supported by the National SKA Program of China(Grant No.2020SKA0120104);the National Key R&D Program of China(Grant No.2022YFA1603104);the National Natural Science Foundation of China(Grant Nos.U2031119,and 12041301);The image of the Gum Nebula comes from the Southern H-Alpha Sky Survey Atlas(SHASSA),which is supported by the National Science Foundation。
The Gum Nebula is a faint supernova remnant extending about 40°across the southern sky,potentially affecting tens of background pulsars.Though the view that the Gum Nebula acts as a potential scattering screen for ba...
supported by the National Natural Science Foundation of China (Grant No. 12305059);supported by the National Natural Science Foundation of China (Grant No. 12305075);supported by the National Natural Science Foundation of China (Grant No. 12403002);the Joint Fund of Henan Province Science and Technology R&D Program (Grant No. 235200810111);the Startup Research Fund of Henan Academy of Sciences (Grant No. 241841224);the Startup Research Fund of Henan Academy of Sciences (Grant No. 241841221)。
Recent observations by pulsar timing array collaborations have detected a stochastic common-spectrum signal, which may originate from scalar-induced gravitational waves generated by primordial curvature perturbations ...
supported in part by the National Natural Science Foundation of China(Nos.61873196,62373030,61772187);the Innovation Program for Quantum Science and Technology(No.2021ZD0303400)。
The traditional orbit determination method based on pulsar profile distortion can determine the six elements of the orbit.However,the estimation accuracies of these methods are limited and the computational load of a ...
supported by National Key Research and Development Program of China(2022YFC2205203);the Major Science and Technology Program of Xinjiang Uygur Autonomous Region(No.2022A03013-1);the National Natural Science Foundation of China(NSFC,grant Nos.U1838109 and 12041304);supported by the Major Science and Technology Program of Xinjiang Uygur Autonomous Region(No.2022A03013-1);National Natural Science Foundation of China(NSFC,Grant No.12303053);the 2021 project Xinjiang Uygur autonomous region of China for Tianshan elites,the Youth Innovation Promotion Association of CAS under No.2023069;the Tianshan Talent Training Program(No.2023TSYCCX0100);supported by the National SKA Program of China(grant No.2020SKA0120200);the National Natural Science Foundation of China(NSFC,grant Nos.12041303,12273100 and12288102);the National Key R&D Program of China(grant No.2022YFC2205201);the West Light Foundation of the Chinese Academy of Sciences(grant No.WLFC 2021-XBQNXZ-027);the Major Science and Technology Program of Xinjiang Uygur Autonomous Region(grant No.2022A03013-4)。
In this paper,the emissions from two pulsars,PSRs J1611-0114 and J1617+1123,were investigated using th Five-hundred-meter Aperture Spherical radio Telescope operating at a central frequency of 1250 MHz.Th average puls...
supported by the National Natural Science Foundation of China(12041303);the National SKA Program of China(2020SKA0120200);the CAS Project for Young Scientists in Basic Research YSBR-063;the National Natural Science Foundation of China(NSFC grant Nos.12203070 and Nos.12203072);the CAS-MPG LEGACY project。
Timing newly discovered pulsars requires gradually building up a timing model that connects observations taken days to months apart.This sometimes can be challenging when our initial knowledge of the pulsar’s positio...
supported by the National Key R&D Program of China Nos.2021YFC2203502 and 2022YFF0711502;the National Natural Science Foundation of China(NSFC,grant Nos.12173077,12073067);the Tianshan Talent Project of Xinjiang Uygur Autonomous Region(2022TSYCCX0095 and2023TSYCCX0112);the Scientific Instrument Developing Project of the Chinese Academy of Sciences,grant No.PTYQ2022YZZD01;China National Astronomical Data Center(NADC);the Operation,Maintenance and Upgrading Fund for Astronomical Telescopes and Facility Instruments,budgeted from the Ministry of Finance of China(MOF)and administrated by the Chinese Academy of Sciences(CAS);Natural Science Foundation of Xinjiang Uygur Autonomous Region(2022D01A360)。
We propose a multi-source radio frequency interference(RFI)mitigation method based on a reference antenna array to address the challenge of RFI from multiple directions in radio observation equipment.It introduces a s...
supported by the National Natural Science Foundation of China (Nos. 61873196 and 62373030);the Innovation Program for Quantum Science and Technology(No. 2021ZD0303400)。
In the two-dimensional positioning method of pulsars, the grid method is used to provide non-sensitive direction and positional estimates. However, the grid method has a high computational load and low accuracy due to...
funded by the Chinese Academy of Sciences(CAS)“Light of West China”Program,the Tianshan talents program(2023TSYCTD0013);The National Natural Science Foundation of China(NSFC,grant No.12288102);The Major Science and Technology Program of Xinjiang Uygur Autonomous Region(No.2022A03013-3)。
Pulsar timing offers a comprehensive avenue for exploring diverse topics in physics and astrophysics.Highprecision solar system planetary ephemeris is crucial for pulsar timing as it provides the positions and velocit...
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 National Key R&D Program of China Nos.2021YFC2203502 and 2022YFF0711502;the National Natural Science Foundation of China(NSFC)(12173077);the Tianshan Talent Project of Xinjiang Uygur Autonomous Region(2022TSYCCX0095 and2023TSYCCX0112);the Scientific Instrument Developing Project of the Chinese Academy of Sciences,grant No.PTYQ2022YZZD01;China National Astronomical Data Center(NADC);the Operation,Maintenance and Upgrading Fund for Astronomical Telescopes and Facility Instruments,budgeted from the Ministry of Finance of China(MOF)and administrated by the Chinese Academy of Sciences(CAS);Natural Science Foundation of Xinjiang Uygur Autonomous Region(2022D01A360)。
For real-time processing of ultra-wide bandwidth low-frequency pulsar baseband data,we designed and implemented an ultra-wide bandwidth low-frequency pulsar data processing pipeline(UWLPIPE)based on the shared ringbuf...