{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:YDLAXVTW34QBA7KXUKHPZRW567","short_pith_number":"pith:YDLAXVTW","schema_version":"1.0","canonical_sha256":"c0d60bd676df20107d57a28efcc6ddf7dadf8525f9d3bbd9b0cd68367428587c","source":{"kind":"arxiv","id":"1005.2091","version":1},"attestation_state":"computed","paper":{"title":"Herschel photometric observations of the low metallicity dwarf galaxy NGC 1705","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"A. Boselli, A. Cooray, A. Papageorgiou, A. Rykala, B. O'Halloran, B. Schulz, C.D. Wilson, D. Cormier, D. Elbaz, D.L. Clements, E. Dwek, E.E. Rigby, F. Galliano, G. J. Bendo, G.S. Wright, H.L. Gomez, H. Roussel, H. Wozniak, I. Perez-Fournon, J.A. Stevens, J. Glenn, J.I. Davies, J.J. Bock, K.G. Isaak, K. Okumura, L. Ciesla, L. Cortese, L.R. Levenson, L. Spinoglio, L. Vigroux, M. Baes, M. Bradford, M. Galametz, M. Griffin, M.J. Barlow, M.J. Page, M. Pohlen, M.R. P. Schirm, M. Sauvage, M. Symeonidis, M. Trichas, M. Vaccari, M.W.L. Smith, N. Castro-Rodriguez, N. Lu, N. Rangwala, N. Sacchi, P. Chanial, P.Panuzzo, R. Auld, S.A. Eales, S. Charlot, S.C. Madden, S. Hony, S. Oliver, S. Sundar, T.J. Parkin, V. Buat, W.K. Gear, W.W. Zeilinger","submitted_at":"2010-05-12T13:32:16Z","abstract_excerpt":"We present Herschel SPIRE and PACS photometeric observations of the low metallicity (Z ~ 0.35 solar) nearby dwarf galaxy, NGC 1705, in six wavelength bands as part of the Dwarf Galaxy Survey guaranteed time Herschel Key Program. We confirm the presence of two dominant circumnuclear IR-bright regions surrounding the central super star cluster that had been previously noted at mid-IR wavelengths and in the sub-mm by LABOCA. On constructing a global spectral energy distribution using the SPIRE and PACS photometry, in conjunction with archival IR measurements, we note the presence of an excess at "},"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":"1005.2091","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2010-05-12T13:32:16Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"2c60d83bb27b7636e4f1c1c2d646470de9ecf1efa6e899c36e0f23f314e8e24c","abstract_canon_sha256":"29185057889c8bab6903a4db931c4b69ca50efe47a7ba0620d9883c94d2dc7c7"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:07:33.747481Z","signature_b64":"qnw2Sv1Ob9e9mYWcfRtiagqXwGTIhfq+cEv1m0vvsAe6QU7dveh4zlivowrmyQLWgtm/9sdrC30OygXnLhKSCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c0d60bd676df20107d57a28efcc6ddf7dadf8525f9d3bbd9b0cd68367428587c","last_reissued_at":"2026-05-18T02:07:33.747020Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:07:33.747020Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Herschel photometric observations of the low metallicity dwarf galaxy NGC 1705","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"A. Boselli, A. Cooray, A. Papageorgiou, A. Rykala, B. O'Halloran, B. Schulz, C.D. Wilson, D. Cormier, D. Elbaz, D.L. Clements, E. Dwek, E.E. Rigby, F. Galliano, G. J. Bendo, G.S. Wright, H.L. Gomez, H. Roussel, H. Wozniak, I. Perez-Fournon, J.A. Stevens, J. Glenn, J.I. Davies, J.J. Bock, K.G. Isaak, K. Okumura, L. Ciesla, L. Cortese, L.R. Levenson, L. Spinoglio, L. Vigroux, M. Baes, M. Bradford, M. Galametz, M. Griffin, M.J. Barlow, M.J. Page, M. Pohlen, M.R. P. Schirm, M. Sauvage, M. Symeonidis, M. Trichas, M. Vaccari, M.W.L. Smith, N. Castro-Rodriguez, N. Lu, N. Rangwala, N. Sacchi, P. Chanial, P.Panuzzo, R. Auld, S.A. Eales, S. Charlot, S.C. Madden, S. Hony, S. Oliver, S. Sundar, T.J. Parkin, V. Buat, W.K. Gear, W.W. Zeilinger","submitted_at":"2010-05-12T13:32:16Z","abstract_excerpt":"We present Herschel SPIRE and PACS photometeric observations of the low metallicity (Z ~ 0.35 solar) nearby dwarf galaxy, NGC 1705, in six wavelength bands as part of the Dwarf Galaxy Survey guaranteed time Herschel Key Program. We confirm the presence of two dominant circumnuclear IR-bright regions surrounding the central super star cluster that had been previously noted at mid-IR wavelengths and in the sub-mm by LABOCA. On constructing a global spectral energy distribution using the SPIRE and PACS photometry, in conjunction with archival IR measurements, we note the presence of an excess at "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1005.2091","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":"1005.2091","created_at":"2026-05-18T02:07:33.747092+00:00"},{"alias_kind":"arxiv_version","alias_value":"1005.2091v1","created_at":"2026-05-18T02:07:33.747092+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1005.2091","created_at":"2026-05-18T02:07:33.747092+00:00"},{"alias_kind":"pith_short_12","alias_value":"YDLAXVTW34QB","created_at":"2026-05-18T12:26:17.028572+00:00"},{"alias_kind":"pith_short_16","alias_value":"YDLAXVTW34QBA7KX","created_at":"2026-05-18T12:26:17.028572+00:00"},{"alias_kind":"pith_short_8","alias_value":"YDLAXVTW","created_at":"2026-05-18T12:26:17.028572+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/YDLAXVTW34QBA7KXUKHPZRW567","json":"https://pith.science/pith/YDLAXVTW34QBA7KXUKHPZRW567.json","graph_json":"https://pith.science/api/pith-number/YDLAXVTW34QBA7KXUKHPZRW567/graph.json","events_json":"https://pith.science/api/pith-number/YDLAXVTW34QBA7KXUKHPZRW567/events.json","paper":"https://pith.science/paper/YDLAXVTW"},"agent_actions":{"view_html":"https://pith.science/pith/YDLAXVTW34QBA7KXUKHPZRW567","download_json":"https://pith.science/pith/YDLAXVTW34QBA7KXUKHPZRW567.json","view_paper":"https://pith.science/paper/YDLAXVTW","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1005.2091&json=true","fetch_graph":"https://pith.science/api/pith-number/YDLAXVTW34QBA7KXUKHPZRW567/graph.json","fetch_events":"https://pith.science/api/pith-number/YDLAXVTW34QBA7KXUKHPZRW567/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/YDLAXVTW34QBA7KXUKHPZRW567/action/timestamp_anchor","attest_storage":"https://pith.science/pith/YDLAXVTW34QBA7KXUKHPZRW567/action/storage_attestation","attest_author":"https://pith.science/pith/YDLAXVTW34QBA7KXUKHPZRW567/action/author_attestation","sign_citation":"https://pith.science/pith/YDLAXVTW34QBA7KXUKHPZRW567/action/citation_signature","submit_replication":"https://pith.science/pith/YDLAXVTW34QBA7KXUKHPZRW567/action/replication_record"}},"created_at":"2026-05-18T02:07:33.747092+00:00","updated_at":"2026-05-18T02:07:33.747092+00:00"}