Zobrazeno 1 - 10
of 83
pro vyhledávání: '"ZHOU Yi-yu"'
Publikováno v:
Tongxin xuebao, Pp 13-18 (2008)
A new direction finding algorithm called conjugate propagator method (COP) for one-dimension signals was proposed. The new algorithm uses the array output and its conjugate form to extend the array aperture so that it can detect more signals than
Externí odkaz:
https://doaj.org/article/f7b3ad7cf046498280e77be30b43c811
Autor:
Lifan Wang, Lei Hu, Hongyan Zhou, Peng Jiang, Zhengyang Li, Xue-Feng Wu, Michael C. B. Ashley, Qiang Liu, Peng Wei, Tianrui Sun, Ming Yang, Zhou-Yi Yu, Qiguo Tian, Jessica Zheng, Robert A. Wittenmyer, Hui Zhang, Ji-Lin Zhou, C. G. Tinney, Xiaoyan Li, Zhaohui Shang, Xiangyan Yuan, Charling Tao, Xiangqun Cui, Xiaofeng Wang, Jon Lawrence, Songhu Wang, Jeremy Mould, Bozhong Gu, Nicholas B. Suntzeff, Duncan J. Wright, Shihai Yang, Hui-Gen Liu, Ce Yu, Fujia Du, Xuefei Gong, En-Si Liang, Lingzhe Xu, S. A. Uddin, Jian-Ning Fu, Zhenxi Zhu, Bin Ma, Yi Hu
Publikováno v:
Astron.J.
Astron.J., 2020, 159 (5), pp.201. ⟨10.3847/1538-3881/ab7ea8⟩
Astron.J., 2020, 159 (5), pp.201. ⟨10.3847/1538-3881/ab7ea8⟩
International audience; The CHinense Exoplanet Searching Program from Antarctica is a ground-based wide-field photometric survey using the AST3 and CSTAR telescopes located at Dome A, Antarctica. Blessed with the unparalleled observing conditions on
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::621f8081414575f9870a6ae88bd275ab
https://hal.science/hal-02542798
https://hal.science/hal-02542798
Autor:
C. G. Tinney, Xiangyan Yuan, Ce Yu, Fujia Du, Qiang Liu, Ji-Lin Zhou, Peng Jiang, Peng Wei, Xuefei Gong, Duncan J. Wright, Jon Lawrence, Lingzhe Xu, Jian-Ning Fu, Xue-Feng Wu, En-Si Liang, Shihai Yang, Syed Uddin, Zhengyang Li, Michael C. B. Ashley, Xiangqun Cui, Xiaofeng Wang, Songhu Wang, Zhou-Yi Yu, Xiaoyan Li, Hui Zhang, Hui-Gen Liu, Qiguo Tian, Lifan Wang, Zhaohui Shang, Charling Tao, Robert A. Wittenmyer, Jessica Zheng, Ming Yang, Zhenxi Zhu, Nicholas B. Suntzeff, Bin Ma, Yi Hu, Jeremy Mould, Bozhong Gu, Hongyan Zhou
Publikováno v:
The Astrophysical Journal Supplement Series, vol 240, iss 2
Astrophys.J.Suppl.
Astrophys.J.Suppl., 2019, 240 (2), pp.16. ⟨10.3847/1538-4365/aaec0c⟩
The Astrophysical Journal Supplement Series
The Astrophysical Journal Supplement Series, IOPscience 2019, 240 (2), pp.16. ⟨10.3847/1538-4365/aaec0c⟩
Astrophys.J.Suppl.
Astrophys.J.Suppl., 2019, 240 (2), pp.16. ⟨10.3847/1538-4365/aaec0c⟩
The Astrophysical Journal Supplement Series
The Astrophysical Journal Supplement Series, IOPscience 2019, 240 (2), pp.16. ⟨10.3847/1538-4365/aaec0c⟩
Located at Dome A, the highest point of the Antarctic plateau, the Chinese Kunlun station is considered to be one of the best ground-based photometric sites because of its extremely cold, dry, and stable atmosphere(Saunders et al. 2009). A target can
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::32d6094f80ca652c37725b2fc002d37d
https://escholarship.org/uc/item/4v58j7vr
https://escholarship.org/uc/item/4v58j7vr
Autor:
Bin Ma, Yi Hu, Zhenxi Zhu, Duncan J. Wright, Xuefei Gong, Nicholas B. Suntzeff, Lingzhe Xu, C. G. Tinney, Jon Lawrence, Xiangyan Yuan, Jian-Ning Fu, Ji-Lin Zhou, Ce Yu, Peng Jiang, Fujia Du, En-Si Liang, Syed Uddin, Zhengyang Li, Ming Yang, Xiangqun Cui, Xiaoyan Li, Zhou-Yi Yu, Bozhong Gu, Qiguo Tian, Charling Tao, Robert A. Wittenmyer, Xiaofeng Wang, Peng Wei, Qiang Liu, Shihai Yang, Hongyan Zhou, Jeremy Mould, Jessica Zheng, Xue-Feng Wu, Hui Zhang, Zhaohui Shang, Michael C. B. Ashley, Hui-Gen Liu, Lifan Wang, Songhu Wang
Publikováno v:
Astrophys.J.Suppl.
