{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:6D7HCPCLZD6ILYSCUXMIKT6NWS","short_pith_number":"pith:6D7HCPCL","schema_version":"1.0","canonical_sha256":"f0fe713c4bc8fc85e242a5d8854fcdb48133e2304878a42155cd096c206d7552","source":{"kind":"arxiv","id":"2506.21335","version":1},"attestation_state":"computed","paper":{"title":"Investigating the clumpy star formation in an interacting dwarf irregular galaxy","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Ana L. Chies-Santos, Ariel Werle, Augusto E. Lassen, Boris H\\\"au{\\ss}ler, Daniel Ruschel-Dutra, Eleazar R. Carrasco, Evelyn J. Johnston, Gabriel M. Azevedo, Jean M. Gomes, Rogemar A. Riffel, Rogerio Riffel, Rubens E. G. Machado","submitted_at":"2025-06-26T14:46:43Z","abstract_excerpt":"Clumpy morphologies are more frequent in distant and low-mass star-forming galaxies. Therefore the less numerous nearby galaxies presenting kpc-sized clumps represent unique laboratories from which to address the mechanisms driving clump formation and study why such structures become less common in the local Universe, and why they tend to exhibit smaller sizes and lower star formation rates compared to their high-$z$ counterparts. We use high spatial resolution Integral Field Unit observations from VLT/MUSE to investigate the properties of several kpc-sized clumps seen in SDSS J020536-081424, "},"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":"2506.21335","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2025-06-26T14:46:43Z","cross_cats_sorted":[],"title_canon_sha256":"cd701e84ef13555482aa2dd66941e533800364cef5b12448d654ce6ba88dfbb6","abstract_canon_sha256":"f5f4fc2bae55f34c6daff9ec4e782316ddf67aa0467000b52e00c69cf9beb5bf"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T11:27:43.885441Z","signature_b64":"H0B/Ze+j3+tsbOJd6S66yXicxurckaHictpO/RNRHORG38LUN7G+VmMCGCVx9V+sPk5gu7yRNJjrB/L4Og6ZDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f0fe713c4bc8fc85e242a5d8854fcdb48133e2304878a42155cd096c206d7552","last_reissued_at":"2026-07-05T11:27:43.884733Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T11:27:43.884733Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Investigating the clumpy star formation in an interacting dwarf irregular galaxy","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Ana L. Chies-Santos, Ariel Werle, Augusto E. Lassen, Boris H\\\"au{\\ss}ler, Daniel Ruschel-Dutra, Eleazar R. Carrasco, Evelyn J. Johnston, Gabriel M. Azevedo, Jean M. Gomes, Rogemar A. Riffel, Rogerio Riffel, Rubens E. G. Machado","submitted_at":"2025-06-26T14:46:43Z","abstract_excerpt":"Clumpy morphologies are more frequent in distant and low-mass star-forming galaxies. Therefore the less numerous nearby galaxies presenting kpc-sized clumps represent unique laboratories from which to address the mechanisms driving clump formation and study why such structures become less common in the local Universe, and why they tend to exhibit smaller sizes and lower star formation rates compared to their high-$z$ counterparts. We use high spatial resolution Integral Field Unit observations from VLT/MUSE to investigate the properties of several kpc-sized clumps seen in SDSS J020536-081424, "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2506.21335","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/2506.21335/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":"2506.21335","created_at":"2026-07-05T11:27:43.884802+00:00"},{"alias_kind":"arxiv_version","alias_value":"2506.21335v1","created_at":"2026-07-05T11:27:43.884802+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2506.21335","created_at":"2026-07-05T11:27:43.884802+00:00"},{"alias_kind":"pith_short_12","alias_value":"6D7HCPCLZD6I","created_at":"2026-07-05T11:27:43.884802+00:00"},{"alias_kind":"pith_short_16","alias_value":"6D7HCPCLZD6ILYSC","created_at":"2026-07-05T11:27:43.884802+00:00"},{"alias_kind":"pith_short_8","alias_value":"6D7HCPCL","created_at":"2026-07-05T11:27:43.884802+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/6D7HCPCLZD6ILYSCUXMIKT6NWS","json":"https://pith.science/pith/6D7HCPCLZD6ILYSCUXMIKT6NWS.json","graph_json":"https://pith.science/api/pith-number/6D7HCPCLZD6ILYSCUXMIKT6NWS/graph.json","events_json":"https://pith.science/api/pith-number/6D7HCPCLZD6ILYSCUXMIKT6NWS/events.json","paper":"https://pith.science/paper/6D7HCPCL"},"agent_actions":{"view_html":"https://pith.science/pith/6D7HCPCLZD6ILYSCUXMIKT6NWS","download_json":"https://pith.science/pith/6D7HCPCLZD6ILYSCUXMIKT6NWS.json","view_paper":"https://pith.science/paper/6D7HCPCL","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2506.21335&json=true","fetch_graph":"https://pith.science/api/pith-number/6D7HCPCLZD6ILYSCUXMIKT6NWS/graph.json","fetch_events":"https://pith.science/api/pith-number/6D7HCPCLZD6ILYSCUXMIKT6NWS/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/6D7HCPCLZD6ILYSCUXMIKT6NWS/action/timestamp_anchor","attest_storage":"https://pith.science/pith/6D7HCPCLZD6ILYSCUXMIKT6NWS/action/storage_attestation","attest_author":"https://pith.science/pith/6D7HCPCLZD6ILYSCUXMIKT6NWS/action/author_attestation","sign_citation":"https://pith.science/pith/6D7HCPCLZD6ILYSCUXMIKT6NWS/action/citation_signature","submit_replication":"https://pith.science/pith/6D7HCPCLZD6ILYSCUXMIKT6NWS/action/replication_record"}},"created_at":"2026-07-05T11:27:43.884802+00:00","updated_at":"2026-07-05T11:27:43.884802+00:00"}