{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2014:JVYEUWD73KASHU2EVDYE2R3DNE","short_pith_number":"pith:JVYEUWD7","canonical_record":{"source":{"id":"1402.1495","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-02-06T21:00:17Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"347f3026ddc6007bcec61872da6a9570932ebfc5f443979ad48c2ec25b66e281","abstract_canon_sha256":"9e445b93fde3b714e5811eabd936531bea5a4ef39231721cdfca937a8f36f068"},"schema_version":"1.0"},"canonical_sha256":"4d704a587fda8123d344a8f04d4763691f3414eb2761f7e44c748c8100f0ba5b","source":{"kind":"arxiv","id":"1402.1495","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1402.1495","created_at":"2026-05-18T01:44:46Z"},{"alias_kind":"arxiv_version","alias_value":"1402.1495v1","created_at":"2026-05-18T01:44:46Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1402.1495","created_at":"2026-05-18T01:44:46Z"},{"alias_kind":"pith_short_12","alias_value":"JVYEUWD73KAS","created_at":"2026-05-18T12:28:35Z"},{"alias_kind":"pith_short_16","alias_value":"JVYEUWD73KASHU2E","created_at":"2026-05-18T12:28:35Z"},{"alias_kind":"pith_short_8","alias_value":"JVYEUWD7","created_at":"2026-05-18T12:28:35Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2014:JVYEUWD73KASHU2EVDYE2R3DNE","target":"record","payload":{"canonical_record":{"source":{"id":"1402.1495","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-02-06T21:00:17Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"347f3026ddc6007bcec61872da6a9570932ebfc5f443979ad48c2ec25b66e281","abstract_canon_sha256":"9e445b93fde3b714e5811eabd936531bea5a4ef39231721cdfca937a8f36f068"},"schema_version":"1.0"},"canonical_sha256":"4d704a587fda8123d344a8f04d4763691f3414eb2761f7e44c748c8100f0ba5b","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:44:46.758539Z","signature_b64":"7dVUsylThEipzPVs4iRTOvccYP3oMr4qIPHN4COEXJh4zC8cy6BN++iLA7xBqYUGzYoII3+Lvk7fFgX4olfAAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4d704a587fda8123d344a8f04d4763691f3414eb2761f7e44c748c8100f0ba5b","last_reissued_at":"2026-05-18T01:44:46.757975Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:44:46.757975Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1402.1495","source_version":1,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T01:44:46Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"TrP7lDfSLDqWVHIYF/rSjkTXDf0OqMWHjjcGOsIVIqhr6kasLLQ4DGKQc4urowrgHqbedK8XctMbIlOY+xqIDQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-26T11:03:26.235307Z"},"content_sha256":"4a4b3d57242d369223aba5f5abc2862c5012d6d4675da00d7c9c3ea613ba712e","schema_version":"1.0","event_id":"sha256:4a4b3d57242d369223aba5f5abc2862c5012d6d4675da00d7c9c3ea613ba712e"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2014:JVYEUWD73KASHU2EVDYE2R3DNE","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"A Two-Parameter Model for the Infrared/Submillimeter/Radio Spectral Energy Distributions of Galaxies and AGN","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"Daniel A. Dale, George Helou, Georgios E. Magdis, Lee Armus, Tanio D\\'iaz-Santos, Yong Shi","submitted_at":"2014-02-06T21:00:17Z","abstract_excerpt":"A two-parameter semi-empirical model is presented for the spectral energy distributions of galaxies with contributions to their infrared-submillimeter-radio emission from both star formation and accretion disk-powered activity. This model builds upon a previous one-parameter family of models for star-forming galaxies, and includes an update to the mid-infrared emission using an average template obtained from Spitzer Space Telescope observations of normal galaxies. Star-forming/AGN diagnostics based on PAH equivalent widths and broadband infrared colors are presented, and example mid-infrared A"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1402.1495","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"},"verdict_id":null},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T01:44:46Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"PskVXXF/xxIjgYjKn6OB6R490vMh5hqfiC/WMAMA67eX7TUXtwWGjV/AF+/3kobPpHXUpRqO1qfIm1f0Q6ITBA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-26T11:03:26.235802Z"},"content_sha256":"030b4b584b17aa8dbc7ae22c116fe1a61d9a2e0814bae4533b370ff7349819cb","schema_version":"1.0","event_id":"sha256:030b4b584b17aa8dbc7ae22c116fe1a61d9a2e0814bae4533b370ff7349819cb"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/JVYEUWD73KASHU2EVDYE2R3DNE/bundle.json","state_url":"https://pith.science/pith/JVYEUWD73KASHU2EVDYE2R3DNE/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/JVYEUWD73KASHU2EVDYE2R3DNE/bundle.json","status":"primary"}],"public_keys":[{"key_id":"pith-v1-2026-05","algorithm":"ed25519","format":"raw","public_key_b64":"stVStoiQhXFxp4s2pdzPNoqVNBMojDU/fJ2db5S3CbM=","public_key_hex":"b2d552b68890857171a78b36a5dccf368a953413288c353f7c9d9d6f94b709b3","fingerprint_sha256_b32_first128bits":"RVFV5Z2OI2J3ZUO7ERDEBCYNKS","fingerprint_sha256_hex":"8d4b5ee74e4693bcd1df2446408b0d54","rotates_at":null,"url":"https://pith.science/pith-signing-key.json","notes":"Pith uses this Ed25519 key to sign canonical record SHA-256 digests. Verify with: ed25519_verify(public_key, message=canonical_sha256_bytes, signature=base64decode(signature_b64))."