Fast radio bursts(FRBs) were first discovered(Lorimer et al. 2007) serendipitously during a search for radio pulses in archival data in 2007. In the intervening period, FRBs have become an active area of astrophysical...Fast radio bursts(FRBs) were first discovered(Lorimer et al. 2007) serendipitously during a search for radio pulses in archival data in 2007. In the intervening period, FRBs have become an active area of astrophysical research that has attracted a diverse community of several hundred astronomers around the world.展开更多
The Five-hundred-meter Aperture Spherical Telescope （FAST） will begin its early-science oper- ations during 2016. Drift-scan pulsar surveys will be carried out during this period using an ultra-wide-band receiver sy...The Five-hundred-meter Aperture Spherical Telescope （FAST） will begin its early-science oper- ations during 2016. Drift-scan pulsar surveys will be carried out during this period using an ultra-wide-band receiver system （covering - 270 to 1620 MHz）. We describe a method for accounting for the changes in the telescope beam shape and the pulsar parameters when searching for pulsars over such a wide bandwidth. We applied this method to simulated data sets of pulsars in globular clusters that are visible to FAST and found that a representative observation would have a sensitivity of -40 ply. Our results showed that a sin- gle drift-scan （lasting less than a minute） is likely to find at least one pulsar for observations of four globular clusters. Repeated observations will increase the likely number of detections. We found that pulsars in - 16 clusters are likely to be found if the data from 100 drift-scan observations of each cluster are incoherently combined.展开更多
文摘Fast radio bursts(FRBs) were first discovered(Lorimer et al. 2007) serendipitously during a search for radio pulses in archival data in 2007. In the intervening period, FRBs have become an active area of astrophysical research that has attracted a diverse community of several hundred astronomers around the world.
基金the support from the professorship award under the Chinese Academy of Sciences(CAS) President's International Fellowship Initiative(PIFI) in 2015the support from the Guizhou Scientific Collaboration Program (No.20130421)+3 种基金the support from the National Natural Science Foundation of China(NSFC, Nos.11305133 and 11273020)the support from NSFC(No.Y411101N01)the support from NSFC(No.11103045)grants from NSFC (No.11373038)the support by National Basic Research Program of China(973 program) Nos.2012CB821800 and 2015CB57100
文摘The Five-hundred-meter Aperture Spherical Telescope （FAST） will begin its early-science oper- ations during 2016. Drift-scan pulsar surveys will be carried out during this period using an ultra-wide-band receiver system （covering - 270 to 1620 MHz）. We describe a method for accounting for the changes in the telescope beam shape and the pulsar parameters when searching for pulsars over such a wide bandwidth. We applied this method to simulated data sets of pulsars in globular clusters that are visible to FAST and found that a representative observation would have a sensitivity of -40 ply. Our results showed that a sin- gle drift-scan （lasting less than a minute） is likely to find at least one pulsar for observations of four globular clusters. Repeated observations will increase the likely number of detections. We found that pulsars in - 16 clusters are likely to be found if the data from 100 drift-scan observations of each cluster are incoherently combined.
