{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:VFXACOYC6XYG6VDCG4OFOBIWAL","short_pith_number":"pith:VFXACOYC","schema_version":"1.0","canonical_sha256":"a96e013b02f5f06f5462371c57051602fa49dfcd65348732168f1123e495c5aa","source":{"kind":"arxiv","id":"2310.13063","version":1},"attestation_state":"computed","paper":{"title":"The Large Array Survey Telescope -- Pipeline. I. Basic image reduction and visit coaddition","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.IM","authors_text":"A. Blumenzweig, A. Krassilchtchikov, A. Sharon, A. Zenin, C. Tishler, D. Elhanati, D. Polishook, E. O. Ofek, E. Segre, E. Zimmerman, G. Nir, N. L. Strotjohann, N. Segev, P. Chen, S. Ben-Ami, S. Garrappa, S. Weimann, V. Fallah Ramazani, Y. Shanni, Y. Shvartzvald, Y. Sofer-Rimalt","submitted_at":"2023-10-19T18:01:47Z","abstract_excerpt":"The Large Array Survey Telescope (LAST) is a wide-field telescope designed to explore the variable and transient sky with a high cadence and to be a test-bed for cost-effective telescope design. A LAST node is composed of 48 (32 already deployed), 28-cm f/2.2 telescopes. A single telescope has a 7.4 deg^2 field of view and reaches a 5-sigma limiting magnitude of 19.6 (21.0) in 20s (20x20s) (filter-less), while the entire system provides a 355 deg^2 field of view. The basic strategy of LAST is to obtain multiple 20-s consecutive exposures of each field (a visit). Each telescope carries a 61 Mpi"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"2310.13063","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.IM","submitted_at":"2023-10-19T18:01:47Z","cross_cats_sorted":[],"title_canon_sha256":"8a3ce92effdeb40f219bdfec0174be940b3fff00f0b585fe4abc05c1de84087e","abstract_canon_sha256":"515a0b3c0d9a34ccaaff28ca8763732ac2b6348060e81268a58357459bb63058"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T07:02:56.509119Z","signature_b64":"DPYqwY2v0tnjlgSe1gjhE+S4OPXvGg2D1mwaBritbHJZ+2Jbzvb4QbrOtnUaleGvzlhNhXVD5H9zjsTW5a8XCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a96e013b02f5f06f5462371c57051602fa49dfcd65348732168f1123e495c5aa","last_reissued_at":"2026-07-05T07:02:56.508635Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T07:02:56.508635Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Large Array Survey Telescope -- Pipeline. I. Basic image reduction and visit coaddition","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.IM","authors_text":"A. Blumenzweig, A. Krassilchtchikov, A. Sharon, A. Zenin, C. Tishler, D. Elhanati, D. Polishook, E. O. Ofek, E. Segre, E. Zimmerman, G. Nir, N. L. Strotjohann, N. Segev, P. Chen, S. Ben-Ami, S. Garrappa, S. Weimann, V. Fallah Ramazani, Y. Shanni, Y. Shvartzvald, Y. Sofer-Rimalt","submitted_at":"2023-10-19T18:01:47Z","abstract_excerpt":"The Large Array Survey Telescope (LAST) is a wide-field telescope designed to explore the variable and transient sky with a high cadence and to be a test-bed for cost-effective telescope design. A LAST node is composed of 48 (32 already deployed), 28-cm f/2.2 telescopes. A single telescope has a 7.4 deg^2 field of view and reaches a 5-sigma limiting magnitude of 19.6 (21.0) in 20s (20x20s) (filter-less), while the entire system provides a 355 deg^2 field of view. The basic strategy of LAST is to obtain multiple 20-s consecutive exposures of each field (a visit). Each telescope carries a 61 Mpi"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2310.13063","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2310.13063/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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"},"aliases":[{"alias_kind":"arxiv","alias_value":"2310.13063","created_at":"2026-07-05T07:02:56.508694+00:00"},{"alias_kind":"arxiv_version","alias_value":"2310.13063v1","created_at":"2026-07-05T07:02:56.508694+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2310.13063","created_at":"2026-07-05T07:02:56.508694+00:00"},{"alias_kind":"pith_short_12","alias_value":"VFXACOYC6XYG","created_at":"2026-07-05T07:02:56.508694+00:00"},{"alias_kind":"pith_short_16","alias_value":"VFXACOYC6XYG6VDC","created_at":"2026-07-05T07:02:56.508694+00:00"},{"alias_kind":"pith_short_8","alias_value":"VFXACOYC","created_at":"2026-07-05T07:02:56.508694+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/VFXACOYC6XYG6VDCG4OFOBIWAL","json":"https://pith.science/pith/VFXACOYC6XYG6VDCG4OFOBIWAL.json","graph_json":"https://pith.science/api/pith-number/VFXACOYC6XYG6VDCG4OFOBIWAL/graph.json","events_json":"https://pith.science/api/pith-number/VFXACOYC6XYG6VDCG4OFOBIWAL/events.json","paper":"https://pith.science/paper/VFXACOYC"},"agent_actions":{"view_html":"https://pith.science/pith/VFXACOYC6XYG6VDCG4OFOBIWAL","download_json":"https://pith.science/pith/VFXACOYC6XYG6VDCG4OFOBIWAL.json","view_paper":"https://pith.science/paper/VFXACOYC","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2310.13063&json=true","fetch_graph":"https://pith.science/api/pith-number/VFXACOYC6XYG6VDCG4OFOBIWAL/graph.json","fetch_events":"https://pith.science/api/pith-number/VFXACOYC6XYG6VDCG4OFOBIWAL/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/VFXACOYC6XYG6VDCG4OFOBIWAL/action/timestamp_anchor","attest_storage":"https://pith.science/pith/VFXACOYC6XYG6VDCG4OFOBIWAL/action/storage_attestation","attest_author":"https://pith.science/pith/VFXACOYC6XYG6VDCG4OFOBIWAL/action/author_attestation","sign_citation":"https://pith.science/pith/VFXACOYC6XYG6VDCG4OFOBIWAL/action/citation_signature","submit_replication":"https://pith.science/pith/VFXACOYC6XYG6VDCG4OFOBIWAL/action/replication_record"}},"created_at":"2026-07-05T07:02:56.508694+00:00","updated_at":"2026-07-05T07:02:56.508694+00:00"}