2022
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Figure 2. The radio spectrum of the VLASS transient VT 1137-0337. This flat-spectrum radio source appeared between FIRST (1998) and VLASS Epoch 1 (2018) and is seen to slowly fade between 2018 and 2022, making it a good candidate for an emerging pulsar wind nebula (Dong et al. arXiv:2206.11911).
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Figure 3. Solar disk images at 1700Å with the Atmospheric Imaging Assembly, and at 0.85mm with ALMA (Allisandrakis et al. 2022 A&A 661, L4).
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Figure 4. Left: astrometric tracks of the star orbits motion in the binary star system GJ896AB made with the VLBA at 8 GHz. These tracks indicate both the star-star orbit, and the planet-induced motion for star A, with an accuracy of ~ ten of microarcseconds. Right: schematic of the surprising retrograde orbit for the planet (Curiel ea. 2022, AJ, 164, 92).
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Figure 5. Images of the Free-Free emission from a Galactic HII region from the GLOSTAR survey at 6 GHz with 1” resolution (left), and in the mid-IR (right; Dzib et al. 2022, arXiv:2210:00560).
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Figure 6. VLA observations of the 22.3 GHz CCS line emission from TMC-1C, plus the Stokes V measurements showing Zeeman splitting (Koley et al. 2022, MNRAS, 516, L48).
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Figure 7. Images of the galaxy M33 at 1.5 GHz, 15” resolution (left), and 6.3 GHz, 9” resolution (right; Tabatabaei et al. 2022, arXiv:2209:01389).
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Figure 8. Location of radio continuum sources and super hot cores within the NGC253 CMZ plotted over the 212 GHz ALCHEMI dust continuum emission. Numbered white circles indicate GMCs identified in the ALMA survey (see Behrens et al 2022, arXiv:2209:06244 and references therein).
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Figure 9. ALMA observations of CO2-1 emission from a post-merger, post-starburst galaxy at z = 0.64. Most of the molecular gas has been stripped into tidal tails extending 64 kpc (Spilker et al. 2022, ApJ 936, L11)
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Figure 10. JWST image of a grand design spiral at z = 3.0. Center: stellar mass surface density (color) and ALMA 150 GHz dust emission (green contours). Right: ALMA detection of molecular gas (Wu et al. arXiv:2208:08473).
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Figure 11. Tentative [OIII] 88um emission seen by ALMA at 256 GHz, from the z = 12.1 JWST galaxy candidate GLASS-z13 (Bakx et al. 2022, arXiv:2208.13642).
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Figure 1. The EHT (including ALMA) image at 240 GHz of the general relativistic shadow of the supermassive black hole at the Galactic Center, Sgr A* (EHT collaboration 2022, ApJ, 930, L12).
