{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2006:OIZJOUPAELHTX2HXRSRYBIOL33","short_pith_number":"pith:OIZJOUPA","schema_version":"1.0","canonical_sha256":"72329751e022cf3be8f78ca380a1cbdef9b57ed23834e61dec5a23054f98797b","source":{"kind":"arxiv","id":"astro-ph/0609483","version":1},"attestation_state":"computed","paper":{"title":"Probing the Density in the Galactic Center Region: Wind-Blown Bubbles and High-Energy Proton Constraints","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Aimee Hungerford, Christopher L. Fryer, Gabriel Rockefeller, Guillaume Belanger, Siming Liu","submitted_at":"2006-09-18T13:37:18Z","abstract_excerpt":"Recent observations of the Galactic center in high-energy gamma-rays (above 0.1TeV) have opened up new ways to study this region, from understanding the emission source of these high-energy photons to constraining the environment in which they are formed. We present a revised theoretical density model of the inner 5pc surrounding Sgr A* based on the fact that the underlying structure of this region is dominated by the winds from the Wolf-Rayet stars orbiting Sgr A*. An ideal probe and application of this density structure is this high energy gamma-ray emission. We assume a proton-scattering mo"},"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":"astro-ph/0609483","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2006-09-18T13:37:18Z","cross_cats_sorted":[],"title_canon_sha256":"c592523d1add8fd66c1afca6fbb25237dd0417e95fcc9fd9aa51cf664439165b","abstract_canon_sha256":"a5dfd1219c2bc1d2350f5740e8ba8c1058b47234129356c24b82805f9c3f72a9"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:28:57.694677Z","signature_b64":"6XTqBFLn3lMPkXkaDfuzHd51IFtxgB+9yQfhtcGobJvxQiCfhm2v2DtdRu2G2GvBMUUznRKXVV/FmuDKDTpKAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"72329751e022cf3be8f78ca380a1cbdef9b57ed23834e61dec5a23054f98797b","last_reissued_at":"2026-05-18T04:28:57.694207Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:28:57.694207Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Probing the Density in the Galactic Center Region: Wind-Blown Bubbles and High-Energy Proton Constraints","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Aimee Hungerford, Christopher L. Fryer, Gabriel Rockefeller, Guillaume Belanger, Siming Liu","submitted_at":"2006-09-18T13:37:18Z","abstract_excerpt":"Recent observations of the Galactic center in high-energy gamma-rays (above 0.1TeV) have opened up new ways to study this region, from understanding the emission source of these high-energy photons to constraining the environment in which they are formed. We present a revised theoretical density model of the inner 5pc surrounding Sgr A* based on the fact that the underlying structure of this region is dominated by the winds from the Wolf-Rayet stars orbiting Sgr A*. An ideal probe and application of this density structure is this high energy gamma-ray emission. We assume a proton-scattering mo"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0609483","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":"astro-ph/0609483","created_at":"2026-05-18T04:28:57.694268+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0609483v1","created_at":"2026-05-18T04:28:57.694268+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0609483","created_at":"2026-05-18T04:28:57.694268+00:00"},{"alias_kind":"pith_short_12","alias_value":"OIZJOUPAELHT","created_at":"2026-05-18T12:25:54.717736+00:00"},{"alias_kind":"pith_short_16","alias_value":"OIZJOUPAELHTX2HX","created_at":"2026-05-18T12:25:54.717736+00:00"},{"alias_kind":"pith_short_8","alias_value":"OIZJOUPA","created_at":"2026-05-18T12:25:54.717736+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/OIZJOUPAELHTX2HXRSRYBIOL33","json":"https://pith.science/pith/OIZJOUPAELHTX2HXRSRYBIOL33.json","graph_json":"https://pith.science/api/pith-number/OIZJOUPAELHTX2HXRSRYBIOL33/graph.json","events_json":"https://pith.science/api/pith-number/OIZJOUPAELHTX2HXRSRYBIOL33/events.json","paper":"https://pith.science/paper/OIZJOUPA"},"agent_actions":{"view_html":"https://pith.science/pith/OIZJOUPAELHTX2HXRSRYBIOL33","download_json":"https://pith.science/pith/OIZJOUPAELHTX2HXRSRYBIOL33.json","view_paper":"https://pith.science/paper/OIZJOUPA","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0609483&json=true","fetch_graph":"https://pith.science/api/pith-number/OIZJOUPAELHTX2HXRSRYBIOL33/graph.json","fetch_events":"https://pith.science/api/pith-number/OIZJOUPAELHTX2HXRSRYBIOL33/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/OIZJOUPAELHTX2HXRSRYBIOL33/action/timestamp_anchor","attest_storage":"https://pith.science/pith/OIZJOUPAELHTX2HXRSRYBIOL33/action/storage_attestation","attest_author":"https://pith.science/pith/OIZJOUPAELHTX2HXRSRYBIOL33/action/author_attestation","sign_citation":"https://pith.science/pith/OIZJOUPAELHTX2HXRSRYBIOL33/action/citation_signature","submit_replication":"https://pith.science/pith/OIZJOUPAELHTX2HXRSRYBIOL33/action/replication_record"}},"created_at":"2026-05-18T04:28:57.694268+00:00","updated_at":"2026-05-18T04:28:57.694268+00:00"}