{"as_of":"2026-08-09T12:02:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:79a50ae653265ff5f1a65ec9f20a4ce99b2dd7b595210f01ab413bd101ef627d","coverage":[{"denominator":19,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":19,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-06T13:10:22.925231Z","state":"measured"},{"denominator":21,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":21,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-09T06:31:02.800959+00:00","state":"measured"},{"denominator":2,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":2,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-04T04:31:49.163149Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2507.20972","last_updated":"2025-07-28T16:34:11Z","snapshot_observed_at":"2026-08-09T05:39:23.831360Z","submitted_at":"2025-07-28T16:34:11Z","title":"Finetuning Stellar Spectra Foundation Models with LoRA","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2507.20972","snapshot_observed_at":"2026-08-02T23:02:30.122460Z","title":"S., & Huang, Y","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2602.15021","last_updated":"2026-07-28T17:24:14Z","snapshot_observed_at":"2026-08-02T23:02:25.719666Z","submitted_at":"2026-02-16T18:58:47Z","title":"Generalization from Low- to Moderate-Resolution Spectra with Neural Networks for Stellar Parameter Estimation: A Case Study with DESI","version":2},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-02T23:02:30.122460Z"},"links":{"cited_paper":"/paper/2507.20972","citing_paper":"/paper/2602.15021"},"observation_digest":"sha256:c9924fda2e9e2e2dfdad7dc433643ad1cff3b5143718275951d172ca43710099","observation_id":"f093f1ce-95a9-49ef-ab66-82906d78db63","resolution":{"observed_at":"2026-08-02T23:02:30.122460Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2507.20972","last_updated":"2025-07-28T16:34:11Z","snapshot_observed_at":"2026-08-09T05:39:23.831360Z","submitted_at":"2025-07-28T16:34:11Z","title":"Finetuning Stellar Spectra Foundation Models with LoRA","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2507.20972","snapshot_observed_at":"2026-08-04T04:31:49.163149Z","title":"Szalay, and Yang Huang","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.02573","last_updated":"2026-08-03T17:49:40Z","snapshot_observed_at":"2026-08-08T09:09:06.432222Z","submitted_at":"2026-08-03T17:49:40Z","title":"Foundation Models for Astrophysics","version":1},"reference_index":148,"source":"pdf_text","source_observed_at":"2026-08-04T04:31:49.163149Z"},"links":{"cited_paper":"/paper/2507.20972","citing_paper":"/paper/2608.02573"},"observation_digest":"sha256:87c21b30bad9e1f629c6b646d90bb036ec14cd302c60cac1c54547215608de23","observation_id":"86be9532-dbed-4f5d-ba5e-aadecbbcbade","resolution":{"observed_at":"2026-08-04T04:31:49.163149Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2507.20972/citation-record","integrity":"/paper/2507.20972/integrity","json":"/paper/2507.20972/citation-record.json","paper":"/paper/2507.20972"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T13:10:22.847822Z","title":"2021.3057097","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2507.20972","last_updated":"2025-07-28T16:34:11Z","snapshot_observed_at":"2026-08-09T05:39:23.831360Z","submitted_at":"2025-07-28T16:34:11Z","title":"Finetuning Stellar Spectra Foundation Models with LoRA","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-06T13:10:22.847822Z"},"links":{"citing_paper":"/paper/2507.20972"},"observation_digest":"sha256:7c17a39beef055e72a21c2d73edff3a1fbbfd55630075015f4f4c7d57d33fe93","observation_id":"057fb720-d857-4262-a52d-c50e60a431a6","resolution":{"observed_at":"2026-08-06T13:10:22.847822Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T13:10:22.863875Z","title":"Ness, M., Hogg, D","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.20972","last_updated":"2025-07-28T16:34:11Z","snapshot_observed_at":"2026-08-09T05:39:23.831360Z","submitted_at":"2025-07-28T16:34:11Z","title":"Finetuning