A spectroscopic dataset for "hump and spike" stars
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These are spectra for a sample of "hump and spike" stars. The data were collected with HERMES spectrograph mounted at the Cassegrain focus of the 1.2-m Mercator telescope located at La Palma, Spain. In a single exposure, this spectrograph records optical spectra in the wavelength (λ) range 377 to 900 nm across the 55 spectral orders. The resolving power of this instrument in the high-resolution mode is R = 85 000 with radial velocity stability of about 50 m/s, and excellent throughput.<br>
创建时间：
2021-01-18
