activity
20032025
most citedThe SCUBA HAlf Degree Extragalactic Survey (SHADES) -- I. Survey motivation, design and data processing

84 citations · 213 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.GA2025

The JWST View of Cygnus A: Jet-Driven Coronal Outflow with a Twist

Patrick M. Ogle, B. Sebastian, A. Aravindan +29

We present first results from James Webb Space Telescope (JWST) Near-Infrared Spectrograph (NIRSpec), Mid-Infrared Instrument (MIRI), and Keck Cosmic Webb Imager (KCWI) integral fi…

astro-ph.GA2023

NOEMA observations of GN-z11: Constraining Neutral Interstellar Medium and Dust Formation in the Heart of Cosmic Reionization at

Y. Fudamoto, P. A. Oesch, F. Walter +17

We present results of dust continuum and [CII] emission line observations of a remarkably UV-luminous () galaxy at : GN-z11. Using the…

astro-ph.GA2022★ 1 cited

Spectroscopy of High Redshift Galaxies with the ngVLA

C. L. Carilli, M. Neeleman

We present simulations of the capabilities of the ngVLA to image at kpc resolution (), molecular line emission from star forming disk galaxies at high redshift.…

astro-ph.GA2022★ 33 cited

The 700 ks Chandra Spiderweb Field II: Evidence for inverse-Compton and thermal diffuse emission in the Spiderweb galaxy

P. Tozzi, R. Gilli, A. Liu +22

We present the X-ray imaging and spectral analysis of the diffuse emission around the Spiderweb galaxy at z=2.16 and of its nuclear emission, based on a deep (700 ks) Chandra obser…

astro-ph.HE2018★ 10 cited

The X-ray Ribs Within the Cocoon Shock of Cygnus A

R. T. Duffy, D. M. Worrall, M. Birkinshaw +15

We use new and archival Chandra observations of Cygnus A, totalling 1.9 Ms, to investigate the distribution and temperature structure of gas lying within the projected extent…

astro-ph.CO2009

High Redshift Radio Galaxies: Laboratories for Massive Galaxy and Cluster Formation in the early Universe

G. Miley, C. Carilli, G. B. Taylor +2

High redshift radio galaxies are among the largest, most luminous, most massive, and most beautiful objects in the Universe. They are generally identified from their radio emission…