{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:FNL7ZONLMNBKDUJWLZEZOMZHKP","short_pith_number":"pith:FNL7ZONL","schema_version":"1.0","canonical_sha256":"2b57fcb9ab6342a1d1365e4997332753d200bdc617616f5fedc9956c458ff1f8","source":{"kind":"arxiv","id":"1010.0020","version":1},"attestation_state":"computed","paper":{"title":"HerMES: SPIRE Science Demonstration Phase Maps","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.IM"],"primary_cat":"astro-ph.CO","authors_text":"A. Amblard, A. Blain, A. Conley, A. Cooray, A. Franceschini, A. Papageorgiou, B. Schulz, C.D. Dowell, C.K. Xu, D.L. Shupe, Douglas Scott, D. Wiebe, E. Chapin, E. Valiante, G. Marsden, G. Wright, H.T. Nguyen, I. Perez-Fournon, J. Bock, J.D. Vieira, J. Glenn, L. Levenson, L. Vigroux, M. Griffin, M. Halpern, M.J. Page, M. Pohlen, M. Rowan-Robinson, M. Zemcov, N. Rangwala, P. Serra, S.J. Oliver, T.P. Ellsworth-Bowers","submitted_at":"2010-09-30T21:36:01Z","abstract_excerpt":"We describe the production and verification of sky maps of the five SPIRE fields observed as part of the Herschel Multi-tiered Extragalactic Survey (HerMES) during the Science Demonstration Phase (SDP) of the Herschel mission. We have implemented an iterative map-making algorithm (SHIM; The SPIRE-HerMES Iterative Mapper) to produce high fidelity maps that preserve extended diffuse emission on the sky while exploiting the repeated observations of the same region of the sky with many detectors in multiple scan directions to minimize residual instrument noise. We specify here the SHIM algorithm a"},"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":"1010.0020","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2010-09-30T21:36:01Z","cross_cats_sorted":["astro-ph.IM"],"title_canon_sha256":"6a342fea53d297c283e409b39077bf7f7343ad7a6a7a9ce73664a63f06468361","abstract_canon_sha256":"21a2baa9dcb93afd256a3c841906e9300a7850e6900958f036b9460a53bf6ca0"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:05:12.908344Z","signature_b64":"tOARwDpcRapfdIu56vKp/ZQNs9W+TeXTLinzwcByMrmyS4aaoHEJPmcfA3bPgo07VMtff8uvqSCLdNceL50ZBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"2b57fcb9ab6342a1d1365e4997332753d200bdc617616f5fedc9956c458ff1f8","last_reissued_at":"2026-05-18T02:05:12.907471Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:05:12.907471Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"HerMES: SPIRE Science Demonstration Phase Maps","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.IM"],"primary_cat":"astro-ph.CO","authors_text":"A. Amblard, A. Blain, A. Conley, A. Cooray, A. Franceschini, A. Papageorgiou, B. Schulz, C.D. Dowell, C.K. Xu, D.L. Shupe, Douglas Scott, D. Wiebe, E. Chapin, E. Valiante, G. Marsden, G. Wright, H.T. Nguyen, I. Perez-Fournon, J. Bock, J.D. Vieira, J. Glenn, L. Levenson, L. Vigroux, M. Griffin, M. Halpern, M.J. Page, M. Pohlen, M. Rowan-Robinson, M. Zemcov, N. Rangwala, P. Serra, S.J. Oliver, T.P. Ellsworth-Bowers","submitted_at":"2010-09-30T21:36:01Z","abstract_excerpt":"We describe the production and verification of sky maps of the five SPIRE fields observed as part of the Herschel Multi-tiered Extragalactic Survey (HerMES) during the Science Demonstration Phase (SDP) of the Herschel mission. We have implemented an iterative map-making algorithm (SHIM; The SPIRE-HerMES Iterative Mapper) to produce high fidelity maps that preserve extended diffuse emission on the sky while exploiting the repeated observations of the same region of the sky with many detectors in multiple scan directions to minimize residual instrument noise. We specify here the SHIM algorithm a"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1010.0020","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":"1010.0020","created_at":"2026-05-18T02:05:12.907572+00:00"},{"alias_kind":"arxiv_version","alias_value":"1010.0020v1","created_at":"2026-05-18T02:05:12.907572+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1010.0020","created_at":"2026-05-18T02:05:12.907572+00:00"},{"alias_kind":"pith_short_12","alias_value":"FNL7ZONLMNBK","created_at":"2026-05-18T12:26:07.630475+00:00"},{"alias_kind":"pith_short_16","alias_value":"FNL7ZONLMNBKDUJW","created_at":"2026-05-18T12:26:07.630475+00:00"},{"alias_kind":"pith_short_8","alias_value":"FNL7ZONL","created_at":"2026-05-18T12:26:07.630475+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/FNL7ZONLMNBKDUJWLZEZOMZHKP","json":"https://pith.science/pith/FNL7ZONLMNBKDUJWLZEZOMZHKP.json","graph_json":"https://pith.science/api/pith-number/FNL7ZONLMNBKDUJWLZEZOMZHKP/graph.json","events_json":"https://pith.science/api/pith-number/FNL7ZONLMNBKDUJWLZEZOMZHKP/events.json","paper":"https://pith.science/paper/FNL7ZONL"},"agent_actions":{"view_html":"https://pith.science/pith/FNL7ZONLMNBKDUJWLZEZOMZHKP","download_json":"https://pith.science/pith/FNL7ZONLMNBKDUJWLZEZOMZHKP.json","view_paper":"https://pith.science/paper/FNL7ZONL","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1010.0020&json=true","fetch_graph":"https://pith.science/api/pith-number/FNL7ZONLMNBKDUJWLZEZOMZHKP/graph.json","fetch_events":"https://pith.science/api/pith-number/FNL7ZONLMNBKDUJWLZEZOMZHKP/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/FNL7ZONLMNBKDUJWLZEZOMZHKP/action/timestamp_anchor","attest_storage":"https://pith.science/pith/FNL7ZONLMNBKDUJWLZEZOMZHKP/action/storage_attestation","attest_author":"https://pith.science/pith/FNL7ZONLMNBKDUJWLZEZOMZHKP/action/author_attestation","sign_citation":"https://pith.science/pith/FNL7ZONLMNBKDUJWLZEZOMZHKP/action/citation_signature","submit_replication":"https://pith.science/pith/FNL7ZONLMNBKDUJWLZEZOMZHKP/action/replication_record"}},"created_at":"2026-05-18T02:05:12.907572+00:00","updated_at":"2026-05-18T02:05:12.907572+00:00"}