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W. N. Brandt

4 papers hereh-index 117 citations7 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 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA4
same name
  • W. N. Brandt — 16 papers, h 6
  • W. N. Brandt — 8 papers, h 4
  • W. N. Brandt — 7 papers, h 6
  • W. N. Brandt — 3 papers, h 4
  • W. N. Brandt — 2 papers, h 6
  • W. N. Brandt — 2 papers, h 3

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

collaborators

4 papers

astro-ph.GA2026

Radial gradients revealed by mutliscale outflows from down-the-barrel spectroscopy toward a quasar at redshift 3.4

Weimin Yi, Paola Rodriguez Hidalgo, Chen Chen +9

Active galactic nucleus(AGN) feedback is a key ingredient in galaxy formation models and simulations. From an observational point of view, however, the channels of AGN feedback cou…

astro-ph.GA2026

Investigating the role of turbulence in the interstellar medium in z∼3 dusty star-forming galaxies using kpc-resolution ALMA dust and gas maps

B. A. Westoby, J. A. Hodge, P. Sharda +29

We present ALMA high-resolution (∼0.25′′/2 kpc) CO(5-4) and CO(4-3) observations of three z∼3 submillimetre-selected dusty galaxies from the ALESS survey.…

astro-ph.GA2026

A Rare Eddington-Limited, Heavily Obscured Low-Mass Active Galactic Nucleus Likely Triggered by a Galaxy Merger

Shouyi Wang, Fan Zou, Chang-Hao Chen +7

We report a detailed analysis of GAMA 376183, a powerful, heavily obscured active galactic nucleus (AGN) hosted by a low-mass galaxy (M⋆​≈1010 M⊙​) likely ex…

astro-ph.GA2026

ALESS--JWST: Dust-driven Morphologies and Hidden Stellar Mass in z∼3 Sub-millimeter Galaxies

J. Li, E. da Cunha, J. A. Hodge +17

We present JWST/NIRCam and MIRI observations of twelve z∼3 sub-millimeter galaxies (SMGs) from the ALESS survey, combined with high-resolution (0.08′′−0.16′′) ALMA 870I^¼m…

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