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researcher

B. Mason

18 papers hereh-index 6225 citations21 works total

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

author position
  • middle author15
  • last author1

Across the 16 of 18 papers where every author was matched, so the position is known.

fields
  • astro-ph.CO7
  • astro-ph.GA6
  • astro-ph3
  • astro-ph.HE2
same name
  • B. Mason — 67 papers, h 25
  • B. Mason — 43 papers, h 39
  • B. Mason — 10 papers, h 6
  • B. Mason — 8 papers, h 6
  • B. Mason — 5 papers, h 6
  • B. Mason — 1 paper, h 15

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
20002026
most citedThe Star Formation in Radio Survey: GBT 33 GHz Observations of Nearby Galaxy Nuclei and Extranuclear Star-Forming Regions

104 citations · 386 across the 18 of their papers we have counts for

collaborators
Showing 2025Show all

3 papers · 1 filter

astro-ph.HE2025

Exploring a Cosmic-Ray Inverse-Compton Origin to the SZ-to-X-Ray Pressure Deficit in the Cool Core Cluster ZwCl 3146

Emily M. Silich, Jack Sayers, Philip F. Hopkins +4

We explore the possibility that inverse-Compton (IC) scattering of cosmic microwave background photons by ∼GeV cosmic rays (CRs) injected by the central active galactic nucleu…

astro-ph.GA2025

The Star Formation in Radio Survey: Adding 90 GHz Data to 3-33 GHz Observations of Star-forming Regions in Nearby Galaxies

Anna Dignan, Eric J. Murphy, Brian Mason +10

We present 90 GHz continuum imaging of 119 star-forming regions in 30 nearby galaxies observed with MUSTANG-2 on the Robert C. Byrd Green Bank Telescope as part of the Star Formati…

astro-ph.GA2025

The SUPERCOLD-CGM survey: II. [\ion{C}{1}](1−0) emission and the physical conditions of cold gas in Enormous Lyα nebulae at z∼2

Jianan Li, Bjorn H. C. Emonts, Zheng Cai +13

We report ALMA and ACA observations of atomic carbon ([\ion{C}{1}](1−0)) and dust continuum in 10 Enormous Lyα Nebulae hosting ultra-luminous Type-I QSOs at z=2.2−2.5, as par…

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