{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:I4ZUA2ZFJCOFZWQMCMJPQXCVK6","short_pith_number":"pith:I4ZUA2ZF","schema_version":"1.0","canonical_sha256":"4733406b25489c5cda0c1312f85c5557a01955215ee8e13442a28df5d92c8737","source":{"kind":"arxiv","id":"1306.6077","version":1},"attestation_state":"computed","paper":{"title":"H2 Excitation Structure on the Sightlines to delta Scorpius and zeta Ophiucus - First Results from the Sub-orbital Local Interstellar Cloud Experiment","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Eric B. Burgh (SOFIA/USRA), James C. Green (Colorado), Kevin France, Matthew Beasley (Planetary Resources), Nicholas Nell, Robert Kane (Colorado)","submitted_at":"2013-06-25T20:00:03Z","abstract_excerpt":"We present the first science results from the Sub-orbital Local Interstellar Cloud Experiment (SLICE): moderate resolution 1020-1070A spectroscopy of four sightlines through the local interstellar medium. High signal-to-noise (S/N) spectra of eta Uma, alpha Vir, delta Sco, and zeta Oph were obtained during a 21 April 2013 rocket flight. The SLICE observations constrain the density, molecular photoexcitation rates, and physical conditions present in the interstellar material towards delta Sco and zeta Oph. Our spectra indicate a factor of two lower total N(H2) than previously reported for delta"},"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":"1306.6077","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2013-06-25T20:00:03Z","cross_cats_sorted":[],"title_canon_sha256":"b7a246cb6d9077a99762f9a9500afc8dd37b643303a8cdb503bf3da30304e250","abstract_canon_sha256":"9521e652d90f0415320ab16f9d87aea0559632f61da96db5cb995823039bf36a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:49:07.892112Z","signature_b64":"J/95l/iXSxlBq7lbKOUmEPcz6lV60BCbcds/3KFBMSY9/tth7mXpicTZ3fsg0Ex3AVayuqiynXCD3C8kibPJBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4733406b25489c5cda0c1312f85c5557a01955215ee8e13442a28df5d92c8737","last_reissued_at":"2026-05-18T01:49:07.891409Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:49:07.891409Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"H2 Excitation Structure on the Sightlines to delta Scorpius and zeta Ophiucus - First Results from the Sub-orbital Local Interstellar Cloud Experiment","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Eric B. Burgh (SOFIA/USRA), James C. Green (Colorado), Kevin France, Matthew Beasley (Planetary Resources), Nicholas Nell, Robert Kane (Colorado)","submitted_at":"2013-06-25T20:00:03Z","abstract_excerpt":"We present the first science results from the Sub-orbital Local Interstellar Cloud Experiment (SLICE): moderate resolution 1020-1070A spectroscopy of four sightlines through the local interstellar medium. High signal-to-noise (S/N) spectra of eta Uma, alpha Vir, delta Sco, and zeta Oph were obtained during a 21 April 2013 rocket flight. The SLICE observations constrain the density, molecular photoexcitation rates, and physical conditions present in the interstellar material towards delta Sco and zeta Oph. Our spectra indicate a factor of two lower total N(H2) than previously reported for delta"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1306.6077","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":"1306.6077","created_at":"2026-05-18T01:49:07.891519+00:00"},{"alias_kind":"arxiv_version","alias_value":"1306.6077v1","created_at":"2026-05-18T01:49:07.891519+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1306.6077","created_at":"2026-05-18T01:49:07.891519+00:00"},{"alias_kind":"pith_short_12","alias_value":"I4ZUA2ZFJCOF","created_at":"2026-05-18T12:27:46.883200+00:00"},{"alias_kind":"pith_short_16","alias_value":"I4ZUA2ZFJCOFZWQM","created_at":"2026-05-18T12:27:46.883200+00:00"},{"alias_kind":"pith_short_8","alias_value":"I4ZUA2ZF","created_at":"2026-05-18T12:27:46.883200+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/I4ZUA2ZFJCOFZWQMCMJPQXCVK6","json":"https://pith.science/pith/I4ZUA2ZFJCOFZWQMCMJPQXCVK6.json","graph_json":"https://pith.science/api/pith-number/I4ZUA2ZFJCOFZWQMCMJPQXCVK6/graph.json","events_json":"https://pith.science/api/pith-number/I4ZUA2ZFJCOFZWQMCMJPQXCVK6/events.json","paper":"https://pith.science/paper/I4ZUA2ZF"},"agent_actions":{"view_html":"https://pith.science/pith/I4ZUA2ZFJCOFZWQMCMJPQXCVK6","download_json":"https://pith.science/pith/I4ZUA2ZFJCOFZWQMCMJPQXCVK6.json","view_paper":"https://pith.science/paper/I4ZUA2ZF","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1306.6077&json=true","fetch_graph":"https://pith.science/api/pith-number/I4ZUA2ZFJCOFZWQMCMJPQXCVK6/graph.json","fetch_events":"https://pith.science/api/pith-number/I4ZUA2ZFJCOFZWQMCMJPQXCVK6/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/I4ZUA2ZFJCOFZWQMCMJPQXCVK6/action/timestamp_anchor","attest_storage":"https://pith.science/pith/I4ZUA2ZFJCOFZWQMCMJPQXCVK6/action/storage_attestation","attest_author":"https://pith.science/pith/I4ZUA2ZFJCOFZWQMCMJPQXCVK6/action/author_attestation","sign_citation":"https://pith.science/pith/I4ZUA2ZFJCOFZWQMCMJPQXCVK6/action/citation_signature","submit_replication":"https://pith.science/pith/I4ZUA2ZFJCOFZWQMCMJPQXCVK6/action/replication_record"}},"created_at":"2026-05-18T01:49:07.891519+00:00","updated_at":"2026-05-18T01:49:07.891519+00:00"}