activity
20242026
most citedHidden in Pixels I: Discovery of dual "little red dots" indicates excess clustering on kilo-parsec scales

3 citations · 3 across the 2 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2026

ASKAP discovery of a pair of large radio bubbles: on the origin of odd radio circles

Renzhi Su, Minfeng Gu, Hengxiao Guo +9

We report the serendipitous discovery of a large, low-surface-brightness radio bubble in 944 MHz continuum data from the ASKAP Evolutionary Map of the Universe (EMU) survey. The st…

cs.AI2026

A systematic evaluation of vision-language models for observational astronomical reasoning tasks

Wenke Ren, Hengxiao Guo, Wenwen Zuo +1

Vision-language models (VLMs) are increasingly proposed as general-purpose tools for scientific data interpretation, yet their reliability on real astronomical observations across…

astro-ph.GA20263 cited

Hidden in Pixels I: Discovery of dual "little red dots" indicates excess clustering on kilo-parsec scales

Takumi S. Tanaka, John D. Silverman, Kazuhiro Shimasaku +56

``Little Red Dots'' (LRDs) are an abundant high-redshift population newly discovered by the James Webb Space Telescope (JWST) and considered to be an early growth phase of supermas…

astro-ph.GA2025

The ALPINE-CRISTAL-JWST Survey: Revealing Less Massive Black Holes in High-Redshift Galaxies

Wenke Ren, John D. Silverman, Andreas L. Faisst +25

We present a systematic search for broad-line active galactic nuclei (AGNs) in the ALPINE-CRISTAL-JWST sample of 18 star-forming galaxies () at redshift…

astro-ph.GA2024

Prior-Informed AGN-Host Spectral Decomposition Using PyQSOFit

Wenke Ren, Hengxiao Guo, Yue Shen +4

We introduce an improved method for decomposing the emission of active galactic nuclei (AGN) and their host galaxies using templates from principal component analysis (PCA). This a…

astro-ph.HE2024

Systematic Collapse of the Accretion Disc Across the Supermassive Black Hole Population

Scott Hagen, Chris Done, John D. Silverman +7

The structure of the accretion flow onto supermassive black holes (SMBH) is not well understood. Standard disc models match to zeroth order in predicting substantial energy dissipa…