Fig. 5

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Comparison of different contributions in the uncertainty of Ṗb for simulated data from 2021 to 2030. The pink, orange and blue lines show the uncertainty of Ṗb using the simulated data from 3ERT (EFF, NC, LT), MeerKAT (MK), and FAST, respectively. The brown line indicates the uncertainty of when using the timing parallax (πx) measured from simulated FAST data. The green lines indicate the uncertainties of
when assuming 10% (dashed) and 3% (dash-dotted) uncertainties in the vertical component of Galactic acceleration Kɀ.
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