{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:I4U3QVUD7YNVE2OZCQFDXLTLJH","short_pith_number":"pith:I4U3QVUD","schema_version":"1.0","canonical_sha256":"4729b85683fe1b5269d9140a3bae6b49e25d35c876f0d1ee21989e344651f6d6","source":{"kind":"arxiv","id":"2208.03383","version":3},"attestation_state":"computed","paper":{"title":"Active Galactic Nuclei signatures in Red Geyser galaxies from Gemini GMOS-IFU observations","license":"http://creativecommons.org/licenses/by-nc-sa/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"G. S. Ilha, J. S. Schimoia, K. Bundy, L. N. da Costa, N. Roy, R. A. Riffel, R. Nemmen, R. Riffel, S. B. Rembold, T. Storchi-Bergmann, T.V. Ricci","submitted_at":"2022-08-05T20:49:46Z","abstract_excerpt":"Red Geysers are quiescent galaxies with galactic scale ionised outflows, likely due to low-luminosity Active Galactic Nuclei (AGN). We used Gemini GMOS-IFU observations of the inner $\\sim 1.0-3.0$ kpc of nine Red Geysers selected from the MaNGA survey to study the gas ionisation and kinematics. The emission-line ratios suggest the presence of Seyfert/LINER (Low Ionisation Nuclear Emission Region) nuclei in all sources. Two galaxies show H$\\alpha$ equivalent width (H$\\alpha$ EW) larger than 3 \\AA (indicative of AGN ionisation) within an aperture 2.5 arcsec of diameter ($1.3-3.7$ kpc at the dist"},"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":"2208.03383","kind":"arxiv","version":3},"metadata":{"license":"http://creativecommons.org/licenses/by-nc-sa/4.0/","primary_cat":"astro-ph.GA","submitted_at":"2022-08-05T20:49:46Z","cross_cats_sorted":[],"title_canon_sha256":"21b5a7b686f76d92f7b561be11019de04967d039bf1416e5212eeb609da9cfcd","abstract_canon_sha256":"11a099b292f98033b13d634dac10fd88c66e3ba8b4f46223de4320cf181975fe"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T04:51:01.634130Z","signature_b64":"X+n95qwtZr/MFXsTe2PCIORi1WBRgGpU0dSDSoURqaMDxKxgL0hyUb+zFaARAD33MsSwUuT1msKl7+RWdcJhAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4729b85683fe1b5269d9140a3bae6b49e25d35c876f0d1ee21989e344651f6d6","last_reissued_at":"2026-07-05T04:51:01.633722Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T04:51:01.633722Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Active Galactic Nuclei signatures in Red Geyser galaxies from Gemini GMOS-IFU observations","license":"http://creativecommons.org/licenses/by-nc-sa/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"G. S. Ilha, J. S. Schimoia, K. Bundy, L. N. da Costa, N. Roy, R. A. Riffel, R. Nemmen, R. Riffel, S. B. Rembold, T. Storchi-Bergmann, T.V. Ricci","submitted_at":"2022-08-05T20:49:46Z","abstract_excerpt":"Red Geysers are quiescent galaxies with galactic scale ionised outflows, likely due to low-luminosity Active Galactic Nuclei (AGN). We used Gemini GMOS-IFU observations of the inner $\\sim 1.0-3.0$ kpc of nine Red Geysers selected from the MaNGA survey to study the gas ionisation and kinematics. The emission-line ratios suggest the presence of Seyfert/LINER (Low Ionisation Nuclear Emission Region) nuclei in all sources. Two galaxies show H$\\alpha$ equivalent width (H$\\alpha$ EW) larger than 3 \\AA (indicative of AGN ionisation) within an aperture 2.5 arcsec of diameter ($1.3-3.7$ kpc at the dist"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2208.03383","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/2208.03383/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":"2208.03383","created_at":"2026-07-05T04:51:01.633786+00:00"},{"alias_kind":"arxiv_version","alias_value":"2208.03383v3","created_at":"2026-07-05T04:51:01.633786+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2208.03383","created_at":"2026-07-05T04:51:01.633786+00:00"},{"alias_kind":"pith_short_12","alias_value":"I4U3QVUD7YNV","created_at":"2026-07-05T04:51:01.633786+00:00"},{"alias_kind":"pith_short_16","alias_value":"I4U3QVUD7YNVE2OZ","created_at":"2026-07-05T04:51:01.633786+00:00"},{"alias_kind":"pith_short_8","alias_value":"I4U3QVUD","created_at":"2026-07-05T04:51:01.633786+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/I4U3QVUD7YNVE2OZCQFDXLTLJH","json":"https://pith.science/pith/I4U3QVUD7YNVE2OZCQFDXLTLJH.json","graph_json":"https://pith.science/api/pith-number/I4U3QVUD7YNVE2OZCQFDXLTLJH/graph.json","events_json":"https://pith.science/api/pith-number/I4U3QVUD7YNVE2OZCQFDXLTLJH/events.json","paper":"https://pith.science/paper/I4U3QVUD"},"agent_actions":{"view_html":"https://pith.science/pith/I4U3QVUD7YNVE2OZCQFDXLTLJH","download_json":"https://pith.science/pith/I4U3QVUD7YNVE2OZCQFDXLTLJH.json","view_paper":"https://pith.science/paper/I4U3QVUD","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2208.03383&json=true","fetch_graph":"https://pith.science/api/pith-number/I4U3QVUD7YNVE2OZCQFDXLTLJH/graph.json","fetch_events":"https://pith.science/api/pith-number/I4U3QVUD7YNVE2OZCQFDXLTLJH/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/I4U3QVUD7YNVE2OZCQFDXLTLJH/action/timestamp_anchor","attest_storage":"https://pith.science/pith/I4U3QVUD7YNVE2OZCQFDXLTLJH/action/storage_attestation","attest_author":"https://pith.science/pith/I4U3QVUD7YNVE2OZCQFDXLTLJH/action/author_attestation","sign_citation":"https://pith.science/pith/I4U3QVUD7YNVE2OZCQFDXLTLJH/action/citation_signature","submit_replication":"https://pith.science/pith/I4U3QVUD7YNVE2OZCQFDXLTLJH/action/replication_record"}},"created_at":"2026-07-05T04:51:01.633786+00:00","updated_at":"2026-07-05T04:51:01.633786+00:00"}