{"as_of":"2026-08-10T23:19:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:7b4c6b5c36951f0cb1f01da39fbc802f494798187a61fe318b421add3e346a71","coverage":[{"denominator":0,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":22,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":22,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-10T06:31:04.303077+00:00","state":"measured"},{"denominator":22,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":22,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-10T21:10:13.841712Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"pith","source_observed_at":"2026-07-07T22:14:11.724134Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1711.06223","last_updated":"2017-11-16T18:05:58Z","snapshot_observed_at":"2026-07-06T06:09:53.105661Z","submitted_at":"2017-11-16T18:05:58Z","title":"Extended gamma-ray sources around pulsars constrain the origin of the positron flux at Earth","version":1},"cited_work":{"arxiv_id":"1711.06223","doi":null,"metadata_source":"pith","pith_arxiv_id":"1711.06223","snapshot_observed_at":"2026-07-07T22:14:11.724134Z","title":"Extended gamma-ray sources around pulsars constrain the origin of the positron flux at Earth","venue":"astro-ph.HE","work_id":"b520aeb4-1f31-495b-958d-05007de45598","year":2017},"citing_paper":{"arxiv_id":"1907.07737","last_updated":"2019-07-17T20:04:01Z","snapshot_observed_at":"2026-07-06T08:08:26.408229Z","submitted_at":"2019-07-17T20:04:01Z","title":"The Southern Wide-Field Gamma-Ray Observatory (SWGO): A Next-Generation Ground-Based Survey Instrument for VHE Gamma-Ray Astronomy","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1711.06223","citing_paper":"/paper/1907.07737"},"observation_digest":"sha256:8bbbcf524474cae91e8290ab88681553b0e1feefc61e2d20d15c0d9093c069cc","observation_id":"e316b8d2-f0d7-49e9-82ba-1a01c477c30b","resolution":{"observed_at":"2026-05-24T19:54:52.682340Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1711.06223","last_updated":"2017-11-16T18:05:58Z","snapshot_observed_at":"2026-07-06T06:09:53.105661Z","submitted_at":"2017-11-16T18:05:58Z","title":"Extended gamma-ray sources around pulsars constrain the origin of the positron flux at Earth","version":1},"cited_work":{"arxiv_id":"1711.06223","doi":null,"metadata_source":"pith","pith_arxiv_id":"1711.06223","snapshot_observed_at":"2026-07-07T22:14:11.724134Z","title":"Extended gamma-ray sources around pulsars constrain the origin of the positron flux at Earth","venue":"astro-ph.HE","work_id":"b520aeb4-1f31-495b-958d-05007de45598","year":2017},"citing_paper":{"arxiv_id":"2310.16594","last_updated":"2024-02-18T06:24:01Z","snapshot_observed_at":"2026-08-10T03:18:26.081433Z","submitted_at":"2023-10-25T12:32:33Z","title":"Constraining the slow-diffusion zone size and electron injection spectral index for the Geminga pulsar halo","version":2},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-05-24T06:48:57.946124Z"},"links":{"cited_paper":"/paper/1711.06223","citing_paper":"/paper/2310.16594"},"observation_digest":"sha256:8aee15d98462a9547a58b21ec9eb07535c273f14bfc18fa1f4eb924e62b419ae","observation_id":"7f2cbd3d-8a4b-452f-853d-43e29f42c074","resolution":{"observed_at":"2026-05-24T06:49:01.944336Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1711.06223","last_updated":"2017-11-16T18:05:58Z","snapshot_observed_at":"2026-07-06T06:09:53.105661Z","submitted_at":"2017-11-16T18:05:58Z","title":"Extended gamma-ray sources around pulsars constrain the origin of the positron flux at