姓名：王军 性别：男
民族：汉族 职称：副研究员
学历：研究生 学位：博士
导师类别：硕士生导师
邮箱地址：wangjun@xao.ac.cn
现任职务：无
主要研究内容：主要从事脉冲星计时和低频望远镜阵列等相关技术研究，承担奇台低频阵列的研发和建设项目。主要研究方向包括脉冲星计时阵列与低频引力波探测研究，低频阵列的波束合成与阵列成像、校准等。
主持、参与科研项目：
1.在研项目
2.已完成项目
代表性科研成果：
[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.