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W. Ho

103 papers hereh-index 469.8k citations178 works total

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

author position
  • sole author8
  • first author30
  • middle author40
  • last author16

Across the 94 of 103 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE67
  • astro-ph18
  • astro-ph.SR13
  • gr-qc3
  • hep-ph1
  • nucl-ex1
same name
  • W. Ho — 34 papers, h 25
  • W. Ho — 19 papers, h 7
  • W. Ho — 10 papers, h 18
  • W. Ho — 9 papers, h 12
  • W. Ho — 3 papers, h 3
  • W. Ho — 2 papers, h 3

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
19982023
most citedA NICER View of PSR J0030+0451: Millisecond Pulsar Parameter Estimation

1.7k citations · 8.6k across the 103 of their papers we have counts for

collaborators
Showing 2001Show all

4 papers · 1 filter

astro-ph2001★ 21 cited

BVRI Photometry of Supernovae

Wynn C. G. Ho, Schuyler D. Van Dyk, Chien Y. Peng +5

We present optical photometry of one Type IIn supernova (1994Y) and nine Type Ia supernovae (1993Y, 1993Z, 1993ae, 1994B, 1994C, 1994M, 1994Q, 1994ae, and 1995D). SN 1993Y and SN 1…

astro-ph2001★ 99 cited

Resonant Conversion of Photon Modes Due to Vacuum Polarization in a Magnetized Plasma: Implications for X-Ray Emission from Magnetars

Dong Lai, Wynn C. G. Ho

It is known that vacuum polarization can modify the photon propagation modes in the atmospheric plasma of a strongly magnetized neutron star. A resonance occurs when the effect of…

astro-ph2001★ 84 cited

A Search for Rapid Photometric Variability in Symbiotic Binaries

J. L. Sokoloski, Lars Bildsten, Wynn C. G. Ho

We report on our survey for rapid (time scale of minutes) photometric variability in symbiotic binaries. These binaries are becoming an increasingly important place to study accret…

astro-ph2001★ 158 cited

Atmospheres and Spectra of Strongly Magnetized Neutron Stars

Wynn C. G. Ho, Dong Lai

We construct atmosphere models for strongly magnetized neutron stars with surface fields B∼1012−1015 G and effective temperatures Teff​∼106−107 K. The atm…

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