Earth","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1711.06223","snapshot_observed_at":"2026-08-10T21:10:13.841712Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2501.06011","last_updated":"2025-07-01T11:50:03Z","snapshot_observed_at":"2026-08-10T21:03:52.464819Z","submitted_at":"2025-01-10T14:48:22Z","title":"SECRET: Stochasticity Emulator for Cosmic Ray Electrons","version":2},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-10T21:10:13.841712Z"},"links":{"cited_paper":"/paper/1711.06223","citing_paper":"/paper/2501.06011"},"observation_digest":"sha256:23b3d625588ea2434a2cff5eabdc2e8a603c835d3b014a8e01e1569e17db31b6","observation_id":"6d6bd7b8-3297-4d88-b6df-e5cebe2d9bd9","resolution":{"observed_at":"2026-08-10T21:10:13.841712Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1711.06223","last_updated":"2017-11-16T18:05:58Z","snapshot_observed_at":"2026-07-06T06:09:53.105661Z","submitted_at":"2017-11-16T18:05:58Z","title":"Extended gamma-ray sources around pulsars constrain the origin of the positron flux at Earth","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1711.06223","snapshot_observed_at":"2026-08-10T19:48:57.578347Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2501.09789","last_updated":"2025-01-16T19:00:01Z","snapshot_observed_at":"2026-08-10T19:37:36.554520Z","submitted_at":"2025-01-16T19:00:01Z","title":"Detecting dark matter sub-halos in the Galactic plane with the Cherenkov Telescope Array Observatory","version":1},"reference_index":121,"source":"pdf_text","source_observed_at":"2026-08-10T19:48:57.578347Z"},"links":{"cited_paper":"/paper/1711.06223","citing_paper":"/paper/2501.09789"},"observation_digest":"sha256:c90c550fa4d61ac75a38cf1b0f710c4e4f312d36bfd899598221190d2f4ae824","observation_id":"e64f172c-abdf-4dbe-ac86-3a208904ab10","resolution":{"observed_at":"2026-08-10T19:48:57.578347Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1711.06223","last_updated":"2017-11-16T18:05:58Z","snapshot_observed_at":"2026-07-06T06:09:53.105661Z","submitted_at":"2017-11-16T18:05:58Z","title":"Extended gamma-ray sources around pulsars constrain the origin of the positron flux at Earth","version":1},"cited_work":{"arxiv_id":"1711.06223","doi":null,"metadata_source":"pith","pith_arxiv_id":"1711.06223","snapshot_observed_at":"2026-07-07T22:14:11.724134Z","title":"Extended gamma-ray sources around pulsars constrain the origin of the positron flux at Earth","venue":"astro-ph.HE","work_id":"b520aeb4-1f31-495b-958d-05007de45598","year":2017},"citing_paper":{"arxiv_id":"2503.15052","last_updated":"2025-03-26T03:58:42Z","snapshot_observed_at":"2026-07-06T20:55:13.966734Z","submitted_at":"2025-03-19T09:42:32Z","title":"Discrete treatment of inverse Compton scattering: implications on parameter estimation in gamma-ray astronomy","version":3},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:06.367210Z"},"links":{"cited_paper":"/paper/1711.06223","citing_paper":"/paper/2503.15052"},"observation_digest":"sha256:9ac0fd841269656610b82f66977f5118bcbc6ad46e046118cc46053302033477","observation_id":"8d212571-80e4-4216-946a-8afefd4c3516","resolution":{"observed_at":"2026-05-23T00:02:17.615900Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1711.06223","last_updated":"2017-11-16T18:05:58Z","snapshot_observed_at":"2026-07-06T06:09:53.105661Z","submitted_at":"2017-11-16T18:05:58Z","title":"Extended gamma-ray sources around pulsars constrain the origin of the positron flux at Earth","version":1},"cited_work":{"arxiv_id":"1711.06223","doi":null,"metadata_source":"pith","pith_arxiv_id":"1711.06223","snapshot_observed_at":"2026-07-07T22:14:11.724134Z","title":"Extended