{"as_of":"2026-08-05T02:05:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:7f0b12b055d89e6718c86190ee6347ed80159e2ab644f1dd76b170c965949124","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":14,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":14,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-04T06:34:03.388597+00:00","state":"measured"},{"denominator":14,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":14,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-03T14:43:18.441055Z","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":"2026-07-04T18:10:02.072633Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1203.2681","last_updated":"2012-03-13T00:38:22Z","snapshot_observed_at":"2026-07-06T02:44:27.243716Z","submitted_at":"2012-03-13T00:38:22Z","title":"Probing the inflaton: Small-scale power spectrum constraints from measurements of the CMB energy spectrum","version":1},"cited_work":{"arxiv_id":"1203.2681","doi":null,"metadata_source":"pith","pith_arxiv_id":"1203.2681","snapshot_observed_at":"2026-07-04T18:10:02.072633Z","title":"Probing the inflaton: Small-scale power spectrum constraints from measurements of the CMB energy spectrum","venue":"astro-ph.CO","work_id":"25ff89f1-1feb-4dd2-877d-0cdc2f9b14f6","year":2012},"citing_paper":{"arxiv_id":"2006.02838","last_updated":"2020-09-04T22:52:13Z","snapshot_observed_at":"2026-07-06T09:26:02.034486Z","submitted_at":"2020-06-03T17:57:28Z","title":"Primordial Black Holes as Dark Matter: Recent Developments","version":3},"reference_index":212,"source":"pdf_text","source_observed_at":"2026-05-16T12:15:12.881226Z"},"links":{"cited_paper":"/paper/1203.2681","citing_paper":"/paper/2006.02838"},"observation_digest":"sha256:71a300539e567beaf15a837e1cf7b27943e782d6a7ef3480116e79688aa4e2f5","observation_id":"8519d953-00f4-41a8-966c-768be8817267","resolution":{"observed_at":"2026-05-16T12:15:12.996576Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1203.2681","last_updated":"2012-03-13T00:38:22Z","snapshot_observed_at":"2026-07-06T02:44:27.243716Z","submitted_at":"2012-03-13T00:38:22Z","title":"Probing the inflaton: Small-scale power spectrum constraints from measurements of the CMB energy spectrum","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1203.2681","snapshot_observed_at":"2026-08-03T14:43:18.441055Z","title":"Chluba, A.L","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2512.19668","last_updated":"2026-06-01T10:28:28Z","snapshot_observed_at":"2026-08-03T14:43:14.081141Z","submitted_at":"2025-12-22T18:48:00Z","title":"Are Primordial Black Holes Truly Fine-Tuned?","version":2},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-03T14:43:18.441055Z"},"links":{"cited_paper":"/paper/1203.2681","citing_paper":"/paper/2512.19668"},"observation_digest":"sha256:e7d36fbc2e280f3e85a7dc75766bca6795f4e46dea381d2953f3726406cdc477","observation_id":"f4787776-b5a4-4b68-b900-4fa84b61b49f","resolution":{"observed_at":"2026-08-03T14:43:18.441055Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1203.2681","last_updated":"2012-03-13T00:38:22Z","snapshot_observed_at":"2026-07-06T02:44:27.243716Z","submitted_at":"2012-03-13T00:38:22Z","title":"Probing the inflaton: Small-scale power spectrum constraints from measurements of the CMB energy spectrum","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1203.2681","snapshot_observed_at":"2026-08-03T09:17:08.598834Z","title":"Chluba, A","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2601.14412","last_updated":"2026-07-03T09:56:53Z","snapshot_observed_at":"2026-08-04T01:33:57.911334Z","submitted_at":"2026-01-20T19:16:41Z","title":"How