We present CCD photometry in the Washington-system C and T1 passbands down to T1 ~ 22.5 mag in the fields of NGC 1697, SL 133, NGC 1997, SL 663, and OHSC 28...
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PublicationWashington photometry of five star clusters in the Large Magellanic Cloud
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PublicationWASP-127b: a misaligned planet with a partly cloudy atmosphere and tenuous sodium signature seen by ESPRESSO
Context. The study of exoplanet atmospheres is essential for understanding the formation, evolution, and composition of exoplanets. The transmission...
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PublicationWASP-92b, WASP-93b and WASP-118b: three new transiting close-in giant planets
We present the discovery of three new transiting giant planets, first detected with the WASP telescopes, and establish their planetary nature with follow up...
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PublicationWater vapor detection in the transmission spectra of HD 209458 b with the CARMENES NIR channel
Aims: We aim at detecting water vapor in the atmosphere of the hot Jupiter HD 209458 b and perform a multi-band study in the near infrared with CARMENES...
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PublicationWave Propagation and Shock Formation in Different Magnetic Structures
Velocity oscillations "measured" simultaneously at the photosphere and the chromosphere—from time series of spectropolarimetric data in the 10830 Å region—of...
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PublicationWhat do galaxies look like beyond 31 mag/arcsec2?
Detection of optical surface brightness structures with magnitudes fainter than 30 mag/arcsec2 has remained elusive in current photometric deep surveys. We are...
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PublicationWhat drives the variance of galaxy spectra?
We present a study aimed at understanding the physical phenomena underlying the formation and evolution of galaxies following a data-driven analysis of...
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PublicationWhen the horseshoe fits: Characterizing 2023 FY<SUB>3</SUB> with the 10.4 m Gran Telescopio Canarias and the Two-meter Twin Telescope
Context. The Arjuna asteroid belt is loosely defined as a diverse group of small asteroids that follow dynamically cold, Earth-like orbits. Most of them are not...
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PublicationWhere are the solar magnetic poles?
Regardless of the physical origin of stellar magnetic fields - fossil or dynamo induced - an inclination angle between the magnetic and rotation axes is very...