(1) Wang N, Peng Q Y, Zhou X, Peng X Y and Peng H W, A distortion solution for the Bok telescope with four CCD chips[J], MNRAS 2019, 485, 1626-1634
(2) Wang N, Peng Q Y, Peng H W, Xie H J, Ma S and Zhang Q F, Precise CCD positions of Triton in 2014-2016 using the newest Gaia DR1 star catalogue[J], MNRAS 2017, 468, 1415-1419
(3) Wang N, Peng Q Y, Zhang X L, Zhang Q F, Li Z and Meng X H, Precise CCD positions of Apophis in 2013[J], MNRAS 2015, 454, 3805-3809
(4) Peng Q Y, Wang N, Vienne A, Zhang Q F, Li Z and Meng X H, Precise CCD positions of Phoebe in 2011-2014[J], MNRAS 2015, 449, 2638-2642
(5) Xie H J, Peng Q Y, Wang N, Vienne A, Li C W, Xie M N and Liu Z W, New CCD astrometric observations of the five major uranian satellites using Gaia DR1 in 2014-2016[J], P&SS 2019, 165, 110-114
(6) Peng H W, Peng Q Y, and Wang N, Precise CCD positions of Himalia using Gaia DR1 in 2015-2016[J], MNRAS 2017, 467, 2266-2273
(7) Lin F R, Peng Q Y, Wang N, Peng H W, Zhang Q F, and Li Z, Generalized derivation of the RRV method and its application[J], AJ 2016, 152, 183 (5 pp)
(8) Peng H W, Wang N, and Peng Q Y, Preliminary results of CCD observations targeting Himalia acquired at Yunnan Observatories in 2015[J], RAA 2016, 16, 186 (8 pp)
(9) Peng H W, Peng Q Y, Wang N, An improved solution to geometric distortion using an orthogonal method[J], RAA 2017, 17, 21(8 pp)