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researcher

M. Ge

122 papers hereh-index 296.4k citations170 works total

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

author position
  • first author2
  • middle author79
  • last author3

Across the 84 of 122 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE97
  • astro-ph.IM21
  • astro-ph.EP2
  • astro-ph.SR1
  • nucl-ex1
same name
  • M. Ge — 79 papers, h 22
  • M. Ge — 52 papers, h 10
  • M. Ge — 41 papers, h 18
  • M. Ge — 12 papers, h 4
  • M. Ge — 9 papers, h 11
  • M. Ge — 5 papers, h 13

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

activity
20112025
most citedThe enhanced X-ray Timing and Polarimetry mission - eXTP

329 citations · 3.4k across the 121 of their papers we have counts for

collaborators
Showing 2017Show all

4 papers · 1 filter

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…

astro-ph.HE2017

Calvera: A low-mass strangeon star torqued by debris disk?

Yunyang Li, Weiyang Wang, Mingyu Ge +3

Calvera is a 59ms isolated pulsar, being unique due to its non-detection in radio, optical and gamma-rays but the purely thermal emission in soft X-rays. It is suggest…

astro-ph.HE2017★ 43 cited

Swift observations of SMC X-3 during its 2016-2017 super-Eddington outburst

Shan-Shan Weng, Ming-Yu Ge, Hai-Hui Zhao +4

The Be X-ray pulsar, SMC X-3 underwent a giant outburst from 2016 August to 2017 March, which was monitored with the Swift satellite. During the outburst, its broadband flux increa…

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