activity
20112018
most citedTesting the chemical tagging technique with open clusters

72 citations · 115 across the 5 of their papers we have counts for

collaborators

12 papers

astro-ph.GA2018

J-PLUS: measuring emission line fluxes in the nearby universe

R. Logroño-García, G. Vilella-Rojo, C. López-Sanjuan +29

In the present paper we aim to validate a methodology designed to extract the Halpha emission line flux from J-PLUS photometric data. J-PLUS is a multi narrow-band filter survey ca…

astro-ph.GA2018

J-PLUS: A wide-field multi-band study of the M15 globular cluster. Evidence of multiple stellar populations in the RGB

Charles Bonatto, Ana L. Chies-Santos, Paula R. T. Coelho +21

The Javalambre Photometric Local Universe Survey (J-PLUS) provides wide field-of-view images in 12 narrow, intermediate and broad-band filters optimized for stellar photometry. Her…

astro-ph.GA2018

J-PLUS: 2-D analysis of the stellar population in NGC 5473 and NGC 5485

I. San Roman, P. Sánchez-Blázquez, A. J. Cenarro +23

The spatial variations of stellar population properties within a galaxy are intimately related to their formation process. Therefore, spatially resolved studies of galaxies are ess…

astro-ph.GA2018

J-PLUS: Morphological star/galaxy classification by PDF analysis

C. López-Sanjuan, H. Vázquez Ramió, J. Varela +29

Our goal is to morphologically classify the sources identified in the images of the J-PLUS early data release (EDR) into compact (stars) or extended (galaxies) using a suited Bayes…

astro-ph.GA2018

J-PLUS: The Javalambre Photometric Local Universe Survey

A. J. Cenarro, M. Moles, D. Cristóbal-Hornillos +119

J-PLUS is an ongoing 12-band photometric optical survey, observing thousands of square degrees of the Northern hemisphere from the dedicated JAST/T80 telescope at the Observatorio…

astro-ph.GA2018

Stellar populations of galaxies in the ALHAMBRA survey up to . III. The stellar content of the quiescent galaxy population during the last Gyr

L. A. Díaz-García, A. J. Cenarro, C. López-Sanjuan +27

We aim at constraining the stellar population properties of quiescent galaxies. These properties reveal how these galaxies evolved and assembled since up to the present ti…