gamma-ray sources around pulsars constrain the origin of the positron flux at Earth","venue":"astro-ph.HE","work_id":"b520aeb4-1f31-495b-958d-05007de45598","year":2017},"citing_paper":{"arxiv_id":"2508.13667","last_updated":"2026-01-30T10:45:06Z","snapshot_observed_at":"2026-08-01T22:15:27.110326Z","submitted_at":"2025-08-19T09:15:39Z","title":"PHECT: A lightweight computation tool for pulsar halo emission","version":2},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-05-18T23:02:15.483780Z"},"links":{"cited_paper":"/paper/1711.06223","citing_paper":"/paper/2508.13667"},"observation_digest":"sha256:371d06d2e9700a17ee59dec11cf7832894faf7b6c29a453013883da3f96e044f","observation_id":"e4882ba3-23a1-411d-8d5f-f608dc31f90a","resolution":{"observed_at":"2026-05-18T23:02:52.534728Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1711.06223","last_updated":"2017-11-16T18:05:58Z","snapshot_observed_at":"2026-07-06T06:09:53.105661Z","submitted_at":"2017-11-16T18:05:58Z","title":"Extended gamma-ray sources around pulsars constrain the origin of the positron flux at Earth","version":1},"cited_work":{"arxiv_id":"1711.06223","doi":null,"metadata_source":"pith","pith_arxiv_id":"1711.06223","snapshot_observed_at":"2026-07-07T22:14:11.724134Z","title":"Extended gamma-ray sources around pulsars constrain the origin of the positron flux at Earth","venue":"astro-ph.HE","work_id":"b520aeb4-1f31-495b-958d-05007de45598","year":2017},"citing_paper":{"arxiv_id":"2511.05409","last_updated":"2026-04-30T09:12:05Z","snapshot_observed_at":"2026-07-06T22:35:13.699594Z","submitted_at":"2025-11-07T16:34:51Z","title":"Charge-dependent spectral softenings of primary cosmic-rays below the knee","version":3},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-05-17T23:49:55.132150Z"},"links":{"cited_paper":"/paper/1711.06223","citing_paper":"/paper/2511.05409"},"observation_digest":"sha256:6cd0686ae8a182534c85d9ada6ecbf9e883cb1dfe2d018d2d1f11a2e49b26fa7","observation_id":"d730ebc2-a797-42bb-aeea-842027e31444","resolution":{"observed_at":"2026-05-17T23:50:31.166570Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1711.06223","last_updated":"2017-11-16T18:05:58Z","snapshot_observed_at":"2026-07-06T06:09:53.105661Z","submitted_at":"2017-11-16T18:05:58Z","title":"Extended gamma-ray sources around pulsars constrain the origin of the positron flux at Earth","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1711.06223","snapshot_observed_at":"2026-08-03T23:17:48.626302Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2511.06733","last_updated":"2026-05-27T08:49:14Z","snapshot_observed_at":"2026-08-06T07:12:48.459744Z","submitted_at":"2025-11-10T05:54:49Z","title":"Implication of multiple source populations of Galactic cosmic rays from proton and helium spectra","version":2},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-03T23:17:48.626302Z"},"links":{"cited_paper":"/paper/1711.06223","citing_paper":"/paper/2511.06733"},"observation_digest":"sha256:c96dd324ca6e759d1999389fb5e8dbd147c5e15a520ed32c081e86fc42271a63","observation_id":"b839f492-27f2-493a-a41a-98af93e9d331","resolution":{"observed_at":"2026-08-03T23:17:48.626302Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1711.06223","last_updated":"2017-11-16T18:05:58Z","snapshot_observed_at":"2026-07-06T06:09:53.105661Z","submitted_at":"2017-11-16T18:05:58Z","title":"Extended gamma-ray sources around pulsars constrain the origin of the positron flux at