The inner mass distribution of late-type spiral galaxies from <monospace>SAURON</monospace> stellar kinematic maps
We infer the central mass distributions within 0.4-1.2 disc scalelengths of 18 late-type spiral galaxies using two different dynamical modelling approaches -...
The Instituto Astrofisica de Canarias-Bartol Cosmic Microwave Background Anisotropy Experiment: Results of the 1994 Campaign
We present the results of a cosmic microwave background (CMB) anisotropy ground-based millimetric experiment sensitive to fluctuations on angular scales of ~2...
The INTEGRAL IBIS/ISGRI System Point Spread Function and Source Location Accuracy
The imager on board INTEGRAL (IBIS) presently provides the most detailed sky images ever obtained at energies above 30 keV. The telescope is based on a coded...
The integrated magnetic field of the Sun as seen by GOLF on board SOHO
An objective of the GOLF experiment (Global Oscillations at Low Frequencies) on-board the SOHO (Solar and Heliospheric Observatory) space mission was to measure...
The intracluster light as a tracer of the total matter density distribution: a view from simulations
By using deep observations of clusters of galaxies, it has been recently found that the projected stellar mass density closely follows the projected total (dark...
The J-PAS survey: The effect of photometric redshift errors on cosmic voids
Aims. We investigated the impact of photometric redshift errors in the ongoing Javalambre Physics of the Accelerating Universe Astrophysical Survey (J-PAS) on...
The Large Magellanic Cloud stellar content with SMASH. I. Assessing the stability of the Magellanic spiral arms
The Large Magellanic Cloud (LMC) is the closest and most studied example of an irregular galaxy. Among its principal defining morphological features, its off...
The LARI Method for ISO-CAM/PHOT Data Reduction and Analysis
The techniques and software tools developed for the reduction and analysis of ISO-CAM/PHOT data with the LARI method are presented together with some highlights...