{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:OV4PZWYEN6TTMJLHGH3WDJHHAY","short_pith_number":"pith:OV4PZWYE","schema_version":"1.0","canonical_sha256":"7578fcdb046fa736256731f761a4e70602268b66213f88fdc5f0dc29539ac515","source":{"kind":"arxiv","id":"1705.03839","version":1},"attestation_state":"computed","paper":{"title":"The effects of the cluster environment on the galaxy mass-size relation in MACSJ J1206.2-0847","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"B. H\\\"au{\\ss}ler, B. Ziegler, M. Verdugo, S. Bamford, U. Kuchner","submitted_at":"2017-05-10T16:09:50Z","abstract_excerpt":"The dense environment of galaxy clusters strongly influences the nature of galaxies. Here, we study the cause of the size distribution of a sample of 560 spectroscopic members spanning a wide dynamical range down to 10^8.5 M_sol (log(M)-2) in the massive CLASH cluster MACSJ 1206.2-0847 at z~0.44. We use Subaru SuprimeCam imaging covering the highest-density core out to the infall regions (3 virial radii) to look for cluster-specific effects. We also compare our measurements to a compatible large field study in order to span extreme environmental densities. This paper presents the trends we ide"},"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":"1705.03839","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-05-10T16:09:50Z","cross_cats_sorted":[],"title_canon_sha256":"671c22b66aa59c3535d3a358596fa3f4c219f80b86398c22a80aeb0576996847","abstract_canon_sha256":"84ee4816169d2f931cc3584763585fd7a8b38459202a4869a6a7ad4a47d83e66"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:38:27.283209Z","signature_b64":"B4xjDo129esVvyie6DI0E7rHYb76l6E4ZspNzfQQcYydakM65/MChvptbpDGPafhzbb4QvYsPDpqxYM7opq6Dw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"7578fcdb046fa736256731f761a4e70602268b66213f88fdc5f0dc29539ac515","last_reissued_at":"2026-05-18T00:38:27.282560Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:38:27.282560Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The effects of the cluster environment on the galaxy mass-size relation in MACSJ J1206.2-0847","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"B. H\\\"au{\\ss}ler, B. Ziegler, M. Verdugo, S. Bamford, U. Kuchner","submitted_at":"2017-05-10T16:09:50Z","abstract_excerpt":"The dense environment of galaxy clusters strongly influences the nature of galaxies. Here, we study the cause of the size distribution of a sample of 560 spectroscopic members spanning a wide dynamical range down to 10^8.5 M_sol (log(M)-2) in the massive CLASH cluster MACSJ 1206.2-0847 at z~0.44. We use Subaru SuprimeCam imaging covering the highest-density core out to the infall regions (3 virial radii) to look for cluster-specific effects. We also compare our measurements to a compatible large field study in order to span extreme environmental densities. This paper presents the trends we ide"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1705.03839","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":"1705.03839","created_at":"2026-05-18T00:38:27.282662+00:00"},{"alias_kind":"arxiv_version","alias_value":"1705.03839v1","created_at":"2026-05-18T00:38:27.282662+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1705.03839","created_at":"2026-05-18T00:38:27.282662+00:00"},{"alias_kind":"pith_short_12","alias_value":"OV4PZWYEN6TT","created_at":"2026-05-18T12:31:34.259226+00:00"},{"alias_kind":"pith_short_16","alias_value":"OV4PZWYEN6TTMJLH","created_at":"2026-05-18T12:31:34.259226+00:00"},{"alias_kind":"pith_short_8","alias_value":"OV4PZWYE","created_at":"2026-05-18T12:31:34.259226+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/OV4PZWYEN6TTMJLHGH3WDJHHAY","json":"https://pith.science/pith/OV4PZWYEN6TTMJLHGH3WDJHHAY.json","graph_json":"https://pith.science/api/pith-number/OV4PZWYEN6TTMJLHGH3WDJHHAY/graph.json","events_json":"https://pith.science/api/pith-number/OV4PZWYEN6TTMJLHGH3WDJHHAY/events.json","paper":"https://pith.science/paper/OV4PZWYE"},"agent_actions":{"view_html":"https://pith.science/pith/OV4PZWYEN6TTMJLHGH3WDJHHAY","download_json":"https://pith.science/pith/OV4PZWYEN6TTMJLHGH3WDJHHAY.json","view_paper":"https://pith.science/paper/OV4PZWYE","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1705.03839&json=true","fetch_graph":"https://pith.science/api/pith-number/OV4PZWYEN6TTMJLHGH3WDJHHAY/graph.json","fetch_events":"https://pith.science/api/pith-number/OV4PZWYEN6TTMJLHGH3WDJHHAY/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/OV4PZWYEN6TTMJLHGH3WDJHHAY/action/timestamp_anchor","attest_storage":"https://pith.science/pith/OV4PZWYEN6TTMJLHGH3WDJHHAY/action/storage_attestation","attest_author":"https://pith.science/pith/OV4PZWYEN6TTMJLHGH3WDJHHAY/action/author_attestation","sign_citation":"https://pith.science/pith/OV4PZWYEN6TTMJLHGH3WDJHHAY/action/citation_signature","submit_replication":"https://pith.science/pith/OV4PZWYEN6TTMJLHGH3WDJHHAY/action/replication_record"}},"created_at":"2026-05-18T00:38:27.282662+00:00","updated_at":"2026-05-18T00:38:27.282662+00:00"}