{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:QYELPAFLLUAPKLBL74P263Z7OQ","short_pith_number":"pith:QYELPAFL","schema_version":"1.0","canonical_sha256":"8608b780ab5d00f52c2bff1faf6f3f74145a7a39acf50fc52987b2dd09df22d7","source":{"kind":"arxiv","id":"2502.19961","version":2},"attestation_state":"computed","paper":{"title":"High-contrast spectroscopy with the new VLT/ERIS instrument: Molecular maps and radial velocity of the gas giant AF Lep b","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.IM"],"primary_cat":"astro-ph.EP","authors_text":"Adrian Glauser, Alexander Agudo Berbel, Alfio Puglisi, Amico Di Cianno, Andrea Baruffolo, Angelo Valentini, Armando Riccardi, Bernardo Salasnich, Christian Rau, Christopher Waring, Christoph Keller, Daniela Fantinel, David Doelman, David Henry, David Lunney, David Pearson, Debora Ferruzzi, Dieter Lutz, Eckhard Sturm, Emily Omaya Garvin, Erich Wiezorrek, Felix Dannert, Filippo Manucci, Frank Eisenhauer, Frans Snik, Gabriele Cugno, Gianluca Di Rico, Gilles Orban De Xivry, Giovanni Cresci, Guido Agapito, Hans Martin Schmid, Heinrich Huber, Helmut Feuchtgruber, Ivan Di Antonio, Jean Hayoz, John Lightfoot, Kateryna Kravchenko, Linda Tacconi, Luca Carbonaro, Marco Bonaglia, Marco Xompero, Markus Johannes Bonse, Martin Black, Matthew Kenworthy, Matthias Deysenroth, Mauro Dolci, Michael Hartl, Mike MacIntosh, Natascha F\\\"orster-Schreiber, Olivier Absil, Paolo Grani, Polychronis Patapis, Reinhard Genzel, Richard Davies, Robert J. De Rosa, Runa Briguglio, Sascha Patrick Quanz, Sebastian Rabien, Simone Esposito, Stefan Gillessen, Taro Shimizu, Thomas Ott, Timothy D. Gebhard, Tomas Stolker, William O. Balmer, William Taylor, Xiaofeng Gao, Yigit Dallilar, Yixian Cao","submitted_at":"2025-02-27T10:36:31Z","abstract_excerpt":"The Enhanced Resolution Imager and Spectrograph (ERIS) is the new Adaptive-Optics (AO) assisted Infrared instrument at the Very Large Telescope (VLT). Its refurbished Integral Field Spectrograph (IFS) SPIFFIER leverages a new AO module, enabling high-contrast imaging applications and giving access to the orbital and atmospheric characterisation of super-Jovian exoplanets. We test the detection limits of ERIS and demonstrate its scientific potential by exploring the atmospheric composition of the young super-Jovian AF Lep b and improving its orbital solution by measuring its radial velocity rel"},"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":"2502.19961","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.EP","submitted_at":"2025-02-27T10:36:31Z","cross_cats_sorted":["astro-ph.IM"],"title_canon_sha256":"88ba5aea847b2e0999d9a002a15cea58ac45668154a9a6729e7d607ec42ab678","abstract_canon_sha256":"1cf227a3ca32dc320334e00d67c76df874efd8060e28717955eb7bab33cb0f86"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T11:16:56.071503Z","signature_b64":"1brMxybqekxYaX5aJxgD4mcd7mfW1wiVU6Bch7xgKrsxSpPiF3AKOjPqMje1cp2fBQx8vgShOQ2knXsMF/yuBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"8608b780ab5d00f52c2bff1faf6f3f74145a7a39acf50fc52987b2dd09df22d7","last_reissued_at":"2026-07-05T11:16:56.070778Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T11:16:56.070778Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"High-contrast spectroscopy with the new VLT/ERIS instrument: Molecular maps and radial velocity of the gas giant AF Lep b","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.IM"],"primary_cat":"astro-ph.EP","authors_text":"Adrian Glauser, Alexander Agudo Berbel, Alfio Puglisi, Amico Di Cianno, Andrea Baruffolo, Angelo Valentini, Armando Riccardi, Bernardo Salasnich, Christian Rau, Christopher Waring, Christoph Keller, Daniela Fantinel, David Doelman, David Henry, David Lunney, David Pearson, Debora Ferruzzi, Dieter Lutz, Eckhard Sturm, Emily Omaya Garvin, Erich Wiezorrek, Felix