{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:SEAMY5AYEHWS6A7KQ3VR77PMMJ","short_pith_number":"pith:SEAMY5AY","schema_version":"1.0","canonical_sha256":"9100cc741821ed2f03ea86eb1ffdec6244e511a9baf59db8b5d7670066208348","source":{"kind":"arxiv","id":"2208.01650","version":4},"attestation_state":"computed","paper":{"title":"Planetary parameters, XUV environments and mass-loss rates for nearby gaseous planets with X-ray detected host-stars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"A. Caldiroli, E. Gallo, E. Rauscher, F. Biassoni, F. Borsa, F. Haardt, R. Spinelli","submitted_at":"2022-08-02T18:00:00Z","abstract_excerpt":"We leverage Gaia DR2 parallactic distances to deliver new or revised estimates of planetary parameters and X-ray irradiation for a distance-limited ($\\lesssim 100$ pc) sample of 27 gaseous planets (from super-Earths to hot Jupiters) with publicly available Chandra and/or XMM observations, for which we carry out a homogeneous data reduction. For 20 planets with X-ray detected host stars we make use of the photoionization hydrodynamics code ATES to derive updated atmospheric mass outflow rates. The newly derived masses/radii are not consistent with the exoplanet.eu values for five systems; HD 14"},"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":"2208.01650","kind":"arxiv","version":4},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2022-08-02T18:00:00Z","cross_cats_sorted":[],"title_canon_sha256":"3a8ff9e1f6d0f3b4fcbf6fbae45dffa558695e47eb24ad9ae49d7774f0b4cb87","abstract_canon_sha256":"1cf3f5eaa270a26388d180e68e89c0b8bc1ad7b8f959b0d3d29f5e5c5a99cee4"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T06:03:56.326560Z","signature_b64":"8J3NZRfNY7sWkA3qNTW99cRnRfNc4BlYkTIAYqyjOgDNZEPmzaoXbjzM9gNDyV6c97kSG9sHg5fZNQd3XVJUCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9100cc741821ed2f03ea86eb1ffdec6244e511a9baf59db8b5d7670066208348","last_reissued_at":"2026-07-05T06:03:56.326062Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T06:03:56.326062Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Planetary parameters, XUV environments and mass-loss rates for nearby gaseous planets with X-ray detected host-stars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"A. Caldiroli, E. Gallo, E. Rauscher, F. Biassoni, F. Borsa, F. Haardt, R. Spinelli","submitted_at":"2022-08-02T18:00:00Z","abstract_excerpt":"We leverage Gaia DR2 parallactic distances to deliver new or revised estimates of planetary parameters and X-ray irradiation for a distance-limited ($\\lesssim 100$ pc) sample of 27 gaseous planets (from super-Earths to hot Jupiters) with publicly available Chandra and/or XMM observations, for which we carry out a homogeneous data reduction. For 20 planets with X-ray detected host stars we make use of the photoionization hydrodynamics code ATES to derive updated atmospheric mass outflow rates. The newly derived masses/radii are not consistent with the exoplanet.eu values for five systems; HD 14"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2208.01650","kind":"arxiv","version":4},"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/2208.01650/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":"2208.01650","created_at":"2026-07-05T06:03:56.326128+00:00"},{"alias_kind":"arxiv_version","alias_value":"2208.01650v4","created_at":"2026-07-05T06:03:56.326128+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2208.01650","created_at":"2026-07-05T06:03:56.326128+00:00"},{"alias_kind":"pith_short_12","alias_value":"SEAMY5AYEHWS","created_at":"2026-07-05T06:03:56.326128+00:00"},{"alias_kind":"pith_short_16","alias_value":"SEAMY5AYEHWS6A7K","created_at":"2026-07-05T06:03:56.326128+00:00"},{"alias_kind":"pith_short_8","alias_value":"SEAMY5AY","created_at":"2026-07-05T06:03:56.326128+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/SEAMY5AYEHWS6A7KQ3VR77PMMJ","json":"https://pith.science/pith/SEAMY5AYEHWS6A7KQ3VR77PMMJ.json","graph_json":"https://pith.science/api/pith-number/SEAMY5AYEHWS6A7KQ3VR77PMMJ/graph.json","events_json":"https://pith.science/api/pith-number/SEAMY5AYEHWS6A7KQ3VR77PMMJ/events.json","paper":"https://pith.science/paper/SEAMY5AY"},"agent_actions":{"view_html":"https://pith.science/pith/SEAMY5AYEHWS6A7KQ3VR77PMMJ","download_json":"https://pith.science/pith/SEAMY5AYEHWS6A7KQ3VR77PMMJ.json","view_paper":"https://pith.science/paper/SEAMY5AY","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2208.01650&json=true","fetch_graph":"https://pith.science/api/pith-number/SEAMY5AYEHWS6A7KQ3VR77PMMJ/graph.json","fetch_events":"https://pith.science/api/pith-number/SEAMY5AYEHWS6A7KQ3VR77PMMJ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/SEAMY5AYEHWS6A7KQ3VR77PMMJ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/SEAMY5AYEHWS6A7KQ3VR77PMMJ/action/storage_attestation","attest_author":"https://pith.science/pith/SEAMY5AYEHWS6A7KQ3VR77PMMJ/action/author_attestation","sign_citation":"https://pith.science/pith/SEAMY5AYEHWS6A7KQ3VR77PMMJ/action/citation_signature","submit_replication":"https://pith.science/pith/SEAMY5AYEHWS6A7KQ3VR77PMMJ/action/replication_record"}},"created_at":"2026-07-05T06:03:56.326128+00:00","updated_at":"2026-07-05T06:03:56.326128+00:00"}