{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:GKQNZDH35URC3VPKA2FFEQ7AV2","short_pith_number":"pith:GKQNZDH3","schema_version":"1.0","canonical_sha256":"32a0dc8cfbed222dd5ea068a5243e0ae9ef5cfdefbbd65c3d8c4f54e76d5d7b3","source":{"kind":"arxiv","id":"2501.12525","version":2},"attestation_state":"computed","paper":{"title":"Detection of Unresolved Strongly Lensed Supernovae with 7-Dimensional Telescope","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","astro-ph.IM"],"primary_cat":"astro-ph.HE","authors_text":"Alex G. Kim, Arman Shafieloo, Elahe Khalouei, Gregory S. H. Paek, Hyung Mok Lee, Myungshin Im, Ryan E. Keeley, William Sheu, Xiaosheng Huang","submitted_at":"2025-01-21T22:28:34Z","abstract_excerpt":"Gravitationally lensed supernovae (glSNe) are a powerful tool for exploring the realms of astronomy and cosmology. Time-delay measurements and lens modeling of glSNe can provide a robust and independent method for constraining the expansion rate of the universe. The study of unresolved glSNe light curves presents a unique opportunity for utilizing small telescopes to investigate these systems. In this work, we investigate diverse observational strategies for the initial detection of glSNe using the 7-Dimensional Telescope (7DT), a multitelescope system composed of twenty 50-cm telescopes. We i"},"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":"2501.12525","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2025-01-21T22:28:34Z","cross_cats_sorted":["astro-ph.CO","astro-ph.IM"],"title_canon_sha256":"e0ab0d6b2eb7fde85c658e49096fe8cf2284961cc394801e1112f1413e3879b4","abstract_canon_sha256":"c8f8c07f0244149db8ea32f35b92b4825a26844a2475b8f272115f245d2fd81c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T11:26:25.645286Z","signature_b64":"yvPHSE9h4W1oVhfpQ+wWkJQaBJSYVTZAe/hhFHQLTJocE0kd+1pILsQ5WPnJM82IfMDbChzKJKf2K+hB7AgGDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"32a0dc8cfbed222dd5ea068a5243e0ae9ef5cfdefbbd65c3d8c4f54e76d5d7b3","last_reissued_at":"2026-07-05T11:26:25.644771Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T11:26:25.644771Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Detection of Unresolved Strongly Lensed Supernovae with 7-Dimensional Telescope","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","astro-ph.IM"],"primary_cat":"astro-ph.HE","authors_text":"Alex G. Kim, Arman Shafieloo, Elahe Khalouei, Gregory S. H. Paek, Hyung Mok Lee, Myungshin Im, Ryan E. Keeley, William Sheu, Xiaosheng Huang","submitted_at":"2025-01-21T22:28:34Z","abstract_excerpt":"Gravitationally lensed supernovae (glSNe) are a powerful tool for exploring the realms of astronomy and cosmology. Time-delay measurements and lens modeling of glSNe can provide a robust and independent method for constraining the expansion rate of the universe. The study of unresolved glSNe light curves presents a unique opportunity for utilizing small telescopes to investigate these systems. In this work, we investigate diverse observational strategies for the initial detection of glSNe using the 7-Dimensional Telescope (7DT), a multitelescope system composed of twenty 50-cm telescopes. We i"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2501.12525","kind":"arxiv","version":2},"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/2501.12525/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":"2501.12525","created_at":"2026-07-05T11:26:25.644831+00:00"},{"alias_kind":"arxiv_version","alias_value":"2501.12525v2","created_at":"2026-07-05T11:26:25.644831+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2501.12525","created_at":"2026-07-05T11:26:25.644831+00:00"},{"alias_kind":"pith_short_12","alias_value":"GKQNZDH35URC","created_at":"2026-07-05T11:26:25.644831+00:00"},{"alias_kind":"pith_short_16","alias_value":"GKQNZDH35URC3VPK","created_at":"2026-07-05T11:26:25.644831+00:00"},{"alias_kind":"pith_short_8","alias_value":"GKQNZDH3","created_at":"2026-07-05T11:26:25.644831+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2604.27511","citing_title":"Finding Strongly Lensed Supernovae from Blended Light Curves","ref_index":35,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/GKQNZDH35URC3VPKA2FFEQ7AV2","json":"https://pith.science/pith/GKQNZDH35URC3VPKA2FFEQ7AV2.json","graph_json":"https://pith.science/api/pith-number/GKQNZDH35URC3VPKA2FFEQ7AV2/graph.json","events_json":"https://pith.science/api/pith-number/GKQNZDH35URC3VPKA2FFEQ7AV2/events.json","paper":"https://pith.science/paper/GKQNZDH3"},"agent_actions":{"view_html":"https://pith.science/pith/GKQNZDH35URC3VPKA2FFEQ7AV2","download_json":"https://pith.science/pith/GKQNZDH35URC3VPKA2FFEQ7AV2.json","view_paper":"https://pith.science/paper/GKQNZDH3","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2501.12525&json=true","fetch_graph":"https://pith.science/api/pith-number/GKQNZDH35URC3VPKA2FFEQ7AV2/graph.json","fetch_events":"https://pith.science/api/pith-number/GKQNZDH35URC3VPKA2FFEQ7AV2/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/GKQNZDH35URC3VPKA2FFEQ7AV2/action/timestamp_anchor","attest_storage":"https://pith.science/pith/GKQNZDH35URC3VPKA2FFEQ7AV2/action/storage_attestation","attest_author":"https://pith.science/pith/GKQNZDH35URC3VPKA2FFEQ7AV2/action/author_attestation","sign_citation":"https://pith.science/pith/GKQNZDH35URC3VPKA2FFEQ7AV2/action/citation_signature","submit_replication":"https://pith.science/pith/GKQNZDH35URC3VPKA2FFEQ7AV2/action/replication_record"}},"created_at":"2026-07-05T11:26:25.644831+00:00","updated_at":"2026-07-05T11:26:25.644831+00:00"}