Image Details
Caption: Figure 9.
The 2–4 GHz data for V2400 Oph on 2025 August 9 (left column) and 2025 August 15 (right column). The top panels show the full-band SEDs, the middle panels show the full-band light curves, and the bottom panels show the dynamic SEDs in Stokes I. Each observation shows distinct behavior in V2400 Oph: at times, emission can be unpolarized, but at others, it can be moderately to highly circularly polarized.
© 2026. The Author(s). Published by the American Astronomical Society.