{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:OBHUJ45LYJX3H7XKC5EH6TYDZX","short_pith_number":"pith:OBHUJ45L","schema_version":"1.0","canonical_sha256":"704f44f3abc26fb3feea17487f4f03cdd7c477f2ed55aae4ffb5cb667279a619","source":{"kind":"arxiv","id":"1302.6589","version":1},"attestation_state":"computed","paper":{"title":"Two Emission Mechanisms in the Fermi Bubbles: A Possible Signal of Annihilating Dark Matter","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-ph"],"primary_cat":"astro-ph.HE","authors_text":"Dan Hooper, Tracy R. Slatyer","submitted_at":"2013-02-26T21:00:01Z","abstract_excerpt":"We study the variation of the spectrum of the Fermi Bubbles with Galactic latitude. Far from the Galactic plane (|b| > 30 degrees), the observed gamma-ray emission is nearly invariant with latitude, and is consistent with arising from inverse Compton scattering of the interstellar radiation field by cosmic-ray electrons with an approximately power-law spectrum. The same electrons in the presence of microgauss-scale magnetic fields can also generate the the observed microwave \"haze\". At lower latitudes (b < 20 degrees), in contrast, the spectrum of the emission correlated with the Bubbles posse"},"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":"1302.6589","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2013-02-26T21:00:01Z","cross_cats_sorted":["astro-ph.CO","hep-ph"],"title_canon_sha256":"ffee749cca2871d3e065e3fbf31b22f294a310aa2a87a6ccd4100dfdc631e28c","abstract_canon_sha256":"2f2b547428d8075810191a8589841f47015c6e7f5f4f0dbcd72840909cfd8fae"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:32:19.373842Z","signature_b64":"u/X+ToLq58D4dOEIXuFlfcCiATBWFsVcAs9Y9nMr45Dri2GcAi2X1Wy6ZHGadgVb289I+jckQ+UuUBAXmg6DCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"704f44f3abc26fb3feea17487f4f03cdd7c477f2ed55aae4ffb5cb667279a619","last_reissued_at":"2026-05-18T03:32:19.372794Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:32:19.372794Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Two Emission Mechanisms in the Fermi Bubbles: A Possible Signal of Annihilating Dark Matter","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-ph"],"primary_cat":"astro-ph.HE","authors_text":"Dan Hooper, Tracy R. Slatyer","submitted_at":"2013-02-26T21:00:01Z","abstract_excerpt":"We study the variation of the spectrum of the Fermi Bubbles with Galactic latitude. Far from the Galactic plane (|b| > 30 degrees), the observed gamma-ray emission is nearly invariant with latitude, and is consistent with arising from inverse Compton scattering of the interstellar radiation field by cosmic-ray electrons with an approximately power-law spectrum. The same electrons in the presence of microgauss-scale magnetic fields can also generate the the observed microwave \"haze\". At lower latitudes (b < 20 degrees), in contrast, the spectrum of the emission correlated with the Bubbles posse"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1302.6589","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":"1302.6589","created_at":"2026-05-18T03:32:19.372931+00:00"},{"alias_kind":"arxiv_version","alias_value":"1302.6589v1","created_at":"2026-05-18T03:32:19.372931+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1302.6589","created_at":"2026-05-18T03:32:19.372931+00:00"},{"alias_kind":"pith_short_12","alias_value":"OBHUJ45LYJX3","created_at":"2026-05-18T12:27:54.935989+00:00"},{"alias_kind":"pith_short_16","alias_value":"OBHUJ45LYJX3H7XK","created_at":"2026-05-18T12:27:54.935989+00:00"},{"alias_kind":"pith_short_8","alias_value":"OBHUJ45L","created_at":"2026-05-18T12:27:54.935989+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":4,"internal_anchor_count":3,"sample":[{"citing_arxiv_id":"2401.00933","citing_title":"Detection of polarized Fermi-bubble synchrotron and dust emission","ref_index":19,"is_internal_anchor":true},{"citing_arxiv_id":"2605.20186","citing_title":"WIMP-like Dark Matter Without Thermalization At Freeze-Out","ref_index":57,"is_internal_anchor":true},{"citing_arxiv_id":"2509.08043","citing_title":"Testing Viability of Benchmark Dark Matter Models for the Galactic Center Excess","ref_index":2,"is_internal_anchor":true},{"citing_arxiv_id":"2605.08010","citing_title":"Producing the GeV Galactic Center Excess via Cosmic Ray-Dark Matter Scattering","ref_index":9,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/OBHUJ45LYJX3H7XKC5EH6TYDZX","json":"https://pith.science/pith/OBHUJ45LYJX3H7XKC5EH6TYDZX.json","graph_json":"https://pith.science/api/pith-number/OBHUJ45LYJX3H7XKC5EH6TYDZX/graph.json","events_json":"https://pith.science/api/pith-number/OBHUJ45LYJX3H7XKC5EH6TYDZX/events.json","paper":"https://pith.science/paper/OBHUJ45L"},"agent_actions":{"view_html":"https://pith.science/pith/OBHUJ45LYJX3H7XKC5EH6TYDZX","download_json":"https://pith.science/pith/OBHUJ45LYJX3H7XKC5EH6TYDZX.json","view_paper":"https://pith.science/paper/OBHUJ45L","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1302.6589&json=true","fetch_graph":"https://pith.science/api/pith-number/OBHUJ45LYJX3H7XKC5EH6TYDZX/graph.json","fetch_events":"https://pith.science/api/pith-number/OBHUJ45LYJX3H7XKC5EH6TYDZX/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/OBHUJ45LYJX3H7XKC5EH6TYDZX/action/timestamp_anchor","attest_storage":"https://pith.science/pith/OBHUJ45LYJX3H7XKC5EH6TYDZX/action/storage_attestation","attest_author":"https://pith.science/pith/OBHUJ45LYJX3H7XKC5EH6TYDZX/action/author_attestation","sign_citation":"https://pith.science/pith/OBHUJ45LYJX3H7XKC5EH6TYDZX/action/citation_signature","submit_replication":"https://pith.science/pith/OBHUJ45LYJX3H7XKC5EH6TYDZX/action/replication_record"}},"created_at":"2026-05-18T03:32:19.372931+00:00","updated_at":"2026-05-18T03:32:19.372931+00:00"}