We report here the main characteristics of a near IR camera devoted to astrophysical solar research, which has been developed by the Instituto de Astrofisica de Canarias (IAC). The system is now being used for photometric and spectroscopic applications, and it will also be used for spectropolarimetry in the near future. The first application is
Esta sección ofrece el acceso a la base de datos de Publicaciones que recopila los artículos del IAC publicados en revistas científicas. Por favor, pulsa la flecha del menú para ver todas las opciones de búsqueda y de ordenación de resultados; autor, revista, año, etc..
Además ofrece acceso al repositorio de preprints del IAC: https://research.iac.es/preprints/l
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Near-infrared camera for solar research: a photometric applicationReyes, Marcos et al.91998
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Near-Infrared Images in the Herbig-Haro 1-2 and 3 Regions
Not Available
Roth, M. et al.Fecha de publicación:
91989 -
Near-infrared images in the Herbig-Haro 1-2 and 3 regions.
Not Available
Roth, M. et al.Fecha de publicación:
91989 -
Near-infrared low-resolution spectroscopy of Pleiades L-type brown dwarfs
Context. The fundamental properties of brown dwarfs evolve with age. Models describing the evolution of luminosities and effective temperatures, among other physical parameters, can be empirically constrained using brown dwarfs of various masses in star clusters of well-determined age and metallicity. Aims: We aim to carry out a spectroscopic and
Bihain, G. et al.Fecha de publicación:
92010 -
Near-InfraRed Planet Searcher to Join HARPS on the ESO 3.6-metre Telescope
The Near-InfraRed Planet Searcher (NIRPS) is a new ultra-stable infrared (YJH) spectrograph that will be installed on ESO's 3.6-metre Telescope in La Silla, Chile. Aiming to achieve a precision of 1 m s-1, NIRPS is designed to find rocky planets orbiting M dwarfs, and will operate together with the High Accuracy Radial velocity Planet Searcher
Bouchy, F. et al.Fecha de publicación:
92017 -
Near-infrared polarimetric adaptive optics observations of NGC 1068: a torus created by a hydromagnetic outflow wind
We present J' and K' imaging linear polarimetric adaptive optics observations of NGC 1068 using MMT-Pol on the 6.5-m MMT. These observations allow us to study the torus from a magnetohydrodynamical (MHD) framework. In a 0.5 arcsec (30 pc) aperture at K', we find that polarization arising from the passage of radiation from the inner edge of the
Lopez-Rodriguez, E. et al.Fecha de publicación:
92015