Image Details
Caption: Figure 1.
Flowchart of the two-level RVZP correction for LAMOST MRS. We compare LAMOST MRS RVs with Gaia-corrected and APOGEE DR17 RVs to derive (1) a spectrograph–exposure correction in (lmjm, planid, spid) units and (2) a fiber–time correction inferred from the good sample after applying the first-level correction.
© 2026. The Author(s). Published by the American Astronomical Society.