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researcher

M. Otsuka

44 papers hereh-index 201.3k citations93 works total

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

author position
  • sole author1
  • first author13
  • middle author17
  • last author9

Across the 40 of 44 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR22
  • astro-ph.GA12
  • astro-ph3
  • astro-ph.CO3
  • astro-ph.HE3
  • astro-ph.IM1
same name
  • M. Otsuka — 5 papers
  • M. Otsuka — 4 papers, h 4
  • M. Otsuka — 3 papers, h 4
  • M. Otsuka — 1 paper, h 1
  • M. Otsuka — 1 paper, h 1
  • M. Otsuka — 1 paper

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
20062023
most citedHerschel Detects a Massive Dust Reservoir in Supernova 1987A

368 citations · 1.3k across the 44 of their papers we have counts for

collaborators
Showing astro-ph.HEShow all

3 papers · 1 filter

astro-ph.HE2021★ 19 cited

Intermediate Luminosity Type Iax SN 2019muj With Narrow Absorption Lines: Long-Lasting Radiation Associated With a Possible Bound Remnant Predicted by the Weak Deflagration Model

Miho Kawabata, Keiichi Maeda, Masayuki Yamanaka +23

We present comprehensive spectroscopic and photometric analyses of the intermediate luminosity Type Iax supernova (SN Iax) 2019muj based on multi-band datasets observed through the…

astro-ph.HE2020★ 20 cited

Calcium-rich Transient SN 2019ehk in A Star-Forming Environment: Yet Another Candidate for An Ultra-Stripped Envelope Supernova

Tatsuya Nakaoka, Keiichi Maeda, Masayuki Yamanaka +20

We present optical and near-infrared observations of SN~Ib~2019ehk. We show that it evolved to a Ca-rich transient according to its spectral properties and evolution in late phases…

astro-ph.HE2019★ 28 cited

Type Ia SN 2019ein: New Insights into the Similarities and diversities among High-Velocity SNe Ia

Miho Kawabata, Keiichi Maeda, Masayuki Yamanaka +38

We present optical observations of type Ia supernova (SN) 2019ein, starting at 2 days after the estimated explosion date. The spectra and the light curves show that SN 2019ein belo…

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