Earth","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1711.06223","snapshot_observed_at":"2026-08-03T15:48:49.866182Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2512.15847","last_updated":"2026-07-16T18:13:20Z","snapshot_observed_at":"2026-08-10T10:46:59.686678Z","submitted_at":"2025-12-17T19:00:00Z","title":"Self-confinement of relativistic pair beams in magnetized interstellar plasmas: the case of pulsar X-ray filaments","version":2},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-03T15:48:49.866182Z"},"links":{"cited_paper":"/paper/1711.06223","citing_paper":"/paper/2512.15847"},"observation_digest":"sha256:5bad4eae49e3b5fd2a608f91fee31e440c8a4bbfde13ef7f99794776bacd0a9a","observation_id":"a695279e-2e2a-4e8b-956f-71b6330517cf","resolution":{"observed_at":"2026-08-03T15:48:49.866182Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1711.06223","last_updated":"2017-11-16T18:05:58Z","snapshot_observed_at":"2026-07-06T06:09:53.105661Z","submitted_at":"2017-11-16T18:05:58Z","title":"Extended gamma-ray sources around pulsars constrain the origin of the positron flux at Earth","version":1},"cited_work":{"arxiv_id":"1711.06223","doi":null,"metadata_source":"pith","pith_arxiv_id":"1711.06223","snapshot_observed_at":"2026-07-07T22:14:11.724134Z","title":"Extended gamma-ray sources around pulsars constrain the origin of the positron flux at Earth","venue":"astro-ph.HE","work_id":"b520aeb4-1f31-495b-958d-05007de45598","year":2017},"citing_paper":{"arxiv_id":"2603.04821","last_updated":"2026-05-20T14:32:07Z","snapshot_observed_at":"2026-08-02T08:55:25.021269Z","submitted_at":"2026-03-05T05:12:25Z","title":"Resolving diffusion signatures in distant pulsar halos with current and future experiments","version":2},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-05-21T12:11:58.523346Z"},"links":{"cited_paper":"/paper/1711.06223","citing_paper":"/paper/2603.04821"},"observation_digest":"sha256:546398779d2c79bb060bc659e1373d45ea3b03b86ec292203fa7dbc7bb95e332","observation_id":"a38001d1-e8d3-40a0-a5d8-32ca7d4e184d","resolution":{"observed_at":"2026-05-21T12:14:11.720039Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1711.06223","last_updated":"2017-11-16T18:05:58Z","snapshot_observed_at":"2026-07-06T06:09:53.105661Z","submitted_at":"2017-11-16T18:05:58Z","title":"Extended gamma-ray sources around pulsars constrain the origin of the positron flux at Earth","version":1},"cited_work":{"arxiv_id":"1711.06223","doi":null,"metadata_source":"pith","pith_arxiv_id":"1711.06223","snapshot_observed_at":"2026-07-07T22:14:11.724134Z","title":"Extended gamma-ray sources around pulsars constrain the origin of the positron flux at Earth","venue":"astro-ph.HE","work_id":"b520aeb4-1f31-495b-958d-05007de45598","year":2017},"citing_paper":{"arxiv_id":"2603.28528","last_updated":"2026-03-30T14:53:58Z","snapshot_observed_at":"2026-07-06T22:51:05.074191Z","submitted_at":"2026-03-30T14:53:58Z","title":"Search for TeV emission from spider millisecond pulsars with HAWC","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-05-14T01:22:04.712990Z"},"links":{"cited_paper":"/paper/1711.06223","citing_paper":"/paper/2603.28528"},"observation_digest":"sha256:762dcc5e1fc8afa0d312afde4765bd4de527bc1b8376917c094cc5f2a28ffd66","observation_id":"6f709017-4141-46ca-a532-25ac3b7bdc72","resolution":{"observed_at":"2026-05-14T01:23:34.675858Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1711.06223","last_updated":"2017-11-16T18:05:58Z","snapshot_observed_at":"2026-07-06T06:09:53.105661Z","submitted_at":"2017-11-16T18:05:58Z","title":"Extended gamma-ray sources around pulsars constrain the origin of the positron flux at