Accès ouvert
2025
article
OpenAlex
Khalid Barkaoui, J. Korth, E. Gaidos, E. Agol et autres
TOI-2015 is a known exoplanetary system around an M4 dwarf star, consisting of a transiting sub-Neptune planet in a 3.35-day orbital period, TOI-2015 b, accompanied by a non-transiting companion, TOI-2015 c. High-precision radial-velocity measurements were taken with the MAROON-X spectrograph, and high-precision …
us, be, es, se, at, jp, ch, it, cl, de, tr, au, fr, gb, Maroc, mx, nl, gr
(code pays fourni par la source)
Accès ouvert
2025
preprint
OpenAlex
Khalid Barkaoui, J. Korth, E. Gaidos, E. Agol et autres
TOI-2015 is a known exoplanetary system around an M4 dwarf star, consisting of a transiting sub-Neptune planet in a 3.35-day orbital period, TOI-2015b, accompanied by a non-transiting companion, TOI-2015c. High-precision RV measurements were taken with the MAROON-X spectrograph, and high-precision photometric data …
2016
article
OpenAlex
Esther Jódar, A. Pérez‐Garrido, A. Díaz‐Sánchez, Isidro Villó-Pérez et autres
Accès ouvert
2015
preprint
OpenAlex
S. Simón‐Díaz, I. Negueruela, J. Maíz Apellániz, N. Castro et autres
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 Galactic massive stars. The project aims at building a large database of high-resolution, multi-epoch, spectra of Galactic OB …
es
(code pays fourni par la source)
Accès ouvert
2015
article
OpenAlex
S. Simón‐Díaz, I. Negueruela, J. Maíz Apellániz, N. Castro et autres
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 Galactic massive stars. The project aims at building a large database of high-resolution, multi-epoch, spectra of Galactic OB …
es
(code pays fourni par la source)
2015
article
OpenAlex
Jonathan Crass, Craig Mackay, David L. King, R. Rébolo et autres
Accès ouvert
2014
article
OpenAlex
Miguel A. Cágigas, Pedro J. Valle, Manuel P. Cagigal, Xesús Prieto-Blanco et autres
We show that the use of apodizing functions at the coronagraph Lyot plane may be useful for improving the image contrast of ground-based coronagraphs. An experimental set-up consisting of a tip–tilt mirror, a coronagraph and a low-noise EMCCD camera was implemented at …
es
(code pays fourni par la source)
2013
article
OpenAlex
A. Díaz‐Sánchez, A. Pérez‐Garrido, Isidro Villó-Pérez, R. Rébolo et autres
2012
article
OpenAlex
Esther Jódar, A. Pérez‐Garrido, A. Díaz‐Sánchez, Isidro Villó-Pérez et autres
We present high-angular-resolution optical I-band imaging of 451 late K to mid-M nearby stars. These observations have been performed with Astralux and FastCam using the lucky imaging technique. We found 70 companions with separations between 0.1 and 3.5 arcsec, out of which …
es
(code pays fourni par la source)
2011
article
OpenAlex
Lucas Labadie, R. Rébolo, Isidro Villó-Pérez, J. A. Pérez-Prieto et autres
High contrast imaging at optical wavelengths is limited by the modest correction of conventional near-IR optimized AO systems.We take advantage of new fast and low-readout-noise detectors to explore the potential of fast imaging coupled to post-processing techniques to detect faint companions to …
es, fr, de
(code pays fourni par la source)
2011
preprint
OpenAlex
Bruno Femenía, R. Rébolo, J. A. Pérez-Prieto, Lucas Labadie et autres
The potential of combining Adaptive Optics (AO) and Lucky Imaging (LI) to achieve high precision astrometry and differential photometry in the optical is investigated by conducting observations of the close 0. ′′ 1 brown dwarf binary GJ569Bab.We took 50000 I-band images with …
es, fr, de
(code pays fourni par la source)
Accès ouvert
2010
conference-paper
OpenAlex
Lucas Labadie, R. Rébolo, Bruno Femenía, Isidro Villó-Pérez et autres
In this paper, we present an original observational approach, which combines, for the first time, traditional speckle imaging with image post-processing to obtain in the optical domain diffraction-limited images with high contrast (10-5) within 0.5 to 2 arcseconds around a bright star. …
es, fr, de
(code pays fourni par la source)