Echelle spectroscopy of δ Vel (Pribulla+, 2011)

Details Echelle spectroscopy of δ Vel (Pribulla+, 2011) Echelle spectroscopy of δ Vel (Pribulla+, 2011)

Jan 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ycat..35289021p&link_type=abstract

VizieR On-line Data Catalog: J/A+A/528/A21. Originally published in: 2011A&A...528A..21P

Physics

Stars: Nearby, Binaries: Eclipsing, Spectroscopy

Scientific paper

The most important dataset used to determine parameters of the eclipsing pair are 63 echelle spectra obtained at the Cerro Armazones Observatory, Chile. The spectra are wavelength-calibrated and normalized to the continuum. The barycentric correction was added. The names of the FITS files containing the spectra are encoded as yymmddnn.fit, where "yymmdd" gives the evening date and "nn" is number of the spectrum within that night.
(2 data files).

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