Detection of solar-like oscillations in the bright red giant stars γ Piscium and θ1 Tauri from a 190-day high-precision spectroscopic multi-site campaign

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Volume 573 (January 2015)

A&A, 573 (2015) A138

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Table 4

Radial velocities of θ¹ Tau from HERMES observations in the high-resolution observing mode.

HJD	RV	error_RV
[d]	[km s^-1]	[km s^-1]


2 455 241.38046	41.645	0.001
2 455 799.74878	43.793	0.002
2 455 806.74723	43.826	0.001
2 455 809.75936	43.865	0.001
2 455 842.75045	44.008	0.001
2 455 870.65140	44.186	0.001
2 456 157.69844	45.671	0.001
2 456 179.69122	45.704	0.001
2 456 305.41881	46.401	0.001
2 456 317.38334	46.396	0.001
2 456 322.38404	46.398	0.001
2 456 374.35806	46.738	0.002
2 456 507.72800	47.417	0.002
2 456 510.72944	47.419	0.001
2 456 518.71171	47.494	0.002
2 456 523.74224	47.481	0.002
2 456 526.74136	47.590	0.002
2 456 576.53391	47.681	0.001

Notes. The radial velocities and their formal uncertainties were determined through the cross-correlation pipeline for the HERMES spectrograph. The average of consecutive measurements is given. The observations were obtained between February 2010 and October 2013.

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