength catalog in GOODS-N: Photometry, Photometric Redshifts, Stellar Masses, Emission line fluxes and Star Formation Rates

Guillermo Barro, Pablo G. Perez-Gonzalez, Antonio Cava +52

We present a WFC3 F160W (-band) selected catalog in the CANDELS/GOODS-N field containing photometry from the ultraviolet (UV) to the far-infrared (IR), photometric redshifts and…

astro-ph.GA2019

Can intrinsic alignments of elongated low-mass galaxies be used to map the cosmic web at high redshift?

Viraj Pandya, Joel Primack, Peter Behroozi +13

Hubble Space Telescope observations show that low-mass () galaxies at high redshift () tend to be elongated (prolate) rather than disky (oblat…

astro-ph.GA2018

Galaxy inclination and the IRX-beta relation: Effects on UV star-formation rate measurements at intermediate to high redshifts

Weichen Wang, Susan A. Kassin, Camilla Pacifici +11

At intermediate and high redshifts, measurements of galaxy star-formation rates are usually based on rest-frame ultraviolet (UV) data. A correction for dust attenuation, A_UV, is n…