{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2000:STXYVUPROEZ22V2A4ISIHXUGFZ","short_pith_number":"pith:STXYVUPR","schema_version":"1.0","canonical_sha256":"94ef8ad1f17133ad5740e22483de862e58e2d1ab2fb39ec74534eef0b14ed8ea","source":{"kind":"arxiv","id":"astro-ph/0004268","version":1},"attestation_state":"computed","paper":{"title":"Near/Mid Infrared-Wavelength Study of the Interacting Galaxy Pair UGC 12914/5 -- \"Taffy\"","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"D. van Buren, E. Valjavec, G. Helou, J.J. Condon, T.H. Jarrett","submitted_at":"2000-04-18T23:49:57Z","abstract_excerpt":"We report on an infrared 1 to 17 micron study of the nearby (cz = 4600 km/s) interacting spiral galaxy system, UGC 12914/12915, using the ground-based Palomar 200\" telescope and PFIRCAM near-infrared detector and space-based mid-infrared imaging and spectral observations using ISOCAM and Phot-S on the Infrared Space Observatory (ISO). Strong line emission from aromatic band features at 6.2, 7.7 and 11.3 microns are seen in both the mid-IR imaging and Phot-S spectro-photometry centered on the nuclei. In the connecting bridge, the mid-infrared imaging reveals dust grains intermixed with the atom"},"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":"astro-ph/0004268","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2000-04-18T23:49:57Z","cross_cats_sorted":[],"title_canon_sha256":"9f3e80406e875ccf374a37a129efb9c24296c04357c680da40c4d08d7a5ff0f1","abstract_canon_sha256":"96ece6e9b432180b27e5e510a2567aa120c62721c89de692079512223fff6695"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T16:16:19.640971Z","signature_b64":"BqD8IKjDPEsHLMZHY/sA3erW3gDmFlKAxwCmcSZ6oB+ETs89eek5lsQlkzytxzAj7NlRqH29+dh+rtxNhGGNBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"94ef8ad1f17133ad5740e22483de862e58e2d1ab2fb39ec74534eef0b14ed8ea","last_reissued_at":"2026-07-04T16:16:19.640515Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T16:16:19.640515Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Near/Mid Infrared-Wavelength Study of the Interacting Galaxy Pair UGC 12914/5 -- \"Taffy\"","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"D. van Buren, E. Valjavec, G. Helou, J.J. Condon, T.H. Jarrett","submitted_at":"2000-04-18T23:49:57Z","abstract_excerpt":"We report on an infrared 1 to 17 micron study of the nearby (cz = 4600 km/s) interacting spiral galaxy system, UGC 12914/12915, using the ground-based Palomar 200\" telescope and PFIRCAM near-infrared detector and space-based mid-infrared imaging and spectral observations using ISOCAM and Phot-S on the Infrared Space Observatory (ISO). Strong line emission from aromatic band features at 6.2, 7.7 and 11.3 microns are seen in both the mid-IR imaging and Phot-S spectro-photometry centered on the nuclei. In the connecting bridge, the mid-infrared imaging reveals dust grains intermixed with the atom"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0004268","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/astro-ph/0004268/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":"astro-ph/0004268","created_at":"2026-07-04T16:16:19.640576+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0004268v1","created_at":"2026-07-04T16:16:19.640576+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0004268","created_at":"2026-07-04T16:16:19.640576+00:00"},{"alias_kind":"pith_short_12","alias_value":"STXYVUPROEZ2","created_at":"2026-07-04T16:16:19.640576+00:00"},{"alias_kind":"pith_short_16","alias_value":"STXYVUPROEZ22V2A","created_at":"2026-07-04T16:16:19.640576+00:00"},{"alias_kind":"pith_short_8","alias_value":"STXYVUPR","created_at":"2026-07-04T16:16:19.640576+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/STXYVUPROEZ22V2A4ISIHXUGFZ","json":"https://pith.science/pith/STXYVUPROEZ22V2A4ISIHXUGFZ.json","graph_json":"https://pith.science/api/pith-number/STXYVUPROEZ22V2A4ISIHXUGFZ/graph.json","events_json":"https://pith.science/api/pith-number/STXYVUPROEZ22V2A4ISIHXUGFZ/events.json","paper":"https://pith.science/paper/STXYVUPR"},"agent_actions":{"view_html":"https://pith.science/pith/STXYVUPROEZ22V2A4ISIHXUGFZ","download_json":"https://pith.science/pith/STXYVUPROEZ22V2A4ISIHXUGFZ.json","view_paper":"https://pith.science/paper/STXYVUPR","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0004268&json=true","fetch_graph":"https://pith.science/api/pith-number/STXYVUPROEZ22V2A4ISIHXUGFZ/graph.json","fetch_events":"https://pith.science/api/pith-number/STXYVUPROEZ22V2A4ISIHXUGFZ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/STXYVUPROEZ22V2A4ISIHXUGFZ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/STXYVUPROEZ22V2A4ISIHXUGFZ/action/storage_attestation","attest_author":"https://pith.science/pith/STXYVUPROEZ22V2A4ISIHXUGFZ/action/author_attestation","sign_citation":"https://pith.science/pith/STXYVUPROEZ22V2A4ISIHXUGFZ/action/citation_signature","submit_replication":"https://pith.science/pith/STXYVUPROEZ22V2A4ISIHXUGFZ/action/replication_record"}},"created_at":"2026-07-04T16:16:19.640576+00:00","updated_at":"2026-07-04T16:16:19.640576+00:00"}