Stellar Spectra Foundation Models with LoRA","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-06T13:10:22.863875Z"},"links":{"citing_paper":"/paper/2507.20972"},"observation_digest":"sha256:6cafe6b9cb48bb0879ad9e6fcdce996b9577c333bcd317b147552512409dbe42","observation_id":"baf3cd74-da72-421e-bba4-95ca1e3d1dba","resolution":{"observed_at":"2026-08-06T13:10:22.863875Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2103.00020","last_updated":"2021-02-26T19:04:58Z","snapshot_observed_at":"2026-07-06T10:45:03.059688Z","submitted_at":"2021-02-26T19:04:58Z","title":"Learning Transferable Visual Models From Natural Language Supervision","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2103.00020","snapshot_observed_at":"2026-08-06T13:10:22.884115Z","title":"Radford, A., Kim, J","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.20972","last_updated":"2025-07-28T16:34:11Z","snapshot_observed_at":"2026-08-09T05:39:23.831360Z","submitted_at":"2025-07-28T16:34:11Z","title":"Finetuning Stellar Spectra Foundation Models with LoRA","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-06T13:10:22.884115Z"},"links":{"cited_paper":"/paper/2103.00020","citing_paper":"/paper/2507.20972"},"observation_digest":"sha256:26b8050b7365adc6f39352273aa62d4f14936e31bda988966dfbbec8b6583270","observation_id":"73d821d1-0216-4dbf-abfb-9a1dc012c448","resolution":{"observed_at":"2026-08-06T13:10:22.884115Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2103.00020","last_updated":"2021-02-26T19:04:58Z","snapshot_observed_at":"2026-07-06T10:45:03.059688Z","submitted_at":"2021-02-26T19:04:58Z","title":"Learning Transferable Visual Models From Natural Language Supervision","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2103.00020","snapshot_observed_at":"2026-08-06T13:10:22.890567Z","title":"R´o˙za´nski, T., Ting, Y .-S., and Jabło´nska, M","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.20972","last_updated":"2025-07-28T16:34:11Z","snapshot_observed_at":"2026-08-09T05:39:23.831360Z","submitted_at":"2025-07-28T16:34:11Z","title":"Finetuning Stellar Spectra Foundation Models with LoRA","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-06T13:10:22.890567Z"},"links":{"cited_paper":"/paper/2103.00020","citing_paper":"/paper/2507.20972"},"observation_digest":"sha256:50f8d249a03b2af7cd599100b86adaed17050b728e5f08a0a355abdbef5539c9","observation_id":"0e6ebcd6-f6fa-4918-bdaf-f8c7aaaaa674","resolution":{"observed_at":"2026-08-06T13:10:22.890567Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T13:10:22.908516Z","title":"Xiang, M","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.20972","last_updated":"2025-07-28T16:34:11Z","snapshot_observed_at":"2026-08-09T05:39:23.831360Z","submitted_at":"2025-07-28T16:34:11Z","title":"Finetuning Stellar Spectra Foundation Models with LoRA","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-06T13:10:22.908516Z"},"links":{"citing_paper":"/paper/2507.20972"},"observation_digest":"sha256:3e0c2e5994ef81a2d08e3a38ddb1dbb2cc896d7409dc5dcec86a9dc7cf683bca","observation_id":"249388ef-ac5a-4af0-97fd-5991ef3f3d1f","resolution":{"observed_at":"2026-08-06T13:10:22.908516Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T13:10:22.914700Z","title":"Zhang, M., Xiang, M., Ting, Y .