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20032019
most citedEmpirical calibration of the near-IR CaII triplet - IV. The stellar population synthesis models

188 citations · 338 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2019★ 51 cited

The Fornax 3D project: Thick disks in a cluster environment

F. Pinna, J. Falcón-Barroso, M. Martig +13

We used deep MUSE observations to perform a stellar-kinematic and population analysis of FCC 153 and FCC 177, two edge-on S0 galaxies in the Fornax cluster. The geometrical definit…

astro-ph.SR2015★ 1 cited

Estimating the magnetic field strength from magnetograms

A. Asensio Ramos, M. J. Martinez Gonzalez, R. Manso Sainz

A properly calibrated longitudinal magnetograph is an instrument that measures circular polarization and gives an estimation of the magnetic flux density in each observed resolutio…

astro-ph2007★ 15 cited

Search for photospheric footpoints of quiet Sun transition region loops

J. Sanchez Almeida, L. Teriaca, P. Suetterlin +3

CONTEXT:The footpoints of quiet Sun Transition Region (TR) loops do not seem to coincide with the photospheric magnetic structures appearing in traditional low-sensitivity magnetog…

astro-ph2007★ 52 cited

A Morphological and Statistical Analysis of Ansae in Barred Galaxies

I. Martinez-Valpuesta, J. H. Knapen, R. Buta

Many barred galaxies show a set of symmetric enhancements at the ends of the stellar bar, called {\it ansae}, or the ``handles'' of the bar. The ansa bars have been in the literatu…

astro-ph2005★ 31 cited

ULTRACAM observations of the black hole X-ray transient XTE J1118+480 in quiescence

T. Shahbaz, V. S. Dhillon, T. R. Marsh +5

We present high time-resolution multicolour observations of the quiescent soft X-ray transient XTE J1118+480 obtained with ULTRACAM. Superimposed on the double-humped continuum g'…

astro-ph2003★ 188 cited

Empirical calibration of the near-IR CaII triplet - IV. The stellar population synthesis models

A. Vazdekis, A. J. Cenarro, J. Gorgas +2

We present a new stellar population synthesis model, which predicts SEDs for single-age single-metallicity stellar populations, SSPs, at resolution 1.5A (FWHM) in the spectral regi…