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W. N. Brandt

4 papers hereh-index 362 citations8 works total

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

author position
  • middle author4

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA3
  • astro-ph.HE1
same name
  • W. N. Brandt — 22 papers, h 6
  • W. N. Brandt — 13 papers, h 6
  • W. N. Brandt — 8 papers, h 4
  • W. N. Brandt — 6 papers, h 1
  • W. N. Brandt — 6 papers, h 3
  • W. N. Brandt — 4 papers, h 4

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
20242026
collaborators

4 papers

astro-ph.HE2026

Systematic Monitoring of Extreme X-ray Variability from Weak-line Quasars

Madison Reich, W. N. Brandt, Bin Luo +4

We present the results of a multi-cycle Chandra program to systematically monitor the X-ray variability of 10 weak-line quasars (WLQs) that previously had limited multi-epoch X-ray…

astro-ph.GA2025

Departures from Standard Disk Predictions in Intensive Ground-Based Monitoring of Three AGN

Diego Gonzalez-Buitrago, Aaron J. Barth, Rick Edelson +42

We present ground-based, multi-band light curves of the AGN Mrk~509, NGC\,4151, and NGC\,4593 obtained contemporaneously with \sw\, monitoring. We measure cross-correlation lags re…

astro-ph.GA2024

A Rapidly Accreting Active Galactic Nucleus Hidden in a Dust-Obscured Galaxy at z∼0.8

Nathan Cristello, Fan Zou, William N. Brandt +3

Dust-obscured galaxies (DOGs) containing central supermassive black holes (SMBHs) that are rapidly accreting (i.e., having high Eddington ratios, I^»Edd​) may represent a…

astro-ph.GA2024

Fast SMBH growth in the SPT2349--56 protocluster at z=4.3

Fabio Vito, William N. Brandt, Andrea Comastri +7

Protoclusters at z>2 are gas-rich regions characterized by high star-formation activity. The same physical properties that enhance star formation in protoclusters are also though…

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