large are curvature perturbations from slow first-order phase transitions? A gauge-invariant analysis","version":2},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-03T09:17:08.598834Z"},"links":{"cited_paper":"/paper/1203.2681","citing_paper":"/paper/2601.14412"},"observation_digest":"sha256:f4c859bf1e3b6a19572cc0c91d5612b707bd9a50a7d815c26a07ab443f66be02","observation_id":"705f5da9-109f-4ed5-b08b-6ce62eca3fbb","resolution":{"observed_at":"2026-08-03T09:17:08.598834Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1203.2681","last_updated":"2012-03-13T00:38:22Z","snapshot_observed_at":"2026-07-06T02:44:27.243716Z","submitted_at":"2012-03-13T00:38:22Z","title":"Probing the inflaton: Small-scale power spectrum constraints from measurements of the CMB energy spectrum","version":1},"cited_work":{"arxiv_id":"1203.2681","doi":null,"metadata_source":"pith","pith_arxiv_id":"1203.2681","snapshot_observed_at":"2026-07-04T18:10:02.072633Z","title":"Probing the inflaton: Small-scale power spectrum constraints from measurements of the CMB energy spectrum","venue":"astro-ph.CO","work_id":"25ff89f1-1feb-4dd2-877d-0cdc2f9b14f6","year":2012},"citing_paper":{"arxiv_id":"2605.11956","last_updated":"2026-05-12T11:08:00Z","snapshot_observed_at":"2026-07-06T23:23:44.276236Z","submitted_at":"2026-05-12T11:08:00Z","title":"Probing the small-scale primordial power spectrum via relic neutrinos and acoustic reheating","version":1},"reference_index":90,"source":"pdf_text","source_observed_at":"2026-05-13T05:32:39.605539Z"},"links":{"cited_paper":"/paper/1203.2681","citing_paper":"/paper/2605.11956"},"observation_digest":"sha256:c9c88b81780956d7e43bd55b96cb2bbe599cda23f80767cc14bf937b46482980","observation_id":"747c0fdf-a210-4a9d-a028-1a1107b3ea79","resolution":{"observed_at":"2026-05-13T05:37:19.401385Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1203.2681","last_updated":"2012-03-13T00:38:22Z","snapshot_observed_at":"2026-07-06T02:44:27.243716Z","submitted_at":"2012-03-13T00:38:22Z","title":"Probing the inflaton: Small-scale power spectrum constraints from measurements of the CMB energy spectrum","version":1},"cited_work":{"arxiv_id":"1203.2681","doi":null,"metadata_source":"pith","pith_arxiv_id":"1203.2681","snapshot_observed_at":"2026-07-04T18:10:02.072633Z","title":"Probing the inflaton: Small-scale power spectrum constraints from measurements of the CMB energy spectrum","venue":"astro-ph.CO","work_id":"25ff89f1-1feb-4dd2-877d-0cdc2f9b14f6","year":2012},"citing_paper":{"arxiv_id":"2605.15197","last_updated":"2026-07-29T13:49:49Z","snapshot_observed_at":"2026-08-02T14:03:29.096476Z","submitted_at":"2026-05-14T17:59:55Z","title":"Primordial Black Hole from Tensor-induced Density Fluctuation: First-order Phase Transitions and Domain Walls","version":1},"reference_index":150,"source":"pdf_text","source_observed_at":"2026-05-15T02:53:41.149271Z"},"links":{"cited_paper":"/paper/1203.2681","citing_paper":"/paper/2605.15197"},"observation_digest":"sha256:531b384780ee763706e0939cbf7539eea86f64d8044c2803025c7db109c12d56","observation_id":"02056784-c201-4ebf-a7db-d5df171c6913","resolution":{"observed_at":"2026-05-15T02:59:42.005450Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1203.2681","last_updated":"2012-03-13T00:38:22Z","snapshot_observed_at":"2026-07-06T02:44:27.243716Z","submitted_at":"2012-03-13T00:38:22Z","title":"Probing the inflaton: Small-scale power spectrum constraints from measurements of the CMB energy