{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:AQKBRBUAKJS7RVENCUV4YED4HO","short_pith_number":"pith:AQKBRBUA","schema_version":"1.0","canonical_sha256":"04141886805265f8d48d152bcc107c3b86055195bd63b1d0bcfcb12ee5822e16","source":{"kind":"arxiv","id":"1710.02439","version":2},"attestation_state":"computed","paper":{"title":"Large Interstellar Polarisation Survey. LIPS I: FORS2 spectropolarimetry in the Southern Hemisphere","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. Cikota, F. Patat, J. Cami, J. Smoker, K.T. Smith, L. Kaper, N.J.L. Cox, N.V. Voshchinnikov, R. Siebenmorgen, S. Bagnulo, S. Taubenberger, the LIPS collaboration","submitted_at":"2017-10-06T15:02:09Z","abstract_excerpt":"Polarimetric studies of light transmitted through interstellar clouds may give constraints on the properties of the interstellar dust grains. Traditionally, broadband linear polarisation (BBLP) measurements have been considered an important diagnostic tool for the study of the interstellar dust, while comparatively less attention has been paid to spectropolarimetric measurements. However, spectropolarimetry may offer stronger constraints than BBLP, for example by revealing narrowband features, and by allowing us to distinguish the contribution of dust from the contribution of interstellar gas."},"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":"1710.02439","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2017-10-06T15:02:09Z","cross_cats_sorted":[],"title_canon_sha256":"f4bcfecd6174ea6ddb8f8cd8bd7ba42c2942779486c85374ce42494956d1c8ae","abstract_canon_sha256":"bd44e2c8f6988f58d18ad5b751c9aa65c3af9dc392097bb6ec0e9486b2619930"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:27:42.845141Z","signature_b64":"mQvZQZcPIaNF05S+VhJjrjFPXLJLWGh6dO8mXvtlm6LbTtn6kZy/+ZUH1JqQzK9jFqzgAAi6owTcSx081ex3CQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"04141886805265f8d48d152bcc107c3b86055195bd63b1d0bcfcb12ee5822e16","last_reissued_at":"2026-05-18T00:27:42.844402Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:27:42.844402Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Large Interstellar Polarisation Survey. LIPS I: FORS2 spectropolarimetry in the Southern Hemisphere","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. Cikota, F. Patat, J. Cami, J. Smoker, K.T. Smith, L. Kaper, N.J.L. Cox, N.V. Voshchinnikov, R. Siebenmorgen, S. Bagnulo, S. Taubenberger, the LIPS collaboration","submitted_at":"2017-10-06T15:02:09Z","abstract_excerpt":"Polarimetric studies of light transmitted through interstellar clouds may give constraints on the properties of the interstellar dust grains. Traditionally, broadband linear polarisation (BBLP) measurements have been considered an important diagnostic tool for the study of the interstellar dust, while comparatively less attention has been paid to spectropolarimetric measurements. However, spectropolarimetry may offer stronger constraints than BBLP, for example by revealing narrowband features, and by allowing us to distinguish the contribution of dust from the contribution of interstellar gas."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1710.02439","kind":"arxiv","version":2},"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":"1710.02439","created_at":"2026-05-18T00:27:42.844491+00:00"},{"alias_kind":"arxiv_version","alias_value":"1710.02439v2","created_at":"2026-05-18T00:27:42.844491+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1710.02439","created_at":"2026-05-18T00:27:42.844491+00:00"},{"alias_kind":"pith_short_12","alias_value":"AQKBRBUAKJS7","created_at":"2026-05-18T12:31:05.417338+00:00"},{"alias_kind":"pith_short_16","alias_value":"AQKBRBUAKJS7RVEN","created_at":"2026-05-18T12:31:05.417338+00:00"},{"alias_kind":"pith_short_8","alias_value":"AQKBRBUA","created_at":"2026-05-18T12:31:05.417338+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/AQKBRBUAKJS7RVENCUV4YED4HO","json":"https://pith.science/pith/AQKBRBUAKJS7RVENCUV4YED4HO.json","graph_json":"https://pith.science/api/pith-number/AQKBRBUAKJS7RVENCUV4YED4HO/graph.json","events_json":"https://pith.science/api/pith-number/AQKBRBUAKJS7RVENCUV4YED4HO/events.json","paper":"https://pith.science/paper/AQKBRBUA"},"agent_actions":{"view_html":"https://pith.science/pith/AQKBRBUAKJS7RVENCUV4YED4HO","download_json":"https://pith.science/pith/AQKBRBUAKJS7RVENCUV4YED4HO.json","view_paper":"https://pith.science/paper/AQKBRBUA","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1710.02439&json=true","fetch_graph":"https://pith.science/api/pith-number/AQKBRBUAKJS7RVENCUV4YED4HO/graph.json","fetch_events":"https://pith.science/api/pith-number/AQKBRBUAKJS7RVENCUV4YED4HO/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/AQKBRBUAKJS7RVENCUV4YED4HO/action/timestamp_anchor","attest_storage":"https://pith.science/pith/AQKBRBUAKJS7RVENCUV4YED4HO/action/storage_attestation","attest_author":"https://pith.science/pith/AQKBRBUAKJS7RVENCUV4YED4HO/action/author_attestation","sign_citation":"https://pith.science/pith/AQKBRBUAKJS7RVENCUV4YED4HO/action/citation_signature","submit_replication":"https://pith.science/pith/AQKBRBUAKJS7RVENCUV4YED4HO/action/replication_record"}},"created_at":"2026-05-18T00:27:42.844491+00:00","updated_at":"2026-05-18T00:27:42.844491+00:00"}