{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2014:S7BSAEYPB5O5ECVLHEYQHBLGVO","short_pith_number":"pith:S7BSAEYP","canonical_record":{"source":{"id":"1406.2599","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-06-10T15:41:35Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"09ab37008ca48d1d206cf453a66edf1d1ced8c2f7a2248c5b7136765229944ae","abstract_canon_sha256":"cc087c60201dc415c92550670f816c66ee20db3dc7b67b3b9b90fc8d1af45ce6"},"schema_version":"1.0"},"canonical_sha256":"97c320130f0f5dd20aab3931038566ab8233a8e37fe0e449b8bfd579f12c2cfb","source":{"kind":"arxiv","id":"1406.2599","version":2},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1406.2599","created_at":"2026-05-18T01:42:58Z"},{"alias_kind":"arxiv_version","alias_value":"1406.2599v2","created_at":"2026-05-18T01:42:58Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1406.2599","created_at":"2026-05-18T01:42:58Z"},{"alias_kind":"pith_short_12","alias_value":"S7BSAEYPB5O5","created_at":"2026-05-18T12:28:49Z"},{"alias_kind":"pith_short_16","alias_value":"S7BSAEYPB5O5ECVL","created_at":"2026-05-18T12:28:49Z"},{"alias_kind":"pith_short_8","alias_value":"S7BSAEYP","created_at":"2026-05-18T12:28:49Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2014:S7BSAEYPB5O5ECVLHEYQHBLGVO","target":"record","payload":{"canonical_record":{"source":{"id":"1406.2599","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-06-10T15:41:35Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"09ab37008ca48d1d206cf453a66edf1d1ced8c2f7a2248c5b7136765229944ae","abstract_canon_sha256":"cc087c60201dc415c92550670f816c66ee20db3dc7b67b3b9b90fc8d1af45ce6"},"schema_version":"1.0"},"canonical_sha256":"97c320130f0f5dd20aab3931038566ab8233a8e37fe0e449b8bfd579f12c2cfb","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:42:58.853343Z","signature_b64":"ClG7uhhIUtVtQXoQVzbpDTLqJbeKC9Q39ZbYksPkY/GMoV4mIptrvnlVwJi49hzu95Syfduhhk0YmAZ/mz+VDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"97c320130f0f5dd20aab3931038566ab8233a8e37fe0e449b8bfd579f12c2cfb","last_reissued_at":"2026-05-18T01:42:58.852680Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:42:58.852680Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1406.2599","source_version":2,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T01:42:58Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"5veJNLif6zllp/f0dJnASl8GaabrrmuO4GmO02xqwN1LqLiAPxuRaePf74pd23NB8BTVbPA0Fv/En7dve5kDCw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-04T13:28:46.943027Z"},"content_sha256":"3e17e3c076c8dcb35ae0dfecac014cda7ab49c2b4013646046b753ec5b7cefb8","schema_version":"1.0","event_id":"sha256:3e17e3c076c8dcb35ae0dfecac014cda7ab49c2b4013646046b753ec5b7cefb8"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2014:S7BSAEYPB5O5ECVLHEYQHBLGVO","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Herschel/PACS Observations of the Host Galaxy of GRB 031203","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"B. O'Halloran, K. Wiersema, M. De Pasquale, M. J. Page, M. Symeonidis, N. Seymour, P. Schady, R. Starling, S. R. Oates","submitted_at":"2014-06-10T15:41:35Z","abstract_excerpt":"We present Herschel/PACS observations of the nearby (z=0.1055) dwarf galaxy that has hosted the long gamma ray burst (LGRB) 031203. Using the PACS data we have been able to place constraints on the dust temperature, dust mass, total infrared luminosity and infrared-derived star-formation rate (SFR) for this object. We find that the GRB host galaxy (GRBH) 031203 has a total infrared luminosity of 3x10^10 L_sun placing it in the regime of the IR-luminous galaxy population. Its dust temperature and specific SFR are comparable to that of many high-redshift (z=0.3-2.5) infrared (IR)-detected GRB ho"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1406.2599","kind":"arxiv","version":2},"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":"2026-05-18T01:42:58Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"e9KEc467p4P9pntqUFbWX3MJTnkWaW9eJvonGY3WuISRgB0ZsqTm++c97DlgGmiQFZLrF99TWx/vFIBX8kKwAA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-04T13:28:46.943621Z"},"content_sha256":"71c94a571ab58a621869f35660ea80c2075d31e6af64ae9c50ca324dc01048f6","schema_version":"1.0","event_id":"sha256:71c94a571ab58a621869f35660ea80c2075d31e6af64ae9c50ca324dc01048f6"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/S7BSAEYPB5O5ECVLHEYQHBLGVO/bundle.json","state_url":"https://pith.science/pith/S7BSAEYPB5O5ECVLHEYQHBLGVO/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