2023年度：
1、The study of eleven contact binaries with mass ratios less than 0.1，MNRAS，2023/01，https://ui.adsabs.harvard.edu/abs/2023MNRAS.tmp…53L/abstract
2、The first photometric and spectroscopic analysis of the neglected totally eclipsing contact binary NSVS 2536063，New Astronomy，2023/01，https://ui.adsabs.harvard.edu/abs/2023NewA…9801914X/abstract
3、Photometric and Spectroscopic Observations of GRB 190106A: Emission from Reverse and Forward Shocks with Late-time Energy Injection，ApJ，2023/05，https://arxiv.org/abs/2302.09722
4、The First Photometric and Spectroscopic Studies of ASASSN-V J015428.67+204247.2 and its Relation to the Population of Low Mass Ratio Contact Binaries，PASP，2023/05，https://iopscience.iop.org/article/10.1088/1538-3873/acc7cb
2022年度：
1、International Asteroid Warning Network Timing Campaign: 2019 XS，PSJ，2022/07，https://iopscience.iop.org/article/10.3847/PSJ/ac7224
2、Extremely low mass ratio contact binaries — I. the first photometric and spectroscopic investigations of ten systems，AJ，2022/09，https://arxiv.org/abs/2209.03653
3、M31N 1926-07c: A Recurrent Nova in M31 with a 2.8 yr Recurrence Time，RNAAS，2022/10，https://iopscience.iop.org/article/10.3847/2515-5172/ac9ab9
4、The First Photometric and Orbital Period Investigation of an Extremely Low Mass Ratio Contact Binary with a Sudden Period Change, TYC 4002-2628-1，MNRAS，2022/10，https://academic.oup.com/mnras/article-abstract/517/2/1928/6758514?redirectedFrom=fulltext
5、Photometric and spectroscopic studies of the long period low mass ratio deep contact binary KN Per，PASP，2022/10，https://arxiv.org/abs/2210.10591
6、M31N 2017-01e: Discovery of a Previous Eruption in this Enigmatic Recurrent Nova，RNAAS，2022/11，https://iopscience.iop.org/article/10.3847/2515-5172/aca2a6
2021年度：
1、Supernovae Detection with Fully Convolutional One-Stage Framework，Sensors，2021/03，https://www.mdpi.com/1424-8220/21/5/1926
2、The first photometric analysis of the totally eclipsing contact binary V811 Cep，RAA，2021/03，https://arxiv.org/abs/2103.12295
3、Photometric Study and Absolute Parameter Estimation of Six Totally Eclipsing Contact Binaries，AJ，2021/07，https://arxiv.org/abs/2104.13759
4、Intermediate-luminosity red transients: Spectrophotometric properties and connection to electron-capture supernova explosions，A&A，2021/08，https://arxiv.org/abs/2108.05087
2020年度：
1、Physical Characterisation of Interstellar Comet 2I/2019 Q4 (Borisov)，AJ，2020/03，https://arxiv.org/abs/2003.14064
2、The first light curve modeling and orbital period change investigation of nine contact binaries around the short period cut-off，AJ，2020/03，https://arxiv.org/abs/2003.02377
3、Observations of Disintegrating Long-Period Comet C/2019 Y4 (ATLAS) — A Sibling of C/1844 Y1 (Great Comet)，AJ，2020/04，https://arxiv.org/abs/2004.10990
4、2000 Herschel A Tumbling Asteroid，MPBu，2020/04，https://ui.adsabs.harvard.edu/abs/2020MPBu…47..142P/abstract
5、Photometry of 2729 Urumqi at The Xingming Observatory in Urumqi City，MPBu，2020/04，https://ui.adsabs.harvard.edu/abs/2020MPBu…47..151G/abstract
6、The first photometric investigation of the contact binary OQ Cam，RAA，2020/05，https://arxiv.org/abs/2005.13966v1
7、The Unusual Eruption of the Extragalactic Classical Nova M31N 2017-09a，The Observatory，2020/06，https://arxiv.org/abs/2006.10118
8、Searching for eclipsing binaries in the area of RA: 02h21m36s, DEC:+57◦11′32′′，MNRAS，2020/07，https://academic.oup.com/mnras/article-abstract/497/3/3381/5876882
9、GJ 3470 c: A Saturn-like Exoplanet Candidate in the Habitable Zone of GJ 3470，arXiv eprint，2020/07，https://arxiv.org/abs/2007.07373
10、The Discovery of an Equal-mass Twin Binary System by Online Sky Survey Images，JDSO，2020/08，http://www.jdso.org/volume16/number4/Sun_401_402.pdf
11、Discovery of new member of WDS 02137-0302，WDS 02137-0302 B may not be physical，JDSO，2020/08，http://www.jdso.org/volume16/number4/Sun_403_404.pdf
