{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2014:B7X25PK7GPNYT67SACRCRPJWJS","short_pith_number":"pith:B7X25PK7","canonical_record":{"source":{"id":"1407.1767","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2014-07-07T16:44:21Z","cross_cats_sorted":[],"title_canon_sha256":"7d6e4b4233c3b2a8abed41ec8135e423d4f1dc2a5edd44e3e97358dffb6db9d9","abstract_canon_sha256":"4da2b146150358a0eac82fcf4c6adcc51c08fdab1528a33698130bf4dd94e9f0"},"schema_version":"1.0"},"canonical_sha256":"0fefaebd5f33db89fbf200a228bd364c8ecc8d212598e2ddf498063d706f2373","source":{"kind":"arxiv","id":"1407.1767","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1407.1767","created_at":"2026-05-18T01:42:41Z"},{"alias_kind":"arxiv_version","alias_value":"1407.1767v1","created_at":"2026-05-18T01:42:41Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1407.1767","created_at":"2026-05-18T01:42:41Z"},{"alias_kind":"pith_short_12","alias_value":"B7X25PK7GPNY","created_at":"2026-05-18T12:28:22Z"},{"alias_kind":"pith_short_16","alias_value":"B7X25PK7GPNYT67S","created_at":"2026-05-18T12:28:22Z"},{"alias_kind":"pith_short_8","alias_value":"B7X25PK7","created_at":"2026-05-18T12:28:22Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2014:B7X25PK7GPNYT67SACRCRPJWJS","target":"record","payload":{"canonical_record":{"source":{"id":"1407.1767","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2014-07-07T16:44:21Z","cross_cats_sorted":[],"title_canon_sha256":"7d6e4b4233c3b2a8abed41ec8135e423d4f1dc2a5edd44e3e97358dffb6db9d9","abstract_canon_sha256":"4da2b146150358a0eac82fcf4c6adcc51c08fdab1528a33698130bf4dd94e9f0"},"schema_version":"1.0"},"canonical_sha256":"0fefaebd5f33db89fbf200a228bd364c8ecc8d212598e2ddf498063d706f2373","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:42:41.319702Z","signature_b64":"B0bI+Q6rzdzjM/AxXGcB/G2vOWUnOrI2ceS46o7dL37dJHZ4KE4ZN6JwE1CxenlD+D1wAcZcjPCindVkx4iGCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0fefaebd5f33db89fbf200a228bd364c8ecc8d212598e2ddf498063d706f2373","last_reissued_at":"2026-05-18T01:42:41.319098Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:42:41.319098Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1407.1767","source_version":1,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T01:42:41Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"8hYc02KNX56sDopvUr4ZV7cfR66aeQ+YAVZw9LEtBsN235q/knKfk7fCXb6Vq6Y4pjkq82yTwrih4vs9EQx8DA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-19T02:11:41.037001Z"},"content_sha256":"0cf1e183254959a649267a11396464ace21f8c9aca02c63f3378b597adfd4fa6","schema_version":"1.0","event_id":"sha256:0cf1e183254959a649267a11396464ace21f8c9aca02c63f3378b597adfd4fa6"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2014:B7X25PK7GPNYT67SACRCRPJWJS","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"LoCuSS: The Near-Infrared Luminosity and Weak-Lensing Mass Scaling Relation of Galaxy Clusters","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Alexis Finoguenov, Arif Babul, Chris P. Haines, Daniel P. Marrone, Eiichi Egami, Graham P. Smith, Maria J. Pereira, Nobuhiro Okabe, Rossella Martino, Sarah L. Mulroy","submitted_at":"2014-07-07T16:44:21Z","abstract_excerpt":"We present the first scaling relation between weak-lensing galaxy cluster mass, $M_{WL}$, and near-infrared luminosity, $L_K$. Our results are based on 17 clusters observed with wide-field instruments on Subaru, the United Kingdom Infrared Telescope, the Mayall Telescope, and the MMT. We concentrate