{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:56EL7IXEQXVYHQHTJLDYTO3D7N","short_pith_number":"pith:56EL7IXE","schema_version":"1.0","canonical_sha256":"ef88bfa2e485eb83c0f34ac789bb63fb69bb5df89a40101053d4af8ff1dfffb0","source":{"kind":"arxiv","id":"2312.03846","version":3},"attestation_state":"computed","paper":{"title":"A New Constraint on the Relative Disorder of Magnetic Fields between Neutral Interstellar Medium Phases","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Minjie Lei, S.E.Clark","submitted_at":"2023-12-06T19:01:07Z","abstract_excerpt":"Utilizing Planck polarized dust emission maps at 353 GHz and new large-area maps of the neutral hydrogen (HI) cold neutral medium (CNM) fraction ($f_\\mathrm{CNM}$), we investigate the relationship between dust polarization fraction ($p_{353}$) and $f_\\mathrm{CNM}$ in the diffuse high latitude ($|b|>30^{\\circ}$) sky. We find that the correlation between $p_{353}$ and $f_\\mathrm{CNM}$ is qualitatively distinct from the $p_{353}$-HI column density ($N_\\mathrm{H\\,I}$) relationship. At low column densities ($N_\\mathrm{H\\,I}<4\\times10^{20}~\\mathrm{cm^{-2}}$) where $p_{353}$ and $N_\\mathrm{H\\,I}$ are"},"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":"2312.03846","kind":"arxiv","version":3},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.GA","submitted_at":"2023-12-06T19:01:07Z","cross_cats_sorted":[],"title_canon_sha256":"d0f7725a5948faf522e3b44317393f0f00beeb31f361dde992a7f0450a65a3db","abstract_canon_sha256":"5a74f89552dc37747936bd5a0e2f4e4f8e840edf335611d91395094b327f763a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T09:56:48.728703Z","signature_b64":"VRt3+wEW2OCvcZWswAnI9IIjKi9mzEwEaREFY0vxiOxO2iCceVZF9nxK2BKfIfgpqn6F6Tlc9htq/9khTym6Bg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ef88bfa2e485eb83c0f34ac789bb63fb69bb5df89a40101053d4af8ff1dfffb0","last_reissued_at":"2026-07-05T09:56:48.728264Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T09:56:48.728264Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A New Constraint on the Relative Disorder of Magnetic Fields between Neutral Interstellar Medium Phases","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Minjie Lei, S.E.Clark","submitted_at":"2023-12-06T19:01:07Z","abstract_excerpt":"Utilizing Planck polarized dust emission maps at 353 GHz and new large-area maps of the neutral hydrogen (HI) cold neutral medium (CNM) fraction ($f_\\mathrm{CNM}$), we investigate the relationship between dust polarization fraction ($p_{353}$) and $f_\\mathrm{CNM}$ in the diffuse high latitude ($|b|>30^{\\circ}$) sky. We find that the correlation between $p_{353}$ and $f_\\mathrm{CNM}$ is qualitatively distinct from the $p_{353}$-HI column density ($N_\\mathrm{H\\,I}$) relationship. At low column densities ($N_\\mathrm{H\\,I}<4\\times10^{20}~\\mathrm{cm^{-2}}$) where $p_{353}$ and $N_\\mathrm{H\\,I}$ are"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2312.03846","kind":"arxiv","version":3},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2312.03846/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"2312.03846","created_at":"2026-07-05T09:56:48.728323+00:00"},{"alias_kind":"arxiv_version","alias_value":"2312.03846v3","created_at":"2026-07-05T09:56:48.728323+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2312.03846","created_at":"2026-07-05T09:56:48.728323+00:00"},{"alias_kind":"pith_short_12","alias_value":"56EL7IXEQXVY","created_at":"2026-07-05T09:56:48.728323+00:00"},{"alias_kind":"pith_short_16","alias_value":"56EL7IXEQXVYHQHT","created_at":"2026-07-05T09:56:48.728323+00:00"},{"alias_kind":"pith_short_8","alias_value":"56EL7IXE","created_at":"2026-07-05T09:56:48.728323+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2411.13325","citing_title":"TPCNet: Representation learning for HI mapping","ref_index":58,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/56EL7IXEQXVYHQHTJLDYTO3D7N","json":"https://pith.science/pith/56EL7IXEQXVYHQHTJLDYTO3D7N.json","graph_json":"https://pith.science/api/pith-number/56EL7IXEQXVYHQHTJLDYTO3D7N/graph.json","events_json":"https://pith.science/api/pith-number/56EL7IXEQXVYHQHTJLDYTO3D7N/events.json","paper":"https://pith.science/paper/56EL7IXE"},"agent_actions":{"view_html":"https://pith.science/pith/56EL7IXEQXVYHQHTJLDYTO3D7N","download_json":"https://pith.science/pith/56EL7IXEQXVYHQHTJLDYTO3D7N.json","view_paper":"https://pith.science/paper/56EL7IXE","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2312.03846&json=true","fetch_graph":"https://pith.science/api/pith-number/56EL7IXEQXVYHQHTJLDYTO3D7N/graph.json","fetch_events":"https://pith.science/api/pith-number/56EL7IXEQXVYHQHTJLDYTO3D7N/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/56EL7IXEQXVYHQHTJLDYTO3D7N/action/timestamp_anchor","attest_storage":"https://pith.science/pith/56EL7IXEQXVYHQHTJLDYTO3D7N/action/storage_attestation","attest_author":"https://pith.science/pith/56EL7IXEQXVYHQHTJLDYTO3D7N/action/author_attestation","sign_citation":"https://pith.science/pith/56EL7IXEQXVYHQHTJLDYTO3D7N/action/citation_signature","submit_replication":"https://pith.science/pith/56EL7IXEQXVYHQHTJLDYTO3D7N/action/replication_record"}},"created_at":"2026-07-05T09:56:48.728323+00:00","updated_at":"2026-07-05T09:56:48.728323+00:00"}