Astrophys.J.Suppl., 2019, 240 (2), pp.17. ⟨10.3847/1538-4365/aaf583⟩
The Astrophysical Journal Supplement Series
The Astrophysical Journal Supplement Series, IOPscience 2019, 240 (2), pp.17. ⟨10.3847/1538-4365/aaf583⟩
The Astrophysical Journal Supplement Series, vol 240, iss 2
Astrophys.J.Suppl., 2019, 240 (2), pp.17. ⟨10.3847/1538-4365/aaf583⟩
The Astrophysical Journal Supplement Series
The Astrophysical Journal Supplement Series, IOPscience 2019, 240 (2), pp.17. ⟨10.3847/1538-4365/aaf583⟩
The Astrophysical Journal Supplement Series, vol 240, iss 2
We report first results from the CHinese Exoplanet Searching Program from Antarctica (CHESPA)---a wide-field high-resolution photometric survey for transiting exoplanets carried out using telescopes of the AST3 (Antarctic Survey Telescopes times 3) p
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::45c393828fbdf3dcf21157d47e533e3b
https://hal.archives-ouvertes.fr/hal-02017058
https://hal.archives-ouvertes.fr/hal-02017058
Autor:
Peng Jiang, Xuefei Gong, Lingzhe Xu, Xiaoyan Li, Jiapeng Zhu, En-Si Liang, Zhengyang Li, Charling Tao, Hui Zhang, Fujia Du, Duncan J. Wright, Tianrui Sun, Shihai Yang, Lifan Wang, Ming Yang, Lei Hu, Hui-Gen Liu, S. A. Uddin, Ji-Lin Zhou, Xiangqun Cui, Xiaofeng Wang, Songhu Wang, Zhenxi Zhu, Bozhong Gu, Nicholas B. Suntzeff, Zhou-Yi Yu, Qiguo Tian, Robert A. Wittenmyer, Hongke Lu, Hongyan Zhou, Xiangyan Yuan, Jeremy Mould, Peng Wei
Publikováno v:
Astron.J.
Astron.J., 2020, 159 (4), pp.172. ⟨10.3847/1538-3881/ab7449⟩
Astron.J., 2020, 159 (4), pp.172. ⟨10.3847/1538-3881/ab7449⟩
International audience; From the experiences learned in three decades of exoplanet search, wide-field transit surveys have proven to be one of the most effective ways to detect exoplanets. Wide field of view, however, suffers from high false-positive
Publikováno v:
Research in Astronomy and Astrophysics. 20:035
HEPS (Habitable ExoPlanet Survey) is a planning astrometry satellite that aims to find Earth-like planets in the solar neighbourhood. In this paper, we selected 140 planet harboring stars within 30 pc of the solar system to be potential targets for H
Autor:
Hui-Gen Liu, Jia-Yi Yang, Di-Chang Chen, Hui Zhang, Ming Yang, En-Si Liang, Ji-Lin Zhou, Zhou-Yi Yu, Ji-Wei Xie
Planetary systems can survive the stellar evolution, as evidenced by the atmospheric metal pollution and dusty disks of single white dwarfs. Recent observations show that 1 to 4 percent of single white dwarfs are accompanied by dusty disks, while the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5f6187ef4bf097e544b529098d4a7b27
Autor:
Zhou-Yi Yu, Zhengyang Li, Qiguo Tian, Ji-Lin Zhou, Xiheng Shi, Hong-fei Zhang, Shaohua Zhang, Haiping Lu, Zhiyong Zhang, Hui-Gen Liu, Xingxing Huang, Minghao Jia, Peng Jiang, Ji Wang, Ming Yang, Bo Liu, Xiang Pan, Fujia Du, Xiaoyan Li, Supachai Awiphan, Bin Li, Tuo Ji, Hongyan Zhou, Jian Wang
Proxima Centauri is known as the closest star from the Sun. Recently, radial velocity observations revealed the existence of an Earth-mass planet around it. With an orbital period of ~11 days, the surface of Proxima Centauri b is temperate and might
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::51830851ca9f6a7ad4706a3429ba6bfb
Publikováno v:
Progress in Natural Science. 15:491-495
When single cycle frequency is employed, the existing spectral correlation-signal subspace fitting (SC-SSF) algorithms usually contain two disadvantages: those single-cycle estimators cannot reach the best performance: it is inconvenient to be applie
Publikováno v:
International Workshop on Communication Technology 2013.