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W. Dunn

3 papers hereh-index 340 citations4 works total

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

author position
  • middle author3

Across the 3 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.EP2
  • astro-ph.SR1
same name
  • W. Dunn — 9 papers, h 16
  • W. Dunn — 3 papers, h 4
  • W. Dunn — 1 paper, h 2
  • W. Dunn — 1 paper, h 5
  • W. Dunn — 1 paper, h 2

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

most citedOriginal Research By Young Twinkle Students (ORBYTS): Ephemeris Refinement of Transiting Exoplanets

36 citations · 48 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.SR2022★ 2 cited

Quantifying the dust in SN 2012aw and iPTF14hls with ORBYTS

Maria Niculescu-Duvaz, M. J. Barlow, W. Dunn +32

Core-collapse supernovae (CCSNe) are potentially capable of producing large quantities of dust, with strong evidence that ejecta dust masses can grow significantly over extended pe…

astro-ph.EP2020★ 10 cited

Original Research By Young Twinkle Students (ORBYTS): Ephemeris Refinement of Transiting Exoplanets II

Billy Edwards, Lara Anisman, Quentin Changeat +60

We report follow-up observations of four transiting exoplanets, TRES-2b, HAT-P-22b, HAT-P-36b and XO-2b, as part of the Original Research By Young Twinkle Students (ORBYTS) program…

astro-ph.EP2020★ 36 cited

Original Research By Young Twinkle Students (ORBYTS): Ephemeris Refinement of Transiting Exoplanets

Billy Edwards, Quentin Changeat, Kai Hou Yip +60

We report follow-up observations of transiting exoplanets that have either large uncertainties (>10 minutes) in their transit times or have not been observed for over three years.…

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