{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:6RFMGC2XSXHG6S3VCZFR2V3NCI","short_pith_number":"pith:6RFMGC2X","schema_version":"1.0","canonical_sha256":"f44ac30b5795ce6f4b75164b1d576d1200b5aaee9a0e6b29be291d99d2409170","source":{"kind":"arxiv","id":"1711.01347","version":1},"attestation_state":"computed","paper":{"title":"Merging Cluster Collaboration: Optical and Spectroscopic Survey of a Radio-Selected Sample of Twenty Nine Merging Galaxy Clusters","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.CO","authors_text":"Annika Peter, Brian Lemaux, Bryant Benson, David M. Wittman, David Sobral, Felipe Andrade-Santos, Francesco de Gasperin, Kyle Finner, Marcus Bruggen, Marusa Bradac, Myungkook J. Jee, Nathan Golovich, Reinout J. van Weeren, William A. Dawson","submitted_at":"2017-11-03T22:12:04Z","abstract_excerpt":"Multi-band photometric and multi-object spectroscopic surveys of merging galaxy clusters allow for the characterization of the distributions of constituent dark matter and galaxy populations, constraints on the dynamics of the merging subclusters, and an understanding of galaxy evolution of member galaxies. We present deep photometric observations from Subaru/SuprimeCam and a catalog of $\\sim$5400 spectroscopic cluster members from Keck/DEIMOS across 29 merging galaxy clusters ranging in redshift from $z=0.07$ to $0.55$. The ensemble is compiled based on the presence of radio relics, which hig"},"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":"1711.01347","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2017-11-03T22:12:04Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"1ec696d906a7d6eeb3c96ae39a40729fa95e28b885e10c90ea4c504c59f50b43","abstract_canon_sha256":"19a807c8af6797128c3191d86c8cc7b998426b184abd85822baa60e06354145d"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:31:18.105666Z","signature_b64":"wQ3j5AqhX6BJcWcieiGQVK4w/fXOBcnpFF6spAZ7IOky0EfabP5ZZUS90sKCM2fWsZfUmt7oFnL2MIYQTPOYDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f44ac30b5795ce6f4b75164b1d576d1200b5aaee9a0e6b29be291d99d2409170","last_reissued_at":"2026-05-18T00:31:18.104967Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:31:18.104967Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Merging Cluster Collaboration: Optical and Spectroscopic Survey of a Radio-Selected Sample of Twenty Nine Merging Galaxy Clusters","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.CO","authors_text":"Annika Peter, Brian Lemaux, Bryant Benson, David M. Wittman, David Sobral, Felipe Andrade-Santos, Francesco de Gasperin, Kyle Finner, Marcus Bruggen, Marusa Bradac, Myungkook J. Jee, Nathan Golovich, Reinout J. van Weeren, William A. Dawson","submitted_at":"2017-11-03T22:12:04Z","abstract_excerpt":"Multi-band photometric and multi-object spectroscopic surveys of merging galaxy clusters allow for the characterization of the distributions of constituent dark matter and galaxy populations, constraints on the dynamics of the merging subclusters, and an understanding of galaxy evolution of member galaxies. We present deep photometric observations from Subaru/SuprimeCam and a catalog of $\\sim$5400 spectroscopic cluster members from Keck/DEIMOS across 29 merging galaxy clusters ranging in redshift from $z=0.07$ to $0.55$. The ensemble is compiled based on the presence of radio relics, which hig"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1711.01347","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":"1711.01347","created_at":"2026-05-18T00:31:18.105071+00:00"},{"alias_kind":"arxiv_version","alias_value":"1711.01347v1","created_at":"2026-05-18T00:31:18.105071+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1711.01347","created_at":"2026-05-18T00:31:18.105071+00:00"},{"alias_kind":"pith_short_12","alias_value":"6RFMGC2XSXHG","created_at":"2026-05-18T12:31:03.183658+00:00"},{"alias_kind":"pith_short_16","alias_value":"6RFMGC2XSXHG6S3V","created_at":"2026-05-18T12:31:03.183658+00:00"},{"alias_kind":"pith_short_8","alias_value":"6RFMGC2X","created_at":"2026-05-18T12:31:03.183658+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/6RFMGC2XSXHG6S3VCZFR2V3NCI","json":"https://pith.science/pith/6RFMGC2XSXHG6S3VCZFR2V3NCI.json","graph_json":"https://pith.science/api/pith-number/6RFMGC2XSXHG6S3VCZFR2V3NCI/graph.json","events_json":"https://pith.science/api/pith-number/6RFMGC2XSXHG6S3VCZFR2V3NCI/events.json","paper":"https://pith.science/paper/6RFMGC2X"},"agent_actions":{"view_html":"https://pith.science/pith/6RFMGC2XSXHG6S3VCZFR2V3NCI","download_json":"https://pith.science/pith/6RFMGC2XSXHG6S3VCZFR2V3NCI.json","view_paper":"https://pith.science/paper/6RFMGC2X","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1711.01347&json=true","fetch_graph":"https://pith.science/api/pith-number/6RFMGC2XSXHG6S3VCZFR2V3NCI/graph.json","fetch_events":"https://pith.science/api/pith-number/6RFMGC2XSXHG6S3VCZFR2V3NCI/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/6RFMGC2XSXHG6S3VCZFR2V3NCI/action/timestamp_anchor","attest_storage":"https://pith.science/pith/6RFMGC2XSXHG6S3VCZFR2V3NCI/action/storage_attestation","attest_author":"https://pith.science/pith/6RFMGC2XSXHG6S3VCZFR2V3NCI/action/author_attestation","sign_citation":"https://pith.science/pith/6RFMGC2XSXHG6S3VCZFR2V3NCI/action/citation_signature","submit_replication":"https://pith.science/pith/6RFMGC2XSXHG6S3VCZFR2V3NCI/action/replication_record"}},"created_at":"2026-05-18T00:31:18.105071+00:00","updated_at":"2026-05-18T00:31:18.105071+00:00"}