{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:VAWJ6772RPCT7UKI5BCDQCZQGS","short_pith_number":"pith:VAWJ6772","schema_version":"1.0","canonical_sha256":"a82c9f7ffa8bc53fd148e844380b3034b4f9627f25124cd862415ecb3eb4496c","source":{"kind":"arxiv","id":"1410.6158","version":1},"attestation_state":"computed","paper":{"title":"The Survey of Lines in M31 (SLIM): Investigating the Origins of [CII] Emission","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Leroy, B. Groves, E. Schinnerer, F. Walter, J. Dalcanton, K. Croxall, K. Kreckel, K. Sandstrom, M. Fouesneau, M. J. Kapala","submitted_at":"2014-10-22T20:00:11Z","abstract_excerpt":"The [CII] 158 micron line is one of the strongest emission lines observed in star-forming galaxies, and has been empirically measured to correlate with the star formation rate (SFR) globally and on ~kpc scales. However, due to the multi-phase origins of [CII], one might expect this relation to break down at small scales. We investigate the origins of [CII] emission by examining high spatial resolution observations of [CII] in M31, with the Survey of Lines in M31 (SLIM). We present five ~700x700 pc (3\"x3\") Fields mapping the [CII] emission, Halpha emission, combined with ancillary infrared (IR)"},"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":"1410.6158","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-10-22T20:00:11Z","cross_cats_sorted":[],"title_canon_sha256":"b8e7aa238fc71d7d85c209904f9b52427b4d8018dea67ea502bfd628fea78c34","abstract_canon_sha256":"4214cc7584605eadad38167025c880b0434a9442e25b6be42c229645d1cf18b8"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:41:40.859870Z","signature_b64":"HkY9RS9/wwplyMhbCRm0h2kk0d1KInJUF93uzh+wssgqhjzGeK5FaWfno3euTqEalhj98LOAeazlwS+Yir6KAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a82c9f7ffa8bc53fd148e844380b3034b4f9627f25124cd862415ecb3eb4496c","last_reissued_at":"2026-05-18T01:41:40.859234Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:41:40.859234Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Survey of Lines in M31 (SLIM): Investigating the Origins of [CII] Emission","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Leroy, B. Groves, E. Schinnerer, F. Walter, J. Dalcanton, K. Croxall, K. Kreckel, K. Sandstrom, M. Fouesneau, M. J. Kapala","submitted_at":"2014-10-22T20:00:11Z","abstract_excerpt":"The [CII] 158 micron line is one of the strongest emission lines observed in star-forming galaxies, and has been empirically measured to correlate with the star formation rate (SFR) globally and on ~kpc scales. However, due to the multi-phase origins of [CII], one might expect this relation to break down at small scales. We investigate the origins of [CII] emission by examining high spatial resolution observations of [CII] in M31, with the Survey of Lines in M31 (SLIM). We present five ~700x700 pc (3\"x3\") Fields mapping the [CII] emission, Halpha emission, combined with ancillary infrared (IR)"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1410.6158","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":"1410.6158","created_at":"2026-05-18T01:41:40.859335+00:00"},{"alias_kind":"arxiv_version","alias_value":"1410.6158v1","created_at":"2026-05-18T01:41:40.859335+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1410.6158","created_at":"2026-05-18T01:41:40.859335+00:00"},{"alias_kind":"pith_short_12","alias_value":"VAWJ6772RPCT","created_at":"2026-05-18T12:28:52.271510+00:00"},{"alias_kind":"pith_short_16","alias_value":"VAWJ6772RPCT7UKI","created_at":"2026-05-18T12:28:52.271510+00:00"},{"alias_kind":"pith_short_8","alias_value":"VAWJ6772","created_at":"2026-05-18T12:28:52.271510+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/VAWJ6772RPCT7UKI5BCDQCZQGS","json":"https://pith.science/pith/VAWJ6772RPCT7UKI5BCDQCZQGS.json","graph_json":"https://pith.science/api/pith-number/VAWJ6772RPCT7UKI5BCDQCZQGS/graph.json","events_json":"https://pith.science/api/pith-number/VAWJ6772RPCT7UKI5BCDQCZQGS/events.json","paper":"https://pith.science/paper/VAWJ6772"},"agent_actions":{"view_html":"https://pith.science/pith/VAWJ6772RPCT7UKI5BCDQCZQGS","download_json":"https://pith.science/pith/VAWJ6772RPCT7UKI5BCDQCZQGS.json","view_paper":"https://pith.science/paper/VAWJ6772","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1410.6158&json=true","fetch_graph":"https://pith.science/api/pith-number/VAWJ6772RPCT7UKI5BCDQCZQGS/graph.json","fetch_events":"https://pith.science/api/pith-number/VAWJ6772RPCT7UKI5BCDQCZQGS/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/VAWJ6772RPCT7UKI5BCDQCZQGS/action/timestamp_anchor","attest_storage":"https://pith.science/pith/VAWJ6772RPCT7UKI5BCDQCZQGS/action/storage_attestation","attest_author":"https://pith.science/pith/VAWJ6772RPCT7UKI5BCDQCZQGS/action/author_attestation","sign_citation":"https://pith.science/pith/VAWJ6772RPCT7UKI5BCDQCZQGS/action/citation_signature","submit_replication":"https://pith.science/pith/VAWJ6772RPCT7UKI5BCDQCZQGS/action/replication_record"}},"created_at":"2026-05-18T01:41:40.859335+00:00","updated_at":"2026-05-18T01:41:40.859335+00:00"}