{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:DUW4CFC2S7ME32GG3XI36QVB4Z","short_pith_number":"pith:DUW4CFC2","schema_version":"1.0","canonical_sha256":"1d2dc1145a97d84de8c6ddd1bf42a1e6449c3244859366a5784fd01be9f3147a","source":{"kind":"arxiv","id":"1208.4260","version":1},"attestation_state":"computed","paper":{"title":"Gemini GMOS--IFU spectroscopy of the compact HII galaxies Tol 0104-388 and Tol 2146-391: The dependence on the properties of the interstellar medium","license":"http://creativecommons.org/licenses/by-nc-sa/3.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Nigoche-Netro, E. R. Carrasco, E. Telles, P. Lagos","submitted_at":"2012-08-21T13:24:03Z","abstract_excerpt":"Using GMOS--IFU spectroscopic observations of the compact HII/BCD galaxies Tol 0104-388 and Tol 2146-391, we study the spatial distribution of emission lines, equivalent width EW(Hb), extinction c(Hb), ionization ratios ([OIII]5007/Hb, [SII]6717,6731/Ha and [NII]6584/Ha), kinematics, and the chemical pattern (O/H, N/H and N/O) of the warm interstellar medium in these galaxies. We also investigate a possible dependence of these properties on the I(HeII4686)/I(Hb) ratio and find no significant correlation between these variables. In fact, the oxygen abundances appear to be uniform in the regions"},"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":"1208.4260","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by-nc-sa/3.0/","primary_cat":"astro-ph.CO","submitted_at":"2012-08-21T13:24:03Z","cross_cats_sorted":[],"title_canon_sha256":"21da59ee9c9fdf265b64e407f36b972faa9d92f0d4283c558061e9d58cad08d8","abstract_canon_sha256":"9f9d1cca056c17f330e7af200194a7abfebfc2fa42472a2679dfbfc69f509127"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:55:08.801403Z","signature_b64":"9CvesUCQkVfUUiSEFy7P7NVlgg3qLOXqK9bxjNH+h4eP10dfrXMFi1ItcvV01Fp+qS3wTU7k4MLkNB55Wz2+Bw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1d2dc1145a97d84de8c6ddd1bf42a1e6449c3244859366a5784fd01be9f3147a","last_reissued_at":"2026-05-18T01:55:08.800963Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:55:08.800963Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Gemini GMOS--IFU spectroscopy of the compact HII galaxies Tol 0104-388 and Tol 2146-391: The dependence on the properties of the interstellar medium","license":"http://creativecommons.org/licenses/by-nc-sa/3.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Nigoche-Netro, E. R. Carrasco, E. Telles, P. Lagos","submitted_at":"2012-08-21T13:24:03Z","abstract_excerpt":"Using GMOS--IFU spectroscopic observations of the compact HII/BCD galaxies Tol 0104-388 and Tol 2146-391, we study the spatial distribution of emission lines, equivalent width EW(Hb), extinction c(Hb), ionization ratios ([OIII]5007/Hb, [SII]6717,6731/Ha and [NII]6584/Ha), kinematics, and the chemical pattern (O/H, N/H and N/O) of the warm interstellar medium in these galaxies. We also investigate a possible dependence of these properties on the I(HeII4686)/I(Hb) ratio and find no significant correlation between these variables. In fact, the oxygen abundances appear to be uniform in the regions"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1208.4260","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":"1208.4260","created_at":"2026-05-18T01:55:08.801024+00:00"},{"alias_kind":"arxiv_version","alias_value":"1208.4260v1","created_at":"2026-05-18T01:55:08.801024+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1208.4260","created_at":"2026-05-18T01:55:08.801024+00:00"},{"alias_kind":"pith_short_12","alias_value":"DUW4CFC2S7ME","created_at":"2026-05-18T12:27:04.183437+00:00"},{"alias_kind":"pith_short_16","alias_value":"DUW4CFC2S7ME32GG","created_at":"2026-05-18T12:27:04.183437+00:00"},{"alias_kind":"pith_short_8","alias_value":"DUW4CFC2","created_at":"2026-05-18T12:27:04.183437+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/DUW4CFC2S7ME32GG3XI36QVB4Z","json":"https://pith.science/pith/DUW4CFC2S7ME32GG3XI36QVB4Z.json","graph_json":"https://pith.science/api/pith-number/DUW4CFC2S7ME32GG3XI36QVB4Z/graph.json","events_json":"https://pith.science/api/pith-number/DUW4CFC2S7ME32GG3XI36QVB4Z/events.json","paper":"https://pith.science/paper/DUW4CFC2"},"agent_actions":{"view_html":"https://pith.science/pith/DUW4CFC2S7ME32GG3XI36QVB4Z","download_json":"https://pith.science/pith/DUW4CFC2S7ME32GG3XI36QVB4Z.json","view_paper":"https://pith.science/paper/DUW4CFC2","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1208.4260&json=true","fetch_graph":"https://pith.science/api/pith-number/DUW4CFC2S7ME32GG3XI36QVB4Z/graph.json","fetch_events":"https://pith.science/api/pith-number/DUW4CFC2S7ME32GG3XI36QVB4Z/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/DUW4CFC2S7ME32GG3XI36QVB4Z/action/timestamp_anchor","attest_storage":"https://pith.science/pith/DUW4CFC2S7ME32GG3XI36QVB4Z/action/storage_attestation","attest_author":"https://pith.science/pith/DUW4CFC2S7ME32GG3XI36QVB4Z/action/author_attestation","sign_citation":"https://pith.science/pith/DUW4CFC2S7ME32GG3XI36QVB4Z/action/citation_signature","submit_replication":"https://pith.science/pith/DUW4CFC2S7ME32GG3XI36QVB4Z/action/replication_record"}},"created_at":"2026-05-18T01:55:08.801024+00:00","updated_at":"2026-05-18T01:55:08.801024+00:00"}