{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2017:5MQHA2RRSSIE6SXSKXRE25YXS3","short_pith_number":"pith:5MQHA2RR","canonical_record":{"source":{"id":"1705.00380","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-04-30T22:13:42Z","cross_cats_sorted":[],"title_canon_sha256":"c407630b0d5934a15b327a8bf324d4449cd9be95175cdd72fb7e675f8de58e02","abstract_canon_sha256":"c6d4d442e63e492c9534668aeed55941e39392e60bd05b92a36a492f592255b7"},"schema_version":"1.0"},"canonical_sha256":"eb20706a3194904f4af255e24d771796c25dd05ed1f9aac8acb5ff96c72ba444","source":{"kind":"arxiv","id":"1705.00380","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1705.00380","created_at":"2026-05-18T00:45:20Z"},{"alias_kind":"arxiv_version","alias_value":"1705.00380v1","created_at":"2026-05-18T00:45:20Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1705.00380","created_at":"2026-05-18T00:45:20Z"},{"alias_kind":"pith_short_12","alias_value":"5MQHA2RRSSIE","created_at":"2026-05-18T12:31:00Z"},{"alias_kind":"pith_short_16","alias_value":"5MQHA2RRSSIE6SXS","created_at":"2026-05-18T12:31:00Z"},{"alias_kind":"pith_short_8","alias_value":"5MQHA2RR","created_at":"2026-05-18T12:31:00Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2017:5MQHA2RRSSIE6SXSKXRE25YXS3","target":"record","payload":{"canonical_record":{"source":{"id":"1705.00380","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-04-30T22:13:42Z","cross_cats_sorted":[],"title_canon_sha256":"c407630b0d5934a15b327a8bf324d4449cd9be95175cdd72fb7e675f8de58e02","abstract_canon_sha256":"c6d4d442e63e492c9534668aeed55941e39392e60bd05b92a36a492f592255b7"},"schema_version":"1.0"},"canonical_sha256":"eb20706a3194904f4af255e24d771796c25dd05ed1f9aac8acb5ff96c72ba444","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:45:20.546419Z","signature_b64":"vPPbh3vqzK+eq0n3Qn3gpDD/WdywAk9UUf9R9bQoqATVmd6PB+xHIfFsLakLbvjI9clPmNsC22eKYlD5IuzSDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"eb20706a3194904f4af255e24d771796c25dd05ed1f9aac8acb5ff96c72ba444","last_reissued_at":"2026-05-18T00:45:20.545718Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:45:20.545718Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1705.00380","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":"2026-05-18T00:45:20Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"Cq+FS9GOKp2rtbOA+rla1e2gWAfsfP4+7itBS+8OCFuD/FQOHixnkSml1IvadkpJ9grX1w+vQ8FwDygYcAvtAg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-29T21:22:40.531612Z"},"content_sha256":"947d6cc43b0456454501e59326c45d2bf8c14ccc7fe7f5030cfc9c3263d87457","schema_version":"1.0","event_id":"sha256:947d6cc43b0456454501e59326c45d2bf8c14ccc7fe7f5030cfc9c3263d87457"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2017:5MQHA2RRSSIE6SXSKXRE25YXS3","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Probing the infrared counterparts of diffuse far-ultraviolet sources in the Galaxy","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Amit Pathak, Gautam Saikia, P. Shalima, Rupjyoti Gogoi","submitted_at":"2017-04-30T22:13:42Z","abstract_excerpt":"Recent availability of high quality infrared (IR) data for diffuse regions in the Galaxy and external galaxies have added to our understanding of interstellar dust. A comparison of ultraviolet (UV) and IR observations may be used to estimate absorption, scattering and thermal emission from interstellar dust. In this paper, we report IR and UV observations for selective diffuse sources in the Galaxy. Using archival mid-infrared (MIR) and far-infrared (FIR) observations from Spitzer Space Telescope, we look for counterparts of diffuse far-ultraviolet (FUV) sources observed by the Voyager, Far Ul"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1705.00380","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":"2026-05-18T00:45:20Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"C0Uvql7W8yzVt+WuXgJUwwo/ft3wjTpzB5HfKgKHjYpFcDm/Rc4xgBMddCW/NT1adKZNJiBEmHGKcANNsjVeDQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-29T21:22:40.532349Z"},"content_sha256":"574fe486616e10b50897848da86d9aefa6e8a85edd5e33a751b6fdd770cac9ef","schema_version":"1.0","event_id":"sha256:574fe486616e10b50897848da86d9aefa6e8a85edd5e33a751b6fdd770cac9ef"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/5MQHA2RRSSIE6SXSKXRE25YXS3/bundle.json","state_url":"https://pith.science/pith/5