{"paper":{"title":"High resolution imaging of the ATLBS regions: the radio source counts","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"K. Thorat, L. Saripalli, R. D. Ekers, R. Subrahmanyan","submitted_at":"2012-02-01T10:09:03Z","abstract_excerpt":"The Australia Telescope Low-brightness survey (ATLBS; \\cite{SESS10}) regions have been mosaic imaged at a radio frequency of 1.4 GHz with $6\\arcsec$ angular resolution and 72 $\\mu$Jy beam$^{-1}$ rms noise. The images (centered at RA: $00^{h}\\ 35^{m}\\ 00^{s}$, DEC: $-67^{\\circ}\\ 00^{'}\\ 00^{\"}$ and RA: $00^{h}\\ 59^{m}\\ 17^{s}$, DEC: $-67^{\\circ}\\ 00^{'}\\ 00^{\"}$ (J2000 epoch)) cover 8.42 square degrees sky area and have no artifacts or imaging errors above the image thermal noise. Multi-resolution radio and optical r-band images (made using the 4-m CTIO Blanco telescope) were used to recognize "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1202.0134","kind":"arxiv","version":2},"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"}