{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:ZQBOFOZ4L6GUAEEGHWNIHAPNAA","short_pith_number":"pith:ZQBOFOZ4","schema_version":"1.0","canonical_sha256":"cc02e2bb3c5f8d4010863d9a8381ed00180fd0daac673d0fd9af8570dcfce421","source":{"kind":"arxiv","id":"1605.00004","version":1},"attestation_state":"computed","paper":{"title":"Tidal stirring of satellites with shallow density profiles prevents them from being too big to fail","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Lucio Mayer, Mihai Tomozeiu, Thomas Quinn","submitted_at":"2016-04-29T20:00:01Z","abstract_excerpt":"The \"too big to fail\" problem is revisited by studying the tidal evolution of populations of dwarf satellites with different density profiles. The high resolution cosmological $\\rm \\Lambda CDM$ \"ErisMod\" set of simulations is used. These simulations can model both the stellar and dark matter components of the satellites, and their evolution under the action of the tides of a MW-sized host halo at a force resolution better than 10 pc. The stronger tidal mass loss and re-shaping of the mass distribution induced in satellites with $\\gamma=0.6$ dark matter density distributions, as those resulting"},"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":"1605.00004","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2016-04-29T20:00:01Z","cross_cats_sorted":[],"title_canon_sha256":"232bdaefa3198cb260a9aca26a85b80b7fe660eafa327c5254786780f3b87659","abstract_canon_sha256":"d49284a6321d60d617c03c48b25b366403d930256c4548f3e01a33689b85bed4"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:08:41.630015Z","signature_b64":"6/WqXSo9v7sAiEXLs/5KeBMfJOo2pl65eNu+x0tc0MpBK2j1u3OLCqZkYpuk3611NNA7xocrXSsvRuER0BY4CA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"cc02e2bb3c5f8d4010863d9a8381ed00180fd0daac673d0fd9af8570dcfce421","last_reissued_at":"2026-05-18T01:08:41.629471Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:08:41.629471Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Tidal stirring of satellites with shallow density profiles prevents them from being too big to fail","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Lucio Mayer, Mihai Tomozeiu, Thomas Quinn","submitted_at":"2016-04-29T20:00:01Z","abstract_excerpt":"The \"too big to fail\" problem is revisited by studying the tidal evolution of populations of dwarf satellites with different density profiles. The high resolution cosmological $\\rm \\Lambda CDM$ \"ErisMod\" set of simulations is used. These simulations can model both the stellar and dark matter components of the satellites, and their evolution under the action of the tides of a MW-sized host halo at a force resolution better than 10 pc. The stronger tidal mass loss and re-shaping of the mass distribution induced in satellites with $\\gamma=0.6$ dark matter density distributions, as those resulting"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1605.00004","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":"1605.00004","created_at":"2026-05-18T01:08:41.629549+00:00"},{"alias_kind":"arxiv_version","alias_value":"1605.00004v1","created_at":"2026-05-18T01:08:41.629549+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1605.00004","created_at":"2026-05-18T01:08:41.629549+00:00"},{"alias_kind":"pith_short_12","alias_value":"ZQBOFOZ4L6GU","created_at":"2026-05-18T12:30:55.937587+00:00"},{"alias_kind":"pith_short_16","alias_value":"ZQBOFOZ4L6GUAEEG","created_at":"2026-05-18T12:30:55.937587+00:00"},{"alias_kind":"pith_short_8","alias_value":"ZQBOFOZ4","created_at":"2026-05-18T12:30:55.937587+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/ZQBOFOZ4L6GUAEEGHWNIHAPNAA","json":"https://pith.science/pith/ZQBOFOZ4L6GUAEEGHWNIHAPNAA.json","graph_json":"https://pith.science/api/pith-number/ZQBOFOZ4L6GUAEEGHWNIHAPNAA/graph.json","events_json":"https://pith.science/api/pith-number/ZQBOFOZ4L6GUAEEGHWNIHAPNAA/events.json","paper":"https://pith.science/paper/ZQBOFOZ4"},"agent_actions":{"view_html":"https://pith.science/pith/ZQBOFOZ4L6GUAEEGHWNIHAPNAA","download_json":"https://pith.science/pith/ZQBOFOZ4L6GUAEEGHWNIHAPNAA.json","view_paper":"https://pith.science/paper/ZQBOFOZ4","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1605.00004&json=true","fetch_graph":"https://pith.science/api/pith-number/ZQBOFOZ4L6GUAEEGHWNIHAPNAA/graph.json","fetch_events":"https://pith.science/api/pith-number/ZQBOFOZ4L6GUAEEGHWNIHAPNAA/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/ZQBOFOZ4L6GUAEEGHWNIHAPNAA/action/timestamp_anchor","attest_storage":"https://pith.science/pith/ZQBOFOZ4L6GUAEEGHWNIHAPNAA/action/storage_attestation","attest_author":"https://pith.science/pith/ZQBOFOZ4L6GUAEEGHWNIHAPNAA/action/author_attestation","sign_citation":"https://pith.science/pith/ZQBOFOZ4L6GUAEEGHWNIHAPNAA/action/citation_signature","submit_replication":"https://pith.science/pith/ZQBOFOZ4L6GUAEEGHWNIHAPNAA/action/replication_record"}},"created_at":"2026-05-18T01:08:41.629549+00:00","updated_at":"2026-05-18T01:08:41.629549+00:00"}