Five-hundred-meter Aperture Spherical radio Telescope (FAST, Nan et al. 2011) is the largest single-dish radio telescope in the world, starting to achieve in the studies of pulsars and fast radio bursts (Qian et al. 2020).

We report the discovery of a highly dispersed fast radio burst (FRB), FRB 181123, from an analysis of ∼1500hr of drift scan survey data taken using the Five-hundred-meter Aperture Spherical radio Telescope (FAST).

innovative feed cabin for China’s Five-hundred-meter Aperture Spherical radio Telescope (FAST), we performed the SETI rst observations with FAST’s newly commisioned 19-beam receiver; we report preliminary results in this paper.

radio Telescope (FAST; Nan 2006; Nan et al. 2011; Jiang et al. 2019) is the largest filled-aperture single-dish radio antenna in the world, with its sensitivity and observable sky coverage both surpassing

The Five-hundred-meter Aperture Spherical radio Telescope (FAST), the largest single-dish radio telescope in the world, has implemented an innovative technology for its huge reflector, which changes the shape of the primary reflector from spherical to

CRAFTS pulsars using FAST radio telescope. The aim of this proposal is to study pulse-shape variability and pulse phenomena, such as timing noises, glitches, mode changing, nulling, and subpulse drifting. The correlation between the rotation irregularities and pulse phenomena will be examined. FAST will enable us to determine

by the Parkes radio telescope on the 10th September, 2017. This pulsar, named PSR J1900-0134, was the first pulsar dis-covered by FAST. The pulsar has a pulse period of 1.8s and a dispersion measure (DM) of 188pccm−3. The search for radio pulsars is one of the main science pursuits for FAST [2]. With the growing population of pul-

environment of FRB progenitor. Using the FAST radio telescope, we detected a few bursts from 2023 to 2024 and confirm the decreasing trends of both DM and RM. Here we propose to continue monitoring FRB 20180301A with the FAST telescope by accomplishing science cases like completing the DM/RM evolution, deciphering the spectro-polarimetric ...

The FAST All Sky HI survey (FASHI) was designed to cover the entire sky observable by the Five-hundred-meter Aperture Spherical radio Telescope (FAST), spanning approximately 22000 square degrees of declination between 14 and +66 , and in the frequency range of 1050-1450MHz, with the expectation of eventually detecting more than 100000 HI ...

The Five-hundred-meter Aperture Spherical radio Telescope (FAST) is expected to complete its commissioning in 2019. FAST will soon begin the Commensal Radio Astronomy FasT Survey (CRAFTS), a novel and unprecedented commensal drift scan survey of …