{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:VHQLUON3OGMXIMWTPUR35RXANF","short_pith_number":"pith:VHQLUON3","schema_version":"1.0","canonical_sha256":"a9e0ba39bb71997432d37d23bec6e06958ab09dc886dfbbe1fced5eb754752fa","source":{"kind":"arxiv","id":"1606.01471","version":2},"attestation_state":"computed","paper":{"title":"MUSE integral-field spectroscopy towards the Frontier Fields cluster Abell S1063: II. Properties of low luminosity Lyman alpha emitters at z>3","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"A. Mercurio, A. M. Koekemoer, C. Grillo, D. Coe, D. McLeod, E. Vanzella, G. B. Caminha, I. Balestra, K. I. Caputi, M. Dijkstra, M. Gronke, M. Nonino, P. Rosati, W. Karman","submitted_at":"2016-06-05T07:26:49Z","abstract_excerpt":"In spite of their conjectured importance for the Epoch of Reionization, the properties of low-mass galaxies are currently still under large debate. In this article, we study the stellar and gaseous properties of faint, low-mass galaxies at z>3. We observed the Frontier Fields cluster Abell S1063 with MUSE over a 2 arcmin^2 field, and combined integral-field spectroscopy with gravitational lensing to perform a blind search for intrinsically faint Lya emitters (LAEs). We determined in total the redshift of 172 galaxies of which 14 are lensed LAEs at z=3-6.1. We increased the number of spectrosco"},"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":"1606.01471","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2016-06-05T07:26:49Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"2c56c0640d194c2ebb81722381968452fe3ef6d5cc0d9b44718846834e1c088a","abstract_canon_sha256":"1a1c99a79f957f89da718502b207131483560db66e5a20dc52cf6891ce8a8a77"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:50:22.240721Z","signature_b64":"WtdkKLH+13LnZWkgZoqST+CJoBmJDo2EOs8Smc2NNb8CnQIucar4XXB3Xy+Zy2mFgv75XyCz8ablTUCqFprtDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a9e0ba39bb71997432d37d23bec6e06958ab09dc886dfbbe1fced5eb754752fa","last_reissued_at":"2026-05-18T00:50:22.239987Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:50:22.239987Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"MUSE integral-field spectroscopy towards the Frontier Fields cluster Abell S1063: II. Properties of low luminosity Lyman alpha emitters at z>3","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"A. Mercurio, A. M. Koekemoer, C. Grillo, D. Coe, D. McLeod, E. Vanzella, G. B. Caminha, I. Balestra, K. I. Caputi, M. Dijkstra, M. Gronke, M. Nonino, P. Rosati, W. Karman","submitted_at":"2016-06-05T07:26:49Z","abstract_excerpt":"In spite of their conjectured importance for the Epoch of Reionization, the properties of low-mass galaxies are currently still under large debate. In this article, we study the stellar and gaseous properties of faint, low-mass galaxies at z>3. We observed the Frontier Fields cluster Abell S1063 with MUSE over a 2 arcmin^2 field, and combined integral-field spectroscopy with gravitational lensing to perform a blind search for intrinsically faint Lya emitters (LAEs). We determined in total the redshift of 172 galaxies of which 14 are lensed LAEs at z=3-6.1. We increased the number of spectrosco"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1606.01471","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":"1606.01471","created_at":"2026-05-18T00:50:22.240096+00:00"},{"alias_kind":"arxiv_version","alias_value":"1606.01471v2","created_at":"2026-05-18T00:50:22.240096+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1606.01471","created_at":"2026-05-18T00:50:22.240096+00:00"},{"alias_kind":"pith_short_12","alias_value":"VHQLUON3OGMX","created_at":"2026-05-18T12:30:48.956258+00:00"},{"alias_kind":"pith_short_16","alias_value":"VHQLUON3OGMXIMWT","created_at":"2026-05-18T12:30:48.956258+00:00"},{"alias_kind":"pith_short_8","alias_value":"VHQLUON3","created_at":"2026-05-18T12:30:48.956258+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/VHQLUON3OGMXIMWTPUR35RXANF","json":"https://pith.science/pith/VHQLUON3OGMXIMWTPUR35RXANF.json","graph_json":"https://pith.science/api/pith-number/VHQLUON3OGMXIMWTPUR35RXANF/graph.json","events_json":"https://pith.science/api/pith-number/VHQLUON3OGMXIMWTPUR35RXANF/events.json","paper":"https://pith.science/paper/VHQLUON3"},"agent_actions":{"view_html":"https://pith.science/pith/VHQLUON3OGMXIMWTPUR35RXANF","download_json":"https://pith.science/pith/VHQLUON3OGMXIMWTPUR35RXANF.json","view_paper":"https://pith.science/paper/VHQLUON3","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1606.01471&json=true","fetch_graph":"https://pith.science/api/pith-number/VHQLUON3OGMXIMWTPUR35RXANF/graph.json","fetch_events":"https://pith.science/api/pith-number/VHQLUON3OGMXIMWTPUR35RXANF/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/VHQLUON3OGMXIMWTPUR35RXANF/action/timestamp_anchor","attest_storage":"https://pith.science/pith/VHQLUON3OGMXIMWTPUR35RXANF/action/storage_attestation","attest_author":"https://pith.science/pith/VHQLUON3OGMXIMWTPUR35RXANF/action/author_attestation","sign_citation":"https://pith.science/pith/VHQLUON3OGMXIMWTPUR35RXANF/action/citation_signature","submit_replication":"https://pith.science/pith/VHQLUON3OGMXIMWTPUR35RXANF/action/replication_record"}},"created_at":"2026-05-18T00:50:22.240096+00:00","updated_at":"2026-05-18T00:50:22.240096+00:00"}