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researcher

L. Ji

4 papers hereh-index 202k citations108 works total

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

author position
  • middle author2

Across the 2 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE3
  • astro-ph.CO1
same name
  • L. Ji — 11 papers, h 20
  • L. Ji — 10 papers, h 11
  • L. Ji — 2 papers, h 20
  • L. Ji — 2 papers, h 16
  • L. Ji — 1 paper
  • L. Ji — 1 paper, h 2

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
20152019
most citedAccretion disks and coronae in the X-ray flashlight

92 citations · 149 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.HE2019★ 35 cited

Insight-HXMT observations of Swift J0243.6+6124 during its 2017-2018 outburst

Yue Zhang, Mingyu Ge, Liming Song +107

The recently discovered neutron star transient Swift J0243.6+6124 has been monitored by {\it the Hard X-ray Modulation Telescope} ({\it Insight-\rm HXMT). Based on the obtained dat…

astro-ph.HE2017★ 92 cited

Accretion disks and coronae in the X-ray flashlight

N. Degenaar, D. R. Ballantyne, T. Belloni +10

Plasma accreted onto the surface of a neutron star can ignite due to unstable thermonuclear burning and produce a bright flash of X-ray emission called a Type-I X-ray burst. Such e…

astro-ph.HE2015★ 20 cited

Diagnosing the burst influence upon accretion in the clocked burster GS 1826--238

Long Ji, Shu Zhang, YuPeng Chen +6

Type-I X-ray bursts on the surface of a neutron star are a unique probe to the accretion in X-ray binary systems. However, we know little about the feedback of the burst emission u…

astro-ph.CO2015★ 2 cited

Chandra and XMM-Newton observations of the merging cluster of galaxies PLCK G036.7+14.9

B. Zhang, L. P. David, C. Jones +13

We present Chandra and XMM-Newton observations of PLCK G036.7+14.9 from the Chandra-Planck Legacy Program. The high resolution X-ray observations reveal two close subclusters, G036…

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