{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:X4N3N3GPZSL2KQVG3AUJI53HDV","short_pith_number":"pith:X4N3N3GP","schema_version":"1.0","canonical_sha256":"bf1bb6eccfcc97a542a6d8289477671d775a1a0bcbdb414cdf9dd62ae5283a6d","source":{"kind":"arxiv","id":"2210.05763","version":2},"attestation_state":"computed","paper":{"title":"GOALS-JWST: Revealing the Buried Star Clusters in the Luminous Infrared Galaxy VV 114","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Aaron S. Evans, Anne M. Medling, Christopher C. Hayward, David Law, David Sanders, David T. Frayer, Eric J. Murphy, Francisca Kemper, George C. Privon, Hanae Inami, Jason Marshall, Jason Surace, Jeffrey A. Rich, Joseph M. Mazzarella, Justin H. Howell, Kazushi Iwasawa, Kirsten L. Larson, Lee Armus, Loreto Barcos-Mu\\~noz, Matthew A. Malkan, Michael J. I. Brown, Paul van der Werf, Philip Appleton, Sabrina Stierwalt, Sean T. Linden, Susanne Aalto, Tanio Diaz-Santos, Thomas Bohn, Thomas Lai, Torsten B\\\"oker, Vassilis Charmandaris, Vivian U, Yiqing Song","submitted_at":"2022-10-11T20:16:21Z","abstract_excerpt":"We present the results of a {\\it James Webb Space Telescope} NIRCam investigation into the young massive star cluster (YMC) population in the luminous infrared galaxy VV 114. We identify 374 compact YMC candidates with a $S/N \\geq 3$, 5, and 5 at F150W, F200W, and F356W respectively. A direct comparison with our {\\it HST} cluster catalog reveals that $\\sim 20\\%$ of these sources are undetected at optical wavelengths. Based on {\\it yggdrasil} stellar population models, we identify 17 YMC candidates in our {\\it JWST} imaging alone with F150W-F200W and F200W-F356W colors suggesting they are all v"},"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":"2210.05763","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.GA","submitted_at":"2022-10-11T20:16:21Z","cross_cats_sorted":[],"title_canon_sha256":"8715f69f13c5fa0f836adb58f878a3656b83b36ca9e083e84c31f269a58737db","abstract_canon_sha256":"753f14d588fb9652c84bf460ad7c5858c4de6c8d09a7f8cef39726a196465689"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T05:46:25.524373Z","signature_b64":"lT+B81j0i6qDGtDuWbPjVnHpLj7KzYqwwKyjxCzIUqQKzS62kPYqx7lTsMiiEzTi8X3Z8Lv8f9ZlrppAvPblAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"bf1bb6eccfcc97a542a6d8289477671d775a1a0bcbdb414cdf9dd62ae5283a6d","last_reissued_at":"2026-07-05T05:46:25.523913Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T05:46:25.523913Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"GOALS-JWST: Revealing the Buried Star Clusters in the Luminous Infrared Galaxy VV 114","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Aaron S. Evans, Anne M. Medling, Christopher C. Hayward, David Law, David Sanders, David T. Frayer, Eric J. Murphy, Francisca Kemper, George C. Privon, Hanae Inami, Jason Marshall, Jason Surace, Jeffrey A. Rich, Joseph M. Mazzarella, Justin H. Howell, Kazushi Iwasawa, Kirsten L. Larson, Lee Armus, Loreto Barcos-Mu\\~noz, Matthew A. Malkan, Michael J. I. Brown, Paul van der Werf, Philip Appleton, Sabrina Stierwalt, Sean T. Linden, Susanne Aalto, Tanio Diaz-Santos, Thomas Bohn, Thomas Lai, Torsten B\\\"oker, Vassilis Charmandaris, Vivian U, Yiqing Song","submitted_at":"2022-10-11T20:16:21Z","abstract_excerpt":"We present the results of a {\\it James Webb Space Telescope} NIRCam investigation into the young massive star cluster (YMC) population in the luminous infrared galaxy VV 114. We identify 374 compact YMC candidates with a $S/N \\geq 3$, 5, and 5 at F150W, F200W, and F356W respectively. A direct comparison with our {\\it HST} cluster catalog reveals that $\\sim 20\\%$ of these sources are undetected at optical wavelengths. Based on {\\it yggdrasil} stellar population models, we identify 17 YMC candidates in our {\\it JWST} imaging alone with F150W-F200W and F200W-F356W colors suggesting they are all v"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2210.05763","kind":"arxiv","version":2},"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/2210.05763/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":"2210.05763","created_at":"2026-07-05T05:46:25.523964+00:00"},{"alias_kind":"arxiv_version","alias_value":"2210.05763v2","created_at":"2026-07-05T05:46:25.523964+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2210.05763","created_at":"2026-07-05T05:46:25.523964+00:00"},{"alias_kind":"pith_short_12","alias_value":"X4N3N3GPZSL2","created_at":"2026-07-05T05:46:25.523964+00:00"},{"alias_kind":"pith_short_16","alias_value":"X4N3N3GPZSL2KQVG","created_at":"2026-07-05T05:46:25.523964+00:00"},{"alias_kind":"pith_short_8","alias_value":"X4N3N3GP","created_at":"2026-07-05T05:46:25.523964+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/X4N3N3GPZSL2KQVG3AUJI53HDV","json":"https://pith.science/pith/X4N3N3GPZSL2KQVG3AUJI53HDV.json","graph_json":"https://pith.science/api/pith-number/X4N3N3GPZSL2KQVG3AUJI53HDV/graph.json","events_json":"https://pith.science/api/pith-number/X4N3N3GPZSL2KQVG3AUJI53HDV/events.json","paper":"https://pith.science/paper/X4N3N3GP"},"agent_actions":{"view_html":"https://pith.science/pith/X4N3N3GPZSL2KQVG3AUJI53HDV","download_json":"https://pith.science/pith/X4N3N3GPZSL2KQVG3AUJI53HDV.json","view_paper":"https://pith.science/paper/X4N3N3GP","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2210.05763&json=true","fetch_graph":"https://pith.science/api/pith-number/X4N3N3GPZSL2KQVG3AUJI53HDV/graph.json","fetch_events":"https://pith.science/api/pith-number/X4N3N3GPZSL2KQVG3AUJI53HDV/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/X4N3N3GPZSL2KQVG3AUJI53HDV/action/timestamp_anchor","attest_storage":"https://pith.science/pith/X4N3N3GPZSL2KQVG3AUJI53HDV/action/storage_attestation","attest_author":"https://pith.science/pith/X4N3N3GPZSL2KQVG3AUJI53HDV/action/author_attestation","sign_citation":"https://pith.science/pith/X4N3N3GPZSL2KQVG3AUJI53HDV/action/citation_signature","submit_replication":"https://pith.science/pith/X4N3N3GPZSL2KQVG3AUJI53HDV/action/replication_record"}},"created_at":"2026-07-05T05:46:25.523964+00:00","updated_at":"2026-07-05T05:46:25.523964+00:00"}