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B. Matthews

9 papers hereh-index 659 citations16 works total

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

author position
  • first author1
  • middle author5
  • last author1

Across the 7 of 9 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA9
same name
  • B. Matthews — 133 papers, h 49
  • B. Matthews — 38 papers, h 13
  • B. Matthews — 13 papers, h 29
  • 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
20202025
most citedPlacing High-Redshift Quasars in Perspective: a Catalog of Spectroscopic Properties from the Gemini Near Infrared Spectrograph -- Distant Quasar Survey

24 citations · 77 across the 9 of their papers we have counts for

collaborators
Showing 2023Show all

3 papers · 1 filter

astro-ph.GA2023★ 13 cited

Gemini Near Infrared Spectrograph -- Distant Quasar Survey: Augmented Spectroscopic Catalog and a Prescription for Correcting UV-Based Quasar Redshifts

Brandon M. Matthews, Cooper Dix, Ohad Shemmer +13

Quasars at z ≳ 1 most often have redshifts measured from rest-frame ultraviolet emission lines. One of the most common such lines, C IV λ1549, shows blueshifts up to ${…

astro-ph.GA2023★ 13 cited

Shedding New Light on Weak Emission-Line Quasars in the CIV​-Hβ Parameter Space

Trung Ha, Cooper Dix, Brandon M. Matthews +20

Weak emission-line quasars (WLQs) are a subset of Type 1 quasars that exhibit extremely weak Lyα+N V λ1240 and/or C IV λ1549 emission lines. We investigate the relationship b…

astro-ph.GA2023★ 8 cited

Gemini Near Infrared Spectrograph - Distant Quasar Survey: Prescriptions for Calibrating UV-Based Estimates of Supermassive Black Hole Masses in High-Redshift Quasars

Cooper Dix, Brandon Matthews, Ohad Shemmer +10

The most reliable single-epoch supermassive black hole mass (MBH​) estimates in quasars are obtained by using the velocity widths of low-ionization emission lines, typicall…

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