Context. The Sloan Digital Sky Survey (SDSS) and Wide-field Infrared Survey Explorer (WISE) provide information about the surface composition of about 100 000 minor planets. The resulting visible colors and albedos enabled us to group them in several major classes, which are a simplified view of the diversity shown by the few existing spectra. A large set of data in the 0.8−2.5 μm, where wide spectral features are expected, is required to refine and complement the global picture of these small bodies of the solar system. Aims. We aim to obtain the near-infrared colors for a large sample of solar system objects using the observations made during the VISTA-VHS survey. Methods. We performed a serendipitous search in VISTA-VHS o...
For faint asteroids, it is not practical to obtain near-infrared spectra. However, it may be possibl...
For faint asteroids, it is not practical to obtain near-infrared spectra. However, it may be possibl...
For faint asteroids, it is not practical to obtain near-infrared spectra. However, it may be possibl...
Context. The MOVIS catalog contains the largest set of near-infrared (NIR) colors for solar system o...
Context. The MOVIS catalog contains the largest set of near-infrared (NIR) colors for solar system o...
We present an update of the visible and near-infrared colour database of Minor Bodies in the Outer S...
The aim of this work is to study the compositional diversity of asteroid families based on their nea...
Context. The study of the surface properties of Centaurs and trans-Neptunian objects (TNOs) provide...
International audienceContext. The study of the surface properties of Centaurs and trans-Neptunian o...
We discuss optical colors of 10,592 asteroids with known orbits selected from a sample of 58,000 mov...
For faint asteroids, it is not practical to obtain near-infrared spectra. However, it may be possibl...
For faint asteroids, it is not practical to obtain near-infrared spectra. However, it may be possibl...
For faint asteroids, it is not practical to obtain near-infrared spectra. However, it may be possibl...
International audienceContext. The study of the surface properties of Centaurs and trans-Neptunian o...
Context. The Javalambre Photometric Local Universe Survey (J-PLUS) is an observational campaign that...
For faint asteroids, it is not practical to obtain near-infrared spectra. However, it may be possibl...
For faint asteroids, it is not practical to obtain near-infrared spectra. However, it may be possibl...
For faint asteroids, it is not practical to obtain near-infrared spectra. However, it may be possibl...
Context. The MOVIS catalog contains the largest set of near-infrared (NIR) colors for solar system o...
Context. The MOVIS catalog contains the largest set of near-infrared (NIR) colors for solar system o...
We present an update of the visible and near-infrared colour database of Minor Bodies in the Outer S...
The aim of this work is to study the compositional diversity of asteroid families based on their nea...
Context. The study of the surface properties of Centaurs and trans-Neptunian objects (TNOs) provide...
International audienceContext. The study of the surface properties of Centaurs and trans-Neptunian o...
We discuss optical colors of 10,592 asteroids with known orbits selected from a sample of 58,000 mov...
For faint asteroids, it is not practical to obtain near-infrared spectra. However, it may be possibl...
For faint asteroids, it is not practical to obtain near-infrared spectra. However, it may be possibl...
For faint asteroids, it is not practical to obtain near-infrared spectra. However, it may be possibl...
International audienceContext. The study of the surface properties of Centaurs and trans-Neptunian o...
Context. The Javalambre Photometric Local Universe Survey (J-PLUS) is an observational campaign that...
For faint asteroids, it is not practical to obtain near-infrared spectra. However, it may be possibl...
For faint asteroids, it is not practical to obtain near-infrared spectra. However, it may be possibl...
For faint asteroids, it is not practical to obtain near-infrared spectra. However, it may be possibl...