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researcher

M. Hayashi

7 papers hereh-index 9598 citations42 works total

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

author position
  • middle author5

Across the 5 of 7 papers where every author was matched, so the position is known.

fields
  • astro-ph.EP3
  • astro-ph.SR3
  • astro-ph.IM1
same name
  • M. Hayashi — 96 papers, h 35
  • M. Hayashi — 90 papers, h 50
  • M. Hayashi — 56 papers, h 39
  • M. Hayashi — 23 papers, h 9
  • M. Hayashi — 17 papers, h 15
  • M. Hayashi — 12 papers, 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
20122018
most citedDirect Imaging Discovery of a `Super-Jupiter' Around the late B-Type Star Kappa And

204 citations · 649 across the 7 of their papers we have counts for

collaborators
Showing 2012Show all

3 papers · 1 filter

astro-ph.SR2012★ 204 cited

Direct Imaging Discovery of a `Super-Jupiter' Around the late B-Type Star Kappa And

J. Carson, C. Thalmann, M. Janson +52

We present the direct imaging discovery of an extrasolar planet, or possible low-mass brown dwarf, at a projected separation of 55 +/- 2 AU (1.058 +/- 0.007 arcsec) from the B9-typ…

astro-ph.IM2012★ 62 cited

New Techniques for High-Contrast Imaging with ADI: the ACORNS-ADI SEEDS Data Reduction Pipeline

Timothy D. Brandt, Michael W. McElwain, Edwin L. Turner +44

We describe Algorithms for Calibration, Optimized Registration, and Nulling the Star in Angular Differential Imaging (ACORNS-ADI), a new, parallelized software package to reduce hi…

astro-ph.SR2012★ 49 cited

High-Contrast NIR Polarization Imaging of MWC480

N. Kusakabe, C. A. Grady, M. L. Sitko +52

One of the key predictions of modeling from the IR excess of Herbig Ae stars is that for protoplanetary disks, where significant grain growth and settling has occurred, the dust di…

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