GRB 200612A could be classified as an ultralong gamma-ray burst due to its prompt emission lasting up to~1020 s and the true timescale of the central engine activity t_(burst)≥4×10^(4) s.The late X-ray light cur...GRB 200612A could be classified as an ultralong gamma-ray burst due to its prompt emission lasting up to~1020 s and the true timescale of the central engine activity t_(burst)≥4×10^(4) s.The late X-ray light curve with a decay index ofα=7.53 is steeper than the steepest possible decay from an external shock model.We propose that this X-ray afterglow can be driven by dipolar radiation from the magnetar spindown during its early stage,while the magnetar collapsed into the black hole before its spindown,resulting in a very steep decay of the late X-ray light curve.The optical data show that the light curve is still rising after 1.1 ks,suggesting a late onset.We show that GRB 200612A’s optical afterglow light curve is fitted with the forward shock model by Gaussian structured off-axis jet.This is a special case among GRBs,as it may be an ultralong gamma-ray burst powered by a magnetar in an off-axis observation scenario.展开更多
GRB 190530A was jointly observed by the High Energy X-ray Telescope of the Hard X-ray Modulation Telescope(Insight-HXMT/HE)and the Ground-Based Wide-Angle Camera network(GWAC-N)with the extremely large field of view.A...GRB 190530A was jointly observed by the High Energy X-ray Telescope of the Hard X-ray Modulation Telescope(Insight-HXMT/HE)and the Ground-Based Wide-Angle Camera network(GWAC-N)with the extremely large field of view.After triggered by Insight-HXMT/HE and Fermi/GBM,we observed the optical emission of GRB 190530A,using the 30 cm telescope of GWAC(GWAC-F30)to search and locate its position.Subsequent observation of the late afterglow of GRB 190530A was made with the 2.16 m telescope at Xinglong Observatory.In this paper,we make a detailed exploration of the origin of GRB 190530A.In the prompt emission,a“double-tracking”pattern is presented both for the low-energy spectral indexαand the peak energy Epin the Band function with Insight-HXMT/HE and Fermi/GBM data;the results of GRB 190530A are consistent with the Amati and Yonetoku correlations;the spectral lag(τ)versus energy(E)can be estimated withτ=-3.0±0.06+(0.17±0.03)logE.The synchrotron radiation can account for the origin of GRB190530A prompt emission behaviors.Theαand Epof the precursor are essentially the same as that of the main prompt emission,implying that they have the same origin.For the afterglow,it can be described with the external forward shock model in ISM circumburst medium.In summary,from precursor,prompt emission to afterglow of GRB 190530A all originated from synchrotron radiation.展开更多
Influenza viruses(FLUV)cause high morbidity and mortality annually in the world and pose a serious threat to the public health.Wuhan,as an important transportation hub in China,has a dense population and suitable clim...Influenza viruses(FLUV)cause high morbidity and mortality annually in the world and pose a serious threat to the public health.Wuhan,as an important transportation hub in China,has a dense population and suitable climate,which also lays a major hidden danger for the outbreak of influenza.To survey and characterize the seasonal FLUV in Wuhan during 2016–2019,we collected 44,738 throat swabs,among which 15.5%were influenza A(FLUAV)positive,6.1%influenza B(FLUBV)and 0.3%co-infection.By monitoring FLUV in each month from June 2016 to May 2019,different with the previously seasonality pattern,only a single influenza peak was appeared in winter of 2017–2018 and 2018–2019,respectively.These data indicated that the complex circulation pattern of seasonal influenza in Wuhan.In addition,we found the age group was skewed towards 5–14 years group whose activity were mostly school based,which suggested school may be an important place for influenza outbreaks.Meanwhile,phylogenic analysis revealed that two subtypes(subclade 3C.2 a2 and 3C.2 a1b)of A(H3N2)were circulating in Wuhan and there was an obvious transition in 2018 because the two subclades were detected simultaneously.Furthermore,by estimating the vaccine effectiveness,we found that the vaccine strain of FLUAV didn’t seem to match very well the current epidemic strain,especially A(H3N2).Hence,more accurate prediction of seasonal outbreak is essential for vaccine design.Taken together,our results provided the current information about seasonal FLUV in Wuhan which form the basis for vaccine updating.展开更多
基金supported by the National Natural Science Foundation of China(Nos.U1938201 and 12373042)。
文摘GRB 200612A could be classified as an ultralong gamma-ray burst due to its prompt emission lasting up to~1020 s and the true timescale of the central engine activity t_(burst)≥4×10^(4) s.The late X-ray light curve with a decay index ofα=7.53 is steeper than the steepest possible decay from an external shock model.We propose that this X-ray afterglow can be driven by dipolar radiation from the magnetar spindown during its early stage,while the magnetar collapsed into the black hole before its spindown,resulting in a very steep decay of the late X-ray light curve.The optical data show that the light curve is still rising after 1.1 ks,suggesting a late onset.We show that GRB 200612A’s optical afterglow light curve is fitted with the forward shock model by Gaussian structured off-axis jet.This is a special case among GRBs,as it may be an ultralong gamma-ray burst powered by a magnetar in an off-axis observation scenario.
