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...
The IACOB spectroscopic database of Northern Galactic OB stars
We present the IACOB spectroscopic database, an homogeneous set of high quality, high resolution spectra of Galactic O- and B-type stars obtained with the FIES...
The IACOB spectroscopic database. New interface and second data release
After almost 12 years gathering data with the 2.56-m Nordic Optical Telescope and the 1.2-m Mercator telescope, the IACOB project has broken the record of...
The IACOB spectroscopic database: recent updates and first data release
The IACOB project is an ambitious long-term project which is contributing to step forward in our knowledge about the physical properties and evolution of...