{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:7DTQIZWDJWLSL3WL7QJVNHYSST","short_pith_number":"pith:7DTQIZWD","schema_version":"1.0","canonical_sha256":"f8e70466c34d9725eecbfc13569f1294efb08048f50b61ee3ce5e2b585161566","source":{"kind":"arxiv","id":"1504.06261","version":2},"attestation_state":"computed","paper":{"title":"GARROTXA Cosmological Simulations of Milky Way-sized Galaxies: General Properties, Hot Gas Distribution, and Missing Baryons","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"Francesca Figueras, Hector Ibarra-Medel, H\\'ector Vel\\'azquez, Octavio Valenzuela, Pedro Col\\'in, Santi Roca-F\\`abrega, Vladimir Avila-Reese, Yair Krongold","submitted_at":"2015-04-23T17:14:48Z","abstract_excerpt":"We introduce a new set of simulations of Milky Way-sized galaxies using the AMR code ART + hydrodynamics in a $\\Lambda$CDM cosmogony. The simulation series is named GARROTXA and follow the formation of a halo/galaxy from z~$=$~60 to z~$=$~0. The final virial mass of the system is $\\sim$7.4$\\times$10$^{11}$M$_{\\odot}$. Our results are as follows: (a) contrary to many previous studies, the circular velocity curve shows no central peak and overall agrees with recent MW observations. (b) Other quantities, such as M$\\_{*}$(6$\\times$10$^{10}$M$_\\odot$) and R$_d$ (2.56 kpc), fall well inside the obse"},"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":"1504.06261","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2015-04-23T17:14:48Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"4aaee71470d44b91437891309560bfb1b43433c2043da6002123170574299d48","abstract_canon_sha256":"acd2875e14e2019bde2505f6f650dac26c2d2dc962a9cea210fde9d73d7110d7"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:12:08.590429Z","signature_b64":"SzNtnuiicQLgEeuKXBnM8HxQOsQv+GYpmhsg/yhITiSehsenAHhyTkynL1Na+2lDY9hMQWcOsaXiTD5LuYvFBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f8e70466c34d9725eecbfc13569f1294efb08048f50b61ee3ce5e2b585161566","last_reissued_at":"2026-05-18T01:12:08.589921Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:12:08.589921Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"GARROTXA Cosmological Simulations of Milky Way-sized Galaxies: General Properties, Hot Gas Distribution, and Missing Baryons","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"Francesca Figueras, Hector Ibarra-Medel, H\\'ector Vel\\'azquez, Octavio Valenzuela, Pedro Col\\'in, Santi Roca-F\\`abrega, Vladimir Avila-Reese, Yair Krongold","submitted_at":"2015-04-23T17:14:48Z","abstract_excerpt":"We introduce a new set of simulations of Milky Way-sized galaxies using the AMR code ART + hydrodynamics in a $\\Lambda$CDM cosmogony. The simulation series is named GARROTXA and follow the formation of a halo/galaxy from z~$=$~60 to z~$=$~0. The final virial mass of the system is $\\sim$7.4$\\times$10$^{11}$M$_{\\odot}$. Our results are as follows: (a) contrary to many previous studies, the circular velocity curve shows no central peak and overall agrees with recent MW observations. (b) Other quantities, such as M$\\_{*}$(6$\\times$10$^{10}$M$_\\odot$) and R$_d$ (2.56 kpc), fall well inside the obse"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1504.06261","kind":"arxiv","version":2},"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":"1504.06261","created_at":"2026-05-18T01:12:08.589997+00:00"},{"alias_kind":"arxiv_version","alias_value":"1504.06261v2","created_at":"2026-05-18T01:12:08.589997+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1504.06261","created_at":"2026-05-18T01:12:08.589997+00:00"},{"alias_kind":"pith_short_12","alias_value":"7DTQIZWDJWLS","created_at":"2026-05-18T12:29:07.941421+00:00"},{"alias_kind":"pith_short_16","alias_value":"7DTQIZWDJWLSL3WL","created_at":"2026-05-18T12:29:07.941421+00:00"},{"alias_kind":"pith_short_8","alias_value":"7DTQIZWD","created_at":"2026-05-18T12:29:07.941421+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/7DTQIZWDJWLSL3WL7QJVNHYSST","json":"https://pith.science/pith/7DTQIZWDJWLSL3WL7QJVNHYSST.json","graph_json":"https://pith.science/api/pith-number/7DTQIZWDJWLSL3WL7QJVNHYSST/graph.json","events_json":"https://pith.science/api/pith-number/7DTQIZWDJWLSL3WL7QJVNHYSST/events.json","paper":"https://pith.science/paper/7DTQIZWD"},"agent_actions":{"view_html":"https://pith.science/pith/7DTQIZWDJWLSL3WL7QJVNHYSST","download_json":"https://pith.science/pith/7DTQIZWDJWLSL3WL7QJVNHYSST.json","view_paper":"https://pith.science/paper/7DTQIZWD","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1504.06261&json=true","fetch_graph":"https://pith.science/api/pith-number/7DTQIZWDJWLSL3WL7QJVNHYSST/graph.json","fetch_events":"https://pith.science/api/pith-number/7DTQIZWDJWLSL3WL7QJVNHYSST/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/7DTQIZWDJWLSL3WL7QJVNHYSST/action/timestamp_anchor","attest_storage":"https://pith.science/pith/7DTQIZWDJWLSL3WL7QJVNHYSST/action/storage_attestation","attest_author":"https://pith.science/pith/7DTQIZWDJWLSL3WL7QJVNHYSST/action/author_attestation","sign_citation":"https://pith.science/pith/7DTQIZWDJWLSL3WL7QJVNHYSST/action/citation_signature","submit_replication":"https://pith.science/pith/7DTQIZWDJWLSL3WL7QJVNHYSST/action/replication_record"}},"created_at":"2026-05-18T01:12:08.589997+00:00","updated_at":"2026-05-18T01:12:08.589997+00:00"}