基金supported by the Open Project Program of the Key Laboratory of Optical Astronomy,National Astronomical Observatories,Chinese Academy of Sciencessupported by the National Key R&D Program of China(grant No.2021YFA0718500)+3 种基金the National Natural Science Foundation of China(grant Nos.U1938201,12103055,11863007 and 11973055)the Guangxi Science Foundation(grant No.2018GXNSFGA281007)the Innovation Project of Guangxi Graduate Education(grant No.YSCW2019050)the Teaching reform project of Guangxi Higher Education(grant No.2019JGZ102)。
文摘GRB 190530A was jointly observed by the High Energy X-ray Telescope of the Hard X-ray Modulation Telescope(Insight-HXMT/HE)and the Ground-Based Wide-Angle Camera network(GWAC-N)with the extremely large field of view.After triggered by Insight-HXMT/HE and Fermi/GBM,we observed the optical emission of GRB 190530A,using the 30 cm telescope of GWAC(GWAC-F30)to search and locate its position.Subsequent observation of the late afterglow of GRB 190530A was made with the 2.16 m telescope at Xinglong Observatory.In this paper,we make a detailed exploration of the origin of GRB 190530A.In the prompt emission,a“double-tracking”pattern is presented both for the low-energy spectral indexαand the peak energy Epin the Band function with Insight-HXMT/HE and Fermi/GBM data;the results of GRB 190530A are consistent with the Amati and Yonetoku correlations;the spectral lag(τ)versus energy(E)can be estimated withτ=-3.0±0.06+(0.17±0.03)logE.The synchrotron radiation can account for the origin of GRB190530A prompt emission behaviors.Theαand Epof the precursor are essentially the same as that of the main prompt emission,implying that they have the same origin.For the afterglow,it can be described with the external forward shock model in ISM circumburst medium.In summary,from precursor,prompt emission to afterglow of GRB 190530A all originated from synchrotron radiation.
基金supported by the Fundamental Research Funds for the Central Universities and the National key research and development program of China(2018TFE0204500)
文摘Influenza viruses(FLUV)cause high morbidity and mortality annually in the world and pose a serious threat to the public health.Wuhan,as an important transportation hub in China,has a dense population and suitable climate,which also lays a major hidden danger for the outbreak of influenza.To survey and characterize the seasonal FLUV in Wuhan during 2016–2019,we collected 44,738 throat swabs,among which 15.5%were influenza A(FLUAV)positive,6.1%influenza B(FLUBV)and 0.3%co-infection.By monitoring FLUV in each month from June 2016 to May 2019,different with the previously seasonality pattern,only a single influenza peak was appeared in winter of 2017–2018 and 2018–2019,respectively.These data indicated that the complex circulation pattern of seasonal influenza in Wuhan.In addition,we found the age group was skewed towards 5–14 years group whose activity were mostly school based,which suggested school may be an important place for influenza outbreaks.Meanwhile,phylogenic analysis revealed that two subtypes(subclade 3C.2 a2 and 3C.2 a1b)of A(H3N2)were circulating in Wuhan and there was an obvious transition in 2018 because the two subclades were detected simultaneously.Furthermore,by estimating the vaccine effectiveness,we found that the vaccine strain of FLUAV didn’t seem to match very well the current epidemic strain,especially A(H3N2).Hence,more accurate prediction of seasonal outbreak is essential for vaccine design.Taken together,our results provided the current information about seasonal FLUV in Wuhan which form the basis for vaccine updating.