Dannert, Filippo Manucci, Frank Eisenhauer, Frans Snik, Gabriele Cugno, Gianluca Di Rico, Gilles Orban De Xivry, Giovanni Cresci, Guido Agapito, Hans Martin Schmid, Heinrich Huber, Helmut Feuchtgruber, Ivan Di Antonio, Jean Hayoz, John Lightfoot, Kateryna Kravchenko, Linda Tacconi, Luca Carbonaro, Marco Bonaglia, Marco Xompero, Markus Johannes Bonse, Martin Black, Matthew Kenworthy, Matthias Deysenroth, Mauro Dolci, Michael Hartl, Mike MacIntosh, Natascha F\\\"orster-Schreiber, Olivier Absil, Paolo Grani, Polychronis Patapis, Reinhard Genzel, Richard Davies, Robert J. De Rosa, Runa Briguglio, Sascha Patrick Quanz, Sebastian Rabien, Simone Esposito, Stefan Gillessen, Taro Shimizu, Thomas Ott, Timothy D. Gebhard, Tomas Stolker, William O. Balmer, William Taylor, Xiaofeng Gao, Yigit Dallilar, Yixian Cao","submitted_at":"2025-02-27T10:36:31Z","abstract_excerpt":"The Enhanced Resolution Imager and Spectrograph (ERIS) is the new Adaptive-Optics (AO) assisted Infrared instrument at the Very Large Telescope (VLT). Its refurbished Integral Field Spectrograph (IFS) SPIFFIER leverages a new AO module, enabling high-contrast imaging applications and giving access to the orbital and atmospheric characterisation of super-Jovian exoplanets. We test the detection limits of ERIS and demonstrate its scientific potential by exploring the atmospheric composition of the young super-Jovian AF Lep b and improving its orbital solution by measuring its radial velocity rel"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2502.19961","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/2502.19961/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":"2502.19961","created_at":"2026-07-05T11:16:56.070868+00:00"},{"alias_kind":"arxiv_version","alias_value":"2502.19961v2","created_at":"2026-07-05T11:16:56.070868+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2502.19961","created_at":"2026-07-05T11:16:56.070868+00:00"},{"alias_kind":"pith_short_12","alias_value":"QYELPAFLLUAP","created_at":"2026-07-05T11:16:56.070868+00:00"},{"alias_kind":"pith_short_16","alias_value":"QYELPAFLLUAPKLBL","created_at":"2026-07-05T11:16:56.070868+00:00"},{"alias_kind":"pith_short_8","alias_value":"QYELPAFL","created_at":"2026-07-05T11:16:56.070868+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2604.09152","citing_title":"Machine Learning as a Transformative Tool for (Exo-)Planetary Science","ref_index":124,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/QYELPAFLLUAPKLBL74P263Z7OQ","json":"https://pith.science/pith/QYELPAFLLUAPKLBL74P263Z7OQ.json","graph_json":"https://pith.science/api/pith-number/QYELPAFLLUAPKLBL74P263Z7OQ/graph.json","events_json":"https://pith.science/api/pith-number/QYELPAFLLUAPKLBL74P263Z7OQ/events.json","paper":"https://pith.science/paper/QYELPAFL"},"agent_actions":{"view_html":"https://pith.science/pith/QYELPAFLLUAPKLBL74P263Z7OQ","download_json":"https://pith.science/pith/QYELPAFLLUAPKLBL74P263Z7OQ.json","view_paper":"https://pith.science/paper/QYELPAFL","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2502.19961&json=true","fetch_graph":"https://pith.science/api/pith-number/QYELPAFLLUAPKLBL74P263Z7OQ/graph.json","fetch_events":"https://pith.science/api/pith-number/QYELPAFLLUAPKLBL74P263Z7OQ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/QYELPAFLLUAPKLBL74P263Z7OQ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/QYELPAFLLUAPKLBL74P263Z7OQ/action/storage_attestation","attest_author":"https://pith.science/pith/QYELPAFLLUAPKLBL74P263Z7OQ/action/author_attestation","sign_citation":"https://pith.science/pith/QYELPAFLLUAPKLBL74P263Z7OQ/action/citation_signature","submit_replication":"https://pith.science/pith/QYELPAFLLUAPKLBL74P263Z7OQ/action/replication_record"}},"created_at":"2026-07-05T11:16:56.070868+00:00","updated_at":"2026-07-05T11:16:56.070868+00:00"}