{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:D7RNIQ72RWJIJORKGGJ3Y23BSC","short_pith_number":"pith:D7RNIQ72","schema_version":"1.0","canonical_sha256":"1fe2d443fa8d9284ba2a3193bc6b619099e3b1e02e9003d786d5e5abb0c9dd4e","source":{"kind":"arxiv","id":"1002.2068","version":1},"attestation_state":"computed","paper":{"title":"Physical and morphological properties of z~3 LBGs: dependence on Lyalpha line emission","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.CO","authors_text":"A. Fontana, A. Grazian, C. Scarlata, E. Giallongo, E. Vanzella, L.Pentericci, M. Castellano","submitted_at":"2010-02-10T10:55:42Z","abstract_excerpt":"We investigate the physical and morphological properties of LBGs at z ~2.5 to ~3.5, to determine if and how they depend on the nature and strength of the Lyalpha emission. We selected U-dropout galaxies from the z-detected GOODS MUSIC catalog, by adapting the classical Lyman Break criteria on the GOODS filter set. We kept only those galaxies with spectroscopic confirmation, mainly from VIMOS and FORS public observations. Using the full multi-wavelength 14-bands photometry, we determined the physical properties of the galaxies, through a standard spectral energy distribution fitting with the up"},"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":"1002.2068","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2010-02-10T10:55:42Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"dba6df7e32b6230595fe412a20dd6af5d0a548392a4397f4e5f5b1d9c0e45343","abstract_canon_sha256":"6f86cb46df9718e24c5241d5fe6533cc06c334511278b2af379ba0768051e666"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:09:10.319439Z","signature_b64":"VmtkGe2cv2dOjrFZp9QuxplnJPykLxNsjCOVHDm3AaUGZsZABhYEf5UvNzRYtq8vo39OcM9S6dTmxOHIGVl9BA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1fe2d443fa8d9284ba2a3193bc6b619099e3b1e02e9003d786d5e5abb0c9dd4e","last_reissued_at":"2026-05-18T02:09:10.319010Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:09:10.319010Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Physical and morphological properties of z~3 LBGs: dependence on Lyalpha line emission","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.CO","authors_text":"A. Fontana, A. Grazian, C. Scarlata, E. Giallongo, E. Vanzella, L.Pentericci, M. Castellano","submitted_at":"2010-02-10T10:55:42Z","abstract_excerpt":"We investigate the physical and morphological properties of LBGs at z ~2.5 to ~3.5, to determine if and how they depend on the nature and strength of the Lyalpha emission. We selected U-dropout galaxies from the z-detected GOODS MUSIC catalog, by adapting the classical Lyman Break criteria on the GOODS filter set. We kept only those galaxies with spectroscopic confirmation, mainly from VIMOS and FORS public observations. Using the full multi-wavelength 14-bands photometry, we determined the physical properties of the galaxies, through a standard spectral energy distribution fitting with the up"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1002.2068","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":"1002.2068","created_at":"2026-05-18T02:09:10.319067+00:00"},{"alias_kind":"arxiv_version","alias_value":"1002.2068v1","created_at":"2026-05-18T02:09:10.319067+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1002.2068","created_at":"2026-05-18T02:09:10.319067+00:00"},{"alias_kind":"pith_short_12","alias_value":"D7RNIQ72RWJI","created_at":"2026-05-18T12:26:06.534383+00:00"},{"alias_kind":"pith_short_16","alias_value":"D7RNIQ72RWJIJORK","created_at":"2026-05-18T12:26:06.534383+00:00"},{"alias_kind":"pith_short_8","alias_value":"D7RNIQ72","created_at":"2026-05-18T12:26:06.534383+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/D7RNIQ72RWJIJORKGGJ3Y23BSC","json":"https://pith.science/pith/D7RNIQ72RWJIJORKGGJ3Y23BSC.json","graph_json":"https://pith.science/api/pith-number/D7RNIQ72RWJIJORKGGJ3Y23BSC/graph.json","events_json":"https://pith.science/api/pith-number/D7RNIQ72RWJIJORKGGJ3Y23BSC/events.json","paper":"https://pith.science/paper/D7RNIQ72"},"agent_actions":{"view_html":"https://pith.science/pith/D7RNIQ72RWJIJORKGGJ3Y23BSC","download_json":"https://pith.science/pith/D7RNIQ72RWJIJORKGGJ3Y23BSC.json","view_paper":"https://pith.science/paper/D7RNIQ72","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1002.2068&json=true","fetch_graph":"https://pith.science/api/pith-number/D7RNIQ72RWJIJORKGGJ3Y23BSC/graph.json","fetch_events":"https://pith.science/api/pith-number/D7RNIQ72RWJIJORKGGJ3Y23BSC/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/D7RNIQ72RWJIJORKGGJ3Y23BSC/action/timestamp_anchor","attest_storage":"https://pith.science/pith/D7RNIQ72RWJIJORKGGJ3Y23BSC/action/storage_attestation","attest_author":"https://pith.science/pith/D7RNIQ72RWJIJORKGGJ3Y23BSC/action/author_attestation","sign_citation":"https://pith.science/pith/D7RNIQ72RWJIJORKGGJ3Y23BSC/action/citation_signature","submit_replication":"https://pith.science/pith/D7RNIQ72RWJIJORKGGJ3Y23BSC/action/replication_record"}},"created_at":"2026-05-18T02:09:10.319067+00:00","updated_at":"2026-05-18T02:09:10.319067+00:00"}