activity
20152026
most citedLACEwING: A New Moving Group Analysis Code

93 citations · 364 across the 65 of their papers we have counts for

collaborators
Showing 2023Show all

8 papers · 1 filter

astro-ph.GA2023

JWST and ALMA discern the assembly of structural and obscured components in a high-redshift starburst galaxy

Zhaoxuan Liu, John D. Silverman, Emanuele Daddi +27

We present observations and analysis of the starburst, PACS-819, at z=1.45 ( M), using high-resolution (; 0.8 kpc) ALMA and multi-wav…

astro-ph.GA20231 cited

ACOSMOS: the infrared luminosity function and dust-obscured star formation rate density at

A. Traina, C. Gruppioni, I. Delvecchio +16

Aims: We leverage the largest available Atacama Large Millimetre/submillimetre Array (ALMA) survey from the archive (ACOSMOS) to study to study infrared luminosity function and…

astro-ph.GA2023

Uncovering a Massive z~7.7 Galaxy Hosting a Heavily Obscured Radio-Loud QSO Candidate in COSMOS-Web

Erini Lambrides, Marco Chiaberge, Arianna Long +47

In this letter, we report the discovery of the highest redshift, heavily obscured, radio-loud AGN candidate selected using JWST NIRCam/MIRI, mid-IR, sub-mm, and radio imaging in th…

astro-ph.GA202312 cited

Efficient NIRCam Selection of Quiescent Galaxies at 3 < z < 6 in CEERS

Arianna S. Long, Jacqueline Antwi-Danso, Erini L. Lambrides +30

Substantial populations of massive quiescent galaxies at challenge our understanding of rapid galaxy growth and quenching over short timescales. In order to piece together…

astro-ph.GA2023

Resolving galactic-scale obscuration of X-ray AGN at with COSMOS-Web

John D. Silverman, Vincenzo Mainieri, Xuheng Ding +25

A large fraction of the accreting supermassive black hole population is shrouded by copious amounts of gas and dust, particularly in the distant () Universe. While much…

astro-ph.GA2023

Powerful Radio-Loud Quasars are Triggered by Galaxy Mergers in the Cosmic Bright Ages

Peter Breiding, Marco Chiaberge, Erini Lambrides +14

While supermassive black holes are ubiquitous features of galactic nuclei, only a small minority are observed during episodes of luminous accretion. The physical mechanism(s) drivi…