{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:7ISRWPHURFXJBS3HEL6BO53KZI","short_pith_number":"pith:7ISRWPHU","schema_version":"1.0","canonical_sha256":"fa251b3cf4896e90cb6722fc17776aca199cb9617f5b238c44672081b16f303d","source":{"kind":"arxiv","id":"1712.05583","version":1},"attestation_state":"computed","paper":{"title":"Data release of UV to submm broadband fluxes for simulated galaxies from the EAGLE project","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Ana Tr\\v{c}ka, James Trayford, Joop Schaye, Maarten Baes, Matthieu Schaller, Peter Camps, Robert A. Crain, Stuart McAlpine, Tom Theuns","submitted_at":"2017-12-15T08:52:32Z","abstract_excerpt":"We present dust-attenuated and dust emission fluxes for sufficiently resolved galaxies in the EAGLE suite of cosmological hydrodynamical simulations, calculated with the SKIRT radiative transfer code. The post-processing procedure includes specific components for star formation regions, stellar sources, and diffuse dust, and takes into account stochastic heating of dust grains to obtain realistic broad-band fluxes in the wavelength range from ultraviolet to sub-millimeter. The mock survey includes nearly half a million simulated galaxies with stellar masses above 10^8.5 solar masses across six"},"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":"1712.05583","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-12-15T08:52:32Z","cross_cats_sorted":[],"title_canon_sha256":"56d5321fd65defe6b033a2acdea2cc1f45a877f0e0ff4d2ea7a92a421b8f0938","abstract_canon_sha256":"2526ba1366310e4f44499428c4f11cdac53a45f5aed59ff44f8980166a29f0e2"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:24:14.685214Z","signature_b64":"ENd8/eS/mB55ZHvLZAgp0rxaQlb4ltLuCk++E9bMRz4IxjS2MkE3kjLhM7NczNs4zAOokJgUSMHM7BCpjsAuCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"fa251b3cf4896e90cb6722fc17776aca199cb9617f5b238c44672081b16f303d","last_reissued_at":"2026-05-18T00:24:14.684673Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:24:14.684673Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Data release of UV to submm broadband fluxes for simulated galaxies from the EAGLE project","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Ana Tr\\v{c}ka, James Trayford, Joop Schaye, Maarten Baes, Matthieu Schaller, Peter Camps, Robert A. Crain, Stuart McAlpine, Tom Theuns","submitted_at":"2017-12-15T08:52:32Z","abstract_excerpt":"We present dust-attenuated and dust emission fluxes for sufficiently resolved galaxies in the EAGLE suite of cosmological hydrodynamical simulations, calculated with the SKIRT radiative transfer code. The post-processing procedure includes specific components for star formation regions, stellar sources, and diffuse dust, and takes into account stochastic heating of dust grains to obtain realistic broad-band fluxes in the wavelength range from ultraviolet to sub-millimeter. The mock survey includes nearly half a million simulated galaxies with stellar masses above 10^8.5 solar masses across six"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1712.05583","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":"1712.05583","created_at":"2026-05-18T00:24:14.684747+00:00"},{"alias_kind":"arxiv_version","alias_value":"1712.05583v1","created_at":"2026-05-18T00:24:14.684747+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1712.05583","created_at":"2026-05-18T00:24:14.684747+00:00"},{"alias_kind":"pith_short_12","alias_value":"7ISRWPHURFXJ","created_at":"2026-05-18T12:31:05.417338+00:00"},{"alias_kind":"pith_short_16","alias_value":"7ISRWPHURFXJBS3H","created_at":"2026-05-18T12:31:05.417338+00:00"},{"alias_kind":"pith_short_8","alias_value":"7ISRWPHU","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/7ISRWPHURFXJBS3HEL6BO53KZI","json":"https://pith.science/pith/7ISRWPHURFXJBS3HEL6BO53KZI.json","graph_json":"https://pith.science/api/pith-number/7ISRWPHURFXJBS3HEL6BO53KZI/graph.json","events_json":"https://pith.science/api/pith-number/7ISRWPHURFXJBS3HEL6BO53KZI/events.json","paper":"https://pith.science/paper/7ISRWPHU"},"agent_actions":{"view_html":"https://pith.science/pith/7ISRWPHURFXJBS3HEL6BO53KZI","download_json":"https://pith.science/pith/7ISRWPHURFXJBS3HEL6BO53KZI.json","view_paper":"https://pith.science/paper/7ISRWPHU","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1712.05583&json=true","fetch_graph":"https://pith.science/api/pith-number/7ISRWPHURFXJBS3HEL6BO53KZI/graph.json","fetch_events":"https://pith.science/api/pith-number/7ISRWPHURFXJBS3HEL6BO53KZI/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/7ISRWPHURFXJBS3HEL6BO53KZI/action/timestamp_anchor","attest_storage":"https://pith.science/pith/7ISRWPHURFXJBS3HEL6BO53KZI/action/storage_attestation","attest_author":"https://pith.science/pith/7ISRWPHURFXJBS3HEL6BO53KZI/action/author_attestation","sign_citation":"https://pith.science/pith/7ISRWPHURFXJBS3HEL6BO53KZI/action/citation_signature","submit_replication":"https://pith.science/pith/7ISRWPHURFXJBS3HEL6BO53KZI/action/replication_record"}},"created_at":"2026-05-18T00:24:14.684747+00:00","updated_at":"2026-05-18T00:24:14.684747+00:00"}