}],"merge_version":"pith-open-graph-merge-v1","built_at":"2026-05-26T11:03:26Z","links":{"resolver":"https://pith.science/pith/JVYEUWD73KASHU2EVDYE2R3DNE","bundle":"https://pith.science/pith/JVYEUWD73KASHU2EVDYE2R3DNE/bundle.json","state":"https://pith.science/pith/JVYEUWD73KASHU2EVDYE2R3DNE/state.json","well_known_bundle":"https://pith.science/.well-known/pith/JVYEUWD73KASHU2EVDYE2R3DNE/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2014:JVYEUWD73KASHU2EVDYE2R3DNE","merge_version":"pith-open-graph-merge-v1","event_count":2,"valid_event_count":2,"invalid_event_count":0,"equivocation_count":0,"current":{"canonical_record":{"metadata":{"abstract_canon_sha256":"9e445b93fde3b714e5811eabd936531bea5a4ef39231721cdfca937a8f36f068","cross_cats_sorted":["astro-ph.CO"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-02-06T21:00:17Z","title_canon_sha256":"347f3026ddc6007bcec61872da6a9570932ebfc5f443979ad48c2ec25b66e281"},"schema_version":"1.0","source":{"id":"1402.1495","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1402.1495","created_at":"2026-05-18T01:44:46Z"},{"alias_kind":"arxiv_version","alias_value":"1402.1495v1","created_at":"2026-05-18T01:44:46Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1402.1495","created_at":"2026-05-18T01:44:46Z"},{"alias_kind":"pith_short_12","alias_value":"JVYEUWD73KAS","created_at":"2026-05-18T12:28:35Z"},{"alias_kind":"pith_short_16","alias_value":"JVYEUWD73KASHU2E","created_at":"2026-05-18T12:28:35Z"},{"alias_kind":"pith_short_8","alias_value":"JVYEUWD7","created_at":"2026-05-18T12:28:35Z"}],"graph_snapshots":[{"event_id":"sha256:030b4b584b17aa8dbc7ae22c116fe1a61d9a2e0814bae4533b370ff7349819cb","target":"graph","created_at":"2026-05-18T01:44:46Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"graph_snapshot":{"author_claims":{"count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","strong_count":0},"builder_version":"pith-number-builder-2026-05-17-v1","claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"paper":{"abstract_excerpt":"A two-parameter semi-empirical model is presented for the spectral energy distributions of galaxies with contributions to their infrared-submillimeter-radio emission from both star formation and accretion disk-powered activity. This model builds upon a previous one-parameter family of models for star-forming galaxies, and includes an update to the mid-infrared emission using an average template obtained from Spitzer Space Telescope observations of normal galaxies. Star-forming/AGN diagnostics based on PAH equivalent widths and broadband infrared colors are presented, and example mid-infrared A","authors_text":"Daniel A. Dale, George Helou, Georgios E. Magdis, Lee Armus, Tanio D\\'iaz-Santos, Yong Shi","cross_cats":["astro-ph.CO"],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-02-06T21:00:17Z","title":"A Two-Parameter Model for the Infrared/Submillimeter/Radio Spectral Energy Distributions of Galaxies and AGN"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1402.1495","kind":"arxiv","version":1},"verdict":{"created_at":null,"id":null,"model_set":{},"one_line_summary":"","pipeline_version":null,"pith_extraction_headline":"","strongest_claim":"","weakest_assumption":""}},"verdict_id":null}}],"author_attestations":[],"timestamp_anchors":[],"storage_attestations":[],"citation_signatures":[],"replication_records":[],"corrections":[],"mirror_hints":[],"record_created":{"event_id":"sha256:4a4b3d57242d369223aba5f5abc2862c5012d6d4675da00d7c9c3ea613ba712e","target":"record","created_at":"2026-05-18T01:44:46Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"attestation_state":"computed","canonical_record":{"metadata":{"abstract_canon_sha256":"9e445b93fde3b714e5811eabd936531bea5a4ef39231721cdfca937a8f36f068","cross_cats_sorted":["astro-ph.CO"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-02-06T21:00:17Z","title_canon_sha256":"347f3026ddc6007bcec61872da6a9570932ebfc5f443979ad48c2ec25b66e281"},"schema_version":"1.0","source":{"id":"1402.1495","kind":"arxiv","version":1}},"canonical_sha256":"4d704a587fda8123d344a8f04d4763691f3414eb2761f7e44c748c8100f0ba5b","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"4d704a587fda8123d344a8f04d4763691f3414eb2761f7e44c748c8100f0ba5b","first_computed_at":"2026-05-18T01:44:46.757975Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T01:44:46.757975Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"7dVUsylThEipzPVs4iRTOvccYP3oMr4qIPHN4COEXJh4zC8cy6BN++iLA7xBqYUGzYoII3+Lvk7fFgX4olfAAA==","signature_status":"signed_v1","signed_at":"2026-05-18T01:44:46.758539Z","signed_message":"canonical_sha256_bytes"},"source_id":"1402.1495","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:4a4b3d57242d369223aba5f5abc2862c5012d6d4675da00d7c9c3ea613ba712e","sha256:030b4b584b17aa8dbc7ae22c116fe1a61d9a2e0814bae4533b370ff7349819cb"],"state_sha256":"d74f577ed1060ea539a0623629e7ffdc0a44cfab1fce6c0f7dc3808d51ec3f64"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"CIzL0nB01qZfqwdaFnxFAPbEXPspTkF+s+4Yf1sbrWTwRbIAwRt53+rg3hp/kQA8PUwDSZgq5P7qi63Qrdq+AA==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-26T11:03:26.239409Z","bundle_sha256":"e16caa945b05a0c0cf982970c53d4e970ce19a31165b3d4fec3472675a254fc2"}}