12、Photometric and Spectroscopic Studies of Flares on Ross 15，RAA，2020/09，https://arxiv.org/abs/2009.06952
2019年度：
1、Photometric Study of Asteroid 4730 Xingming from Gaoyazi Observatories and Xingming Observatories，MPBu，2019/01，http://articles.adsabs.harvard.edu/pdf/2019MPBu…46…82T
2、The Rotation Period of (32209) 2000 OW9，MPBu，2019/04，http://adsabs.harvard.edu/abs/2019MPBu…46..215G
3、Photometric investigations on two totally eclipsing contact binaries：V342 UMa and V509 Cam，RAA，2019/05，https://arxiv.org/abs/1905.01646
4、Asteroid (3200) Phaethon: Colors，Phase Curve，Limits on CometaryActivity，and Fragmentation，AJ，2019/06，https://iopscience.iop.org/article/10.3847/1538-3881/ab245d
5、New active asteroid (6478) Gault，MNRAS，2019/07，https://academic.oup.com/mnrasl/article-abstract/488/1/L143/5532375?redirectedFrom=fulltext
6、V1005 Her：a solar-type shallow-contact binary in a triply fossil system，MNRAS，2019/08，https://academic.oup.com/mnras/article/489/2/2677/5551498
7、The long-lived Type IIn SN 2015da：Infrared echoes and strong interaction within an extended massive shell，A&A，2019/08，https://arxiv.org/abs/1908.08580
2018年度：
1、Asteroid Lightcurves from Xingming Observatory: 2017 – 2017 June，MPBu，2018/01，https://ui.adsabs.harvard.edu/abs/2018MPBu…45…57T/abstract
2、Breaking the habit – the peculiar 2016 eruption of the unique recurrent nova M31N 2008-12a，APJ，2018/03，https://arxiv.org/abs/1803.00181
3、Lightcurve Analysis for Near-Earth Asteroid 2012 TC4，MPBu，2018/07，https://ui.adsabs.harvard.edu/abs/2018MPBu…45..220T/abstract
4、Two Hyperbolic Baldheads in the Solar System: 2017 U7 and 2018 C2，2018/08，AJ, https://iopscience.iop.org/article/10.3847/1538-3881/aacdf3/pdf
2017年度：
1、The Rotation Period of 1117 Reginita，MPBu，2017/10，https://ui.adsabs.harvard.edu/abs/2017MPBu…44..307T/abstract
2016年度：
1、When comets get old: A synthesis of comet and meteor observations of the low activity comet 209P/LINEAR，Icarus，2016/01，https://ui.adsabs.harvard.edu/abs/2016Icar..264…48Y/abstract
2、Massive stars exploding in a He-rich circumstellar medium – IX. SN 2014av, and characterization of Type Ibn SNe，MNRAS，2016/02，https://ui.adsabs.harvard.edu/abs/2016MNRAS.456..853P/abstract
3、M31N 2008-12a – the remarkable recurrent nova in M31: Pan-chromatic observations of the 2015 eruption，APJ，2016/12，https://ui.adsabs.harvard.edu/abs/2016ApJ…833..149D/abstract
4、POPULAR SUPERNOVA PROJECT: A CITIZEN SCIENCE PROGRAM BASED ON AMATEUR ASTRONOMICAL OBSERVATIONS，INTED2016，https://library.iated.org/view/LI2016POP
2015年度：
1、A remarkable recurrent nova in M 31: The 2010 eruption recovered and evidence of a six-month period，A&A，2015/10，https://ui.adsabs.harvard.edu/abs/2015A%26A…582L…8H/abstract
2、Gone in a Blaze of Glory: The Demise of Comet C/2015 D1 (SOHO)，APJ，2015/11，https://ui.adsabs.harvard.edu/link_gateway/2015ApJ…813…73H/EPRINT_PDF
3、Bangs and Meteors from the Quiet Comet 15P/Finlay，APJ，2015/11，https://ui.adsabs.harvard.edu/abs/2015ApJ…814…79Y/abstract
4、SN 2011fu: A type IIb Supernova with a luminous double-peaked light curve，MNRAS，2015/11，https://ui.adsabs.harvard.edu/abs/2015MNRAS.454…95M/abstract
5、Results from the worldwide coma morphology campaign for comet ISON (C/2012 S1)，P&SS，2015/12，https://arxiv.org/abs/1511.07592
2014年度：
1、An Early Look of Comet C/2013 A1 (Siding Spring): Breathtaker or Nightmare?，APJ，2014/06，https://ui.adsabs.harvard.edu/link_gateway/2014ApJ…787..115Y/EPRINT_PDF
2013年度：
1、Supersoft X-rays reveal a classical nova in the M 31 globular cluster Bol 126，A&A，2013/01，https://ui.adsabs.harvard.edu/abs/2013A%26A…549A.120H/abstract
2011年度：
1、Forecasting Cloud Cover and Atmospheric Seeing for Astronomical Observing: Application and Evaluation of the Global Forecast System，PASP，2011/01，https://ui.adsabs.harvard.edu/link_gateway/2011PASP..123..113Y/PUB_PDF