MQHA2RRSSIE6SXSKXRE25YXS3/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/5MQHA2RRSSIE6SXSKXRE25YXS3/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":"2026-05-29T21:22:40Z","links":{"resolver":"https://pith.science/pith/5MQHA2RRSSIE6SXSKXRE25YXS3","bundle":"https://pith.science/pith/5MQHA2RRSSIE6SXSKXRE25YXS3/bundle.json","state":"https://pith.science/pith/5MQHA2RRSSIE6SXSKXRE25YXS3/state.json","well_known_bundle":"https://pith.science/.well-known/pith/5MQHA2RRSSIE6SXSKXRE25YXS3/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2017:5MQHA2RRSSIE6SXSKXRE25YXS3","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":"c6d4d442e63e492c9534668aeed55941e39392e60bd05b92a36a492f592255b7","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-04-30T22:13:42Z","title_canon_sha256":"c407630b0d5934a15b327a8bf324d4449cd9be95175cdd72fb7e675f8de58e02"},"schema_version":"1.0","source":{"id":"1705.00380","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1705.00380","created_at":"2026-05-18T00:45:20Z"},{"alias_kind":"arxiv_version","alias_value":"1705.00380v1","created_at":"2026-05-18T00:45:20Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1705.00380","created_at":"2026-05-18T00:45:20Z"},{"alias_kind":"pith_short_12","alias_value":"5MQHA2RRSSIE","created_at":"2026-05-18T12:31:00Z"},{"alias_kind":"pith_short_16","alias_value":"5MQHA2RRSSIE6SXS","created_at":"2026-05-18T12:31:00Z"},{"alias_kind":"pith_short_8","alias_value":"5MQHA2RR","created_at":"2026-05-18T12:31:00Z"}],"graph_snapshots":[{"event_id":"sha256:574fe486616e10b50897848da86d9aefa6e8a85edd5e33a751b6fdd770cac9ef","target":"graph","created_at":"2026-05-18T00:45:20Z","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":"Recent availability of high quality infrared (IR) data for diffuse regions in the Galaxy and external galaxies have added to our understanding of interstellar dust. A comparison of ultraviolet (UV) and IR observations may be used to estimate absorption, scattering and thermal emission from interstellar dust. In this paper, we report IR and UV observations for selective diffuse sources in the Galaxy. Using archival mid-infrared (MIR) and far-infrared (FIR) observations from Spitzer Space Telescope, we look for counterparts of diffuse far-ultraviolet (FUV) sources observed by the Voyager, Far Ul","authors_text":"Amit Pathak, Gautam Saikia, P. Shalima, Rupjyoti Gogoi","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-04-30T22:13:42Z","title":"Probing the infrared counterparts of diffuse far-ultraviolet sources in the Galaxy"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1705.00380","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":"sha256:947d6cc43b0456454501e59326c45d2bf8c14ccc7fe7f5030cfc9c3263d87457","target":"record","created_at":"2026-05-18T00:45:20Z","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":"c6d4d442e63e492c9534668aeed55941e39392e60bd05b92a36a492f592255b7","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-04-30T22:13:42Z","title_canon_sha256":"c407630b0d5934a15b327a8bf324d4449cd9be95175cdd72fb7e675f8de58e02"},"schema_version":"1.0","source":{"id":"1705.00380","kind":"arxiv","version":1}},"canonical_sha256":"eb20706a3194904f4af255e24d771796c25dd05ed1f9aac8acb5ff96c72ba444","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"eb20706a3194904f4af255e24d771796c25dd05ed1f9aac8acb5ff96c72ba444","first_computed_at":"2026-05-18T00:45:20.545718Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T00:45:20.545718Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"vPPbh3vqzK+eq0n3Qn3gpDD/WdywAk9UUf9R9bQoqATVmd6PB+xHIfFsLakLbvjI9clPmNsC22eKYlD5IuzSDA==","signature_status":"signed_v1","signed_at":"2026-05-18T00:45:20.546419Z","signed_message":"canonical_sha256_bytes"},"source_id":"1705.00380","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:947d6cc43b0456454501e59326c45d2bf8c14ccc7fe7f5030cfc9c3263d87457","sha256:574fe486616e10b50897848da86d9aefa6e8a85edd5e33a751b6fdd770cac9ef"],"state_sha256":"447dd92374c8aba3a74416a65c43fad25b8bbaf8709ebd3f9e4e489d8487e9b9"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"6bTTobOTgVFC+CBxYf5doqRXmCvEWj2ovHxxh7kXvrXuqzPJk0ymJ6nAE5rrws1EVHAXrYFBPwD37kEW+uw4DQ==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-29T21:22:40.536714Z","bundle_sha256":"a3ca1bd3326d6e601eb337937cd96fb5b8a03b758cf81b0be42b60e131c3c9cb"}}