In July 2001, AutoFib-2 (AF2), the prime focus robotic fiber positioner for the Isaac Newton Group's (ING) 4.2m William Hershel Telescope (WHT) had its new...
Classical model-atmosphere analyses of stellar spectra usually begin by measuring equivalent widths, and then proceed into a loop in which 1) model spectra are...
Automated analysis of stellar spectra: application to the GAUDI
In this paper we describe a methodology to be used for the automated analysis of the spectroscopic contents of the GAUDI archive. We perform chi-square...
Automated Stellar Spectral Classification and Parameter-Ization for the Masses
Stellar spectroscopic classification has been successfully automated by a number of groups. Automated classification and parameterization work best when applied...
Automatic determination of atmospheric turbulence wind profiles using wavelets
Adaptive optics devices in astronomy compensate the distortions introduced by the atmosphere in the quality and resolution of images taken by ground-based...
Automatic scattered field estimation for the Stripe82 survey
The low surface brightness Universe is one of the last frontiers in observational Astronomy, even a deep large multi-band survey such as the SDSS/Stripe82 is...
More than 2000 stars distributed in the field of view of 35 planetary nebulae, and 31 stars from the spectral catalog of Jacoby et al. (1984, Cat. III/92) were...