Professional:
Associate Research Professor
Master Supervisor
Education:
2017-2021 Bielefeld University Ph.D.
2014-2017 University of Chinese Academy of Sciences M.S.
2010-2014 Hainan University B. Eng.
Contact:
E-mail: wangjun@xao.ac.cn
Postal Address: 150 Science 1-Street, Urumqi, Xinjiang 830011, China
Research Interests:
Selected Publications:
[1] Wang, J.*, Norden, M., and Donker, P., “Real-time station monitor and stationtest pipelines for LOFAR 2.0”, Journal of Astronomical Telescopes, Instruments, and Systems, vol. 11, Art. no. 017002, 2025. doi:10.1117/1.JATIS.11.1.017002.
[2] Wang, J.*, Verbiest, J. P. W., Shaifullah, G. M., and Yuan, J. P., “Effect of Matching Algorithm and Profile Shape on Pulsar Pulse Time of Arrival Uncertainties”, Research in Astronomy and Astrophysics, vol. 23, no. 12, Art. no. 125020, IOP, 2023. doi:10.1088/1674-4527/ad013d.
[3] Wang, J.*, et. al., “A comparative analysis of pulse time-of-arrival creation methods”, Astronomy and Astrophysics, vol. 658, Art. no. A181, EDP, 2022. doi:10.1051/0004-6361/202141121.
[4] Wang, J.*, et. al., “Improving pulsar timing precision through superior time-of-arrival creation”, Astronomy and Astrophysics, vol. 687, Art. no. A154, EDP, 2024. doi:10.1051/0004-6361/202449366.
[5] Wang, J.*, et. al., “Noise analysis of six pulsars and a limit on the gravitational wave background”, Physica Scripta, vol. 99, no. 8, Art. no. 085024, IOP, 2024. doi:10.1088/1402-4896/ad5ec5.
[6] Iraci, F., et. al., “Combining the second data release of the European Pulsar Timing Array with low-frequency pulsar data”, Astronomy and Astrophysics, vol. 704, Art. no. A109, EDP, 2025. doi:10.1051/0004-6361/202555516.
[7] Larsen, B., et. al., “Rapid construction of joint pulsar timing array data sets: the Lite method”, Monthly Notices of the Royal Astronomical Society, vol. 542, no. 4, OUP, pp. 3028–3048, 2025. doi:10.1093/mnras/staf1420.
[8] Porayko, N. K., et. al., “Searches for signatures of ultralight axion dark matter in polarimetry data of the European Pulsar Timing Array”, Physical Review D, vol. 111, no. 6, Art. no. 062005, APS, 2025. doi:10.1103/PhysRevD.111.062005.
[9] Liu, K., et. al., “The impact on astrometry by solar-wind effect in pulsar timing”, Monthly Notices of the Royal Astronomical Society, vol. 536, no. 3, OUP, pp. 2603–2617, 2025. doi:10.1093/mnras/stae2727.
[10] EPTA Collaboration, et. al., “The second data release from the European Pulsar Timing Array. V. Search for continuous gravitational wave signals”, Astronomy and Astrophysics, vol. 690, Art. no. A118, EDP, 2024. doi:10.1051/0004-6361/202348568.
[11] EPTA Collaboration, et. al., “The second data release from the European Pulsar Timing Array. IV. Implications for massive black holes, dark matter, and the early Universe”, Astronomy and Astrophysics, vol. 685, Art. no. A94, EDP, 2024. doi:10.1051/0004-6361/202347433.
[12] Agazie, G., et. al., “Comparing Recent Pulsar Timing Array Results on the Nanohertz Stochastic Gravitational-wave Background”, The Astrophysical Journal, vol. 966, no. 1, Art. no. 105, IOP, 2024. doi:10.3847/1538-4357/ad36be.
