{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:NV6CZGYMPFZPCHLPASXFY7ZUI3","short_pith_number":"pith:NV6CZGYM","schema_version":"1.0","canonical_sha256":"6d7c2c9b0c7972f11d6f04ae5c7f3446d440fb034f5ad3a32a28279446913796","source":{"kind":"arxiv","id":"1105.2492","version":1},"attestation_state":"computed","paper":{"title":"The Spitzer discovery of a galaxy with infrared emission solely due to AGN activity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. A. Zijlstra, A. G. G. M. Tielens, B. Shiao, F. Kemper, G. C. Sloan, J. Mullaney, J. Roman-Duval, J. Th. van Loon, K. D. Gordon, M. Marengo, M. Meixner, Paul M. Woods, P. Panuzzo, R. Indebetouw, S. C. Madden, S. Hony, V. Gorjian","submitted_at":"2011-05-12T14:46:17Z","abstract_excerpt":"We present a galaxy (SAGE1CJ053634.78-722658.5) at a redshift of 0.14 of which the IR is entirely dominated by emission associated with the AGN. We present the 5-37 um Spitzer/IRS spectrum and broad wavelength SED of SAGE1CJ053634, an IR point-source detected by Spitzer/SAGE (Meixner et al 2006). The source was observed in the SAGE-Spec program (Kemper et al., 2010) and was included to determine the nature of sources with deviant IR colours. The spectrum shows a redshifted (z=0.14+-0.005) silicate emission feature with an exceptionally high feature-to-continuum ratio and weak polycyclic aromat"},"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":"1105.2492","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2011-05-12T14:46:17Z","cross_cats_sorted":[],"title_canon_sha256":"fdc5513e6543d85d477a6c8f33b325433298e3f238966b5c1f2b94a2a5c26da8","abstract_canon_sha256":"c62d8d53be95d98db478c4b14c3cca3aa22cd8561a6d54adca6c7367abefaa33"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:01:59.120459Z","signature_b64":"9vaZCohPO6fzOliFKxXoKEiCvPpGeIunLv3RYm5+XLuhS9JE0qYKs4VObCz+b/EU0Zw5gN5U44SGDwbYIaTOCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6d7c2c9b0c7972f11d6f04ae5c7f3446d440fb034f5ad3a32a28279446913796","last_reissued_at":"2026-05-18T02:01:59.120005Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:01:59.120005Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Spitzer discovery of a galaxy with infrared emission solely due to AGN activity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. A. Zijlstra, A. G. G. M. Tielens, B. Shiao, F. Kemper, G. C. Sloan, J. Mullaney, J. Roman-Duval, J. Th. van Loon, K. D. Gordon, M. Marengo, M. Meixner, Paul M. Woods, P. Panuzzo, R. Indebetouw, S. C. Madden, S. Hony, V. Gorjian","submitted_at":"2011-05-12T14:46:17Z","abstract_excerpt":"We present a galaxy (SAGE1CJ053634.78-722658.5) at a redshift of 0.14 of which the IR is entirely dominated by emission associated with the AGN. We present the 5-37 um Spitzer/IRS spectrum and broad wavelength SED of SAGE1CJ053634, an IR point-source detected by Spitzer/SAGE (Meixner et al 2006). The source was observed in the SAGE-Spec program (Kemper et al., 2010) and was included to determine the nature of sources with deviant IR colours. The spectrum shows a redshifted (z=0.14+-0.005) silicate emission feature with an exceptionally high feature-to-continuum ratio and weak polycyclic aromat"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1105.2492","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":"1105.2492","created_at":"2026-05-18T02:01:59.120077+00:00"},{"alias_kind":"arxiv_version","alias_value":"1105.2492v1","created_at":"2026-05-18T02:01:59.120077+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1105.2492","created_at":"2026-05-18T02:01:59.120077+00:00"},{"alias_kind":"pith_short_12","alias_value":"NV6CZGYMPFZP","created_at":"2026-05-18T12:26:37.096874+00:00"},{"alias_kind":"pith_short_16","alias_value":"NV6CZGYMPFZPCHLP","created_at":"2026-05-18T12:26:37.096874+00:00"},{"alias_kind":"pith_short_8","alias_value":"NV6CZGYM","created_at":"2026-05-18T12:26:37.096874+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/NV6CZGYMPFZPCHLPASXFY7ZUI3","json":"https://pith.science/pith/NV6CZGYMPFZPCHLPASXFY7ZUI3.json","graph_json":"https://pith.science/api/pith-number/NV6CZGYMPFZPCHLPASXFY7ZUI3/graph.json","events_json":"https://pith.science/api/pith-number/NV6CZGYMPFZPCHLPASXFY7ZUI3/events.json","paper":"https://pith.science/paper/NV6CZGYM"},"agent_actions":{"view_html":"https://pith.science/pith/NV6CZGYMPFZPCHLPASXFY7ZUI3","download_json":"https://pith.science/pith/NV6CZGYMPFZPCHLPASXFY7ZUI3.json","view_paper":"https://pith.science/paper/NV6CZGYM","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1105.2492&json=true","fetch_graph":"https://pith.science/api/pith-number/NV6CZGYMPFZPCHLPASXFY7ZUI3/graph.json","fetch_events":"https://pith.science/api/pith-number/NV6CZGYMPFZPCHLPASXFY7ZUI3/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/NV6CZGYMPFZPCHLPASXFY7ZUI3/action/timestamp_anchor","attest_storage":"https://pith.science/pith/NV6CZGYMPFZPCHLPASXFY7ZUI3/action/storage_attestation","attest_author":"https://pith.science/pith/NV6CZGYMPFZPCHLPASXFY7ZUI3/action/author_attestation","sign_citation":"https://pith.science/pith/NV6CZGYMPFZPCHLPASXFY7ZUI3/action/citation_signature","submit_replication":"https://pith.science/pith/NV6CZGYMPFZPCHLPASXFY7ZUI3/action/replication_record"}},"created_at":"2026-05-18T02:01:59.120077+00:00","updated_at":"2026-05-18T02:01:59.120077+00:00"}