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20202023
most citedRe-estimating the Spin Parameter of the Black Hole in Cygnus X-1

57 citations · 184 across the 6 of their papers we have counts for

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6 papers · 1 filter

astro-ph.HE2023★ 11 cited

X-ray spectral correlations in a sample of Low-mass black hole X-ray binaries in the hard state

Bei You, Yanting Dong, Zhen Yan +4

The power-law emission and reflection component provide valuable insights into the accretion process around a black hole. In this work, thanks to the broadband spectra coverage of…

astro-ph.HE2022★ 17 cited

Analysis of the reflection spectra of MAXI J1535-571 in the hard and intermediate states

Yanting Dong, Zhu Liu, Youli Tuo +4

We report results on the joint-fit of the NuSTAR and HXMT data for the black hole X-ray binary candidate MAXI J1535-571. The observations were obtained in 2017 when the source evol…

astro-ph.HE2021★ 57 cited

Re-estimating the Spin Parameter of the Black Hole in Cygnus X-1

Xueshan Zhao, Lijun Gou, Yanting Dong +6

Cygnus X-1 is a well-studied persistent black hole X-ray binary. Recently, the three parameters needed to estimate the black hole spin of this system, namely the black hole mass $M…

astro-ph.HE2020★ 51 cited

Estimating the black hole spin for the X-ray binary MAXI J1820+070

Xueshan Zhao, Lijun Gou, Yanting Dong +6

MAXI J1820+070 is a newly-discovered black hole X-ray binary, whose dynamical parameters, namely the black hole mass, the inclination angle and the source distance, have been estim…

astro-ph.HE2020★ 33 cited

The spin measurement of the black hole in 4U 1543-47 constrained with the X-ray reflected emission

Yanting Dong, Javier A. García, James F. Steiner +1

4U 1543-47 is a low mass X-ray binary which harbours a stellar-mass black hole located in our Milky Way galaxy. In this paper, we revisit 7 data sets which were in the Steep Power…

astro-ph.HE2020★ 15 cited

A detailed study on the reflection component for the Black Hole Candidate MAXI J1836-194

Yanting Dong, Javier A. García, Zhu Liu +3

We present a detailed spectral analysis of the black hole candidate MAXI J1836-194. The source was caught in the intermediate state during its 2011 outburst by Suzaku and RXTE. We…