{"paper":{"title":"Radio Monitoring and High Resolution Observations of the Soft Gamma Ray Repeater 1806-20. by Vasisht et al. Postscript file, 13 pages","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"D. A. Frail, G. Vasisht, S. R. Kulkarni","submitted_at":"1994-12-01T02:03:50Z","abstract_excerpt":"We report the results of radio flux-monitoring and high resolution observations at 3.6 cm with the VLA, of the central condensation in G10.0-0.3, the radio nebula surrounding the soft gamma ray repeater (SGR) 1806-20. The quiescent X-ray source AX1805.7-2025 is coincident with the radio core suggesting that G10.0-0.3 is a plerionic supernova remnant. The monitoring experiment was performed in 10 epochs spread over five months, starting just before the latest reactivation of SGR 1806-20 in gamma-rays. There is no apparent increase in the radio flux density from the central region of G10.0-0.3 o"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/9411117","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}