activity
20172020
most citedEAS age determination from the study of the lateral distribution of charged particles near the shower axis with the ARGO-YBJ experiment

11 citations · 14 across the 6 of their papers we have counts for

collaborators

8 papers

astro-ph.SR2020

Estimates of current helicity and tilt of solar active regions and Joy's law

K. Kuzanyan, N. Kleeorin, I. Rogachevskii +2

The tilt angle, current helicity and twist of solar magnetic fields can be observed in solar active regions. We carried out estimates of these parameters by two ways. Firstly, we c…

astro-ph.HE2020

HXMT Identification of a non-thermal X-ray burst from SGR J1935+2154 and with FRB 200428

C. K. Li, L. Lin, S. L. Xiong +117

Fast radio bursts (FRBs) are short pulses observed in radio band from cosmological distances. One class of models invoke soft gamma-ray repeaters (SGRs), or magnetars, as the sourc…

astro-ph.HE20203 cited

Insight-HXMT insight into switch of the accretion mode: the case of the X-ray pulsar 4U 1901+03

Y. L. Tuo, L. Ji, S. S. Tsygankov +116

We use the In data collected during the 2019 outburst from X-ray pulsar 4U 1901+03 to complement the orbital parameters reported by Fermi/GBM. Using the Insight-HXMT, we examine th…

astro-ph.HE2020

Joint Analysis of Energy and RMS Spectra from MAXI J1535-571 with Insight-HXMT

L. D. Kong, S. Zhang, Y. P. Chen +115

A new black hole X-ray binary (BHXRB) MAXI J1535-571 was discovered by MAXI during its outburst in 2017. Using observations taken by the first Chinese X-ray satellite, the Hard X-r…

astro-ph.HE2019

Diagnostic of the spectral properties of Aquila X-1 by Insight-HXMT snapshots during the early propeller phase

C. Güngör, M. Y. Ge, S. Zhang +108

We study the 2018 outburst of Aql X-1 via the monitor of all sky X-ray image (MAXI) data. We show that the outburst starting in February 2018 is a member of short-low class in the…

astro-ph.HE2019

-HXMT study of the timing properties of Sco X-1

S. M. Jia, Q. C. Bu, J. L. Qu +106

We present a detailed timing study of the brightest persistent X-ray source Sco X-1 using the data collected by the Hard X-ray Modulation Telescope (-HXMT) from July 2017…