Abstract
We present an Echelle+CCD, high signal-to-noise ratio, high-resolution (R = 20,000) spectroscopic atlas of 108 well-known objects representative of the most common types of peculiar and variable stars. The wavelength interval extends from 4600 to 9400Å and includes the RAVE, Gaia, and HERMES wavelength ranges.Multi-epoch spectra are provided for the majority of the observed stars. A total of 425 spectra of peculiar stars, which were collected during 56 observing nights between 1998 November and 2002 August, are presented. The spectra are given in FITS format and heliocentric wavelengths, with accurate subtraction of both the sky background and the scattered light. Auxiliary material useful for custom applications (telluric dividers, spectrophotometric stars, flat-field tracings) is also provided. The atlas aims to provide a homogeneous database of the spectral appearance of stellar peculiarities, a tool useful both for classification purposes and inter-comparison studies. It could also serve in the planning and development of automated classification algorithms designed for RAVE, Gaia, HERMES, and other large-scale spectral surveys. The spectrum ofXXOph is discussed in some detail as an example of the content of the present atlas.
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Tomasella, L., Munari, U., & Zwitter, T. (2010). A high-resolution, multi-epoch spectral atlas of peculiar stars including RAVE, Gaia, and HERMES wavelength ranges. Astronomical Journal, 140(6), 1758–1765. https://doi.org/10.1088/0004-6256/140/6/1758
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