{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:HKBFEYR7WLLZ3FYC3RLN5OGWQZ","short_pith_number":"pith:HKBFEYR7","schema_version":"1.0","canonical_sha256":"3a8252623fb2d79d9702dc56deb8d6865cdcc4ab5e22ca2ba6788d57bdc5b5c5","source":{"kind":"arxiv","id":"1503.07504","version":1},"attestation_state":"computed","paper":{"title":"Data Reduction Pipeline for the MMT and Magellan Infrared Spectrograph","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.IM","authors_text":"Brian McLeod, Daniel Fabricant, Igor Chilingarian, Sean Moran, Warren Brown, Yuri Beletsky","submitted_at":"2015-03-25T19:18:31Z","abstract_excerpt":"We describe the new spectroscopic data reduction pipeline for the multi-object MMT/Magellan Infrared Spectrograph. The pipeline is implemented in idl as a stand-alone package and is publicly available in both stable and development versions. We describe novel algorithms for sky subtraction and correction for telluric absorption. We demonstrate that our sky subtraction technique reaches the Poisson limit set by the photon statistics. Our telluric correction uses a hybrid approach by first computing a correction function from an observed stellar spectrum, and then differentially correcting it us"},"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":"1503.07504","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.IM","submitted_at":"2015-03-25T19:18:31Z","cross_cats_sorted":[],"title_canon_sha256":"cfd018c3991c795c618a659e9588d6d1ce7e02e8655c552259522c33b6c763e4","abstract_canon_sha256":"69b30c40f36aa99fc620d92d53c1f425fc30b99234b42972d717c5e5551f10f0"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:40:49.884038Z","signature_b64":"HlGsS/9kTkzyk2wRKaUdvDda7iY7bhq3KrC/iHoLd/KwV3DesnFbt2rkOFgsJi72/CIkYOVvK+cVXSoY2j0VDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"3a8252623fb2d79d9702dc56deb8d6865cdcc4ab5e22ca2ba6788d57bdc5b5c5","last_reissued_at":"2026-05-18T01:40:49.883397Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:40:49.883397Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Data Reduction Pipeline for the MMT and Magellan Infrared Spectrograph","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.IM","authors_text":"Brian McLeod, Daniel Fabricant, Igor Chilingarian, Sean Moran, Warren Brown, Yuri Beletsky","submitted_at":"2015-03-25T19:18:31Z","abstract_excerpt":"We describe the new spectroscopic data reduction pipeline for the multi-object MMT/Magellan Infrared Spectrograph. The pipeline is implemented in idl as a stand-alone package and is publicly available in both stable and development versions. We describe novel algorithms for sky subtraction and correction for telluric absorption. We demonstrate that our sky subtraction technique reaches the Poisson limit set by the photon statistics. Our telluric correction uses a hybrid approach by first computing a correction function from an observed stellar spectrum, and then differentially correcting it us"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1503.07504","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":"1503.07504","created_at":"2026-05-18T01:40:49.883498+00:00"},{"alias_kind":"arxiv_version","alias_value":"1503.07504v1","created_at":"2026-05-18T01:40:49.883498+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1503.07504","created_at":"2026-05-18T01:40:49.883498+00:00"},{"alias_kind":"pith_short_12","alias_value":"HKBFEYR7WLLZ","created_at":"2026-05-18T12:29:25.134429+00:00"},{"alias_kind":"pith_short_16","alias_value":"HKBFEYR7WLLZ3FYC","created_at":"2026-05-18T12:29:25.134429+00:00"},{"alias_kind":"pith_short_8","alias_value":"HKBFEYR7","created_at":"2026-05-18T12:29:25.134429+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2605.17040","citing_title":"PEARLS: JWST Counterparts of Micro-Jy Radio Sources in the NEP Time Domain Field. II. All Four Spokes","ref_index":63,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/HKBFEYR7WLLZ3FYC3RLN5OGWQZ","json":"https://pith.science/pith/HKBFEYR7WLLZ3FYC3RLN5OGWQZ.json","graph_json":"https://pith.science/api/pith-number/HKBFEYR7WLLZ3FYC3RLN5OGWQZ/graph.json","events_json":"https://pith.science/api/pith-number/HKBFEYR7WLLZ3FYC3RLN5OGWQZ/events.json","paper":"https://pith.science/paper/HKBFEYR7"},"agent_actions":{"view_html":"https://pith.science/pith/HKBFEYR7WLLZ3FYC3RLN5OGWQZ","download_json":"https://pith.science/pith/HKBFEYR7WLLZ3FYC3RLN5OGWQZ.json","view_paper":"https://pith.science/paper/HKBFEYR7","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1503.07504&json=true","fetch_graph":"https://pith.science/api/pith-number/HKBFEYR7WLLZ3FYC3RLN5OGWQZ/graph.json","fetch_events":"https://pith.science/api/pith-number/HKBFEYR7WLLZ3FYC3RLN5OGWQZ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/HKBFEYR7WLLZ3FYC3RLN5OGWQZ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/HKBFEYR7WLLZ3FYC3RLN5OGWQZ/action/storage_attestation","attest_author":"https://pith.science/pith/HKBFEYR7WLLZ3FYC3RLN5OGWQZ/action/author_attestation","sign_citation":"https://pith.science/pith/HKBFEYR7WLLZ3FYC3RLN5OGWQZ/action/citation_signature","submit_replication":"https://pith.science/pith/HKBFEYR7WLLZ3FYC3RLN5OGWQZ/action/replication_record"}},"created_at":"2026-05-18T01:40:49.883498+00:00","updated_at":"2026-05-18T01:40:49.883498+00:00"}