spectrum","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1203.2681","snapshot_observed_at":"2026-08-02T14:03:43.873407Z","title":"Chluba, A","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2605.15197","last_updated":"2026-07-29T13:49:49Z","snapshot_observed_at":"2026-08-02T14:03:29.096476Z","submitted_at":"2026-05-14T17:59:55Z","title":"Primordial Black Hole from Tensor-induced Density Fluctuation: First-order Phase Transitions and Domain Walls","version":2},"reference_index":150,"source":"pdf_text","source_observed_at":"2026-08-02T14:03:43.873407Z"},"links":{"cited_paper":"/paper/1203.2681","citing_paper":"/paper/2605.15197"},"observation_digest":"sha256:4a42e40b709574e345328010f7ef11de4ed9b34b0963c5d3c999f27913110818","observation_id":"3cedc2aa-217a-4d17-b8c1-23ff5463e3d0","resolution":{"observed_at":"2026-08-02T14:03:43.873407Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1203.2681","last_updated":"2012-03-13T00:38:22Z","snapshot_observed_at":"2026-07-06T02:44:27.243716Z","submitted_at":"2012-03-13T00:38:22Z","title":"Probing the inflaton: Small-scale power spectrum constraints from measurements of the CMB energy spectrum","version":1},"cited_work":{"arxiv_id":"1203.2681","doi":null,"metadata_source":"pith","pith_arxiv_id":"1203.2681","snapshot_observed_at":"2026-07-04T18:10:02.072633Z","title":"Probing the inflaton: Small-scale power spectrum constraints from measurements of the CMB energy spectrum","venue":"astro-ph.CO","work_id":"25ff89f1-1feb-4dd2-877d-0cdc2f9b14f6","year":2012},"citing_paper":{"arxiv_id":"2605.27231","last_updated":"2026-05-26T16:11:50Z","snapshot_observed_at":"2026-08-03T01:55:34.476811Z","submitted_at":"2026-05-26T16:11:50Z","title":"A Fast Method to Compute Scalar Induced Gravitational Waves on a Lattice with Primordial Non-Gaussianities","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-06-29T15:37:34.480455Z"},"links":{"cited_paper":"/paper/1203.2681","citing_paper":"/paper/2605.27231"},"observation_digest":"sha256:5ec6db3f9f97fd56c9f431e56b96743b08ecf9bdc447ddf5383b6d8c541e34da","observation_id":"6b776240-0854-4f8b-9cb1-151f2e7ca29f","resolution":{"observed_at":"2026-06-29T15:43:32.726459Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1203.2681","last_updated":"2012-03-13T00:38:22Z","snapshot_observed_at":"2026-07-06T02:44:27.243716Z","submitted_at":"2012-03-13T00:38:22Z","title":"Probing the inflaton: Small-scale power spectrum constraints from measurements of the CMB energy spectrum","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1203.2681","snapshot_observed_at":"2026-07-12T14:05:11.011544Z","title":"Chluba, A","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2606.14827","last_updated":"2026-07-09T09:33:51Z","snapshot_observed_at":"2026-07-12T23:17:34.647107Z","submitted_at":"2026-06-12T14:29:14Z","title":"Probing the fate of large primordial perturbations with exoplanets","version":2},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-07-12T14:05:11.011544Z"},"links":{"cited_paper":"/paper/1203.2681","citing_paper":"/paper/2606.14827"},"observation_digest":"sha256:15ccd6d00328cce94a9b5b88b385a9eb7c151781cd074ea7fb91f6534b932dd4","observation_id":"00a238b9-6f71-4d0d-b401-3fa3526eeddf","resolution":{"observed_at":"2026-07-12T14:05:11.011544Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1203.2681","last_updated":"2012-03-13T00:38:22Z","snapshot_observed_at":"2026-07-06T02:44:27.243716Z","submitted_at":"2012-03-13T00:38:22Z","title":"Probing the inflaton: Small-scale power spectrum constraints from measurements of the CMB energy spectrum","version":1},"cited_work":{"arxiv_id":"1203.2681","doi":null,"metadata_source":"pith","pith_arxiv_id":"1203.2681","snapshot_observed_at":"2026-07-04T18:10:02.072633Z","title":"Probing