{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:WLZV6LUAS4LWSFJGCN625EVMWT","short_pith_number":"pith:WLZV6LUA","schema_version":"1.0","canonical_sha256":"b2f35f2e809717691526137dae92acb4fdb4ddfa4e0ea36916df43429cad00d9","source":{"kind":"arxiv","id":"1308.6496","version":1},"attestation_state":"computed","paper":{"title":"A near-infrared census of the multi-component stellar structure of early-type dwarf galaxies in the Virgo cluster","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Boselli, A. Ry\\'s, E. Laurikainen, E. Toloba, G. Hensler, H. Salo, H. T. Meyer, J. Falc\\'on-Barroso, J. Janz, K. S. A. Hansson, M. den Brok, R. F. Peletier, S.-M. Niemi, S. Paudel, T. Lisker","submitted_at":"2013-08-29T15:29:14Z","abstract_excerpt":"The fraction of star-forming to quiescent dwarf galaxies varies from almost infinity in the field to zero in the centers of rich galaxy clusters. What is causing this pronounced morphology-density relation? What do quiescent dwarf galaxies look like when studied in detail, and what conclusions can be drawn about their formation mechanism? Here we study a nearly magnitude-complete sample (-19 < M_r < -16 mag) of 121 Virgo cluster early types with deep near-infrared images from the SMAKCED project. We fit two-dimensional models with optional inner and outer components, as well as bar and lens co"},"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":"1308.6496","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2013-08-29T15:29:14Z","cross_cats_sorted":[],"title_canon_sha256":"9850ebb2b9e02e15043cb5738e913be325d5e836251a83462f965c6602358928","abstract_canon_sha256":"e3960a7e13ccdf4bb19704d50f23f1786c022b4eb219d0cb7644150026363e67"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:47:56.883922Z","signature_b64":"6SLORtI+y9/ljgacXvR9DtqSrdQWJJ4zpbIQf8UUxVQY50BKI69ibUn2XyPPkeBtdnpu2MOr6IPpzcL7I7ayAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"b2f35f2e809717691526137dae92acb4fdb4ddfa4e0ea36916df43429cad00d9","last_reissued_at":"2026-05-18T01:47:56.883452Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:47:56.883452Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A near-infrared census of the multi-component stellar structure of early-type dwarf galaxies in the Virgo cluster","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Boselli, A. Ry\\'s, E. Laurikainen, E. Toloba, G. Hensler, H. Salo, H. T. Meyer, J. Falc\\'on-Barroso, J. Janz, K. S. A. Hansson, M. den Brok, R. F. Peletier, S.-M. Niemi, S. Paudel, T. Lisker","submitted_at":"2013-08-29T15:29:14Z","abstract_excerpt":"The fraction of star-forming to quiescent dwarf galaxies varies from almost infinity in the field to zero in the centers of rich galaxy clusters. What is causing this pronounced morphology-density relation? What do quiescent dwarf galaxies look like when studied in detail, and what conclusions can be drawn about their formation mechanism? Here we study a nearly magnitude-complete sample (-19 < M_r < -16 mag) of 121 Virgo cluster early types with deep near-infrared images from the SMAKCED project. We fit two-dimensional models with optional inner and outer components, as well as bar and lens co"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1308.6496","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":"1308.6496","created_at":"2026-05-18T01:47:56.883529+00:00"},{"alias_kind":"arxiv_version","alias_value":"1308.6496v1","created_at":"2026-05-18T01:47:56.883529+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1308.6496","created_at":"2026-05-18T01:47:56.883529+00:00"},{"alias_kind":"pith_short_12","alias_value":"WLZV6LUAS4LW","created_at":"2026-05-18T12:28:04.890932+00:00"},{"alias_kind":"pith_short_16","alias_value":"WLZV6LUAS4LWSFJG","created_at":"2026-05-18T12:28:04.890932+00:00"},{"alias_kind":"pith_short_8","alias_value":"WLZV6LUA","created_at":"2026-05-18T12:28:04.890932+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/WLZV6LUAS4LWSFJGCN625EVMWT","json":"https://pith.science/pith/WLZV6LUAS4LWSFJGCN625EVMWT.json","graph_json":"https://pith.science/api/pith-number/WLZV6LUAS4LWSFJGCN625EVMWT/graph.json","events_json":"https://pith.science/api/pith-number/WLZV6LUAS4LWSFJGCN625EVMWT/events.json","paper":"https://pith.science/paper/WLZV6LUA"},"agent_actions":{"view_html":"https://pith.science/pith/WLZV6LUAS4LWSFJGCN625EVMWT","download_json":"https://pith.science/pith/WLZV6LUAS4LWSFJGCN625EVMWT.json","view_paper":"https://pith.science/paper/WLZV6LUA","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1308.6496&json=true","fetch_graph":"https://pith.science/api/pith-number/WLZV6LUAS4LWSFJGCN625EVMWT/graph.json","fetch_events":"https://pith.science/api/pith-number/WLZV6LUAS4LWSFJGCN625EVMWT/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/WLZV6LUAS4LWSFJGCN625EVMWT/action/timestamp_anchor","attest_storage":"https://pith.science/pith/WLZV6LUAS4LWSFJGCN625EVMWT/action/storage_attestation","attest_author":"https://pith.science/pith/WLZV6LUAS4LWSFJGCN625EVMWT/action/author_attestation","sign_citation":"https://pith.science/pith/WLZV6LUAS4LWSFJGCN625EVMWT/action/citation_signature","submit_replication":"https://pith.science/pith/WLZV6LUAS4LWSFJGCN625EVMWT/action/replication_record"}},"created_at":"2026-05-18T01:47:56.883529+00:00","updated_at":"2026-05-18T01:47:56.883529+00:00"}