{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:HVRLKGPVSWJ2XTWRM2QFB5UUJB","short_pith_number":"pith:HVRLKGPV","schema_version":"1.0","canonical_sha256":"3d62b519f59593abced166a050f694486a32bc9b7fe72ec0231185e41bb4793c","source":{"kind":"arxiv","id":"1107.1713","version":1},"attestation_state":"computed","paper":{"title":"The XDSPRES CL-based package for reducing OSIRIS cross-dispersed spectra","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.IM","authors_text":"Daniel Ruschel-Dutra, Jorge Ricardo Ducati, Miriani Pastoriza, Rog\\'erio Riffel","submitted_at":"2011-07-08T19:59:29Z","abstract_excerpt":"We present a description of the CL-based package XDSPRES, which aims at being a complete reducing facility for cross-dispersed spectra taken with the Ohio State Infrared Imager/Spectrometer, as installed at the SOAR telescope. This instrument provides spectra in the range between 1.2um and 2.35um in a single exposure, with resolving power of R ~ 1200. XDSPRES consists of two tasks, namely xdflat and doosiris. The former is a completely automated code for preparing normalized flat field images from raw flat field exposures. Doosiris was designed to be a complete reduction pipeline, requiring a "},"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":"1107.1713","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.IM","submitted_at":"2011-07-08T19:59:29Z","cross_cats_sorted":[],"title_canon_sha256":"3eb414f8c646255f5515e018c1f79c4de0b6b19ff792bcd429c7f97d24be2b4d","abstract_canon_sha256":"dbaed0bdf70fc681b810e5697625f565f102a8845602cf1effdf1d82f505d23c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:01:21.129708Z","signature_b64":"o0OsYvJfdg0UmMibvB2v1E614nxbnWHen2R06clpuyHE9PwBwMcFfxkQo2adbstT6jRAtxP0SuOFxa7BOMm4Bg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"3d62b519f59593abced166a050f694486a32bc9b7fe72ec0231185e41bb4793c","last_reissued_at":"2026-05-18T02:01:21.129220Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:01:21.129220Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The XDSPRES CL-based package for reducing OSIRIS cross-dispersed spectra","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.IM","authors_text":"Daniel Ruschel-Dutra, Jorge Ricardo Ducati, Miriani Pastoriza, Rog\\'erio Riffel","submitted_at":"2011-07-08T19:59:29Z","abstract_excerpt":"We present a description of the CL-based package XDSPRES, which aims at being a complete reducing facility for cross-dispersed spectra taken with the Ohio State Infrared Imager/Spectrometer, as installed at the SOAR telescope. This instrument provides spectra in the range between 1.2um and 2.35um in a single exposure, with resolving power of R ~ 1200. XDSPRES consists of two tasks, namely xdflat and doosiris. The former is a completely automated code for preparing normalized flat field images from raw flat field exposures. Doosiris was designed to be a complete reduction pipeline, requiring a "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1107.1713","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"},"aliases":[{"alias_kind":"arxiv","alias_value":"1107.1713","created_at":"2026-05-18T02:01:21.129288+00:00"},{"alias_kind":"arxiv_version","alias_value":"1107.1713v1","created_at":"2026-05-18T02:01:21.129288+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1107.1713","created_at":"2026-05-18T02:01:21.129288+00:00"},{"alias_kind":"pith_short_12","alias_value":"HVRLKGPVSWJ2","created_at":"2026-05-18T12:26:30.835961+00:00"},{"alias_kind":"pith_short_16","alias_value":"HVRLKGPVSWJ2XTWR","created_at":"2026-05-18T12:26:30.835961+00:00"},{"alias_kind":"pith_short_8","alias_value":"HVRLKGPV","created_at":"2026-05-18T12:26:30.835961+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/HVRLKGPVSWJ2XTWRM2QFB5UUJB","json":"https://pith.science/pith/HVRLKGPVSWJ2XTWRM2QFB5UUJB.json","graph_json":"https://pith.science/api/pith-number/HVRLKGPVSWJ2XTWRM2QFB5UUJB/graph.json","events_json":"https://pith.science/api/pith-number/HVRLKGPVSWJ2XTWRM2QFB5UUJB/events.json","paper":"https://pith.science/paper/HVRLKGPV"},"agent_actions":{"view_html":"https://pith.science/pith/HVRLKGPVSWJ2XTWRM2QFB5UUJB","download_json":"https://pith.science/pith/HVRLKGPVSWJ2XTWRM2QFB5UUJB.json","view_paper":"https://pith.science/paper/HVRLKGPV","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1107.1713&json=true","fetch_graph":"https://pith.science/api/pith-number/HVRLKGPVSWJ2XTWRM2QFB5UUJB/graph.json","fetch_events":"https://pith.science/api/pith-number/HVRLKGPVSWJ2XTWRM2QFB5UUJB/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/HVRLKGPVSWJ2XTWRM2QFB5UUJB/action/timestamp_anchor","attest_storage":"https://pith.science/pith/HVRLKGPVSWJ2XTWRM2QFB5UUJB/action/storage_attestation","attest_author":"https://pith.science/pith/HVRLKGPVSWJ2XTWRM2QFB5UUJB/action/author_attestation","sign_citation":"https://pith.science/pith/HVRLKGPVSWJ2XTWRM2QFB5UUJB/action/citation_signature","submit_replication":"https://pith.science/pith/HVRLKGPVSWJ2XTWRM2QFB5UUJB/action/replication_record"}},"created_at":"2026-05-18T02:01:21.129288+00:00","updated_at":"2026-05-18T02:01:21.129288+00:00"}