In this contribution I describe the main characteristics of the inversion codes developed at the Instituto de Astrofísica de Canarias for the analisys of Stokes...
We present new deep co-adds of data taken within Stripe 82 of the Sloan Digital Sky Survey (SDSS), especially stacked to reach the faintest surface brightness...
The IAC Stripe82 Legacy Survey: Improved Sky-rectified Images
The IAC Stripe 82 Legacy Survey is a new co-addition of the SDSS Stripe 82 data (Abazajian et al. 2009), especially reduced to preserve the faintest surface...
Here we report the main characteristics of the recently acquired near infrared camera. It is based on a 256x256 HgCdTe Nicmos-3 array, sensitive from 1 mu m to...
The IACOB project: A grid-based automatic tool for the quantitative spectroscopic analysis of O-stars
We present the IACOB grid-based automatic tool for the quantitative spectroscopic analysis of O-stars. The tool consists of an extensive grid of FASTWIND models...
The IACOB project: Hunting for spectroscopic binaries in the OB supergiant domain. The pulsational variability menace
A large percentage of massive stars are born as part of binary or multiple systems. This statement, which has been defended by some authors during the last 3...
The IACOB project: searching for empirical signatures of binarity in fast-rotating Galactic O stars and B supergiants
Rotation is one of the important parameters affecting the evolution and final fate of massive stars. Still the origin of fast- rotating stars in the massive OB...
The IACOB spectroscopic survey of Galactic OB stars is an ambitious observational project aimed at compiling a large, homogeneous, high-resolution database of...
The IACOB spectroscopic database of galactic OB stars
We present the IACOB spectroscopic database, the largest homogeneous database of high-resolution, high signal-to-noise ratio spectra of Northern Galactic OB...