We present X-ray and radio observations following SGR J1935+2154's October 2022 outburst. Using XMM-Newton and NuSTAR data, we found persistent emission well-described by a blackbody (kT_BB ≈ 0.4 keV, R_BB ≈ 1.9 km) plus power-law model up to 25 keV. We detected X-ray pulsations and measured a spin-down rate of Ṗ = 5.52×10⁻¹¹ s s⁻¹, 3.8 times larger than after its 2014 outburst. Despite 92.5 hours of radio monitoring with 25-32m telescopes, no radio bursts or pulsed emission were detected.

We present a long-term X-ray monitoring campaign of Swift J1818.0−1607, a very young radio-loud magnetar (P=1.36s, B≈3×10¹⁴G) using XMM-Newton, NuSTAR, and Swift, from its 2020 March outburst through 2021 October. The 1-10 keV spectrum is modeled with an absorbed blackbody (kT_BB≈1.1 keV) showing a shrinking emitting region (0.6 to 0.2 km). We observed large torque variability and detected bright diffuse X-ray emission extending 50″-110″ around the source. VLA observations revealed a radio counterpart (4.38±0.05 mJy at 3 GHz) and a half-ring radio structure ~90″ west of the magnetar, potentially associated with its supernova remnant.