{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:324PPNSCMQIUYDWVKMAKTBOS5V","short_pith_number":"pith:324PPNSC","schema_version":"1.0","canonical_sha256":"deb8f7b64264114c0ed55300a985d2ed4de753fd4d3451bebd3046f8dbca0d78","source":{"kind":"arxiv","id":"1303.5490","version":3},"attestation_state":"computed","paper":{"title":"The Supermassive Black Hole Mass - Spheroid Stellar Mass Relation for S\\'ersic and Core-S\\'ersic Galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Alister W. Graham, James Schombert, Nicholas Scott","submitted_at":"2013-03-22T00:44:35Z","abstract_excerpt":"We have examined the relationship between supermassive black hole mass (M$_{BH}$) and the stellar mass of the host spheroid (M$_{sph,*}$) for a sample of 75 nearby galaxies. To derive the spheroid stellar masses we used improved 2MASS K$_s$-band photometry from the ARCHANGEL photometry pipeline. Dividing our sample into core-S\\'ersic and S\\'ersic galaxies, we find that they are described by very different M$_{BH}$-M$_{sph,*}$ relations. For core-S\\'ersic galaxies - which are typically massive and luminous, with M$_{BH} \\gtrsim 2x10^8 M_\\odot$ - we find M$_{BH} \\propto M_{sph,*}^{(0.97 \\pm 0.14"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"1303.5490","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2013-03-22T00:44:35Z","cross_cats_sorted":[],"title_canon_sha256":"49db889f5539837e9ffa4b5905d916a3180c604f075d32f0ce86902ca48a7ec7","abstract_canon_sha256":"b0a90a8d34f56997ef838091ea97a2cc9a7e67fd0e0fb4990dc2ddc95156c5d8"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:46:04.691670Z","signature_b64":"zrj/5a4LOAFwYwHPQXkmjBvXnzEtI/ncvt0lPewozTmwuVsIcVx4XqRuJbD2K1DyCyRi6jTCcKSI1C+17WGsBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"deb8f7b64264114c0ed55300a985d2ed4de753fd4d3451bebd3046f8dbca0d78","last_reissued_at":"2026-05-18T02:46:04.691121Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:46:04.691121Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Supermassive Black Hole Mass - Spheroid Stellar Mass Relation for S\\'ersic and Core-S\\'ersic Galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Alister W. Graham, James Schombert, Nicholas Scott","submitted_at":"2013-03-22T00:44:35Z","abstract_excerpt":"We have examined the relationship between supermassive black hole mass (M$_{BH}$) and the stellar mass of the host spheroid (M$_{sph,*}$) for a sample of 75 nearby galaxies. To derive the spheroid stellar masses we used improved 2MASS K$_s$-band photometry from the ARCHANGEL photometry pipeline. Dividing our sample into core-S\\'ersic and S\\'ersic galaxies, we find that they are described by very different M$_{BH}$-M$_{sph,*}$ relations. For core-S\\'ersic galaxies - which are typically massive and luminous, with M$_{BH} \\gtrsim 2x10^8 M_\\odot$ - we find M$_{BH} \\propto M_{sph,*}^{(0.97 \\pm 0.14"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1303.5490","kind":"arxiv","version":3},"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":"1303.5490","created_at":"2026-05-18T02:46:04.691199+00:00"},{"alias_kind":"arxiv_version","alias_value":"1303.5490v3","created_at":"2026-05-18T02:46:04.691199+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1303.5490","created_at":"2026-05-18T02:46:04.691199+00:00"},{"alias_kind":"pith_short_12","alias_value":"324PPNSCMQIU","created_at":"2026-05-18T12:27:32.513160+00:00"},{"alias_kind":"pith_short_16","alias_value":"324PPNSCMQIUYDWV","created_at":"2026-05-18T12:27:32.513160+00:00"},{"alias_kind":"pith_short_8","alias_value":"324PPNSC","created_at":"2026-05-18T12:27:32.513160+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/324PPNSCMQIUYDWVKMAKTBOS5V","json":"https://pith.science/pith/324PPNSCMQIUYDWVKMAKTBOS5V.json","graph_json":"https://pith.science/api/pith-number/324PPNSCMQIUYDWVKMAKTBOS5V/graph.json","events_json":"https://pith.science/api/pith-number/324PPNSCMQIUYDWVKMAKTBOS5V/events.json","paper":"https://pith.science/paper/324PPNSC"},"agent_actions":{"view_html":"https://pith.science/pith/324PPNSCMQIUYDWVKMAKTBOS5V","download_json":"https://pith.science/pith/324PPNSCMQIUYDWVKMAKTBOS5V.json","view_paper":"https://pith.science/paper/324PPNSC","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1303.5490&json=true","fetch_graph":"https://pith.science/api/pith-number/324PPNSCMQIUYDWVKMAKTBOS5V/graph.json","fetch_events":"https://pith.science/api/pith-number/324PPNSCMQIUYDWVKMAKTBOS5V/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/324PPNSCMQIUYDWVKMAKTBOS5V/action/timestamp_anchor","attest_storage":"https://pith.science/pith/324PPNSCMQIUYDWVKMAKTBOS5V/action/storage_attestation","attest_author":"https://pith.science/pith/324PPNSCMQIUYDWVKMAKTBOS5V/action/author_attestation","sign_citation":"https://pith.science/pith/324PPNSCMQIUYDWVKMAKTBOS5V/action/citation_signature","submit_replication":"https://pith.science/pith/324PPNSCMQIUYDWVKMAKTBOS5V/action/replication_record"}},"created_at":"2026-05-18T02:46:04.691199+00:00","updated_at":"2026-05-18T02:46:04.691199+00:00"}