{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:AXG3VRNKJN7LRVDSR6JHABDB2F","short_pith_number":"pith:AXG3VRNK","schema_version":"1.0","canonical_sha256":"05cdbac5aa4b7eb8d4728f92700461d163929bdee7a6fb442fa694c6f8e375ab","source":{"kind":"arxiv","id":"1904.02733","version":1},"attestation_state":"computed","paper":{"title":"MASCARA-4 b/bRing-1b - A retrograde hot Jupiter around the bright A3V star HD 85628","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"A. Jord\\'an, A. Wyttenbach, A. Zapata, B.Lomberg, D. Osip, E. E. Mamajek, G.A. Bakos, G.J.J. Talens, G.P.P.L. Otten, H. James, I. Snellen, J. Bailey, L. Paredes, L. Vanzi, M. Ireland, M. Kenworthy, P. Dorval, R. Brahm, R. Hinojosa, R. Kuhn, R. Stuik, S. Crawford, S. N. Mellon, T. Henry, V. Suc, W. Bhatti, W.C. Jao, Z. Csubry","submitted_at":"2019-04-04T18:13:54Z","abstract_excerpt":"In this paper, we aim to characterize a transiting planetary candidate in the southern skies found in the combined MASCARA and bRing data sets of HD 85628, an A3V star of V = 8.2 mag at a distance 172 pc, to confirm its planetary nature. The candidate was originally detected in data obtained jointly with the MASCARA and bRing instruments using a BLS search for transit events. Further photometry was taken by the 0.7 m CHAT, and radial velocity measurements with FIDEOS on the ESO 1.0 m Telescope. High resolution spectra during a transit were taken with CHIRON on the SMARTS 1.5 m telescope to tar"},"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":"1904.02733","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2019-04-04T18:13:54Z","cross_cats_sorted":[],"title_canon_sha256":"42bd1117dd7a9a417c6ebb71f7f8e5bc45b6fceccc904e6614957c96d1922a7b","abstract_canon_sha256":"395597f033fe6a418cde4c61398f16ae155b89223779dbc47bf9799a40dddc58"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T00:46:45.341830Z","signature_b64":"H6nTjJgBJr4MkHeuaRtbcRqf4GtfGIXfdLhAmcuz1vIubgXh0H+RDz5ttTCfFf7O2OSTAFiPXLCXWUag3RF9Ag==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"05cdbac5aa4b7eb8d4728f92700461d163929bdee7a6fb442fa694c6f8e375ab","last_reissued_at":"2026-07-05T00:46:45.341434Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T00:46:45.341434Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"MASCARA-4 b/bRing-1b - A retrograde hot Jupiter around the bright A3V star HD 85628","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"A. Jord\\'an, A. Wyttenbach, A. Zapata, B.Lomberg, D. Osip, E. E. Mamajek, G.A. Bakos, G.J.J. Talens, G.P.P.L. Otten, H. James, I. Snellen, J. Bailey, L. Paredes, L. Vanzi, M. Ireland, M. Kenworthy, P. Dorval, R. Brahm, R. Hinojosa, R. Kuhn, R. Stuik, S. Crawford, S. N. Mellon, T. Henry, V. Suc, W. Bhatti, W.C. Jao, Z. Csubry","submitted_at":"2019-04-04T18:13:54Z","abstract_excerpt":"In this paper, we aim to characterize a transiting planetary candidate in the southern skies found in the combined MASCARA and bRing data sets of HD 85628, an A3V star of V = 8.2 mag at a distance 172 pc, to confirm its planetary nature. The candidate was originally detected in data obtained jointly with the MASCARA and bRing instruments using a BLS search for transit events. Further photometry was taken by the 0.7 m CHAT, and radial velocity measurements with FIDEOS on the ESO 1.0 m Telescope. High resolution spectra during a transit were taken with CHIRON on the SMARTS 1.5 m telescope to tar"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1904.02733","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/1904.02733/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":"1904.02733","created_at":"2026-07-05T00:46:45.341485+00:00"},{"alias_kind":"arxiv_version","alias_value":"1904.02733v1","created_at":"2026-07-05T00:46:45.341485+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1904.02733","created_at":"2026-07-05T00:46:45.341485+00:00"},{"alias_kind":"pith_short_12","alias_value":"AXG3VRNKJN7L","created_at":"2026-07-05T00:46:45.341485+00:00"},{"alias_kind":"pith_short_16","alias_value":"AXG3VRNKJN7LRVDS","created_at":"2026-07-05T00:46:45.341485+00:00"},{"alias_kind":"pith_short_8","alias_value":"AXG3VRNK","created_at":"2026-07-05T00:46:45.341485+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/AXG3VRNKJN7LRVDSR6JHABDB2F","json":"https://pith.science/pith/AXG3VRNKJN7LRVDSR6JHABDB2F.json","graph_json":"https://pith.science/api/pith-number/AXG3VRNKJN7LRVDSR6JHABDB2F/graph.json","events_json":"https://pith.science/api/pith-number/AXG3VRNKJN7LRVDSR6JHABDB2F/events.json","paper":"https://pith.science/paper/AXG3VRNK"},"agent_actions":{"view_html":"https://pith.science/pith/AXG3VRNKJN7LRVDSR6JHABDB2F","download_json":"https://pith.science/pith/AXG3VRNKJN7LRVDSR6JHABDB2F.json","view_paper":"https://pith.science/paper/AXG3VRNK","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1904.02733&json=true","fetch_graph":"https://pith.science/api/pith-number/AXG3VRNKJN7LRVDSR6JHABDB2F/graph.json","fetch_events":"https://pith.science/api/pith-number/AXG3VRNKJN7LRVDSR6JHABDB2F/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/AXG3VRNKJN7LRVDSR6JHABDB2F/action/timestamp_anchor","attest_storage":"https://pith.science/pith/AXG3VRNKJN7LRVDSR6JHABDB2F/action/storage_attestation","attest_author":"https://pith.science/pith/AXG3VRNKJN7LRVDSR6JHABDB2F/action/author_attestation","sign_citation":"https://pith.science/pith/AXG3VRNKJN7LRVDSR6JHABDB2F/action/citation_signature","submit_replication":"https://pith.science/pith/AXG3VRNKJN7LRVDSR6JHABDB2F/action/replication_record"}},"created_at":"2026-07-05T00:46:45.341485+00:00","updated_at":"2026-07-05T00:46:45.341485+00:00"}