-S., Wang, J., Li, H., Zou, H., Nie, J., Mou, L., Wu, T., Wu, Y ., and Liu, J","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.20972","last_updated":"2025-07-28T16:34:11Z","snapshot_observed_at":"2026-08-09T05:39:23.831360Z","submitted_at":"2025-07-28T16:34:11Z","title":"Finetuning Stellar Spectra Foundation Models with LoRA","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-06T13:10:22.914700Z"},"links":{"citing_paper":"/paper/2507.20972"},"observation_digest":"sha256:95cd17b4e292bf35a8d062b2a9cb0a2732da6c85bc01089cb7c26c02720e004c","observation_id":"e3dd5ad3-24d4-49fa-9ef1-535d7ca79990","resolution":{"observed_at":"2026-08-06T13:10:22.914700Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T13:10:22.920121Z","title":"Zhao, X., Huang, Y ., Xue, G., Kong, X., Liu, J., Tang, X., Beers, T","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.20972","last_updated":"2025-07-28T16:34:11Z","snapshot_observed_at":"2026-08-09T05:39:23.831360Z","submitted_at":"2025-07-28T16:34:11Z","title":"Finetuning Stellar Spectra Foundation Models with LoRA","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-06T13:10:22.920121Z"},"links":{"citing_paper":"/paper/2507.20972"},"observation_digest":"sha256:08f184749540063b293c3e29ce2ca5b53de6ce4454a0b825bf2188da9f205735","observation_id":"acebe60f-3ee1-4429-b853-d7900de5a1d4","resolution":{"observed_at":"2026-08-06T13:10:22.920121Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T13:10:22.925231Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.20972","last_updated":"2025-07-28T16:34:11Z","snapshot_observed_at":"2026-08-09T05:39:23.831360Z","submitted_at":"2025-07-28T16:34:11Z","title":"Finetuning Stellar Spectra Foundation Models with LoRA","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-06T13:10:22.925231Z"},"links":{"citing_paper":"/paper/2507.20972"},"observation_digest":"sha256:7e67f07097fdc5887cb353a517931aa531f72d7331de891c0b597322690e09ee","observation_id":"ae201a59-502f-446f-b2b2-436ab31dadb0","resolution":{"observed_at":"2026-08-06T13:10:22.925231Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2106.09685","last_updated":"2021-10-16T18:40:34Z","snapshot_observed_at":"2026-08-07T07:43:16.294957Z","submitted_at":"2021-06-17T17:37:18Z","title":"LoRA: Low-Rank Adaptation of Large Language Models","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2106.09685","snapshot_observed_at":"2026-08-06T13:10:22.834491Z","title":"J., Shen, Y ., Wallis, P., Allen-Zhu, Z., Li, Y ., Wang, S., Wang, L., and Chen, W","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.20972","last_updated":"2025-07-28T16:34:11Z","snapshot_observed_at":"2026-08-09T05:39:23.831360Z","submitted_at":"2025-07-28T16:34:11Z","title":"Finetuning Stellar Spectra Foundation Models with LoRA","version":1},"reference_index":1983,"source":"pdf_text","source_observed_at":"2026-08-06T13:10:22.834491Z"},"links":{"cited_paper":"/paper/2106.09685","citing_paper":"/paper/2507.20972"},"observation_digest":"sha256:51773fc50960e6570929f0b206577716b679ef2a3048767a655b6d0650e1dc12","observation_id":"658ab082-cfeb-4e45-bf7c-bdd41abd39a5","resolution":{"observed_at":"2026-08-06T13:10:22.834491Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T13:10:22.858478Z","title":"Koposov, S","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.20972","last_updated":"2025-07-28T16:34:11Z","snapshot_observed_at":"2026-08-09T05:39:23.831360Z","submitted_at":"2025-07-28T16:34:11Z","title":"Finetuning Stellar Spectra Foundation Models with LoRA","version":1},"reference_index":2009,"source":"pdf_text","source_observed_at":"2026-08-06T13:10:22.858478Z"},"links":{"citing_paper":"/paper/2507.20972"},"observation_digest":"sha256:ec8db90e1cd9bd624423d2c896b9cfc018a720e959dffb62c65582d181c655d5","observation_id":"536b0858-6565-4004-80d3-a7546d5d4f5d","resolution":{"observed_at":"2026-08-06T13:10:22.858478Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T13:10:22.822351Z","title":"URL https://doi.org/ 10.1117/12.2057445","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.20972","last_updated":"2025-07-28T16:34:11Z","snapshot_observed_at":"2026-08-09T05:39:23.831360Z","submitted_at":"2025-07-28T16:34:11Z","title":"Finetuning Stellar Spectra Foundation Models with