support of the National SKA program of China(Nos.2022SKA0110100 and 2022SKA0110101);the National Natural Science Foundation of China(NSFC,Grant Nos.1236114814,12203061,12273070,and 12303004)。
This paper presents the design,calibration,and survey strategy of the Fast Radio Burst(FRB)digital backend and its real-time data processing pipeline employed in the Tianlai Cylinder Pathfinder Array.The array,consist...
supported by the Specialized Research Fund for State Key Laboratories under Grant 202217;the Key Laboratory of Solar Activity and Space Weather(NSSC)under Grant E26600021S。
Ground-based radio observations below 30 MHz are susceptible to the ionosphere of the Earth and the radio frequency interference.Compared with other space mission concepts,making low frequency observations using an in...
supported by the Joint Funds of the National Natural Science Foundation of China(U1931107);supported by the National Key Research and Development Program of China No.2021YFA1600500。
A Fourier transform spectrometer(FTS)has been used to observe solar activities due to its ultra-high spectral resolution.However,the FTS in-band spectra are usually distorted and some artifacts appear in out-of-band r...
supported by the National SKA Program of China(2020SKA0110300);the Joint Research Fund in Astronomy(U1831204 and U1931141);the National Natural Science Foundation of China(NSFC);the Chinese Academy of Sciences(CAS);the Funds for International Cooperation and Exchange of the NSFC(11961141001);the NSFC(Grant No.11903009)。
As a dedicated solar radioheliograph,the MingantU SpEctral RadioHeliograph(MUSER)has a maximum baseline of more than 3000 m and a frequency range of 400 MHz–15 GHz.According to the classical radio interferometry theo...
supported by NSFC grants(11790301,11790305,11773043,U2031134,and 12003049);the National Key R&D Program of China(2021YFA1600500,2021YFA1600503,and 2018YFA0404602);supported by the National Major Scientific Research Facility Program of China with the Grant No.ZDYZ2009-3;The MUSER calibration system is a part of the Chinese Meridian Project funded by China’s National Development and Reform Commission。
The Mingantu Spectral Radioheliograph(MUSER),a new generation of solar dedicated radio imagingspectroscopic telescope,has realized high-time,high-angular,and high-frequency resolution imaging of the Sun over an ultra-...
supported by the National Natural Science Foundation of China(Grant Nos.11903067,11973011,11573057,U1831137 and 11703070);Shanghai Outstanding Academic Leaders Plan,the Strategic Priority Research Program of the Chinese Academy of Sciences(Grant No.XDB23010200);the Shanghai Key Laboratory of Space Navigation and Positioning Techniques(ZZXT-201902)。
By sending one or more telescopes into space,Space-VLBI(SVLBI)is able to achieve even higher angular resolution and is therefore the trend of the VLBI technique.For the SVLBI program,the design of satellite orbits pla...
supported by the National Natural Science Foundation of China(Grant Nos.11703033,11673051,11603001 and U1831136);the West Light Foundation of the Chinese Academy of Sciences(XAB2016A06);supported by the 100 Talents Project of the Chinese Academy of Sciences(CAS)。
In order to measure the Universal Time(UT1)in real time,National Time Service Center(NTSC)has built a VGOS-like(VLBI Global Observing System)broadband VLBI network,which includes three13-m radio telescopes located in ...
Supported by the National Natural Science Foundation of China
Recently, a configuration using atomic interferometers (AIs) had been sug- gested for the detection of gravitational waves. A new AI with some additional laser pulses for implementing large momentum transfer was als...