Image Details
Caption: Figure 2.
Top panel: distribution of pairwise RV difference is shown for three different RV error bins—blue for the 35 km s−1 bin, orange for the 55 km s−1 bin, and green for the 95 km s−1 bin. Bottom panel: the fit to the distribution of pairwise RV difference, σRV,fit, for different corrected CORV RV error bins, δRV. After correcting the RV errors, as explained in the text, we find that CORV RV errors agree with the fitted errors from the pair subtraction test to within 10%.
© 2026. The Author(s). Published by the American Astronomical Society.