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A JWST, ALMA, and VLA Survey of the Ophiuchus A Star-forming Region: Unveiling Hidden Dust Mass and Connecting Infrared Outflows to Their Radio Origins

  • Authors: Isaac C. Radley, John D. Ilee, Gemma Busquet, Hauyu Baobab Liu, Klaus M. Pontoppidan, Alvaro Ribas, Marc Audard, Eleonora Bianchi, Tyler L. Bourke, Claudio Codella, Audrey Coutens, Josep M. Girart, Melvin G. Hoare, Izaskun Jiménez-Serra, Doug Johnstone, Laurent Loinard, Olja Panić, Jaime E. Pineda, Linda Podio, John J. Tobin, David J. Wilner

Isaac C. Radley et al 2026 The Astronomical Journal 172 .

  • Provider: AAS Journals

Caption: Figure C1.

VLA continuum images for the Q (44 GHz), K (22 GHz), and X (10 GHz) bands and respective 3σ and 5σ contours broken into two blocks. rms values in mJy beam−1 are shown in the top right of each panel. For the nondetection (ND) in SM1, we indicate the expected position with a white cross. Image beam sizes and PAs are shown as the hatched ellipse in the bottom left of each panel. We include a 50 au scale bar in the bottom-right panel of each block shared across all images. Each row corresponds to a single frequency and each column, per block, to a single object. Object names and classes are found in the column title.

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