{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:4G4U4QSECWEOSMCFYF32JZSB5D","short_pith_number":"pith:4G4U4QSE","schema_version":"1.0","canonical_sha256":"e1b94e42441588e93045c177a4e641e8ff2c7b0e0a0fd39431f28a49dcd45056","source":{"kind":"arxiv","id":"2002.12870","version":3},"attestation_state":"computed","paper":{"title":"Mid-Infrared Diagnostics of the Circumnuclear Environments of the Youngest Radio Galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.HE","authors_text":"A. Siemiginowska, A. Wojtowicz, C.C. Cheung, D. Koziel-Wierzbowska, E. Kosmaczewski, L. Ostorero, L. Stawarz, M. Sobolewska, V. Marchenko","submitted_at":"2020-02-28T17:11:31Z","abstract_excerpt":"We present a systematic analysis of the mid-infrared (MIR) properties of the youngest radio galaxies, based on low-resolution data provided by the {\\it WISE} and {\\it IRAS} satellites. We restrict our analysis to sources with available X-ray data that constitute the earliest phase of radio galaxy evolution, i.e. those classified as Gigahertz Peaked Spectrum (GPS) and/or Compact Symmetric Objects (CSOs). In our sample of 29 objects, we find that the host galaxies are predominantly red/yellow ellipticals, with some of them displaying distorted morphology. We find a variety of MIR colors, and obs"},"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":"2002.12870","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2020-02-28T17:11:31Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"71d88425b00c8bb6368916358276cadfd54fe4a42548004bd618c2cd66f28909","abstract_canon_sha256":"3c459df79ffe24c51630a7eda6cf689b46f1179099c0086cffe1601a89ad2f1f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T01:20:54.077204Z","signature_b64":"xB2HuRg8Z2zHgaqYYvAnI8GrPlnZPPtOcKVKllTtuTuR1zplOTn8K3uKyOXalELF5sNUTpgtYki7LVyDTV6oAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e1b94e42441588e93045c177a4e641e8ff2c7b0e0a0fd39431f28a49dcd45056","last_reissued_at":"2026-07-05T01:20:54.076362Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T01:20:54.076362Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Mid-Infrared Diagnostics of the Circumnuclear Environments of the Youngest Radio Galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.HE","authors_text":"A. Siemiginowska, A. Wojtowicz, C.C. Cheung, D. Koziel-Wierzbowska, E. Kosmaczewski, L. Ostorero, L. Stawarz, M. Sobolewska, V. Marchenko","submitted_at":"2020-02-28T17:11:31Z","abstract_excerpt":"We present a systematic analysis of the mid-infrared (MIR) properties of the youngest radio galaxies, based on low-resolution data provided by the {\\it WISE} and {\\it IRAS} satellites. We restrict our analysis to sources with available X-ray data that constitute the earliest phase of radio galaxy evolution, i.e. those classified as Gigahertz Peaked Spectrum (GPS) and/or Compact Symmetric Objects (CSOs). In our sample of 29 objects, we find that the host galaxies are predominantly red/yellow ellipticals, with some of them displaying distorted morphology. We find a variety of MIR colors, and obs"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2002.12870","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/2002.12870/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":"2002.12870","created_at":"2026-07-05T01:20:54.076425+00:00"},{"alias_kind":"arxiv_version","alias_value":"2002.12870v3","created_at":"2026-07-05T01:20:54.076425+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2002.12870","created_at":"2026-07-05T01:20:54.076425+00:00"},{"alias_kind":"pith_short_12","alias_value":"4G4U4QSECWEO","created_at":"2026-07-05T01:20:54.076425+00:00"},{"alias_kind":"pith_short_16","alias_value":"4G4U4QSECWEOSMCF","created_at":"2026-07-05T01:20:54.076425+00:00"},{"alias_kind":"pith_short_8","alias_value":"4G4U4QSE","created_at":"2026-07-05T01:20:54.076425+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/4G4U4QSECWEOSMCFYF32JZSB5D","json":"https://pith.science/pith/4G4U4QSECWEOSMCFYF32JZSB5D.json","graph_json":"https://pith.science/api/pith-number/4G4U4QSECWEOSMCFYF32JZSB5D/graph.json","events_json":"https://pith.science/api/pith-number/4G4U4QSECWEOSMCFYF32JZSB5D/events.json","paper":"https://pith.science/paper/4G4U4QSE"},"agent_actions":{"view_html":"https://pith.science/pith/4G4U4QSECWEOSMCFYF32JZSB5D","download_json":"https://pith.science/pith/4G4U4QSECWEOSMCFYF32JZSB5D.json","view_paper":"https://pith.science/paper/4G4U4QSE","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2002.12870&json=true","fetch_graph":"https://pith.science/api/pith-number/4G4U4QSECWEOSMCFYF32JZSB5D/graph.json","fetch_events":"https://pith.science/api/pith-number/4G4U4QSECWEOSMCFYF32JZSB5D/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/4G4U4QSECWEOSMCFYF32JZSB5D/action/timestamp_anchor","attest_storage":"https://pith.science/pith/4G4U4QSECWEOSMCFYF32JZSB5D/action/storage_attestation","attest_author":"https://pith.science/pith/4G4U4QSECWEOSMCFYF32JZSB5D/action/author_attestation","sign_citation":"https://pith.science/pith/4G4U4QSECWEOSMCFYF32JZSB5D/action/citation_signature","submit_replication":"https://pith.science/pith/4G4U4QSECWEOSMCFYF32JZSB5D/action/replication_record"}},"created_at":"2026-07-05T01:20:54.076425+00:00","updated_at":"2026-07-05T01:20:54.076425+00:00"}