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M. Ge

3 papers here

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • middle author2

Across the 2 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE3
same name
  • M. Ge — 41 papers, h 22
  • M. Ge — 3 papers, h 13
  • M. Ge — 2 papers, h 10
  • M. Ge — 1 paper, h 11
  • M. Ge — 1 paper
  • M. Ge — 1 paper, h 47

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

most citedInsight-HXMT observations of the first binary neutron star merger GW170817

64 citations · 81 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.HE2018★ 7 cited

Pulse phase-resolved analysis of SMC X-3 during its 2016--2017 super-Eddington outburst

Hai-Hui Zhao, Shan-Shan Weng, Ming-Yu Ge +2

The Be X-ray pulsar SMC X-3 underwent an extra long and ultraluminous giant outburst from 2016 August to 2017 March. The peak X-ray luminosity is up to ∼1039 erg/s, sugges…

astro-ph.HE2017★ 10 cited

Disc-corona interaction in the heartbeat state of GRS 1915+105

Shu-Ping Yan, Li Ji, Si-Ming Liu +10

Timing analysis provides information about the dynamics of matter accreting on to neutron stars and black holes, and hence is crucial for studying the physics of the accretion flow…

astro-ph.HE2017★ 64 cited

Insight-HXMT observations of the first binary neutron star merger GW170817

TiPei Li, ShaoLin Xiong, ShuangNan Zhang +107

Finding the electromagnetic (EM) counterpart of binary compact star merger, especially the binary neutron star (BNS) merger, is critically important for gravitational wave (GW) ast…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.