activity
20132026
most citedOverview of the Instrumentation for the Dark Energy Spectroscopic Instrument

465 citations · 2k across the 125 of their papers we have counts for

collaborators
Showing 2022Show all

12 papers · 1 filter

astro-ph.GA2022★ 54 cited

Overmassive black holes in dwarf galaxies out to z0.9 in the VIPERS survey

M. Mezcua, M. Siudek, H. Suh +3

Supermassive black holes (SMBHs) are thought to originate from early Universe seed black holes of mass -10 M and grown through cosmic time. S…

astro-ph.GA2022★ 10 cited

DESI Survey Validation Spectra Reveal an Increasing Fraction of Recently Quenched Galaxies at

David J. Setton, Biprateep Dey, Gourav Khullar +24

We utilize bright Luminous Red Galaxies (LRGs) from the novel Dark Energy Spectroscopic Instrument Survey Validation spectroscopic sample, leveraging its deep ($\sim2.5…

astro-ph.GA2022★ 26 cited

DEVILS: Cosmic evolution of SED-derived metallicities and their connection to star-formation histories

Jessica E. Thorne, Aaron S. G. Robotham, Sabine Bellstedt +6

Gas-phase metallicities of galaxies are typically measured through auroral or nebular emission lines, but metallicity also leaves an imprint on the overall spectral energy distribu…

astro-ph.GA2022★ 25 cited

The environment of AGN dwarf galaxies at z0.7 from the VIPERS survey

M. Siudek, M. Mezcua, J. Krywult

Dwarf galaxies are ideal laboratories to study the relationship between the environment and AGN activity. However, the type of environments in which dwarf galaxies hosting AGN resi…

astro-ph.GA2022★ 11 cited

Lessons Learned from the Two Largest Galaxy Morphological Classification Catalogues built by Convolutional Neural Networks

Ting-Yun Cheng, H. Domínguez Sánchez, J. Vega-Ferrero +54

We compare the two largest galaxy morphology catalogues, which separate early and late type galaxies at intermediate redshift. The two catalogues were built by applying supervised…

astro-ph.IM2022

The PAU Survey & Euclid: Improving broad-band photometric redshifts with multi-task learning

L. Cabayol, M. Eriksen, J. Carretero +123

Current and future imaging surveys require photometric redshifts (photo-zs) to be estimated for millions of galaxies. Improving the photo-z quality is a major challenge but is need…