activity
20162022
most citedSpace very long baseline interferometry in China

23 citations · 83 across the 5 of their papers we have counts for

collaborators

7 papers

astro-ph.GA202215 cited

A Q-band line survey towards Orion KL using the Tianma radio telescope

Xunchuan Liu, Tie Liu, Zhiqiang Shen +28

We have conducted a line survey towards Orion KL using the Q-band receiver of Tianma 65 m radio telescope (TMRT), covering 34.8--50 GHz with a velocity resolution between 0.79 km s…

astro-ph.GA2021

East Asian VLBI Network Observations of Active Galactic Nuclei Jets: Imaging with KaVA+Tianma+Nanshan

Yuzhu Cui, Kazuhiro Hada, Motoki Kino +74

The East Asian very-long-baseline interferometry (VLBI) Network (EAVN) is a rapidly evolving international VLBI array that is currently promoted under joint efforts among China, Ja…

astro-ph.SR201914 cited

Carbon-Chain Molecules in Molecular Outflows and Lupus I Region--New Producing Region and New Forming Mechanism

Yuefang Wu, Xunchuan Liu, Xi Chen +18

Using the new equipment of the Shanghai Tian Ma Radio Telescope, we have searched for carbon-chain molecules (CCMs) towards five outflow sources and six Lupus I starless dust cores…

astro-ph.SR201910 cited

A particular carbon-chain-producing region: L1489 starless core

Yuefang Wu, Lianghao Lin, Xunchuan Liu +14

We detected carbon-chain molecules (CCMs) HC2n+1N (n=1-3) and C3S in Ku band as well as {high-energy excitation lines including C4H N=9-8, J=17/2-15/2, 19/2-17/2, and CH3CCH J=5-4,…

astro-ph.IM201923 cited

Space very long baseline interferometry in China

Tao An, Xiaoyu Hong, Weimin Zheng +19

Space very long baseline interferometry (VLBI) has unique applications in high-resolution imaging of fine structure of astronomical objects and high-precision astrometry due to the…

astro-ph.HE201721 cited

TMRT observations of 26 pulsars at 8.6 GHz

Ru-Shuang Zhao, Xin-Ji Wu, Zhen Yan +18

Integrated pulse profiles at 8.6~GHz obtained with the Shanghai Tian Ma Radio Telescope (TMRT) are presented for a sample of 26 pulsars. Mean flux densities and pulse width paramet…