{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:AR76PJBR4BE3CXRAPV6OTWRGEI","short_pith_number":"pith:AR76PJBR","schema_version":"1.0","canonical_sha256":"047fe7a431e049b15e207d7ce9da26222ce6e77734f06dca33976741f3143e90","source":{"kind":"arxiv","id":"2310.03048","version":1},"attestation_state":"computed","paper":{"title":"DRAGONS -- A Quick Overview","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.IM","authors_text":"Bruno Quint, Chris Simpson, Daniel Berke, James Turner, Joanna Thomas-Osip, Kathleen Labrie, Monika Soraisam, Olesja Smirnova, Oliver Oberdorf, Ricardo Cardenes, Simon Conseil, Vinicius M. Placco, William D. Vacca","submitted_at":"2023-10-03T23:04:57Z","abstract_excerpt":"DRAGONS (Data Reduction for Astronomy from Gemini Observatory North and South) is a platform for the reduction and processing of astronomical data. The Python-based, open-source package includes infrastructure for automation and algorithms for the processing of imaging and spectroscopic data, up to the analysis-ready stage. DRAGONS currently focuses on the reduction of Gemini data, although it allows for support of data from other instruments and telescopes through third-party extensions. Its latest release (v3.1) enables automated reduction of all currently-active Gemini imaging facility inst"},"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":"2310.03048","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.IM","submitted_at":"2023-10-03T23:04:57Z","cross_cats_sorted":[],"title_canon_sha256":"42ea5f3ca710b2ab4f3ff68e1aa7180c3847403595db14e7df96c6b0673fa352","abstract_canon_sha256":"a59dde05dc91e148c030aa0534816033b5b6df8d701ff3abfcbfbb64be559a57"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T06:57:28.191522Z","signature_b64":"o7w+eDrCB5vxy8o3wnzr5YE23Zx+WQ2aELv0tSPpAbmsfpz1XmCqfRyc11bJYt50VW1XYm4fa087fuk39x0fDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"047fe7a431e049b15e207d7ce9da26222ce6e77734f06dca33976741f3143e90","last_reissued_at":"2026-07-05T06:57:28.191051Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T06:57:28.191051Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"DRAGONS -- A Quick Overview","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.IM","authors_text":"Bruno Quint, Chris Simpson, Daniel Berke, James Turner, Joanna Thomas-Osip, Kathleen Labrie, Monika Soraisam, Olesja Smirnova, Oliver Oberdorf, Ricardo Cardenes, Simon Conseil, Vinicius M. Placco, William D. Vacca","submitted_at":"2023-10-03T23:04:57Z","abstract_excerpt":"DRAGONS (Data Reduction for Astronomy from Gemini Observatory North and South) is a platform for the reduction and processing of astronomical data. The Python-based, open-source package includes infrastructure for automation and algorithms for the processing of imaging and spectroscopic data, up to the analysis-ready stage. DRAGONS currently focuses on the reduction of Gemini data, although it allows for support of data from other instruments and telescopes through third-party extensions. Its latest release (v3.1) enables automated reduction of all currently-active Gemini imaging facility inst"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2310.03048","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/2310.03048/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":"2310.03048","created_at":"2026-07-05T06:57:28.191109+00:00"},{"alias_kind":"arxiv_version","alias_value":"2310.03048v1","created_at":"2026-07-05T06:57:28.191109+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2310.03048","created_at":"2026-07-05T06:57:28.191109+00:00"},{"alias_kind":"pith_short_12","alias_value":"AR76PJBR4BE3","created_at":"2026-07-05T06:57:28.191109+00:00"},{"alias_kind":"pith_short_16","alias_value":"AR76PJBR4BE3CXRA","created_at":"2026-07-05T06:57:28.191109+00:00"},{"alias_kind":"pith_short_8","alias_value":"AR76PJBR","created_at":"2026-07-05T06:57:28.191109+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.06673","citing_title":"A redshift of z=3.20 for the bright arc in eMACSJ2229.9-0808: Comment on Wagner & Falco (2026) \"Hamilton's Object revisited: A challenging source redshift of a strong lensing configuration\"","ref_index":11,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/AR76PJBR4BE3CXRAPV6OTWRGEI","json":"https://pith.science/pith/AR76PJBR4BE3CXRAPV6OTWRGEI.json","graph_json":"https://pith.science/api/pith-number/AR76PJBR4BE3CXRAPV6OTWRGEI/graph.json","events_json":"https://pith.science/api/pith-number/AR76PJBR4BE3CXRAPV6OTWRGEI/events.json","paper":"https://pith.science/paper/AR76PJBR"},"agent_actions":{"view_html":"https://pith.science/pith/AR76PJBR4BE3CXRAPV6OTWRGEI","download_json":"https://pith.science/pith/AR76PJBR4BE3CXRAPV6OTWRGEI.json","view_paper":"https://pith.science/paper/AR76PJBR","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2310.03048&json=true","fetch_graph":"https://pith.science/api/pith-number/AR76PJBR4BE3CXRAPV6OTWRGEI/graph.json","fetch_events":"https://pith.science/api/pith-number/AR76PJBR4BE3CXRAPV6OTWRGEI/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/AR76PJBR4BE3CXRAPV6OTWRGEI/action/timestamp_anchor","attest_storage":"https://pith.science/pith/AR76PJBR4BE3CXRAPV6OTWRGEI/action/storage_attestation","attest_author":"https://pith.science/pith/AR76PJBR4BE3CXRAPV6OTWRGEI/action/author_attestation","sign_citation":"https://pith.science/pith/AR76PJBR4BE3CXRAPV6OTWRGEI/action/citation_signature","submit_replication":"https://pith.science/pith/AR76PJBR4BE3CXRAPV6OTWRGEI/action/replication_record"}},"created_at":"2026-07-05T06:57:28.191109+00:00","updated_at":"2026-07-05T06:57:28.191109+00:00"}