the inflaton: Small-scale power spectrum constraints from measurements of the CMB energy spectrum","venue":"astro-ph.CO","work_id":"25ff89f1-1feb-4dd2-877d-0cdc2f9b14f6","year":2012},"citing_paper":{"arxiv_id":"2606.25014","last_updated":"2026-07-08T17:34:31Z","snapshot_observed_at":"2026-07-12T12:25:42.844259Z","submitted_at":"2026-06-23T18:00:00Z","title":"Probing Confining Dark Sectors with Cosmological Perturbations","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-06-25T23:01:42.890617Z"},"links":{"cited_paper":"/paper/1203.2681","citing_paper":"/paper/2606.25014"},"observation_digest":"sha256:7a2516922028a726315a39b0330caf67b5abe8bf6e845b7261626d6cc1f572c7","observation_id":"a2de9107-dc76-4e7c-851b-59771a598cc7","resolution":{"observed_at":"2026-07-04T18:10:02.074114Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1203.2681","last_updated":"2012-03-13T00:38:22Z","snapshot_observed_at":"2026-07-06T02:44:27.243716Z","submitted_at":"2012-03-13T00:38:22Z","title":"Probing the inflaton: Small-scale power spectrum constraints from measurements of the CMB energy spectrum","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1203.2681","snapshot_observed_at":"2026-07-12T12:25:43.531687Z","title":"Chluba, A","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2606.25014","last_updated":"2026-07-08T17:34:31Z","snapshot_observed_at":"2026-07-12T12:25:42.844259Z","submitted_at":"2026-06-23T18:00:00Z","title":"Probing Confining Dark Sectors with Cosmological Perturbations","version":2},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-07-12T12:25:43.531687Z"},"links":{"cited_paper":"/paper/1203.2681","citing_paper":"/paper/2606.25014"},"observation_digest":"sha256:c23af8fc1078aeaa14220f3e08a6df6a97610c9e3984c79834a7ae288cab4284","observation_id":"a3c32547-9078-47e3-a6fa-f977a2396bd3","resolution":{"observed_at":"2026-07-12T12:25:43.531687Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1203.2681","last_updated":"2012-03-13T00:38:22Z","snapshot_observed_at":"2026-07-06T02:44:27.243716Z","submitted_at":"2012-03-13T00:38:22Z","title":"Probing the inflaton: Small-scale power spectrum constraints from measurements of the CMB energy spectrum","version":1},"cited_work":{"arxiv_id":"1203.2681","doi":null,"metadata_source":"pith","pith_arxiv_id":"1203.2681","snapshot_observed_at":"2026-07-04T18:10:02.072633Z","title":"Probing the inflaton: Small-scale power spectrum constraints from measurements of the CMB energy spectrum","venue":"astro-ph.CO","work_id":"25ff89f1-1feb-4dd2-877d-0cdc2f9b14f6","year":2012},"citing_paper":{"arxiv_id":"2606.28296","last_updated":"2026-06-26T17:40:06Z","snapshot_observed_at":"2026-07-07T00:02:24.342539Z","submitted_at":"2026-06-26T17:40:06Z","title":"Memoirs of the curvaton: non-perturbative non-Gaussianity and supermassive primordial black holes","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-06-29T02:29:32.722846Z"},"links":{"cited_paper":"/paper/1203.2681","citing_paper":"/paper/2606.28296"},"observation_digest":"sha256:96655fc6908240dbc139c5d456894a427b94c7ad044263caf4fa9ed26c5214e4","observation_id":"44ab6fe7-5e31-40ca-91e0-b841f115fea2","resolution":{"observed_at":"2026-07-01T18:15:57.784379Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1203.2681","last_updated":"2012-03-13T00:38:22Z","snapshot_observed_at":"2026-07-06T02:44:27.243716Z","submitted_at":"2012-03-13T00:38:22Z","title":"Probing the inflaton: Small-scale power spectrum constraints from measurements of the CMB energy