/S7BSAEYPB5O5ECVLHEYQHBLGVO/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":"2026-06-04T13:28:46Z","links":{"resolver":"https://pith.science/pith/S7BSAEYPB5O5ECVLHEYQHBLGVO","bundle":"https://pith.science/pith/S7BSAEYPB5O5ECVLHEYQHBLGVO/bundle.json","state":"https://pith.science/pith/S7BSAEYPB5O5ECVLHEYQHBLGVO/state.json","well_known_bundle":"https://pith.science/.well-known/pith/S7BSAEYPB5O5ECVLHEYQHBLGVO/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2014:S7BSAEYPB5O5ECVLHEYQHBLGVO","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":"cc087c60201dc415c92550670f816c66ee20db3dc7b67b3b9b90fc8d1af45ce6","cross_cats_sorted":["astro-ph.CO"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-06-10T15:41:35Z","title_canon_sha256":"09ab37008ca48d1d206cf453a66edf1d1ced8c2f7a2248c5b7136765229944ae"},"schema_version":"1.0","source":{"id":"1406.2599","kind":"arxiv","version":2}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1406.2599","created_at":"2026-05-18T01:42:58Z"},{"alias_kind":"arxiv_version","alias_value":"1406.2599v2","created_at":"2026-05-18T01:42:58Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1406.2599","created_at":"2026-05-18T01:42:58Z"},{"alias_kind":"pith_short_12","alias_value":"S7BSAEYPB5O5","created_at":"2026-05-18T12:28:49Z"},{"alias_kind":"pith_short_16","alias_value":"S7BSAEYPB5O5ECVL","created_at":"2026-05-18T12:28:49Z"},{"alias_kind":"pith_short_8","alias_value":"S7BSAEYP","created_at":"2026-05-18T12:28:49Z"}],"graph_snapshots":[{"event_id":"sha256:71c94a571ab58a621869f35660ea80c2075d31e6af64ae9c50ca324dc01048f6","target":"graph","created_at":"2026-05-18T01:42:58Z","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":"We present Herschel/PACS observations of the nearby (z=0.1055) dwarf galaxy that has hosted the long gamma ray burst (LGRB) 031203. Using the PACS data we have been able to place constraints on the dust temperature, dust mass, total infrared luminosity and infrared-derived star-formation rate (SFR) for this object. We find that the GRB host galaxy (GRBH) 031203 has a total infrared luminosity of 3x10^10 L_sun placing it in the regime of the IR-luminous galaxy population. Its dust temperature and specific SFR are comparable to that of many high-redshift (z=0.3-2.5) infrared (IR)-detected GRB ho","authors_text":"B. O'Halloran, K. Wiersema, M. De Pasquale, M. J. Page, M. Symeonidis, N. Seymour, P. Schady, R. Starling, S. R. Oates","cross_cats":["astro-ph.CO"],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-06-10T15:41:35Z","title":"Herschel/PACS Observations of the Host Galaxy of GRB 031203"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1406.2599","kind":"arxiv","version":2},"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":"sha256:3e17e3c076c8dcb35ae0dfecac014cda7ab49c2b4013646046b753ec5b7cefb8","target":"record","created_at":"2026-05-18T01:42:58Z","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":"cc087c60201dc415c92550670f816c66ee20db3dc7b67b3b9b90fc8d1af45ce6","cross_cats_sorted":["astro-ph.CO"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-06-10T15:41:35Z","title_canon_sha256":"09ab37008ca48d1d206cf453a66edf1d1ced8c2f7a2248c5b7136765229944ae"},"schema_version":"1.0","source":{"id":"1406.2599","kind":"arxiv","version":2}},"canonical_sha256":"97c320130f0f5dd20aab3931038566ab8233a8e37fe0e449b8bfd579f12c2cfb","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"97c320130f0f5dd20aab3931038566ab8233a8e37fe0e449b8bfd579f12c2cfb","first_computed_at":"2026-05-18T01:42:58.852680Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T01:42:58.852680Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"ClG7uhhIUtVtQXoQVzbpDTLqJbeKC9Q39ZbYksPkY/GMoV4mIptrvnlVwJi49hzu95Syfduhhk0YmAZ/mz+VDw==","signature_status":"signed_v1","signed_at":"2026-05-18T01:42:58.853343Z","signed_message":"canonical_sha256_bytes"},"source_id":"1406.2599","source_kind":"arxiv","source_version":2}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:3e17e3c076c8dcb35ae0dfecac014cda7ab49c2b4013646046b753ec5b7cefb8","sha256:71c94a571ab58a621869f35660ea80c2075d31e6af64ae9c50ca324dc01048f6"],"state_sha256":"995e95feacce19752ab65a2a3c73327c3492fd8b58f35e5a6490a199ae886a37"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"/Ye+lmdW9fF+o4wU+x4h1E4IbAeiNnkRVotsVrw0XPkVDeg5H958GxhutVGqtTXXSDFx5/MXL/2LK+hAA6u7Bw==","signed_message":"bundle_sha256_bytes","signed_at":"2026-06-04T13:28:46.946613Z","bundle_sha256":"fc8b030ba177092c2956133a450c92788d15a3109380dbf2b025e764d97433e9"}}