activity
20172020
most citedUsing Gaia DR2 to solve differential color refraction and charge transfer efficiency issues

24 citations · 76 across the 5 of their papers we have counts for

collaborators

6 papers

astro-ph.IM202024 cited

Using Gaia DR2 to solve differential color refraction and charge transfer efficiency issues

F. R. Lin, Q. Y. Peng, Z. J. Zheng

The Gaia DR2 catalog released in 2018 gives information about more than one billion stars, including their extremely precise positions that are not affected by the atmosphere, as w…

astro-ph.IM2020

Automatic removal of false image stars in disk-resolved images of the Cassini Imaging Science Subsystem

Qingfeng Zhang, Zhicong Lu, Xiaomei Zhou +5

Taking a large amount of images, the Cassini Imaging Science Subsystem (ISS) has been routinely used in astrometry. In ISS images, disk-resolved objects often lead to false detecti…

astro-ph.GA201919 cited

Characterization of precision premium in astrometry

F. R. Lin, J. H. Peng, Z. J. Zheng +1

Precision premium, a concept in astrometry that was firstly presented by Pascu in 1994, initially means that the relative positional measurement of the Galilean satellites of Jupit…

astro-ph.IM20198 cited

A distortion solution for the Bok telescope with four CCD chips

N. Wang, Q. Y. Peng, X. Zhou +2

The Beijing-Arizona Sky Survey (BASS) is an imaging survey and uses the 2.3 m Bok telescope at Kitt Peak. In order to tap the astrometric potential of the Bok telescope and improve…

astro-ph.EP201719 cited

Precise CCD positions of Triton in 2014-2016 using the newest Gaia DR1 star catalogue

N. Wang, Q. Y. Peng, H. W. Peng +3

755 new CCD observations during the years 2014-2016 have been reduced to derive the precise positions of Triton, the first satellite of Neptune. The observations were made by the 1…

astro-ph.EP20176 cited

Precise CCD positions of Himalia using Gaia DR1 in 2015-2016

H. W. Peng, Q. Y. Peng, N. Wang

In order to obtain high precision CCD positions of Himalia, the sixth Jovian satellite, a total of 598 CCD observations have been obtained during the years 2015-2016. The observati…