2024年度：
1、M31N 2013-10c: A Newly Identified Recurrent Nova in M31, RNAAS, 2024/01, https://iopscience.iop.org/article/10.3847/2515-5172/ad19de
2、Confirmation of a Sub-Saturn-size transiting exoplanet orbiting a G dwarf: TOI-1194 b and a very low mass companion star: TOI-1251 B from TESS, RAA, 2024/02, https://iopscience.iop.org/article/10.1088/1674-4527/ad057b
3、New constraints on Triton’s atmosphere from the 6 October 2022 stellar occultation, A&A, 2024/04, https://www.aanda.org/10.1051/0004-6361/202348460
4、Spectroscopic and photometric investigations of the totally eclipsing contact binary V1320 Cas, NewA, 2024/06, https://authors.elsevier.com/a/1jCc%7E_VU94Kt54
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、TOI-4562 b: A highly eccentric temperate Jupiter analog orbiting a young field star, AJ, 2023/02, http://dx.doi.org/10.3847/1538-3881/acb5a2
4、Photometric and Spectroscopic Observations of GRB 190106A: Emission from Reverse and Forward Shocks with Late-time Energy Injection, ApJ, 2023/05, https://iopscience.iop.org/article/10.3847/1538-4357/acbd96
5、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
6、Flares confirmed for the first time to be from the primary component of an eclipsing binary, MNRAS, 2023/10, https://doi.org/10.1093/mnras/stad3251
7、The first analysis of three long-period low mass-ratio Contact Binaries, MNRAS, 2023/11, https://doi.org/10.1093/mnras/stad3591
8、Harnessing Edge-Enhanced Attention Mechanisms for Supernova Detection in Deep Learning Frameworks, ASCOM, 2023/12, https://www.sciencedirect.com/science/article/pii/S2213133723000999
9、Optical and Near-infrared Observations of the Distant but Bright “New Year’s Burst” GRB 220101A, ApJ, 2023/12, https://iopscience.iop.org/article/10.3847/1538-4357/ad05c8
10、A Shock Flash Breaking Out of a Dusty Red Supergiant, Nature, 2023/12, https://doi.org/10.1038/s41586-023-06843-6
11、Discovery of the Closest Ultrastripped Supernova: SN 2021agco in UGC 3855, ApJL, 2023/12, https://iopscience.iop.org/article/10.3847/2041-8213/ad0cc3
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