Earth","version":1},"cited_work":{"arxiv_id":"1711.06223","doi":null,"metadata_source":"pith","pith_arxiv_id":"1711.06223","snapshot_observed_at":"2026-07-07T22:14:11.724134Z","title":"Extended gamma-ray sources around pulsars constrain the origin of the positron flux at Earth","venue":"astro-ph.HE","work_id":"b520aeb4-1f31-495b-958d-05007de45598","year":2017},"citing_paper":{"arxiv_id":"2604.15537","last_updated":"2026-04-16T21:34:54Z","snapshot_observed_at":"2026-07-06T23:03:02.938732Z","submitted_at":"2026-04-16T21:34:54Z","title":"On the contribution of the bow shock pulsar wind nebula PSR J0437-4715 to the observed fluxes of GeV-TeV positrons and antiprotons","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-05-10T09:41:35.845413Z"},"links":{"cited_paper":"/paper/1711.06223","citing_paper":"/paper/2604.15537"},"observation_digest":"sha256:df67e7332c28c1106d1b79c10fc6e592e0944da468672d7d6b837517c8e57f5e","observation_id":"c866f6d5-056d-40df-8f40-1ce77b394516","resolution":{"observed_at":"2026-05-10T09:43:49.022923Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1711.06223","last_updated":"2017-11-16T18:05:58Z","snapshot_observed_at":"2026-07-06T06:09:53.105661Z","submitted_at":"2017-11-16T18:05:58Z","title":"Extended gamma-ray sources around pulsars constrain the origin of the positron flux at Earth","version":1},"cited_work":{"arxiv_id":"1711.06223","doi":null,"metadata_source":"pith","pith_arxiv_id":"1711.06223","snapshot_observed_at":"2026-07-07T22:14:11.724134Z","title":"Extended gamma-ray sources around pulsars constrain the origin of the positron flux at Earth","venue":"astro-ph.HE","work_id":"b520aeb4-1f31-495b-958d-05007de45598","year":2017},"citing_paper":{"arxiv_id":"2605.17636","last_updated":"2026-05-17T20:07:07Z","snapshot_observed_at":"2026-08-05T22:35:13.903215Z","submitted_at":"2026-05-17T20:07:07Z","title":"Diffuse gamma-ray emission in the vicinity of open cluster Berkeley 87","version":1},"reference_index":84,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1711.06223","citing_paper":"/paper/2605.17636"},"observation_digest":"sha256:2b079f9ea5dca4c0288011221463afaffcb950176d57835621b9a98bd4d5aa1e","observation_id":"2203c40b-2ceb-4b3b-b70c-6e6c01b6f093","resolution":{"observed_at":"2026-05-19T22:17:49.109502Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1711.06223","last_updated":"2017-11-16T18:05:58Z","snapshot_observed_at":"2026-07-06T06:09:53.105661Z","submitted_at":"2017-11-16T18:05:58Z","title":"Extended gamma-ray sources around pulsars constrain the origin of the positron flux at Earth","version":1},"cited_work":{"arxiv_id":"1711.06223","doi":null,"metadata_source":"pith","pith_arxiv_id":"1711.06223","snapshot_observed_at":"2026-07-07T22:14:11.724134Z","title":"Extended gamma-ray sources around pulsars constrain the origin of the positron flux at Earth","venue":"astro-ph.HE","work_id":"b520aeb4-1f31-495b-958d-05007de45598","year":2017},"citing_paper":{"arxiv_id":"2605.18122","last_updated":"2026-05-18T09:29:09Z","snapshot_observed_at":"2026-08-02T16:13:58.000124Z","submitted_at":"2026-05-18T09:29:09Z","title":"Spectral energy-loss bump and $\\gamma$-ray pulsar halos","version":1},"reference_index":2,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1711.06223","citing_paper":"/paper/2605.18122"},"observation_digest":"sha256:57888a02050065a4990ddc54f405f185429a36a84104abdb8117e632aac4e08c","observation_id":"3eac4249-b655-4f65-b053-582c3d3f2a47","resolution":{"observed_at":"2026-05-20T09:13:09.600735Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1711.06223","last_updated":"2017-11-16T18:05:58Z","snapshot_observed_at":"2026-07-06T06:09:53.105661Z","submitted_at":"2017-11-16T18:05:58Z","title":"Extended