Image Details
Caption: Figure 1.
Nightly binned RVs of 70 Oph A (48 nights) and 70 Oph B (44 nights) derived from PFS spectra, shown as a function of time. Each night’s data are represented by a single weighted-average measurement, with weights computed as the inverse square of the RV uncertainties. The time of each binned point corresponds to the weighted average of the observation times. Error bars are smaller than the symbol size and are therefore not visible.
© 2026. The Author(s). Published by the American Astronomical Society.