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Peng Q.Y., Mao W., A Method for Determining Precisely the Barycentric Position of Uranus Observed with CCD systems, 1998,ApSS, 257, 278-281
Peng Q.Y., Vienne A., and Shen K.X., Positional measuring procedure and CCD observations for Saturnian satellites, 2002, A&A 383, 296-301 (IF2005: 4.223; IDS Number: 527JT)
Peng Q.Y., Han Y.B., Zhang C.L. and Li Z.L., Image-processing techniques in precisely measuring positions of Jupiter and its Galilean satellites, 2003, A&A 401, 773-779 (IF2005: 4.223; IDS Number: 658EN)
Peng Q.Y., Image-processing techniques in precisely measuring positions of Saturn and its satellites, 2003, Science in China (G) 46, 362-370 (IF2005: 0.292; IDS Number: 706LY)
Peng Q.Y., Vienne A., Han Y.B. and Li Z.L., Precise calibration of CCD images with a small field of view, 2004, A&A 424, 339-344 (IF2005: 4.223; IDS Number: 857DD)
Peng Q.Y., New confirmation of image-processing techniques for astrometry of Saturn and its satellites, 2005, MNRAS 359, 1597-1600 (IF2005: 5.352; IDS Number: 933NQ)
Peng Q.Y., Zhang Q.F., Precise positions of Phoebe determined with CCD image-overlapping calibration, 2006, MNRAS 366, 208-212 (IF2005: 5.352; IDS Number: 006DW)
Peng Q.Y., Noyelles B., Eclipses and occultations of Galilean satellites observed at Yunnan observatory in 2003, 2007, ChJAA 7, 317-324 (IF2005: 0.672; IDS Number: 162ZY)
Peng Q.Y., Vienne A., Lainey V. and Noyelles B., New evidence of precision premium for Galilean satellites from CCD imaging, 2008, Planetary & Space Science 56. 1807-1811 (SCI, IF2008: 2.506)
Arlot, J. -E.; Jin, W. J.; Zhu, J.; Peng, Q. Y.; Colas, F.; Shen, K. X.; Tang, Z. H.; Zhu, Z.; Lainey, V.; Thuillot, W.; Vienne, A., 2008, A project of teaching ground-based astrometry, 2008, IAUsymp.248, 521-522
Peng Q.Y., Emelyanov N.V., Zhou L., Gu W. R., Astrometry from mutual event and small-separation CCD imaging, 2008, IAUsymp. 248, 114-115
Peng Q.Y., Vienne A., Wu X. P., Gan L. L., and Desmars J., CCD Positions of Saturn and its major satellites in 2002-2006, 2008, AJ 136, 2214-2221 (SCI IF2007: 5.019)
Arlot J.-E. et al. (118 authors,including Peng Q.Y., Vienne A. ), The Phemu03 catalogue of observations of the mutual phemena of the Galilean satellites of Jupiter,2009,A&A 493, 1171-1182 ( SCI IF2007: 4.259; IDS Number: 857DD)
Peng Q.Y., Fan L.Y., Accurate determination of plate model based on CCD images with different orientations, 2010, Chinese Science Bulletin, 55, 791-796
Peng Q.Y., He H. F., Lainey V., & Vienne A., Precise CCD positions of Galilean satellite-pairs, 2012, MNRAS, 419, 1977-1982
Zhang Q.F., Peng Q.Y., Zhu Z., Preliminary results of solving the problem of geometric distortion for the 2.4 m telescope at Yunnan Observatory, 2012,RAA, 12, 1451
Peng Q.Y., Vienne A., Zhang Q.F., Desmars J., Yang C.Y., He H.F., Convenient solution to Geometric Distortion and its application to the observations of Phoebe, 2012, AJ, 144:170
Desmars J., Li S.N., Tajeddine R., Peng Q.Y., and Tang Z.H., Phoebe’s orbit from ground-based and space-based observations, 2013, A&A,553, A36
Peng Q.Y., Wang N., Vienne A., Zhang Q.F., Li Z. and Meng X.H., Precise CCD positions of Phoebe in 2011-2014, 2015, MNRAS, 449, 2638-2642
Wang N., Peng Q.Y.*, Zhang X.L., Zhang Q.F., Li Z., and Meng X.H., Precise CCD positions of Apophis in 2013, 2015, MNRAS 454,3805