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B. Matthews

38 papers hereh-index 132k citations36 works total

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

author position
  • first author1
  • middle author22
  • last author2

Across the 25 of 38 papers where every author was matched, so the position is known.

fields
  • astro-ph.EP28
  • astro-ph.SR6
  • astro-ph1
  • astro-ph.CO1
  • astro-ph.GA1
  • astro-ph.IM1
same name
  • B. Matthews — 133 papers, h 49
  • B. Matthews — 13 papers, h 29
  • B. Matthews — 9 papers, h 6
  • B. Matthews — 2 papers, h 17
  • B. Matthews — 1 paper, h 3
  • B. Matthews — 1 paper, h 19

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
19972026
most citedDiscovery and spectroscopy of the young Jovian planet 51 Eri b with the Gemini Planet Imager

559 citations · 2.2k across the 35 of their papers we have counts for

collaborators
Showing 2026Show all

3 papers · 1 filter

astro-ph.IM2026

Ushering in high angular resolution observatories in the far-infrared: The case for a double-Fourier interferometer

C. S. Benson, M. Bonato, T. A. Davis +14

A far-infrared (far-IR) interferometer from a space-based platform would bring about a transformational improvement in the spatial detail of astronomical observations that are inac…

astro-ph.EP2026

The JWST Early Release Science Program for Direct Observations of Exoplanetary Systems VIII: patchy forsterite and enstatite clouds in the atmosphere of VHS 1256 b, retrieval lessons learned and outlook to the future

Niall Whiteford, Jacqueline K. Faherty, Ben Burningham +123

JWST defines a new era for the data-driven approach of retrieval modelling, which has become a cornerstone tool for the statistical inference of exoplanetary and brown dwarf proper…

astro-ph.EP2026

A radially broad collisional cascade in the debris disk of γ Ophiuchi observed by JWST

Yinuo Han, Mark Wyatt, Kate Y. L. Su +13

The A1V star γ Oph, at a distance of 29.7 pc, is known from Spitzer imaging to host a debris disk with a large radial extent and from its spectral energy distribution to host inn…

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