gamma-ray sources around pulsars constrain the origin of the positron flux at Earth","version":1},"cited_work":{"arxiv_id":"1711.06223","doi":null,"metadata_source":"pith","pith_arxiv_id":"1711.06223","snapshot_observed_at":"2026-07-07T22:14:11.724134Z","title":"Extended gamma-ray sources around pulsars constrain the origin of the positron flux at Earth","venue":"astro-ph.HE","work_id":"b520aeb4-1f31-495b-958d-05007de45598","year":2017},"citing_paper":{"arxiv_id":"2606.17690","last_updated":"2026-06-26T11:50:42Z","snapshot_observed_at":"2026-08-02T22:36:40.221535Z","submitted_at":"2026-06-16T09:00:21Z","title":"A catalogue of TeV pulsar environments","version":1},"reference_index":75,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1711.06223","citing_paper":"/paper/2606.17690"},"observation_digest":"sha256:9cca59292dc50cd883d0fad482f598d5e34998d5e279febd96dcec6458760640","observation_id":"86c9a1cf-ab05-4996-89fa-fc36ba501298","resolution":{"observed_at":"2026-06-26T23:50:15.336488Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1711.06223","last_updated":"2017-11-16T18:05:58Z","snapshot_observed_at":"2026-07-06T06:09:53.105661Z","submitted_at":"2017-11-16T18:05:58Z","title":"Extended gamma-ray sources around pulsars constrain the origin of the positron flux at Earth","version":1},"cited_work":{"arxiv_id":"1711.06223","doi":null,"metadata_source":"pith","pith_arxiv_id":"1711.06223","snapshot_observed_at":"2026-07-07T22:14:11.724134Z","title":"Extended gamma-ray sources around pulsars constrain the origin of the positron flux at Earth","venue":"astro-ph.HE","work_id":"b520aeb4-1f31-495b-958d-05007de45598","year":2017},"citing_paper":{"arxiv_id":"2606.17690","last_updated":"2026-06-26T11:50:42Z","snapshot_observed_at":"2026-08-02T22:36:40.221535Z","submitted_at":"2026-06-16T09:00:21Z","title":"A catalogue of TeV pulsar environments","version":2},"reference_index":75,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1711.06223","citing_paper":"/paper/2606.17690"},"observation_digest":"sha256:661fa3a9316d3bc5e8317ad4c98d1caba40cc80977b7e010e1ccdee110915c3d","observation_id":"6bb0f220-2a61-4f37-bd6f-c063def9d751","resolution":{"observed_at":"2026-06-29T05:23:07.459375Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1711.06223","last_updated":"2017-11-16T18:05:58Z","snapshot_observed_at":"2026-07-06T06:09:53.105661Z","submitted_at":"2017-11-16T18:05:58Z","title":"Extended gamma-ray sources around pulsars constrain the origin of the positron flux at Earth","version":1},"cited_work":{"arxiv_id":"1711.06223","doi":null,"metadata_source":"pith","pith_arxiv_id":"1711.06223","snapshot_observed_at":"2026-07-07T22:14:11.724134Z","title":"Extended gamma-ray sources around pulsars constrain the origin of the positron flux at Earth","venue":"astro-ph.HE","work_id":"b520aeb4-1f31-495b-958d-05007de45598","year":2017},"citing_paper":{"arxiv_id":"2606.19701","last_updated":"2026-06-18T01:52:52Z","snapshot_observed_at":"2026-08-02T20:38:02.898818Z","submitted_at":"2026-06-18T01:52:52Z","title":"On the Contribution of Local Sources to the Galactic Cosmic-Ray Spectrum: An Exact Series Solution for Two-Zone Diffusion","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-06-26T16:43:02.409335Z"},"links":{"cited_paper":"/paper/1711.06223","citing_paper":"/paper/2606.19701"},"observation_digest":"sha256:232553b4b183f0e8e6ad3bf086104d2bbac0b05c95edcf09fd7dc92276702b68","observation_id":"73656088-1850-4480-bdf5-07bbb8475d4d","resolution":{"observed_at":"2026-07-04T04:49:35.783814Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1711.06223","last_updated":"2017-11-16T18:05:58Z","snapshot_observed_at":"2026-07-06T06:09:53.105661Z","submitted_at":"2017-11-16T18:05:58Z","title":"Extended