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researcher

B. Norris

65 papers hereh-index 263.2k citations167 works total

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

author position
  • first author5
  • middle author51
  • last author1

Across the 57 of 65 papers where every author was matched, so the position is known.

fields
  • astro-ph.IM55
  • astro-ph.SR6
  • astro-ph.EP1
  • astro-ph.GA1
  • physics.optics1
  • physics.pop-ph1
same name
  • B. Norris — 23 papers, h 25
  • B. Norris — 5 papers, h 10
  • B. Norris — 3 papers
  • B. Norris — 1 paper, h 2
  • B. Norris — 1 paper, h 3
  • B. Norris — 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

activity
20102026
most citedSouthern Massive Stars at High Angular Resolution: Observational Campaign and Companion Detection

615 citations · 2.7k across the 64 of their papers we have counts for

collaborators
Showing 2012Show all

3 papers · 1 filter

astro-ph.IM2012★ 67 cited

Starlight Demonstration of the Dragonfly Instrument: an Integrated Photonic Pupil Remapping Interferometer for High Contrast Imaging

N. Jovanovic, P. G. Tuthill, B. Norris +13

In the two decades since the first extra-solar planet was discovered, the detection and characterization of extra-solar planets has become one of the key endeavors in all of modern…

astro-ph.IM2012★ 26 cited

Design of Optically Path Length Matched, Three-Dimensional Photonic Circuits Comprising Uniquely Routed Waveguides

Ned Charles, Nemanja Jovanovic, Simon Gross +6

A method for designing physically path length matched, three-dimensional photonic circuits is described. We focus specifically on the case where all the waveguides are uniquely rou…

astro-ph.SR2012★ 198 cited

A close halo of large transparent grains around extreme red giant stars

Barnaby R. M. Norris, Peter G. Tuthill, Michael J. Ireland +6

Intermediate-mass stars end their lives by ejecting the bulk of their envelope via a slow dense wind back into the interstellar medium, to form the next generation of stars and pla…

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