Abundance analysis of LSS 3378 (Pandey+, 2006) (original) (raw)

2007

Abstract

The spectrum of LSS 3378 was obtained on 2002 June 19 with the 4-m Blanco telescope and the Cassegrain echelle spectrograph at Cerro Tololo Inter-American Observatory (CTIO) in Chile. Three exposures of 25-min each, spectra covering the wavelength interval 50008200{AA} without gaps, were recorded at a resolving power of R=30000. The Image Reduction and Analysis Facility (IRAF) software packages were used to reduce the recorded spectra. (1 data file).

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