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Fang Lu

5 papers hereh-index 219 citations3 works total

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

author position
  • first author1
  • middle author2
  • last author1

Across the 4 of 5 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE3
  • astro-ph1
  • astro-ph.GA1
same name
  • Fang Lu — 3 papers
  • Fang Lu — 3 papers, h 4
  • Fang Lu — 2 papers, h 6
  • Fang Lu — 2 papers, h 7
  • Fang Lu — 2 papers, h 3
  • Fang Lu — 1 paper, h 4

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
20042026
most citedEvolution of the X-ray Profile of the Crab Pulsar

21 citations · 48 across the 5 of their papers we have counts for

collaborators
Showing astro-ph.HEShow all

3 papers · 1 filter

astro-ph.HE2021★ 9 cited

Timing and spectral variability of high mass X-ray pulsar GX 301--2 over orbital phases observed by Insight-HXMT

Y. Z. Ding, W. Wang, P. R. Epili +7

We report the orbital X-ray variability of high mass X-ray binary (HMXB) GX301--2. GX301--2 undergone a spin up process in 2018--2020 with the period evolving from ∼ 685 s to…

astro-ph.HE2019★ 21 cited

Evolution of the X-ray Profile of the Crab Pulsar

M. Y. Ge, L. L. Yan, F. J. Lu +5

Using the archive data from the Rossi X-ray Timing Explorer ({\sl RXTE}), we have studied the evolution of the X-ray profile of the Crab pulsar in a time span of 11 years. The X-ra…

astro-ph.HE2015★ 4 cited

Reverse-Shock in Tycho's Supernova Remnant

F. J. Lu, M. Y. Ge, S. J. Zheng +3

Thermal X-ray emission from young supernova remnants (SNRs) is usually dominated by the emission lines of the supernova (SN) ejecta, which are widely believed being crossed and thu…

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