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A. Gil de Paz

Researcher at Complutense University of Madrid

Publications -  210
Citations -  14408

A. Gil de Paz is an academic researcher from Complutense University of Madrid. The author has contributed to research in topics: Galaxy & Star formation. The author has an hindex of 56, co-authored 200 publications receiving 13290 citations. Previous affiliations of A. Gil de Paz include Carnegie Learning & Jet Propulsion Laboratory.

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Journal ArticleDOI

MEGARA-GTC stellar spectral library – II. MEGASTAR first release

TL;DR: The first release of the MEGASTAR catalogue is presented in this article, consisting of the spectra of 414 stars observed with R - 20 000 in the spectral intervals 6420-6790 A and 8370-8885 A, and obtained with a continuum average signal-to-noise ratio around 260.
Journal ArticleDOI

The First Gamma-ray Emitting BL Lacertae Object at the Cosmic Dawn

TL;DR: In this article, the authors reported the identification of the first high-gamma-ray emitting BL Lacertae object, 4FGL~J1219, beyond the first two billion years of the universe.
Proceedings ArticleDOI

MEGARA fiber bundles

TL;DR: MEGARA (Multi Espectrografo en GTC de Alta Resolucion para Astronomia) is the future optical Integral Field Unit (IFU) and Multi-Object Spectrograph (MOS) for the 10.4m Gran Telescopio CANARIAS (GTC) as mentioned in this paper.
Proceedings ArticleDOI

Cryostat and CCD for MEGARA at GTC

TL;DR: In this article, the authors describe the full preliminary design of the cryostat which will harbor the CCD detector for the MEGARA spectrograph, as well as all the vacuum and temperature sub-systems to operate it.
Proceedings ArticleDOI

VIENTOS: a feasibility study of innovative pupil systems for the new generation of instruments in the large telescopes

TL;DR: The VIENTOS project tries to identify the current scientific needs, to understand why some of them have not been fulfilled yet and to propose optomechanical solutions for these pupil elements that could produce a qualitative leap in the performance of the instruments to operate in the large telescopes.