L. P. Xin(NAOC), J. Wang(GXU), C. Gao(GXU), X. H. Han(NAOC), J. Y. Wei(NAOC),
G. W. LI(NAOC), L. H. Li(NAOC), C. Wu(NAOC), X. G. Wang(GXU),
E. W. Liang (GXU), R. S. Zhang(NAOC), Y. L. Qiu(NAOC),
and J. S. Deng(NAOC) report:
We began to observe GRB 210218A (Sbarufatti al., GCN 29529)
with Xinglong GWAC-F60A telescope, China, at 11:37:45 (UT),
18th. Feb. 2021, about 146 sec after the burst, under bad seeing condition.
A series of R, I images were obtained.
Preliminary analysis shows that no any new optical source
was found in single images within the Swift errorbox (Sbarufatti al., GCN 29529),
down to the 3 sigma upper limit of 15.0 mag in R band.
The upper limit is calibrated to the USNO B1.0 catalog.
This result is consistent with the previous report (Zhu et al., GCN 29530).