gamma-ray sources around pulsars constrain the origin of the positron flux at Earth","version":1},"cited_work":{"arxiv_id":"1711.06223","doi":null,"metadata_source":"pith","pith_arxiv_id":"1711.06223","snapshot_observed_at":"2026-07-07T22:14:11.724134Z","title":"Extended gamma-ray sources around pulsars constrain the origin of the positron flux at Earth","venue":"astro-ph.HE","work_id":"b520aeb4-1f31-495b-958d-05007de45598","year":2017},"citing_paper":{"arxiv_id":"2606.23476","last_updated":"2026-06-22T15:22:06Z","snapshot_observed_at":"2026-08-02T21:35:47.442014Z","submitted_at":"2026-06-22T15:22:06Z","title":"TeV-PeV Gamma-ray and Neutrino Emission in the Galactic Plane","version":1},"reference_index":175,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1711.06223","citing_paper":"/paper/2606.23476"},"observation_digest":"sha256:77ff65f21fc11d8ae616af548124bcd96e5bb8450e4b0243fd893a0de47b59e9","observation_id":"06a9742b-8842-4c1b-8c09-c60499ad5775","resolution":{"observed_at":"2026-06-26T07:29:08.280443Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1711.06223","last_updated":"2017-11-16T18:05:58Z","snapshot_observed_at":"2026-07-06T06:09:53.105661Z","submitted_at":"2017-11-16T18:05:58Z","title":"Extended gamma-ray sources around pulsars constrain the origin of the positron flux at Earth","version":1},"cited_work":{"arxiv_id":"1711.06223","doi":null,"metadata_source":"pith","pith_arxiv_id":"1711.06223","snapshot_observed_at":"2026-07-07T22:14:11.724134Z","title":"Extended gamma-ray sources around pulsars constrain the origin of the positron flux at Earth","venue":"astro-ph.HE","work_id":"b520aeb4-1f31-495b-958d-05007de45598","year":2017},"citing_paper":{"arxiv_id":"2606.25077","last_updated":"2026-06-23T18:35:44Z","snapshot_observed_at":"2026-08-08T14:52:38.897535Z","submitted_at":"2026-06-23T18:35:44Z","title":"Small-scale Magnetic Fields in the Milky Way and Nearby Galaxies","version":1},"reference_index":11,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1711.06223","citing_paper":"/paper/2606.25077"},"observation_digest":"sha256:a43f1223d06d5cf67d25ab614c66ba386aa84030d6ddb994a94adcd9303345ac","observation_id":"7186db00-55ab-4e5a-bb8a-0c72534882f6","resolution":{"observed_at":"2026-06-26T00:48:45.379662Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1711.06223","last_updated":"2017-11-16T18:05:58Z","snapshot_observed_at":"2026-07-06T06:09:53.105661Z","submitted_at":"2017-11-16T18:05:58Z","title":"Extended gamma-ray sources around pulsars constrain the origin of the positron flux at Earth","version":1},"cited_work":{"arxiv_id":"1711.06223","doi":null,"metadata_source":"pith","pith_arxiv_id":"1711.06223","snapshot_observed_at":"2026-07-07T22:14:11.724134Z","title":"Extended gamma-ray sources around pulsars constrain the origin of the positron flux at Earth","venue":"astro-ph.HE","work_id":"b520aeb4-1f31-495b-958d-05007de45598","year":2017},"citing_paper":{"arxiv_id":"2606.26597","last_updated":"2026-06-25T04:53:51Z","snapshot_observed_at":"2026-07-30T03:43:17.560575Z","submitted_at":"2026-06-25T04:53:51Z","title":"A Boundary-Consistent Two-Zone Electron Kernel for Distant Pulsar Contributions to Positron Flux and