During the post-AGB phase the dust shell detaches from the central star and dust temperatures varies between 100 and 200 K. In order to study the onset of photo...
The Onset of Star Formation in the Universe: Constraints from Nearby Isolated Dwarf Galaxies.
The details of the early star formation histories of tiny dwarf galaxies can shed light on the role in galaxy formation of the reionization which occured at...
The Open Cluster Chemical Abundances and Mapping (OCCAM) Survey: Galactic Gradients using SDSS-IV/DR13 and Gaia
The Open Cluster Chemical Analysis and Mapping (OCCAM) survey aims to produce a comprehensive, uniform, infrared-based data set forhundreds of open clusters...
The Open Cluster Chemical Abundances and Mapping (OCCAM) Survey: Overview and Membership Methods
The Open Cluster Chemical Analysis and Mapping (OCCAM) survey aims to produce a comprehensive, uniform, infrared-based data set for hundreds of open clusters...
The Open Cluster Chemical Abundances from Spanish Observatories survey (OCCASO)
We present the motivation, design and current status of the Open Cluster Chemical Abundances from Spanish Observatories survey (OCCASO). Using the high...
The Open Cluster Chemical Abundances from Spanish Observatories Survey (OCCASO)
We present the motivation, design and current status of the Open Cluster Chemical Abundances from Spanish Observatories survey (OCCASO). Using the high...
The optical AIV of the infrared multi-slit spectrophotometer for GTC, EMIR
EMIR is a second generation GTC instrument. EMIR's external structure is a huge cylindrical vacuum chamber of 2.2m length and 1.8m in diameter with a weight of...
The optical counterpart of the accreting millisecond X-ray pulsar IGR J17498-2921
We report the optical detection of a faint star consistent with the known position of the 401 Hz transient accreting millisecond X-ray pulsar IGR J17498-2921...