activity
19972025
most citedOptical Spectroscopy of Type Ia Supernovae

148 citations · 1.1k across the 35 of their papers we have counts for

collaborators

35 papers

astro-ph.HE2025

Accretion and Jet Coupling in Powerful Radio Quasars at Cosmic Noon

Mojegan Azadi, Belinda Wilkes, Joanna Kuraszkiewicz +2

We present bolometric corrections, as a function of wavelength, for powerful radio-loud quasars from the Revised Third Cambridge Catalogue of Radio Galaxies (3CRR) at 1 < z < 2. Th…

astro-ph.GA2025

A Bolometric Luminosity Correction Recipe for AGN at Any Epoch

Mojegan Azadi, Belinda Wilkes, Joanna Kuraszkiewicz +2

Understanding how active galactic nuclei (AGN) affect their host galaxies requires determining their total radiative power across all wavelengths (i.e., bolometric luminosities). W…

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.GA2024★ 1 cited

A Multiwavelength Portrait of the 3C 220.3 Lensed System

Sóley Ó. Hyman, Belinda J. Wilkes, S. P. Willner +10

The 3C 220.3 system is a rare case of a foreground narrow-line radio galaxy ("galaxy A," ) lensing a background submillimeter galaxy (). New spe…

astro-ph.SR2023

The Mass-Temperature Relation for B and Early A Stars Based on IUE Spectra of Detached Eclipsing Binaries

Nancy Remage Evans, Mckenzie G. Ferrari, Joanna Kuraszkiewicz +4

Ultraviolet spectra were taken of 25 Detached Eclipsing Binaries (DEBs) with spectral types O, B, and early A with the International Ultraviolet Explorer (IUE) satellite in the 115…

astro-ph.GA2022★ 2 cited

The Bolometric Luminosity Correction of Radio-Quiet and Radio-Loud Quasars at 1<z<2

Mojegan Azadi, Belinda Wilkes, Joanna Kuraszkiewicz +2

To understand the impact of active galactic nuclei (AGN) on their host galaxies and large scale environment it is crucial to determine their total radiative power across all wavele…