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Table · dataset · 2014

Spectroscopy of WASP planet host stars

Listed in IVOA Registry (Virtual Observatory)

We have made a detailed spectral analysis of 11 Wide Angle Search for Planets (WASP) planet host stars using high signal-to-noise ratio (S/N) HARPS spectra.

Description

Our line list was carefully selected from the spectra of the Sun and Procyon, and we made a critical evaluation of the atomic data. The spectral lines were measured using equivalent widths.

The procedures were tested on the Sun and Procyon prior to be being used on the WASP stars. The effective temperature (Teff), surface gravity (logg), microturbulent velocity (v_mic_) and metallicity were determined for all the stars.

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Optical
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Astronomical sciences 73%
Provenance · 1 source records, 9 field assertions
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IVOA Registry (Virtual Observatory)ivo://cds.vizier/j/mnras/428/316413 d agoJSON v1
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