Image Details
Caption: Figure 8.
Residuals of Mars orbiter VLBI data against DE440, showing the Goldstone–Madrid baseline (top) and the Goldstone–Canberra baseline (bottom). The rms residual of the Goldstone–Madrid baseline is about 0.25 mas and the rms residual of the Goldstone–Canberra baseline is about 0.18 mas.
© 2021 The Author(s). Published by The American Astronomical Society.