LoRA","version":1},"reference_index":2014,"source":"pdf_text","source_observed_at":"2026-08-06T13:10:22.822351Z"},"links":{"citing_paper":"/paper/2507.20972"},"observation_digest":"sha256:f5c63916f2fc4530e30aa37ae74e45be9af3e7117f8278c5ed2e8ac6d1abadb9","observation_id":"92e61e26-79a4-497f-84de-9f85d7d084d5","resolution":{"observed_at":"2026-08-06T13:10:22.822351Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T13:10:22.869551Z","title":"Nikutta, R., Fitzpatrick, M., Scott, A., and Weaver, B","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.20972","last_updated":"2025-07-28T16:34:11Z","snapshot_observed_at":"2026-08-09T05:39:23.831360Z","submitted_at":"2025-07-28T16:34:11Z","title":"Finetuning Stellar Spectra Foundation Models with LoRA","version":1},"reference_index":2015,"source":"pdf_text","source_observed_at":"2026-08-06T13:10:22.869551Z"},"links":{"citing_paper":"/paper/2507.20972"},"observation_digest":"sha256:eb16ed3d80c31f24506fe31613b950eca37c3467d70e9e58237a7c22a6305e1e","observation_id":"d4b7cb5f-eb77-4adb-83b9-c592bf503ef6","resolution":{"observed_at":"2026-08-06T13:10:22.869551Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1810.04805","last_updated":"2019-05-24T20:37:26Z","snapshot_observed_at":"2026-07-30T09:12:38.100527Z","submitted_at":"2018-10-11T00:50:01Z","title":"BERT: Pre-training of Deep Bidirectional Transformers for Language Understanding","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1810.04805","snapshot_observed_at":"2026-08-06T13:10:22.817158Z","title":"1810.04805","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.20972","last_updated":"2025-07-28T16:34:11Z","snapshot_observed_at":"2026-08-09T05:39:23.831360Z","submitted_at":"2025-07-28T16:34:11Z","title":"Finetuning Stellar Spectra Foundation Models with LoRA","version":1},"reference_index":2018,"source":"pdf_text","source_observed_at":"2026-08-06T13:10:22.817158Z"},"links":{"cited_paper":"/paper/1810.04805","citing_paper":"/paper/2507.20972"},"observation_digest":"sha256:2c9a513e4b53a18890b52bb986fe905aae72f58d370219fb1f4f38774e075d2e","observation_id":"35e5c145-e791-48d6-86b1-4fa7ced2a18b","resolution":{"observed_at":"2026-08-06T13:10:22.817158Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T13:10:22.902394Z","title":"Xiang, M., Ting, Y .-S., Rix, H.-W., Sandford, N., Buder, S., Lind, K., Liu, X.-W., Shi, J.-R., and Zhang, H.-W","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.20972","last_updated":"2025-07-28T16:34:11Z","snapshot_observed_at":"2026-08-09T05:39:23.831360Z","submitted_at":"2025-07-28T16:34:11Z","title":"Finetuning Stellar Spectra Foundation Models with LoRA","version":1},"reference_index":2019,"source":"pdf_text","source_observed_at":"2026-08-06T13:10:22.902394Z"},"links":{"citing_paper":"/paper/2507.20972"},"observation_digest":"sha256:38cdddaefc572c3b7a6e9bbb437897b52dd488c2eb4d3add3cc822b7c0db0900","observation_id":"391ba551-3a76-4617-a15d-12eb28af5026","resolution":{"observed_at":"2026-08-06T13:10:22.902394Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T13:10:22.876346Z","title":"doi: https://doi.org/10.1016/j.ascom.2020.100411","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2507.20972","last_updated":"2025-07-28T16:34:11Z","snapshot_observed_at":"2026-08-09T05:39:23.831360Z","submitted_at":"2025-07-28T16:34:11Z","title":"Finetuning Stellar Spectra Foundation Models with LoRA","version":1},"reference_index":2020,"source":"pdf_text","source_observed_at":"2026-08-06T13:10:22.876346Z"},"links":{"citing_paper":"/paper/2507.20972"},"observation_digest":"sha256:f1eaadad5267cdbe205883646dfb437953c996edcc4b5294120fedfd4adc6702","observation_id":"a0217b25-5cc8-46ce-b386-f1d9e52f9d6c","resolution":{"observed_at":"2026-08-06T13:10:22.876346Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T13:10:22.839661Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.20972","last_updated":"2025-07-28T16:34:11Z","snapshot_observed_at":"2026-08-09T05:39:23.831360Z","submitted_at":"2025-07-28T16:34:11Z","title":"Finetuning Stellar Spectra Foundation Models with