Anisotropy","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-06-26T04:33:12.240034Z"},"links":{"cited_paper":"/paper/1711.06223","citing_paper":"/paper/2606.26597"},"observation_digest":"sha256:bf58fe86e53bac2ff8fa2a8b402f3d22e1519a63175a221bae8c958949a2ce13","observation_id":"478204ba-7963-46c1-a05d-4795b5418bbf","resolution":{"observed_at":"2026-07-04T14:09:52.785132Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1711.06223","last_updated":"2017-11-16T18:05:58Z","snapshot_observed_at":"2026-07-06T06:09:53.105661Z","submitted_at":"2017-11-16T18:05:58Z","title":"Extended gamma-ray sources around pulsars constrain the origin of the positron flux at Earth","version":1},"cited_work":{"arxiv_id":"1711.06223","doi":null,"metadata_source":"pith","pith_arxiv_id":"1711.06223","snapshot_observed_at":"2026-07-07T22:14:11.724134Z","title":"Extended gamma-ray sources around pulsars constrain the origin of the positron flux at Earth","venue":"astro-ph.HE","work_id":"b520aeb4-1f31-495b-958d-05007de45598","year":2017},"citing_paper":{"arxiv_id":"2607.00042","last_updated":"2026-06-29T17:25:56Z","snapshot_observed_at":"2026-08-02T13:28:22.137868Z","submitted_at":"2026-06-29T17:25:56Z","title":"Understanding Pulsar Wind Nebulae with the SKA","version":1},"reference_index":4,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1711.06223","citing_paper":"/paper/2607.00042"},"observation_digest":"sha256:b59f80b8af9e6ee60149609602dda93a17ef825f14233647d3f7d847a45b6986","observation_id":"8abca6c8-8bc2-487d-8739-afcd05b0001d","resolution":{"observed_at":"2026-07-02T20:37:21.960036Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1711.06223","last_updated":"2017-11-16T18:05:58Z","snapshot_observed_at":"2026-07-06T06:09:53.105661Z","submitted_at":"2017-11-16T18:05:58Z","title":"Extended gamma-ray sources around pulsars constrain the origin of the positron flux at Earth","version":1},"cited_work":{"arxiv_id":"1711.06223","doi":null,"metadata_source":"pith","pith_arxiv_id":"1711.06223","snapshot_observed_at":"2026-07-07T22:14:11.724134Z","title":"Extended gamma-ray sources around pulsars constrain the origin of the positron flux at Earth","venue":"astro-ph.HE","work_id":"b520aeb4-1f31-495b-958d-05007de45598","year":2017},"citing_paper":{"arxiv_id":"2607.05245","last_updated":"2026-07-06T15:55:09Z","snapshot_observed_at":"2026-08-07T02:18:45.404914Z","submitted_at":"2026-07-06T15:55:09Z","title":"Geminga and Monogem in the CTAO Era: Probing TeV Halos and Cosmic-Ray Transport","version":1},"reference_index":1,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1711.06223","citing_paper":"/paper/2607.05245"},"observation_digest":"sha256:6592731c5850c3f594e165cd9e11e3f6f8fb083c708ab3b021665ec4208172c5","observation_id":"dcf5e101-54d1-4268-8a21-cd63d7cf246b","resolution":{"observed_at":"2026-07-07T22:14:11.727520Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/1711.06223/citation-record","integrity":"/paper/1711.06223/integrity","json":"/paper/1711.06223/citation-record.json","paper":"/paper/1711.06223"},"outbound":[],"paper":{"arxiv_id":"1711.06223","last_updated":"2017-11-16T18:05:58Z","latest_version":1,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-07-06T06:09:53.105661Z","submitted_at":"2017-11-16T18:05:58Z","title":"Extended gamma-ray sources around pulsars constrain the origin of the positron flux at Earth"},"reference_resolution":{"displayed":0,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":0,"verified_exact":0,"verified_fuzzy":0},"total_outbound_references":0},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"thesis":"As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 22 inbound Pith citation observations for arXiv:1711.06223."}