{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:S26JT7WDX467NQLB5UMVAYTH6H","short_pith_number":"pith:S26JT7WD","schema_version":"1.0","canonical_sha256":"96bc99fec3bf3df6c161ed19506267f1c4f193867906c89cad4c0a7c5179084b","source":{"kind":"arxiv","id":"1207.1195","version":1},"attestation_state":"computed","paper":{"title":"NGC 3627: a galaxy-dwarf collision?","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.CO","authors_text":"D. J. Bomans, M. Soida, M. Wezgowiec","submitted_at":"2012-07-05T08:53:37Z","abstract_excerpt":"Group galaxies very often show distinct signs of interaction with both companion galaxies and the intragroup medium. X-ray observations are particularly helpful because they provide information on the temperatures and the densities of the hot gas in galaxies and intergalactic space. This can put important constraints on the nature and timescales of these interactions. We use the XMM-Newton X-ray observations of NGC 3627 in the Leo Triplet galaxy group to explain peculiar features visible in the polarized radio maps. We analyzed soft X-ray (0.2-1 keV) emission from NGC 3627 to study the distrib"},"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":"1207.1195","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2012-07-05T08:53:37Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"63d406451ee9e5a931fe1a7400ab94b60415d5a50c462d2b7d7fe412c9bca4ab","abstract_canon_sha256":"8cdfb48dce3ac59b3c0c6ce2cf0c5892146d1e30ca9f060dbcaded45b3b60bff"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:56:34.487297Z","signature_b64":"FD3Inv1zz8lhWPv/Kjh63xzJ2FFis87Byk90fzIRk3zdB6+pjrZi73F/Ko/xWLQ38J70N8IP0mRqTN/G6GSOCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"96bc99fec3bf3df6c161ed19506267f1c4f193867906c89cad4c0a7c5179084b","last_reissued_at":"2026-05-18T01:56:34.486631Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:56:34.486631Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"NGC 3627: a galaxy-dwarf collision?","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.CO","authors_text":"D. J. Bomans, M. Soida, M. Wezgowiec","submitted_at":"2012-07-05T08:53:37Z","abstract_excerpt":"Group galaxies very often show distinct signs of interaction with both companion galaxies and the intragroup medium. X-ray observations are particularly helpful because they provide information on the temperatures and the densities of the hot gas in galaxies and intergalactic space. This can put important constraints on the nature and timescales of these interactions. We use the XMM-Newton X-ray observations of NGC 3627 in the Leo Triplet galaxy group to explain peculiar features visible in the polarized radio maps. We analyzed soft X-ray (0.2-1 keV) emission from NGC 3627 to study the distrib"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1207.1195","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":"1207.1195","created_at":"2026-05-18T01:56:34.486730+00:00"},{"alias_kind":"arxiv_version","alias_value":"1207.1195v1","created_at":"2026-05-18T01:56:34.486730+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1207.1195","created_at":"2026-05-18T01:56:34.486730+00:00"},{"alias_kind":"pith_short_12","alias_value":"S26JT7WDX467","created_at":"2026-05-18T12:27:20.899486+00:00"},{"alias_kind":"pith_short_16","alias_value":"S26JT7WDX467NQLB","created_at":"2026-05-18T12:27:20.899486+00:00"},{"alias_kind":"pith_short_8","alias_value":"S26JT7WD","created_at":"2026-05-18T12:27:20.899486+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/S26JT7WDX467NQLB5UMVAYTH6H","json":"https://pith.science/pith/S26JT7WDX467NQLB5UMVAYTH6H.json","graph_json":"https://pith.science/api/pith-number/S26JT7WDX467NQLB5UMVAYTH6H/graph.json","events_json":"https://pith.science/api/pith-number/S26JT7WDX467NQLB5UMVAYTH6H/events.json","paper":"https://pith.science/paper/S26JT7WD"},"agent_actions":{"view_html":"https://pith.science/pith/S26JT7WDX467NQLB5UMVAYTH6H","download_json":"https://pith.science/pith/S26JT7WDX467NQLB5UMVAYTH6H.json","view_paper":"https://pith.science/paper/S26JT7WD","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1207.1195&json=true","fetch_graph":"https://pith.science/api/pith-number/S26JT7WDX467NQLB5UMVAYTH6H/graph.json","fetch_events":"https://pith.science/api/pith-number/S26JT7WDX467NQLB5UMVAYTH6H/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/S26JT7WDX467NQLB5UMVAYTH6H/action/timestamp_anchor","attest_storage":"https://pith.science/pith/S26JT7WDX467NQLB5UMVAYTH6H/action/storage_attestation","attest_author":"https://pith.science/pith/S26JT7WDX467NQLB5UMVAYTH6H/action/author_attestation","sign_citation":"https://pith.science/pith/S26JT7WDX467NQLB5UMVAYTH6H/action/citation_signature","submit_replication":"https://pith.science/pith/S26JT7WDX467NQLB5UMVAYTH6H/action/replication_record"}},"created_at":"2026-05-18T01:56:34.486730+00:00","updated_at":"2026-05-18T01:56:34.486730+00:00"}