{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:HYMZYJDYHG5JILMIUAUZN4WGBW","short_pith_number":"pith:HYMZYJDY","schema_version":"1.0","canonical_sha256":"3e199c247839ba942d88a02996f2c60da200c6654e469ce9721689a5988c15f8","source":{"kind":"arxiv","id":"1802.04305","version":2},"attestation_state":"computed","paper":{"title":"Local measurements of the mean interstellar polarization at high Galactic latitudes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","astro-ph.SR"],"primary_cat":"astro-ph.GA","authors_text":"D. Blinov, G. V. Panopoulou, I. Komis, I. Liodakis, K. Tassis, R. Skalidis, V. Pavlidou","submitted_at":"2018-02-12T19:04:37Z","abstract_excerpt":"We conduct a small-scale pathfinding survey designed to identify the average polarization properties of the diffuse ISM locally at the lowest dust content regions. We perform deep optopolarimetric surveys within three $\\sim 15' \\times 15'$ regions located at $b > 48^\\circ$, using the RoboPol instrument. The observed samples of stars are photometrically complete to $\\sim$16 mag in the R-band. The selected regions exhibit low dust emission at 353 GHz and low total reddening compared to the majority of high-latitude sightlines. We measure the level of systematic uncertainty for all observing epoc"},"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":"1802.04305","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2018-02-12T19:04:37Z","cross_cats_sorted":["astro-ph.CO","astro-ph.SR"],"title_canon_sha256":"29e5c05dbf170bf01a1c09e1e989a76066ce45e4e83328e7125b4fde3d44fe05","abstract_canon_sha256":"c53a96ea0137e475a8cb7fd39ecc56550bf1fa89dc2f65ca292da61825093866"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:08:10.300313Z","signature_b64":"ztQw1muowB1mqK43b+6cGKUCdIrI8wp0bXS8owrxPVhkHNgtDysemy4RbieMHBTUZdt0PACp9YV7Z0uI7bleDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"3e199c247839ba942d88a02996f2c60da200c6654e469ce9721689a5988c15f8","last_reissued_at":"2026-05-18T00:08:10.299832Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:08:10.299832Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Local measurements of the mean interstellar polarization at high Galactic latitudes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","astro-ph.SR"],"primary_cat":"astro-ph.GA","authors_text":"D. Blinov, G. V. Panopoulou, I. Komis, I. Liodakis, K. Tassis, R. Skalidis, V. Pavlidou","submitted_at":"2018-02-12T19:04:37Z","abstract_excerpt":"We conduct a small-scale pathfinding survey designed to identify the average polarization properties of the diffuse ISM locally at the lowest dust content regions. We perform deep optopolarimetric surveys within three $\\sim 15' \\times 15'$ regions located at $b > 48^\\circ$, using the RoboPol instrument. The observed samples of stars are photometrically complete to $\\sim$16 mag in the R-band. The selected regions exhibit low dust emission at 353 GHz and low total reddening compared to the majority of high-latitude sightlines. We measure the level of systematic uncertainty for all observing epoc"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1802.04305","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":"1802.04305","created_at":"2026-05-18T00:08:10.299944+00:00"},{"alias_kind":"arxiv_version","alias_value":"1802.04305v2","created_at":"2026-05-18T00:08:10.299944+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1802.04305","created_at":"2026-05-18T00:08:10.299944+00:00"},{"alias_kind":"pith_short_12","alias_value":"HYMZYJDYHG5J","created_at":"2026-05-18T12:32:28.185984+00:00"},{"alias_kind":"pith_short_16","alias_value":"HYMZYJDYHG5JILMI","created_at":"2026-05-18T12:32:28.185984+00:00"},{"alias_kind":"pith_short_8","alias_value":"HYMZYJDY","created_at":"2026-05-18T12:32:28.185984+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/HYMZYJDYHG5JILMIUAUZN4WGBW","json":"https://pith.science/pith/HYMZYJDYHG5JILMIUAUZN4WGBW.json","graph_json":"https://pith.science/api/pith-number/HYMZYJDYHG5JILMIUAUZN4WGBW/graph.json","events_json":"https://pith.science/api/pith-number/HYMZYJDYHG5JILMIUAUZN4WGBW/events.json","paper":"https://pith.science/paper/HYMZYJDY"},"agent_actions":{"view_html":"https://pith.science/pith/HYMZYJDYHG5JILMIUAUZN4WGBW","download_json":"https://pith.science/pith/HYMZYJDYHG5JILMIUAUZN4WGBW.json","view_paper":"https://pith.science/paper/HYMZYJDY","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1802.04305&json=true","fetch_graph":"https://pith.science/api/pith-number/HYMZYJDYHG5JILMIUAUZN4WGBW/graph.json","fetch_events":"https://pith.science/api/pith-number/HYMZYJDYHG5JILMIUAUZN4WGBW/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/HYMZYJDYHG5JILMIUAUZN4WGBW/action/timestamp_anchor","attest_storage":"https://pith.science/pith/HYMZYJDYHG5JILMIUAUZN4WGBW/action/storage_attestation","attest_author":"https://pith.science/pith/HYMZYJDYHG5JILMIUAUZN4WGBW/action/author_attestation","sign_citation":"https://pith.science/pith/HYMZYJDYHG5JILMIUAUZN4WGBW/action/citation_signature","submit_replication":"https://pith.science/pith/HYMZYJDYHG5JILMIUAUZN4WGBW/action/replication_record"}},"created_at":"2026-05-18T00:08:10.299944+00:00","updated_at":"2026-05-18T00:08:10.299944+00:00"}