on the relation between projected 2D weak-lensing mass and spectroscopically confirmed luminosity within 1Mpc, modelled as $M_{WL} \\propto L_{K}^b$, obtaining a power law slope of $b=0.83^{+0.27}_{-0.24}$ and an intrinsic scatter of $\\sigma_{lnM_{WL}|L_{K}}=10^{+8}_{-5}\\%$. Intrinsic scatter of ~10"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1407.1767","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"},"verdict_id":null},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T01:42:41Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"zkQDN1q28qHlCdu2uihplplmwKVXF/y7bj9hLW3hNmr6Y99x5JeMIw53CFoM/iCOSo2XlxINVBBwauJ9l6JBCQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-19T02:11:41.037382Z"},"content_sha256":"5de0ce8358df2eb6df8a15b1ba28b4bb4437aec3a7358f6856210d22260c93c1","schema_version":"1.0","event_id":"sha256:5de0ce8358df2eb6df8a15b1ba28b4bb4437aec3a7358f6856210d22260c93c1"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/B7X25PK7GPNYT67SACRCRPJWJS/bundle.json","state_url":"https://pith.science/pith/B7X25PK7GPNYT67SACRCRPJWJS/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/B7X25PK7GPNYT67SACRCRPJWJS/bundle.json","status":"primary"}],"public_keys":[{"key_id":"pith-v1-2026-05","algorithm":"ed25519","format":"raw","public_key_b64":"stVStoiQhXFxp4s2pdzPNoqVNBMojDU/fJ2db5S3CbM=","public_key_hex":"b2d552b68890857171a78b36a5dccf368a953413288c353f7c9d9d6f94b709b3","fingerprint_sha256_b32_first128bits":"RVFV5Z2OI2J3ZUO7ERDEBCYNKS","fingerprint_sha256_hex":"8d4b5ee74e4693bcd1df2446408b0d54","rotates_at":null,"url":"https://pith.science/pith-signing-key.json","notes":"Pith uses this Ed25519 key to sign canonical record SHA-256 digests. Verify with: ed25519_verify(public_key, message=canonical_sha256_bytes, signature=base64decode(signature_b64))."}],"merge_version":"pith-open-graph-merge-v1","built_at":"2026-05-19T02:11:41Z","links":{"resolver":"https://pith.science/pith/B7X25PK7GPNYT67SACRCRPJWJS","bundle":"https://pith.science/pith/B7X25PK7GPNYT67SACRCRPJWJS/bundle.json","state":"https://pith.science/pith/B7X25PK7GPNYT67SACRCRPJWJS/state.json","well_known_bundle":"https://pith.science/.well-known/pith/B7X25PK7GPNYT67SACRCRPJWJS/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2014:B7X25PK7GPNYT67SACRCRPJWJS","merge_version":"pith-open-graph-merge-v1","event_count":2,"valid_event_count":2,"invalid_event_count":0,"equivocation_count":0,"current":{"canonical_record":{"metadata":{"abstract_canon_sha256":"4da2b146150358a0eac82fcf4c6adcc51c08fdab1528a33698130bf4dd94e9f0","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2014-07-07T16:44:21Z","title_canon_sha256":"7d6e4b4233c3b2a8abed41ec8135e423d4f1dc2a5edd44e3e97358dffb6db9d9"},"schema_version":"1.0","source":{"id":"1407.1767","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1407.1767","created_at":"2026-05-18T01:42:41Z"},{"alias_kind":"arxiv_version","alias_value":"1407.1767v1","created_at":"2026-05-18T01:42:41Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1407.1767","created_at":"2026-05-18T01:42:41Z"},{"alias_kind":"pith_short_12","alias_value":"B7X25PK7GPNY","created_at":"2026-05-18T12:28:22Z"},{"alias_kind":"pith_short_16","alias_value":"B7X25PK7GPNYT67S","created_at":"2026-05-18T12:28:22Z"},{"alias_kind":"pith_short_8","alias_value":"B7X25PK7","created_at":"2026-05-18T12:28:22Z"}],"graph_snapshots":[{"event_id":"sha256:5de0ce8358df2eb6df8a15b1ba28b4bb4437aec3a7358f6856210d22260c93c1","target":"graph","created_at":"2026-05-18T01:42:41Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"graph_snapshot":{"author_claims":{"count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","strong_count":0},"builder_version":"pith-number-builder-2026-05-17-v1","claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"paper":{"abstract_excerpt":"We