{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:7IKZZIM3FCBUIKGP6BHJXS4OHJ","short_pith_number":"pith:7IKZZIM3","schema_version":"1.0","canonical_sha256":"fa159ca19b28834428cff04e9bcb8e3a6e7f527e32a5acc73fdb372391ff7e45","source":{"kind":"arxiv","id":"1711.07496","version":1},"attestation_state":"computed","paper":{"title":"The globular cluster NGC7492 and the Sagittarius tidal stream: together but unmixed","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.GA","authors_text":"Antonio Sollima, Camila Navarrete, David Mart\\'inez-Delgado, Jes\\'us M. Corral-Santana, Julio A. Carballo-Bello, Marcelo D. Mora, M\\'arcio Catelan, Patrick C\\^ot\\'e, Ricardo R. Mu\\~noz, Sonia Duffau","submitted_at":"2017-11-20T19:00:10Z","abstract_excerpt":"We have derived from VIMOS spectroscopy the radial velocities for a sample of 71 stars selected from CFHT/Megacam photometry around the Galactic globular cluster NGC7492. In the resulting velocity distribution, it is possible to distinguish two relevant non-Galactic kinematic components along the same line of sight: a group of stars at $\\langle{v_{\\rm r}}\\rangle \\sim 125$km s$^{-1}$ which is compatible with the velocity of the old leading arm of the Sagittarius tidal stream, and a larger number of objects at $\\langle{v_{\\rm r}}\\rangle \\sim -110$km s$^{-1}$ that might be identified as members o"},"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":"1711.07496","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-11-20T19:00:10Z","cross_cats_sorted":["astro-ph.SR"],"title_canon_sha256":"c2c4849883230be46430b81abfd81792527e4fded4aeb34715616c215624112e","abstract_canon_sha256":"5a42b10e69439bad46ffd5c70c2d29ab467dbfe14236f54b26f4c893f79bba93"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:26:23.826125Z","signature_b64":"mXOhuBVDbaeB0/3rvdszfDOQg5Njw48kyYDtspbBy9Fvl5sS20/b4nalunj4SwQBnaQ3azN8F3iDpNrVmzkEBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"fa159ca19b28834428cff04e9bcb8e3a6e7f527e32a5acc73fdb372391ff7e45","last_reissued_at":"2026-05-18T00:26:23.825419Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:26:23.825419Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The globular cluster NGC7492 and the Sagittarius tidal stream: together but unmixed","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.GA","authors_text":"Antonio Sollima, Camila Navarrete, David Mart\\'inez-Delgado, Jes\\'us M. Corral-Santana, Julio A. Carballo-Bello, Marcelo D. Mora, M\\'arcio Catelan, Patrick C\\^ot\\'e, Ricardo R. Mu\\~noz, Sonia Duffau","submitted_at":"2017-11-20T19:00:10Z","abstract_excerpt":"We have derived from VIMOS spectroscopy the radial velocities for a sample of 71 stars selected from CFHT/Megacam photometry around the Galactic globular cluster NGC7492. In the resulting velocity distribution, it is possible to distinguish two relevant non-Galactic kinematic components along the same line of sight: a group of stars at $\\langle{v_{\\rm r}}\\rangle \\sim 125$km s$^{-1}$ which is compatible with the velocity of the old leading arm of the Sagittarius tidal stream, and a larger number of objects at $\\langle{v_{\\rm r}}\\rangle \\sim -110$km s$^{-1}$ that might be identified as members o"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1711.07496","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":"1711.07496","created_at":"2026-05-18T00:26:23.825551+00:00"},{"alias_kind":"arxiv_version","alias_value":"1711.07496v1","created_at":"2026-05-18T00:26:23.825551+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1711.07496","created_at":"2026-05-18T00:26:23.825551+00:00"},{"alias_kind":"pith_short_12","alias_value":"7IKZZIM3FCBU","created_at":"2026-05-18T12:31:05.417338+00:00"},{"alias_kind":"pith_short_16","alias_value":"7IKZZIM3FCBUIKGP","created_at":"2026-05-18T12:31:05.417338+00:00"},{"alias_kind":"pith_short_8","alias_value":"7IKZZIM3","created_at":"2026-05-18T12:31:05.417338+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/7IKZZIM3FCBUIKGP6BHJXS4OHJ","json":"https://pith.science/pith/7IKZZIM3FCBUIKGP6BHJXS4OHJ.json","graph_json":"https://pith.science/api/pith-number/7IKZZIM3FCBUIKGP6BHJXS4OHJ/graph.json","events_json":"https://pith.science/api/pith-number/7IKZZIM3FCBUIKGP6BHJXS4OHJ/events.json","paper":"https://pith.science/paper/7IKZZIM3"},"agent_actions":{"view_html":"https://pith.science/pith/7IKZZIM3FCBUIKGP6BHJXS4OHJ","download_json":"https://pith.science/pith/7IKZZIM3FCBUIKGP6BHJXS4OHJ.json","view_paper":"https://pith.science/paper/7IKZZIM3","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1711.07496&json=true","fetch_graph":"https://pith.science/api/pith-number/7IKZZIM3FCBUIKGP6BHJXS4OHJ/graph.json","fetch_events":"https://pith.science/api/pith-number/7IKZZIM3FCBUIKGP6BHJXS4OHJ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/7IKZZIM3FCBUIKGP6BHJXS4OHJ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/7IKZZIM3FCBUIKGP6BHJXS4OHJ/action/storage_attestation","attest_author":"https://pith.science/pith/7IKZZIM3FCBUIKGP6BHJXS4OHJ/action/author_attestation","sign_citation":"https://pith.science/pith/7IKZZIM3FCBUIKGP6BHJXS4OHJ/action/citation_signature","submit_replication":"https://pith.science/pith/7IKZZIM3FCBUIKGP6BHJXS4OHJ/action/replication_record"}},"created_at":"2026-05-18T00:26:23.825551+00:00","updated_at":"2026-05-18T00:26:23.825551+00:00"}