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Two Exciting High-redshift Galaxy Candidates Turn Out to Be Two Exciting Brown Dwarfs

  • Authors: Maruša Bradac, Chris Willott, Yoshihisa Asada, Loïc Albert, Gregor Rihtaršič, Anishya Harshan, Jon Judež, Nicholas S. Martis, Andrea Ferrara, Kevin Hainline, Abdurro'uf, Joseph F. V. Allingham, Volker Bromm, John Chisholm, Dan Coe, Guillaume Desprez, Jose M. Diego, Andreas L. Faisst, Seiji Fujimoto, Lukas J. Furtak, Tiger Yu-Yang Hsiao, Kohei Inayoshi, Anton M. Koekemoer, Vasily Kokorev, Brian C. Lemaux, Paulo A. A. Lopes, Ray A. Lucas, Danilo Marchesini, Vladan Markov, Gaël Noirot, Richard Pan, Scott W. Randall, Johan Richard, Luke Robbins, Ghassan T. E. Sarrouh, Marcin Sawicki, Tim Schrabback, Roberta Tripodi, Eros Vanzella, Rogier A. Windhorst

Maruša Bradac et al 2026 The Astrophysical Journal Letters 1010 .

  • Provider: AAS Journals

Caption: Figure 3.

Detected proper motion of the two objects. Top: shown is a 16″ × 16″ cutout of the field with Bullet-BD1 and Bullet-BD2 marked. Left column (a) shows the original F444W image taken by the JWST Silver Bullet collaboration (epoch 1), middle column (b) is the image taken ∼1 yr later by the VENUS collaboration (epoch 2), and right panel (c) shows the difference image between epochs 2 and 1 with zoomed insets for the two objects of interest. Middle and bottom: zoom in to the same images (for difference, red is positive, blue is negative). Both objects can be seen moving (white circular aperture is for epoch 1, red for epoch 2; crosses denote their centroids) in a similar direction (20° measured north through east) with proper motion of (49 ± 8) mas yr−1 for Bullet-BD1 and (24 ± 3) mas yr−1 for Bullet-BD2.

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