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researcher

N. Wang

4 papers hereh-index 00 citations0 works total

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

author position
  • middle author4

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

fields
  • astro-ph.HE3
  • hep-ph1
same name
  • N. Wang — 95 papers, h 3
  • N. Wang — 66 papers, h 21
  • N. Wang — 35 papers, h 56
  • N. Wang — 24 papers, h 13
  • N. Wang — 21 papers, h 18
  • N. Wang — 11 papers, h 7

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
20152021
most citedThe Spin-down State Change and Mode Change Associated with Glitch Activity of PSR B2035+36

37 citations · 79 across the 3 of their papers we have counts for

collaborators

4 papers

astro-ph.HE2021★ 22 cited

Unusual Emission Variations Near the Eclipse of A Black Widow PSR J1720−0533

S. Q. Wang, J. B. Wang, N. Wang +15

We report on an {unusually} bright observation of PSR J1720−0533 using the Five-hundred-meter Aperture Spherical radio Telescope (FAST). The pulsar is in a black widow system tha…

astro-ph.HE2018★ 37 cited

The Spin-down State Change and Mode Change Associated with Glitch Activity of PSR B2035+36

F. F. Kou, J. P. Yuan, N. Wang +2

We presented timing results of PSR B2035+36 using ~9-yr observations with the Nanshan 25-m radio telescope. PSR B2035+36 was reported to exhibit significant changes in pulse profil…

astro-ph.HE2016★ 20 cited

Pulse profiles and timing of PSR J1757−2421

J. P. Yuan, R. N. Manchester, N. Wang +4

Pulse arrival time measurements over fourteen years with the Nanshan 25-m and Parkes 64-m radio telescopes have been used to determine the average profile and timing properties for…

hep-ph2015

The Effects of Superhigh Magnetic Fields on Equations of States of Neutron Stars

Z. F. Gao, N. Wang, Y. Xu +2

By introducing Dirac ?-function in superhigh magnetic field, we deduce a general formula for pressure of degenerate and relativistic electrons, Pe, which is suitable for superhigh…

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