present the first scaling relation between weak-lensing galaxy cluster mass, $M_{WL}$, and near-infrared luminosity, $L_K$. Our results are based on 17 clusters observed with wide-field instruments on Subaru, the United Kingdom Infrared Telescope, the Mayall Telescope, and the MMT. We concentrate on the relation between projected 2D weak-lensing mass and spectroscopically confirmed luminosity within 1Mpc, modelled as $M_{WL} \\propto L_{K}^b$, obtaining a power law slope of $b=0.83^{+0.27}_{-0.24}$ and an intrinsic scatter of $\\sigma_{lnM_{WL}|L_{K}}=10^{+8}_{-5}\\%$. Intrinsic scatter of ~10","authors_text":"Alexis Finoguenov, Arif Babul, Chris P. Haines, Daniel P. Marrone, Eiichi Egami, Graham P. Smith, Maria J. Pereira, Nobuhiro Okabe, Rossella Martino, Sarah L. Mulroy","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2014-07-07T16:44:21Z","title":"LoCuSS: The Near-Infrared Luminosity and Weak-Lensing Mass Scaling Relation of Galaxy Clusters"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1407.1767","kind":"arxiv","version":1},"verdict":{"created_at":null,"id":null,"model_set":{},"one_line_summary":"","pipeline_version":null,"pith_extraction_headline":"","strongest_claim":"","weakest_assumption":""}},"verdict_id":null}}],"author_attestations":[],"timestamp_anchors":[],"storage_attestations":[],"citation_signatures":[],"replication_records":[],"corrections":[],"mirror_hints":[],"record_created":{"event_id":"sha256:0cf1e183254959a649267a11396464ace21f8c9aca02c63f3378b597adfd4fa6","target":"record","created_at":"2026-05-18T01:42:41Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"attestation_state":"computed","canonical_record":{"metadata":{"abstract_canon_sha256":"4da2b146150358a0eac82fcf4c6adcc51c08fdab1528a33698130bf4dd94e9f0","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2014-07-07T16:44:21Z","title_canon_sha256":"7d6e4b4233c3b2a8abed41ec8135e423d4f1dc2a5edd44e3e97358dffb6db9d9"},"schema_version":"1.0","source":{"id":"1407.1767","kind":"arxiv","version":1}},"canonical_sha256":"0fefaebd5f33db89fbf200a228bd364c8ecc8d212598e2ddf498063d706f2373","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"0fefaebd5f33db89fbf200a228bd364c8ecc8d212598e2ddf498063d706f2373","first_computed_at":"2026-05-18T01:42:41.319098Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T01:42:41.319098Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"B0bI+Q6rzdzjM/AxXGcB/G2vOWUnOrI2ceS46o7dL37dJHZ4KE4ZN6JwE1CxenlD+D1wAcZcjPCindVkx4iGCw==","signature_status":"signed_v1","signed_at":"2026-05-18T01:42:41.319702Z","signed_message":"canonical_sha256_bytes"},"source_id":"1407.1767","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:0cf1e183254959a649267a11396464ace21f8c9aca02c63f3378b597adfd4fa6","sha256:5de0ce8358df2eb6df8a15b1ba28b4bb4437aec3a7358f6856210d22260c93c1"],"state_sha256":"15e0c8e42b37b1940658ecbd172023116a5ea4492d153a55d563ff0f632e1205"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"o/H/dax7r9ElGmUGswlWDJnKpYKrEiO8mFkNbNiraTlzw7PqCRSxf8g7E1z7yy46KdX9EbsTrfI210Y3Ru22BA==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-19T02:11:41.038690Z","bundle_sha256":"b38aeb9be24e7b6eb0b93cb093e70d989274c6252464b8529d0037f3150c4d03"}}