{"paper":{"title":"The RoboPol Pipeline and Control System","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.IM","authors_text":"A. C. S. Readhead, A. Kougentakis, A. Kus, A. N. Ramaprakash, A. Steiakaki, B. Pazderska, C. Rajarshi, D. Blinov, E. Angelakis, E. Paleologou, E. Pazderski, G. Panopoulou, G. Paterakis, I. Myserlis, I. Papadakis, I. Papamastorakis, J. A. Zensus, K. Tassis, L. Fuhrmann, M. Balokovi\\'c, N. Kylafis, O. G. King, P. Khodade, P. Reig, R. Feiler, R. Rouneq, T. Hovatta, T. J. Pearson, V. Pavlidou","submitted_at":"2013-10-28T19:49:40Z","abstract_excerpt":"We describe the data reduction pipeline and control system for the RoboPol project. The RoboPol project is monitoring the optical $R$-band magnitude and linear polarization of a large sample of active galactic nuclei that is dominated by blazars. The pipeline calibrates and reduces each exposure frame, producing a measurement of the magnitude and linear polarization of every source in the $13'\\times 13'$ field of view. The control system combines a dynamic scheduler, real-time data reduction, and telescope automation to allow high-efficiency unassisted observations."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1310.7555","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"}