{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2026:G3HGT3DZNIYJHA6ECP6BPA6VW6","short_pith_number":"pith:G3HGT3DZ","schema_version":"1.0","canonical_sha256":"36ce69ec796a309383c413fc1783d5b78d6ce139d37512136f4aec080bd8589a","source":{"kind":"arxiv","id":"2606.19862","version":1},"attestation_state":"computed","paper":{"title":"Multi-band Structural Analysis of KiDS-selected Low Surface Brightness Galaxies with Hyper Suprime-Cam Imaging","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Dipanjan Mitra, Kanak Saha","submitted_at":"2026-06-18T07:16:55Z","abstract_excerpt":"We present a homogeneous multi-band structural analysis of 205 KiDS-selected low surface brightness galaxy (LSBG) candidates using deep Hyper Suprime-Cam (HSC) $G$, $R$, and $I$-band imaging. Structural parameters were derived using single-component S\\'ersic modeling with GALFIT. The sample is dominated by diffuse systems with low S\\'ersic indices, with the distributions consistently peaking near $n\\approx0.7$ across all bands. The estimated $B$-band central surface brightness distribution has a median value of $\\tilde{\\mu}_{0,B}=24.55$ mag arcsec$^{-2}$, indicating that the galaxies lie firml"},"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":"2606.19862","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.GA","submitted_at":"2026-06-18T07:16:55Z","cross_cats_sorted":[],"title_canon_sha256":"067f2ebe4e08cf7484efff5bdb1718095e98e1acd8136d1fd84d07c7fe33fb72","abstract_canon_sha256":"4717c6e98b1e4e0a0f54d75d3c92ce219392a22845bd361ba2310a496d35b81f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-06-19T16:12:37.237457Z","signature_b64":"kH3B82gqz0hGaZZZeAyo3tfmto3gLmoMsCFiXor/2q7YS9/8kuyPAl1Wz2paABVRz7/ih1IX9Mc83Z5UhZISCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"36ce69ec796a309383c413fc1783d5b78d6ce139d37512136f4aec080bd8589a","last_reissued_at":"2026-06-19T16:12:37.237120Z","signature_status":"signed_v1","first_computed_at":"2026-06-19T16:12:37.237120Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Multi-band Structural Analysis of KiDS-selected Low Surface Brightness Galaxies with Hyper Suprime-Cam Imaging","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Dipanjan Mitra, Kanak Saha","submitted_at":"2026-06-18T07:16:55Z","abstract_excerpt":"We present a homogeneous multi-band structural analysis of 205 KiDS-selected low surface brightness galaxy (LSBG) candidates using deep Hyper Suprime-Cam (HSC) $G$, $R$, and $I$-band imaging. Structural parameters were derived using single-component S\\'ersic modeling with GALFIT. The sample is dominated by diffuse systems with low S\\'ersic indices, with the distributions consistently peaking near $n\\approx0.7$ across all bands. The estimated $B$-band central surface brightness distribution has a median value of $\\tilde{\\mu}_{0,B}=24.55$ mag arcsec$^{-2}$, indicating that the galaxies lie firml"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2606.19862","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2606.19862/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"2606.19862","created_at":"2026-06-19T16:12:37.237174+00:00"},{"alias_kind":"arxiv_version","alias_value":"2606.19862v1","created_at":"2026-06-19T16:12:37.237174+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2606.19862","created_at":"2026-06-19T16:12:37.237174+00:00"},{"alias_kind":"pith_short_12","alias_value":"G3HGT3DZNIYJ","created_at":"2026-06-19T16:12:37.237174+00:00"},{"alias_kind":"pith_short_16","alias_value":"G3HGT3DZNIYJHA6E","created_at":"2026-06-19T16:12:37.237174+00:00"},{"alias_kind":"pith_short_8","alias_value":"G3HGT3DZ","created_at":"2026-06-19T16:12:37.237174+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/G3HGT3DZNIYJHA6ECP6BPA6VW6","json":"https://pith.science/pith/G3HGT3DZNIYJHA6ECP6BPA6VW6.json","graph_json":"https://pith.science/api/pith-number/G3HGT3DZNIYJHA6ECP6BPA6VW6/graph.json","events_json":"https://pith.science/api/pith-number/G3HGT3DZNIYJHA6ECP6BPA6VW6/events.json","paper":"https://pith.science/paper/G3HGT3DZ"},"agent_actions":{"view_html":"https://pith.science/pith/G3HGT3DZNIYJHA6ECP6BPA6VW6","download_json":"https://pith.science/pith/G3HGT3DZNIYJHA6ECP6BPA6VW6.json","view_paper":"https://pith.science/paper/G3HGT3DZ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2606.19862&json=true","fetch_graph":"https://pith.science/api/pith-number/G3HGT3DZNIYJHA6ECP6BPA6VW6/graph.json","fetch_events":"https://pith.science/api/pith-number/G3HGT3DZNIYJHA6ECP6BPA6VW6/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/G3HGT3DZNIYJHA6ECP6BPA6VW6/action/timestamp_anchor","attest_storage":"https://pith.science/pith/G3HGT3DZNIYJHA6ECP6BPA6VW6/action/storage_attestation","attest_author":"https://pith.science/pith/G3HGT3DZNIYJHA6ECP6BPA6VW6/action/author_attestation","sign_citation":"https://pith.science/pith/G3HGT3DZNIYJHA6ECP6BPA6VW6/action/citation_signature","submit_replication":"https://pith.science/pith/G3HGT3DZNIYJHA6ECP6BPA6VW6/action/replication_record"}},"created_at":"2026-06-19T16:12:37.237174+00:00","updated_at":"2026-06-19T16:12:37.237174+00:00"}