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researcher

K. Ohmori

47 papers hereh-index 333k citations66 works total

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

author position
  • sole author2
  • first author11
  • middle author19
  • last author11

Across the 43 of 47 papers where every author was matched, so the position is known.

fields
  • hep-th36
  • astro-ph.EP3
  • cond-mat.str-el3
  • astro-ph.GA1
  • astro-ph.SR1
  • cond-mat.stat-mech1
same name
  • K. Ohmori — 8 papers, h 8
  • K. Ohmori — 8 papers, h 5
  • K. Ohmori — 5 papers, h 25
  • K. Ohmori — 1 paper, h 4
  • K. Ohmori — 1 paper, 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
20112023
most citedKramers-Wannier-like duality defects in (3+1)d gauge theories

281 citations · 2.5k across the 47 of their papers we have counts for

collaborators
Showing astro-ph.EPShow all

3 papers · 1 filter

astro-ph.EP2012★ 77 cited

MOA-2010-BLG-477Lb: constraining the mass of a microlensing planet from microlensing parallax, orbital motion and detection of blended light

E. Bachelet, I. -G. Shin, C. Han +138

Microlensing detections of cool planets are important for the construction of an unbiased sample to estimate the frequency of planets beyond the snow line, which is where giant pla…

astro-ph.EP2012★ 27 cited

A New Type of Ambiguity in the Planet and Binary Interpretations of Central Perturbations of High-Magnification Gravitational Microlensing Events

J. -Y. Choi, I. -G. Shin, C. Han +118

High-magnification microlensing events provide an important channel to detect planets. Perturbations near the peak of a high-magnification event can be produced either by a planet…

astro-ph.EP2012★ 235 cited

MOA-2011-BLG-293Lb: A test of pure survey microlensing planet detections

J. C. Yee, Y. Shvartzvald, A. Gal-Yam +10

Because of the development of large-format, wide-field cameras, microlensing surveys are now able to monitor millions of stars with sufficient cadence to detect planets. These new…

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