{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:PENJRS6IBDMZ5DKYP4Y42COXAC","short_pith_number":"pith:PENJRS6I","schema_version":"1.0","canonical_sha256":"791a98cbc808d99e8d587f31cd09d7008951f363c39edb3456aa827612e3d636","source":{"kind":"arxiv","id":"1203.6784","version":1},"attestation_state":"computed","paper":{"title":"A peculiar class of debris disks from Herschel/DUNES - A steep fall off in the far infrared","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.EP"],"primary_cat":"astro-ph.SR","authors_text":"A. Bayo, A. Mora, A. V. Krivov, B. Montesinos, C. del Burgo, C. Eiroa, D. Ardila, G. Bryden, G. J. White, G. Kennedy, G. L. Pilbratt, J.-C. Augereau, J. Greaves, J. Lebreton, J. Maldonado, J. P. Marshall, J. Sanz-Forcada, K. Stapelfeldt, M. Arevalo, O. Absil, R. Liseau, S. Ertel, S. Wolf, T. Loehne","submitted_at":"2012-03-30T12:07:50Z","abstract_excerpt":"Aims. We present photometric data of debris disks around HIP 103389 (HD 199260), HIP 107350 (HN Peg, HD206860), and HIP 114948 (HD 219482), obtained in the context of our Herschel Open Time Key Program DUNES (DUst around NEarby Stars). Methods. We used Herschel/PACS to detect the thermal emission of the three debris disks with a 3 sigma sensitivity of a few mJy at 100 um and 160 um. In addition, we obtained Herschel/PACS photometric data at 70 um for HIP 103389. Two different approaches are applied to reduce the Herschel data to investigate the impact of data reduction on the photometry. We fi"},"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":"1203.6784","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2012-03-30T12:07:50Z","cross_cats_sorted":["astro-ph.EP"],"title_canon_sha256":"18321eb6c36c8fcff0e4b7ce835766474801bdcd5a2624a74ae03658ec30b8d8","abstract_canon_sha256":"5e945cbbb6dc9a4cc6e329e2379d31f6c570a074055576757671fe5f7cf593d9"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:58:00.129854Z","signature_b64":"p/v9sKTta1sl6/GBgW1yOuBXeR67pM8X69tCxoXl1GxfM44Er+hGfMiKqWWoYDWwb8LrVDiewbmAkcgPcWhNAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"791a98cbc808d99e8d587f31cd09d7008951f363c39edb3456aa827612e3d636","last_reissued_at":"2026-05-18T01:58:00.129271Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:58:00.129271Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A peculiar class of debris disks from Herschel/DUNES - A steep fall off in the far infrared","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.EP"],"primary_cat":"astro-ph.SR","authors_text":"A. Bayo, A. Mora, A. V. Krivov, B. Montesinos, C. del Burgo, C. Eiroa, D. Ardila, G. Bryden, G. J. White, G. Kennedy, G. L. Pilbratt, J.-C. Augereau, J. Greaves, J. Lebreton, J. Maldonado, J. P. Marshall, J. Sanz-Forcada, K. Stapelfeldt, M. Arevalo, O. Absil, R. Liseau, S. Ertel, S. Wolf, T. Loehne","submitted_at":"2012-03-30T12:07:50Z","abstract_excerpt":"Aims. We present photometric data of debris disks around HIP 103389 (HD 199260), HIP 107350 (HN Peg, HD206860), and HIP 114948 (HD 219482), obtained in the context of our Herschel Open Time Key Program DUNES (DUst around NEarby Stars). Methods. We used Herschel/PACS to detect the thermal emission of the three debris disks with a 3 sigma sensitivity of a few mJy at 100 um and 160 um. In addition, we obtained Herschel/PACS photometric data at 70 um for HIP 103389. Two different approaches are applied to reduce the Herschel data to investigate the impact of data reduction on the photometry. We fi"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1203.6784","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":"1203.6784","created_at":"2026-05-18T01:58:00.129365+00:00"},{"alias_kind":"arxiv_version","alias_value":"1203.6784v1","created_at":"2026-05-18T01:58:00.129365+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1203.6784","created_at":"2026-05-18T01:58:00.129365+00:00"},{"alias_kind":"pith_short_12","alias_value":"PENJRS6IBDMZ","created_at":"2026-05-18T12:27:18.751474+00:00"},{"alias_kind":"pith_short_16","alias_value":"PENJRS6IBDMZ5DKY","created_at":"2026-05-18T12:27:18.751474+00:00"},{"alias_kind":"pith_short_8","alias_value":"PENJRS6I","created_at":"2026-05-18T12:27:18.751474+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/PENJRS6IBDMZ5DKYP4Y42COXAC","json":"https://pith.science/pith/PENJRS6IBDMZ5DKYP4Y42COXAC.json","graph_json":"https://pith.science/api/pith-number/PENJRS6IBDMZ5DKYP4Y42COXAC/graph.json","events_json":"https://pith.science/api/pith-number/PENJRS6IBDMZ5DKYP4Y42COXAC/events.json","paper":"https://pith.science/paper/PENJRS6I"},"agent_actions":{"view_html":"https://pith.science/pith/PENJRS6IBDMZ5DKYP4Y42COXAC","download_json":"https://pith.science/pith/PENJRS6IBDMZ5DKYP4Y42COXAC.json","view_paper":"https://pith.science/paper/PENJRS6I","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1203.6784&json=true","fetch_graph":"https://pith.science/api/pith-number/PENJRS6IBDMZ5DKYP4Y42COXAC/graph.json","fetch_events":"https://pith.science/api/pith-number/PENJRS6IBDMZ5DKYP4Y42COXAC/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/PENJRS6IBDMZ5DKYP4Y42COXAC/action/timestamp_anchor","attest_storage":"https://pith.science/pith/PENJRS6IBDMZ5DKYP4Y42COXAC/action/storage_attestation","attest_author":"https://pith.science/pith/PENJRS6IBDMZ5DKYP4Y42COXAC/action/author_attestation","sign_citation":"https://pith.science/pith/PENJRS6IBDMZ5DKYP4Y42COXAC/action/citation_signature","submit_replication":"https://pith.science/pith/PENJRS6IBDMZ5DKYP4Y42COXAC/action/replication_record"}},"created_at":"2026-05-18T01:58:00.129365+00:00","updated_at":"2026-05-18T01:58:00.129365+00:00"}