LoRA","version":1},"reference_index":2021,"source":"pdf_text","source_observed_at":"2026-08-06T13:10:22.839661Z"},"links":{"citing_paper":"/paper/2507.20972"},"observation_digest":"sha256:b1a92eca428dd74ca74f9220c8a1e6159d399bde9776e85ab5309c551af97b18","observation_id":"df313894-781b-41df-b74e-92fb338bef6d","resolution":{"observed_at":"2026-08-06T13:10:22.839661Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1810.04805","last_updated":"2019-05-24T20:37:26Z","snapshot_observed_at":"2026-07-30T09:12:38.100527Z","submitted_at":"2018-10-11T00:50:01Z","title":"BERT: Pre-training of Deep Bidirectional Transformers for Language Understanding","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1810.04805","snapshot_observed_at":"2026-08-06T13:10:22.810294Z","title":"Devlin, J., Chang, M.-W., Lee, K., and Toutanova, K","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.20972","last_updated":"2025-07-28T16:34:11Z","snapshot_observed_at":"2026-08-09T05:39:23.831360Z","submitted_at":"2025-07-28T16:34:11Z","title":"Finetuning Stellar Spectra Foundation Models with LoRA","version":1},"reference_index":2022,"source":"pdf_text","source_observed_at":"2026-08-06T13:10:22.810294Z"},"links":{"cited_paper":"/paper/1810.04805","citing_paper":"/paper/2507.20972"},"observation_digest":"sha256:f89222ac7192487b3bfd2f289f0b83a6bfbbba4bf873c2d2266b48b56b19f1e2","observation_id":"d2de5298-6b78-4601-802a-d71f05b25c3b","resolution":{"observed_at":"2026-08-06T13:10:22.810294Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T13:10:22.828692Z","title":"Hoaglin, D","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.20972","last_updated":"2025-07-28T16:34:11Z","snapshot_observed_at":"2026-08-09T05:39:23.831360Z","submitted_at":"2025-07-28T16:34:11Z","title":"Finetuning Stellar Spectra Foundation Models with LoRA","version":1},"reference_index":2023,"source":"pdf_text","source_observed_at":"2026-08-06T13:10:22.828692Z"},"links":{"citing_paper":"/paper/2507.20972"},"observation_digest":"sha256:9259b6947c8378c1bd4673f8ed935eb4fb47b79878253599f83332d489d62906","observation_id":"923c1961-2cd3-44f3-978f-bf85879f3889","resolution":{"observed_at":"2026-08-06T13:10:22.828692Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2401.05576","last_updated":"2025-02-10T22:55:14Z","snapshot_observed_at":"2026-08-05T19:49:28.448011Z","submitted_at":"2024-01-10T23:00:03Z","title":"SPARCL: SPectra Analysis and Retrievable Catalog Lab","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2401.05576","snapshot_observed_at":"2026-08-06T13:10:22.852946Z","title":"Koleva, M., Prugniel, P., Bouchard, A., and Wu, Y","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.20972","last_updated":"2025-07-28T16:34:11Z","snapshot_observed_at":"2026-08-09T05:39:23.831360Z","submitted_at":"2025-07-28T16:34:11Z","title":"Finetuning Stellar Spectra Foundation Models with LoRA","version":1},"reference_index":2024,"source":"pdf_text","source_observed_at":"2026-08-06T13:10:22.852946Z"},"links":{"cited_paper":"/paper/2401.05576","citing_paper":"/paper/2507.20972"},"observation_digest":"sha256:18bf30b6521316b050818d3c306cdcd2b6b7711422aeac4bb5288ab8ae201d05","observation_id":"010b8760-79d7-4272-a530-6b319c09cbb5","resolution":{"observed_at":"2026-08-06T13:10:22.852946Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2507.20972","last_updated":"2025-07-28T16:34:11Z","latest_version":1,"primary_category":"astro-ph.IM","snapshot_observed_at":"2026-08-09T05:39:23.831360Z","submitted_at":"2025-07-28T16:34:11Z","title":"Finetuning Stellar Spectra Foundation Models with LoRA"},"reference_resolution":{"displayed":19,"state_counts":{"malformed_identifier":3,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":16,"verified_exact":0,"verified_fuzzy":0},"total_outbound_references":19},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"thesis":"As of 9 August 2026, this Paper Citation Record lists 19 of 19 outbound references and 2 inbound Pith citation observations for arXiv:2507.20972."}