{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:JLRL44N4OKUOYNY4O6UUQDBMJU","short_pith_number":"pith:JLRL44N4","schema_version":"1.0","canonical_sha256":"4ae2be71bc72a8ec371c77a9480c2c4d0a8955a62b3fe3463dcbdeb5a0f0ab6f","source":{"kind":"arxiv","id":"1410.5825","version":1},"attestation_state":"computed","paper":{"title":"Radial velocities from VLT-KMOS spectra of giant stars in the globular cluster NGC 6388","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.SR","authors_text":"Alessio Mucciarelli (UNIBo), Barbara Lanzoni (UNIBO), Elena Valenti (ESO), Emanuele Dalessandro (UNIBO), Emilio Lapenna (UNIBo), Francesco Rosario Ferraro (UNIBO), Livia Origlia (INAF-OABo), Michele Cirasuolo (ATC-Edinburgh)","submitted_at":"2014-10-21T20:00:08Z","abstract_excerpt":"We present new radial velocity measurements for 82 stars, members of the Galactic globular cluster NGC 6388, obtained from ESO-VLT KMOS spectra acquired during the instrument Science Verification. The accuracy of the wavelength calibration is discussed and a number of tests of the KMOS response are presented. The cluster systemic velocity obtained (81.3 +/- 1.5 km/sec) is in very good agreement with previous determinations. While a hint of ordered rotation is found between 9'' and 20'' from the cluster centre, where the distribution of radial velocities is clearly bimodal, more data are needed"},"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":"1410.5825","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2014-10-21T20:00:08Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"844bd7ef54a24a4c5bd7eefb4fef728cb0942f408fb18fe073ae5d87c1bb382e","abstract_canon_sha256":"2ee3d798233d60e9c8f7d29b04d983ef2b1ed29107229ad6cd4ad2b3439ca743"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:41:41.294051Z","signature_b64":"f1eXhJDZw2soY6NMgcYxJUUbYtYok+zhUuJQNgHq6l1d5zb26d2O1nmNnxZd0WfH6f3gmA3CS91hD+BEIpzECw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4ae2be71bc72a8ec371c77a9480c2c4d0a8955a62b3fe3463dcbdeb5a0f0ab6f","last_reissued_at":"2026-05-18T01:41:41.293445Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:41:41.293445Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Radial velocities from VLT-KMOS spectra of giant stars in the globular cluster NGC 6388","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.SR","authors_text":"Alessio Mucciarelli (UNIBo), Barbara Lanzoni (UNIBO), Elena Valenti (ESO), Emanuele Dalessandro (UNIBO), Emilio Lapenna (UNIBo), Francesco Rosario Ferraro (UNIBO), Livia Origlia (INAF-OABo), Michele Cirasuolo (ATC-Edinburgh)","submitted_at":"2014-10-21T20:00:08Z","abstract_excerpt":"We present new radial velocity measurements for 82 stars, members of the Galactic globular cluster NGC 6388, obtained from ESO-VLT KMOS spectra acquired during the instrument Science Verification. The accuracy of the wavelength calibration is discussed and a number of tests of the KMOS response are presented. The cluster systemic velocity obtained (81.3 +/- 1.5 km/sec) is in very good agreement with previous determinations. While a hint of ordered rotation is found between 9'' and 20'' from the cluster centre, where the distribution of radial velocities is clearly bimodal, more data are needed"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1410.5825","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":"1410.5825","created_at":"2026-05-18T01:41:41.293541+00:00"},{"alias_kind":"arxiv_version","alias_value":"1410.5825v1","created_at":"2026-05-18T01:41:41.293541+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1410.5825","created_at":"2026-05-18T01:41:41.293541+00:00"},{"alias_kind":"pith_short_12","alias_value":"JLRL44N4OKUO","created_at":"2026-05-18T12:28:33.132498+00:00"},{"alias_kind":"pith_short_16","alias_value":"JLRL44N4OKUOYNY4","created_at":"2026-05-18T12:28:33.132498+00:00"},{"alias_kind":"pith_short_8","alias_value":"JLRL44N4","created_at":"2026-05-18T12:28:33.132498+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/JLRL44N4OKUOYNY4O6UUQDBMJU","json":"https://pith.science/pith/JLRL44N4OKUOYNY4O6UUQDBMJU.json","graph_json":"https://pith.science/api/pith-number/JLRL44N4OKUOYNY4O6UUQDBMJU/graph.json","events_json":"https://pith.science/api/pith-number/JLRL44N4OKUOYNY4O6UUQDBMJU/events.json","paper":"https://pith.science/paper/JLRL44N4"},"agent_actions":{"view_html":"https://pith.science/pith/JLRL44N4OKUOYNY4O6UUQDBMJU","download_json":"https://pith.science/pith/JLRL44N4OKUOYNY4O6UUQDBMJU.json","view_paper":"https://pith.science/paper/JLRL44N4","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1410.5825&json=true","fetch_graph":"https://pith.science/api/pith-number/JLRL44N4OKUOYNY4O6UUQDBMJU/graph.json","fetch_events":"https://pith.science/api/pith-number/JLRL44N4OKUOYNY4O6UUQDBMJU/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/JLRL44N4OKUOYNY4O6UUQDBMJU/action/timestamp_anchor","attest_storage":"https://pith.science/pith/JLRL44N4OKUOYNY4O6UUQDBMJU/action/storage_attestation","attest_author":"https://pith.science/pith/JLRL44N4OKUOYNY4O6UUQDBMJU/action/author_attestation","sign_citation":"https://pith.science/pith/JLRL44N4OKUOYNY4O6UUQDBMJU/action/citation_signature","submit_replication":"https://pith.science/pith/JLRL44N4OKUOYNY4O6UUQDBMJU/action/replication_record"}},"created_at":"2026-05-18T01:41:41.293541+00:00","updated_at":"2026-05-18T01:41:41.293541+00:00"}