activity
20102023
most citedA comparison between the soft X-ray and [O III] morphologies of active galactic nuclei

24 citations · 40 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.GA2023★ 1 cited

COALAS II. Extended molecular gas reservoirs are common in a distant, forming galaxy cluster

Zhengyi Chen, Helmut Dannerbauer, Matthew Lehnert +24

This paper presents the results of 475 hours of interferometric observations with the Australia Telescope Compact Array towards the Spiderweb protocluster at \(z=2.16\). We search…

astro-ph.GA2023★ 1 cited

The PAU Survey: Classifying low-z SEDs using Machine Learning clustering

A. L. González-Morán, P. Arrabal Haro, C. Muñóz-Tuñón +15

We present an application of unsupervised Machine Learning Clustering to the PAU Survey of galaxy spectral energy distribution (SED) within the COSMOS field. The clustering algorit…

astro-ph.GA2017★ 24 cited

A comparison between the soft X-ray and [O III] morphologies of active galactic nuclei

Carlos Gómez-Guijarro, Omaira González-Martín, Cristina Ramos Almeida +2

Several studies of nearby active galactic nuclei (AGN) have shown that the soft X-ray emission presents a size and morphology that resembles that of the narrow-line region (NLR) tr…

astro-ph.GA2015★ 13 cited

GLACE survey: OSIRIS/GTC Tuneable Filter H imaging of the rich galaxy cluster ZwCl 0024.0+1652 at z = 0.395. Part I -- Survey presentation, TF data reduction techniques and catalogue

Miguel Sánchez-Portal, Irene Pintos-Castro, Ricardo Pérez-Martínez +35

The cores of clusters at 0 z 1 are dominated by quiescent early-type galaxies, whereas the field is dominated by star-forming late-type ones. Galaxy propertie…

astro-ph.CO2010★ 1 cited

The GaLAxy Cluster Evolution Survey (GLACE): introduction and first results

M. Sánchez-Portal, J. Cepa, I. Pintos-Castro +27

Aimed at understanding the evolution of galaxies in clusters, the GLACE survey is mapping a set of optical lines ([OII]3727, [OIII]5007, Hbeta and Halpha/[NII] when possible) in se…