activity
20062026
most citedStellar populations of galaxies in the ALHAMBRA survey up to . I. MUFFIT: A Multi-Filter Fitting code for stellar population diagnostics

24 citations · 62 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.GA2026★ 1 cited

PKS 2155-304: Long-Term Optical Photometric Monitoring and Variability Analysis

J. L. Weiss, I. Andruchow, E. J. Marchesini +6

Through the detailed study of the optical flux behaviour in blazars over time, it is possible to infer the conditions responsible for their observed emission. PKS 2155-304, a BL La…

astro-ph.GA2016★ 20 cited

The ALHAMBRA survey : band luminosity function of quiescent and star-forming galaxies at by PDF analysis

C. López-Sanjuan, E. Tempel, N. Benítez +34

Our goal is to study the evolution of the band luminosity function (LF) since using ALHAMBRA data. We used the photometric redshift and the band selection magnitude p…

astro-ph.GA2015★ 12 cited

The ALHAMBRA survey : Estimation of the clustering signal encoded in the cosmic variance

C. López-Sanjuan, A. J. Cenarro, C. Hernández-Monteagudo +30

The relative cosmic variance () is a fundamental source of uncertainty in pencil-beam surveys and, as a particular case of count-in-cell statistics, can be used to estimate th…

astro-ph.GA2015★ 24 cited

Stellar populations of galaxies in the ALHAMBRA survey up to . I. MUFFIT: A Multi-Filter Fitting code for stellar population diagnostics

L. A. Díaz-García, A. J. Cenarro, C. López-Sanjuan +29

We present MUFFIT, a new generic code optimized to retrieve the main stellar population parameters of galaxies in photometric multi-filter surveys, and we check its reliability and…

astro-ph2006★ 5 cited

The scaling relation of early-type galaxies in clusters. II: Spectroscopic data for galaxies in eight nearby clusters

D. Bettoni, M. Moles, P. Kjaergaard +2

AIMS: We present in this work low and intermediate resolution spectroscopic data collected for 152 early type galaxies in 8 nearby clusters with z 0.10. METHODS: We use low…