{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:3HNOVYH6W6AF6BBOVCEVRQKL2J","short_pith_number":"pith:3HNOVYH6","schema_version":"1.0","canonical_sha256":"d9daeae0feb7805f042ea88958c14bd24dee5b604595fee25361f022688b3ca9","source":{"kind":"arxiv","id":"2406.07180","version":1},"attestation_state":"computed","paper":{"title":"Detailed chemical abundances of the globular cluster Terzan 6 in the inner bulge","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.GA","authors_text":"A. Mucciarelli, B. Lanzoni, C. Fanelli, C. Pallanca, D. Massari, E. Dalessandro, F. R. Ferraro, L. Origlia, M. Loriga, R. M. Rich","submitted_at":"2024-06-11T11:44:36Z","abstract_excerpt":"We used near-infrared spectroscopy at medium-high resolution (R=8,000$-$25,000) to perform the first comprehensive chemical study of the intermediate luminosity bulge globular cluster Terzan~6. We derived detailed abundances and abundance patterns of 27 giant stars, likely members of Terzan~6, based on their accurate Hubble Space Telescope proper motions and line-of-sight radial velocities. From the spectral analysis of these stars, we determined an average heliocentric radial velocity of 143.3$\\pm$1.0 km s$^{-1}$ with a velocity dispersion of 5.1$\\pm$0.7 km s$^{-1}$ and an average [Fe/H]=$-0."},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"2406.07180","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2024-06-11T11:44:36Z","cross_cats_sorted":["astro-ph.SR"],"title_canon_sha256":"b484f2336c874c679d6a9c9f5cd11dd83b0bc7865b5c84cbf25683d435ff4953","abstract_canon_sha256":"ac6a3493c66cab220f8529d4b646c41aff9d61e17d71d891fb3f03cf1378b1f7"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T08:30:19.606496Z","signature_b64":"B7dTNIaM0oGo/wy72xSIILAJYyctyZr6D6apoeIpacRoZHw5xXcuuVRSz+HnCiDttusokjFXUoxzm/7DrcvVAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d9daeae0feb7805f042ea88958c14bd24dee5b604595fee25361f022688b3ca9","last_reissued_at":"2026-07-05T08:30:19.605962Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T08:30:19.605962Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Detailed chemical abundances of the globular cluster Terzan 6 in the inner bulge","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.GA","authors_text":"A. Mucciarelli, B. Lanzoni, C. Fanelli, C. Pallanca, D. Massari, E. Dalessandro, F. R. Ferraro, L. Origlia, M. Loriga, R. M. Rich","submitted_at":"2024-06-11T11:44:36Z","abstract_excerpt":"We used near-infrared spectroscopy at medium-high resolution (R=8,000$-$25,000) to perform the first comprehensive chemical study of the intermediate luminosity bulge globular cluster Terzan~6. We derived detailed abundances and abundance patterns of 27 giant stars, likely members of Terzan~6, based on their accurate Hubble Space Telescope proper motions and line-of-sight radial velocities. From the spectral analysis of these stars, we determined an average heliocentric radial velocity of 143.3$\\pm$1.0 km s$^{-1}$ with a velocity dispersion of 5.1$\\pm$0.7 km s$^{-1}$ and an average [Fe/H]=$-0."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2406.07180","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2406.07180/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"2406.07180","created_at":"2026-07-05T08:30:19.606023+00:00"},{"alias_kind":"arxiv_version","alias_value":"2406.07180v1","created_at":"2026-07-05T08:30:19.606023+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2406.07180","created_at":"2026-07-05T08:30:19.606023+00:00"},{"alias_kind":"pith_short_12","alias_value":"3HNOVYH6W6AF","created_at":"2026-07-05T08:30:19.606023+00:00"},{"alias_kind":"pith_short_16","alias_value":"3HNOVYH6W6AF6BBO","created_at":"2026-07-05T08:30:19.606023+00:00"},{"alias_kind":"pith_short_8","alias_value":"3HNOVYH6","created_at":"2026-07-05T08:30:19.606023+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/3HNOVYH6W6AF6BBOVCEVRQKL2J","json":"https://pith.science/pith/3HNOVYH6W6AF6BBOVCEVRQKL2J.json","graph_json":"https://pith.science/api/pith-number/3HNOVYH6W6AF6BBOVCEVRQKL2J/graph.json","events_json":"https://pith.science/api/pith-number/3HNOVYH6W6AF6BBOVCEVRQKL2J/events.json","paper":"https://pith.science/paper/3HNOVYH6"},"agent_actions":{"view_html":"https://pith.science/pith/3HNOVYH6W6AF6BBOVCEVRQKL2J","download_json":"https://pith.science/pith/3HNOVYH6W6AF6BBOVCEVRQKL2J.json","view_paper":"https://pith.science/paper/3HNOVYH6","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2406.07180&json=true","fetch_graph":"https://pith.science/api/pith-number/3HNOVYH6W6AF6BBOVCEVRQKL2J/graph.json","fetch_events":"https://pith.science/api/pith-number/3HNOVYH6W6AF6BBOVCEVRQKL2J/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/3HNOVYH6W6AF6BBOVCEVRQKL2J/action/timestamp_anchor","attest_storage":"https://pith.science/pith/3HNOVYH6W6AF6BBOVCEVRQKL2J/action/storage_attestation","attest_author":"https://pith.science/pith/3HNOVYH6W6AF6BBOVCEVRQKL2J/action/author_attestation","sign_citation":"https://pith.science/pith/3HNOVYH6W6AF6BBOVCEVRQKL2J/action/citation_signature","submit_replication":"https://pith.science/pith/3HNOVYH6W6AF6BBOVCEVRQKL2J/action/replication_record"}},"created_at":"2026-07-05T08:30:19.606023+00:00","updated_at":"2026-07-05T08:30:19.606023+00:00"}