spectrum","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1203.2681","snapshot_observed_at":"2026-08-02T07:54:46.976988Z","title":"Chluba, A","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2607.09285","last_updated":"2026-07-22T09:21:46Z","snapshot_observed_at":"2026-08-02T07:54:40.995317Z","submitted_at":"2026-07-10T10:51:32Z","title":"Primordial Black Hole mass growth from neutrinos during the radiation era","version":2},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-02T07:54:46.976988Z"},"links":{"cited_paper":"/paper/1203.2681","citing_paper":"/paper/2607.09285"},"observation_digest":"sha256:c69353918a43d3bbb9be6323913fb50bc0e9d8b3d871b1072e45bba2fea69d1b","observation_id":"ed64e3b4-1811-4717-a17f-fccd4f05e677","resolution":{"observed_at":"2026-08-02T07:54:46.976988Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1203.2681","last_updated":"2012-03-13T00:38:22Z","snapshot_observed_at":"2026-07-06T02:44:27.243716Z","submitted_at":"2012-03-13T00:38:22Z","title":"Probing the inflaton: Small-scale power spectrum constraints from measurements of the CMB energy spectrum","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1203.2681","snapshot_observed_at":"2026-08-01T15:56:22.631300Z","title":"Chluba, A","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2607.18185","last_updated":"2026-07-20T17:23:48Z","snapshot_observed_at":"2026-08-01T15:56:15.184642Z","submitted_at":"2026-07-20T17:23:48Z","title":"Wide binaries in ultra-faint dwarf galaxies as a probe of extended dark objects","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-01T15:56:22.631300Z"},"links":{"cited_paper":"/paper/1203.2681","citing_paper":"/paper/2607.18185"},"observation_digest":"sha256:ec6092d41883ec48aa3e4e38e694de9ae229636ae42f25ab83d04c6cb1ddb565","observation_id":"8ed705d0-8243-4bd9-9175-7878cd87e639","resolution":{"observed_at":"2026-08-01T15:56:22.631300Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1203.2681","last_updated":"2012-03-13T00:38:22Z","snapshot_observed_at":"2026-07-06T02:44:27.243716Z","submitted_at":"2012-03-13T00:38:22Z","title":"Probing the inflaton: Small-scale power spectrum constraints from measurements of the CMB energy spectrum","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1203.2681","snapshot_observed_at":"2026-08-01T09:11:23.298003Z","title":"Chluba, A","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2607.20884","last_updated":"2026-07-23T03:18:02Z","snapshot_observed_at":"2026-08-04T08:11:58.976766Z","submitted_at":"2026-07-23T03:18:02Z","title":"A lower bound on primordial power spectrum from halo substructure","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-01T09:11:23.298003Z"},"links":{"cited_paper":"/paper/1203.2681","citing_paper":"/paper/2607.20884"},"observation_digest":"sha256:a0d7033b97341884194bb1cf7afff9674eec03ce0a45449cf638728f460323c3","observation_id":"37e21cac-2c36-4013-8dfd-4b0e790dddbc","resolution":{"observed_at":"2026-08-01T09:11:23.298003Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1203.2681/citation-record","integrity":"/paper/1203.2681/integrity","json":"/paper/1203.2681/citation-record.json","paper":"/paper/1203.2681"},"outbound":[],"paper":{"arxiv_id":"1203.2681","last_updated":"2012-03-13T00:38:22Z","latest_version":1,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-07-06T02:44:27.243716Z","submitted_at":"2012-03-13T00:38:22Z","title":"Probing the inflaton: Small-scale power spectrum constraints from measurements of the CMB energy spectrum"},"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":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"thesis":"As of 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 14 inbound Pith citation observations for arXiv:1203.2681."}