{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2005:X32LS327YILY37VRIWLF2IHWZK","short_pith_number":"pith:X32LS327","schema_version":"1.0","canonical_sha256":"bef4b96f5fc2178dfeb145965d20f6ca867a0c63eba1e3fce5d4971fa27fd831","source":{"kind":"arxiv","id":"astro-ph/0506176","version":1},"attestation_state":"computed","paper":{"title":"The Intrinsic Properties of SMMJ14011+0252","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Durham), Edinburgh), G.P. Smith (Caltech) & R.J. Ivison (IfA/ROE, Ian Smail (ICC","submitted_at":"2005-06-08T19:11:41Z","abstract_excerpt":"We discuss the properties of the bright submillimeter source SMMJ14011+0252 at z=2.56 which lies behind the central regions of the z=0.25 lensing cluster A1835. This system has a complex optical morphology consisting of at least five separate components. We reassess the extensive multiwavelength observations of this system and find strong support for the suggestion that one of these five components represents a foreground galaxy. The spectral and morphological properties of the foreground galaxy indicate that it is a low-luminosity, passive early-type disk member of the A1835 cluster. We estim"},"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/0506176","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2005-06-08T19:11:41Z","cross_cats_sorted":[],"title_canon_sha256":"99466287df6d4cb98be17e5490807cb31f9435ea7dd7408a755006567019142a","abstract_canon_sha256":"e499e97db6ef21083a7d6c83ebe36d8e967a9801640a575c4b18efa74e1af620"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T16:52:31.202474Z","signature_b64":"2xD0V5ODCgYFPmxkhRKCkf8h9iV54ERpnC/Zsz+3qcHGdEX0ytf3XEO9q0XIUjy5oJt1Q+bPU46XVkfo+iqTCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"bef4b96f5fc2178dfeb145965d20f6ca867a0c63eba1e3fce5d4971fa27fd831","last_reissued_at":"2026-07-04T16:52:31.202087Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T16:52:31.202087Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Intrinsic Properties of SMMJ14011+0252","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Durham), Edinburgh), G.P. Smith (Caltech) & R.J. Ivison (IfA/ROE, Ian Smail (ICC","submitted_at":"2005-06-08T19:11:41Z","abstract_excerpt":"We discuss the properties of the bright submillimeter source SMMJ14011+0252 at z=2.56 which lies behind the central regions of the z=0.25 lensing cluster A1835. This system has a complex optical morphology consisting of at least five separate components. We reassess the extensive multiwavelength observations of this system and find strong support for the suggestion that one of these five components represents a foreground galaxy. The spectral and morphological properties of the foreground galaxy indicate that it is a low-luminosity, passive early-type disk member of the A1835 cluster. We estim"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0506176","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/0506176/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/0506176","created_at":"2026-07-04T16:52:31.202162+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0506176v1","created_at":"2026-07-04T16:52:31.202162+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0506176","created_at":"2026-07-04T16:52:31.202162+00:00"},{"alias_kind":"pith_short_12","alias_value":"X32LS327YILY","created_at":"2026-07-04T16:52:31.202162+00:00"},{"alias_kind":"pith_short_16","alias_value":"X32LS327YILY37VR","created_at":"2026-07-04T16:52:31.202162+00:00"},{"alias_kind":"pith_short_8","alias_value":"X32LS327","created_at":"2026-07-04T16:52:31.202162+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.06673","citing_title":"A redshift of z=3.20 for the bright arc in eMACSJ2229.9-0808: Comment on Wagner & Falco (2026) \"Hamilton's Object revisited: A challenging source redshift of a strong lensing configuration\"","ref_index":10,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/X32LS327YILY37VRIWLF2IHWZK","json":"https://pith.science/pith/X32LS327YILY37VRIWLF2IHWZK.json","graph_json":"https://pith.science/api/pith-number/X32LS327YILY37VRIWLF2IHWZK/graph.json","events_json":"https://pith.science/api/pith-number/X32LS327YILY37VRIWLF2IHWZK/events.json","paper":"https://pith.science/paper/X32LS327"},"agent_actions":{"view_html":"https://pith.science/pith/X32LS327YILY37VRIWLF2IHWZK","download_json":"https://pith.science/pith/X32LS327YILY37VRIWLF2IHWZK.json","view_paper":"https://pith.science/paper/X32LS327","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0506176&json=true","fetch_graph":"https://pith.science/api/pith-number/X32LS327YILY37VRIWLF2IHWZK/graph.json","fetch_events":"https://pith.science/api/pith-number/X32LS327YILY37VRIWLF2IHWZK/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/X32LS327YILY37VRIWLF2IHWZK/action/timestamp_anchor","attest_storage":"https://pith.science/pith/X32LS327YILY37VRIWLF2IHWZK/action/storage_attestation","attest_author":"https://pith.science/pith/X32LS327YILY37VRIWLF2IHWZK/action/author_attestation","sign_citation":"https://pith.science/pith/X32LS327YILY37VRIWLF2IHWZK/action/citation_signature","submit_replication":"https://pith.science/pith/X32LS327YILY37VRIWLF2IHWZK/action/replication_record"}},"created_at":"2026-07-04T16:52:31.202162+00:00","updated_at":"2026-07-04T16:52:31.202162+00:00"}