{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2010:DZODEZJFVLJIIMVRTQD3WHL22Z","short_pith_number":"pith:DZODEZJF","canonical_record":{"source":{"id":"1010.2774","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2010-10-13T21:05:29Z","cross_cats_sorted":[],"title_canon_sha256":"657690225030ec0ff049ad6967a63f1e6f90fe024c268c5c11b068055d7c647e","abstract_canon_sha256":"425573f9ec0c96e3b1f5baa1405f5d6a80495b7f976612a75cf2d42fb3ac77be"},"schema_version":"1.0"},"canonical_sha256":"1e5c326525aad28432b19c07bb1d7ad6630970282815643011a6420c203fb1a4","source":{"kind":"arxiv","id":"1010.2774","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1010.2774","created_at":"2026-05-18T02:05:05Z"},{"alias_kind":"arxiv_version","alias_value":"1010.2774v1","created_at":"2026-05-18T02:05:05Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1010.2774","created_at":"2026-05-18T02:05:05Z"},{"alias_kind":"pith_short_12","alias_value":"DZODEZJFVLJI","created_at":"2026-05-18T12:26:06Z"},{"alias_kind":"pith_short_16","alias_value":"DZODEZJFVLJIIMVR","created_at":"2026-05-18T12:26:06Z"},{"alias_kind":"pith_short_8","alias_value":"DZODEZJF","created_at":"2026-05-18T12:26:06Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2010:DZODEZJFVLJIIMVRTQD3WHL22Z","target":"record","payload":{"canonical_record":{"source":{"id":"1010.2774","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2010-10-13T21:05:29Z","cross_cats_sorted":[],"title_canon_sha256":"657690225030ec0ff049ad6967a63f1e6f90fe024c268c5c11b068055d7c647e","abstract_canon_sha256":"425573f9ec0c96e3b1f5baa1405f5d6a80495b7f976612a75cf2d42fb3ac77be"},"schema_version":"1.0"},"canonical_sha256":"1e5c326525aad28432b19c07bb1d7ad6630970282815643011a6420c203fb1a4","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:05:05.301637Z","signature_b64":"V4lU4AsltoFrspMZem5sqfv2iAuPzmhFsWRJWm3zSydmZzO/E9NLv5hsU8oWObxpDgAILGasx9K4AMhx9CScCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1e5c326525aad28432b19c07bb1d7ad6630970282815643011a6420c203fb1a4","last_reissued_at":"2026-05-18T02:05:05.300780Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:05:05.300780Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1010.2774","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":"2026-05-18T02:05:05Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"U0JS2TRKXnpgwXY/dwBuuwFFxnaASrTru9Y/eM+1bWdUiwIBhx/b7gFPqSzaP8R6oRBBNp9wJNX5kxmyHkCuAg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-28T06:13:26.934878Z"},"content_sha256":"8d59c1f246cf08ef0e5cebd9e4f554ffbef233862a296ac701aaf30172d726e7","schema_version":"1.0","event_id":"sha256:8d59c1f246cf08ef0e5cebd9e4f554ffbef233862a296ac701aaf30172d726e7"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2010:DZODEZJFVLJIIMVRTQD3WHL22Z","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Dust in the diffuse emission of the galactic plane - The Herschel/Spitzer SED fitting","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Noriega-Crespo, J.-P. Bernard, M. Compiegne, N. Flagey, P. G. Martin, R. Paladini, S. Molinari","submitted_at":"2010-10-13T21:05:29Z","abstract_excerpt":"The first Herschel Hi-Gal images of the galactic plane unveil the far-infrared diffuse emission of the interstellar medium with an unprecedented angular resolution and sensitivity. In this paper, we present the first analysis of these data in combination with that of Spitzer Glimpse & Mipsgal. We selected a relatively diffuse and low excitation region of the l~59\\,^{\\circ} Hi-Gal Science Demonstration Phase field to perform a pixel by pixel fitting of the 8 to 500 microns SED using the DustEM dust emission model. We derived maps of the Very Small Grains (VSG) and PAH abundances from the model."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1010.2774","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":"2026-05-18T02:05:05Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"SGn0cwKREVPqD5vnJaYAuaNJ1AuPjEsgcJCqorcpxF2e9GMQTkBjDqYZf0cyRrljPRn+ntTMTflDoJQ3u8w9AA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-28T06:13:26.935444Z"},"content_sha256":"8a8416aeaf2a3c70082556076fb9db1f9686c8edd02a4f701d773e38e6fe3ef8","schema_version":"1.0","event_id":"sha256:8a8416aeaf2a3c70082556076fb9db1f9686c8edd02a4f701d773e38e6fe3ef8"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/DZODEZJFVLJIIMVRTQD3WHL22Z/bundle.json","state_url":"https://pith.science/pith/DZODEZJFVLJIIMVRTQD3WHL22Z/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/DZODEZJFVLJIIMVRTQD3WHL22Z/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":"2026-05-28T06:13:26Z","links":{"resolver":"https://pith.science/pith/DZODEZJFVLJIIMVRTQD3WHL22Z","bundle":"https://pith.science/pith/DZODEZJFVLJIIMVRTQD3WHL22Z/bundle.json","state":"https://pith.science/pith/DZODEZJFVLJIIMVRTQD3WHL22Z/state.json","well_known_bundle":"https://pith.science/.well-known/pith/DZODEZJFVLJIIMVRTQD3WHL22Z/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2010:DZODEZJFVLJIIMVRTQD3WHL22Z","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":"425573f9ec0c96e3b1f5baa1405f5d6a80495b7f976612a75cf2d42fb3ac77be","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2010-10-13T21:05:29Z","title_canon_sha256":"657690225030ec0ff049ad6967a63f1e6f90fe024c268c5c11b068055d7c647e"},"schema_version":"1.0","source":{"id":"1010.2774","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1010.2774","created_at":"2026-05-18T02:05:05Z"},{"alias_kind":"arxiv_version","alias_value":"1010.2774v1","created_at":"2026-05-18T02:05:05Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1010.2774","created_at":"2026-05-18T02:05:05Z"},{"alias_kind":"pith_short_12","alias_value":"DZODEZJFVLJI","created_at":"2026-05-18T12:26:06Z"},{"alias_kind":"pith_short_16","alias_value":"DZODEZJFVLJIIMVR","created_at":"2026-05-18T12:26:06Z"},{"alias_kind":"pith_short_8","alias_value":"DZODEZJF","created_at":"2026-05-18T12:26:06Z"}],"graph_snapshots":[{"event_id":"sha256:8a8416aeaf2a3c70082556076fb9db1f9686c8edd02a4f701d773e38e6fe3ef8","target":"graph","created_at":"2026-05-18T02:05:05Z","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":"The first Herschel Hi-Gal images of the galactic plane unveil the far-infrared diffuse emission of the interstellar medium with an unprecedented angular resolution and sensitivity. In this paper, we present the first analysis of these data in combination with that of Spitzer Glimpse & Mipsgal. We selected a relatively diffuse and low excitation region of the l~59\\,^{\\circ} Hi-Gal Science Demonstration Phase field to perform a pixel by pixel fitting of the 8 to 500 microns SED using the DustEM dust emission model. We derived maps of the Very Small Grains (VSG) and PAH abundances from the model.","authors_text":"A. Noriega-Crespo, J.-P. Bernard, M. Compiegne, N. Flagey, P. G. Martin, R. Paladini, S. Molinari","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2010-10-13T21:05:29Z","title":"Dust in the diffuse emission of the galactic plane - The Herschel/Spitzer SED fitting"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1010.2774","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":"sha256:8d59c1f246cf08ef0e5cebd9e4f554ffbef233862a296ac701aaf30172d726e7","target":"record","created_at":"2026-05-18T02:05:05Z","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":"425573f9ec0c96e3b1f5baa1405f5d6a80495b7f976612a75cf2d42fb3ac77be","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2010-10-13T21:05:29Z","title_canon_sha256":"657690225030ec0ff049ad6967a63f1e6f90fe024c268c5c11b068055d7c647e"},"schema_version":"1.0","source":{"id":"1010.2774","kind":"arxiv","version":1}},"canonical_sha256":"1e5c326525aad28432b19c07bb1d7ad6630970282815643011a6420c203fb1a4","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"1e5c326525aad28432b19c07bb1d7ad6630970282815643011a6420c203fb1a4","first_computed_at":"2026-05-18T02:05:05.300780Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T02:05:05.300780Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"V4lU4AsltoFrspMZem5sqfv2iAuPzmhFsWRJWm3zSydmZzO/E9NLv5hsU8oWObxpDgAILGasx9K4AMhx9CScCA==","signature_status":"signed_v1","signed_at":"2026-05-18T02:05:05.301637Z","signed_message":"canonical_sha256_bytes"},"source_id":"1010.2774","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:8d59c1f246cf08ef0e5cebd9e4f554ffbef233862a296ac701aaf30172d726e7","sha256:8a8416aeaf2a3c70082556076fb9db1f9686c8edd02a4f701d773e38e6fe3ef8"],"state_sha256":"4f7bab487b805e842d022a6951f8dc85c300f55abc471631c66deee77a770d7c"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"rJePry6tcsmZqInL6bLNGg15OSlG7Vyr77Oc9tsbvdYQVxcEQjw42spZ0rASuNZC3gjVesE1oqvHRjXOHi1BDQ==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-28T06:13:26.938200Z","bundle_sha256":"25a25a82c0c6398a271f4fac390efbef42721ac5389ab35a8cd5e687cf581bf3"}}