{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:4UOODGVUG545FDBBMYW7FXSW4F","short_pith_number":"pith:4UOODGVU","schema_version":"1.0","canonical_sha256":"e51ce19ab43779d28c21662df2de56e153d68d142f87ab67f8e4bf412780d36d","source":{"kind":"arxiv","id":"2407.15807","version":1},"attestation_state":"computed","paper":{"title":"A biconical ionised gas outflow and evidence for positive feedback in NGC 7172 uncovered by MIRI/JWST","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Alonso-Herrero, A. Audibert, A. J. Bunker, A. Labiano, B. Garc\\'ia-Lorenzo, C. Packham, C. Ramos Almeida, C. Ricci, D. Esparza-Arredondo, D. Rigopoulou, D. Rosario, D. Rouan, E. Bellocchi, E. K. S. Hicks, E. L\\'opez-Rodr\\'iguez, F. Combes, H. Haidar, I. Garc\\'ia-Bernete, L. Fuller, L. Hermosa Mu\\~noz, L. Zhang, M. Imanishi, M.J. Ward, M. Leist, M. Pereira-Santaella, M. Stalevski, M. Villar-Mart\\'in, N.A. Levenson, O. Gonz\\'alez-Mart\\'in, P. Boorman, P. Gandhi, R. Davies, S. Campbell, S. Garc\\'ia-Burillo, S. H\\\"onig, T. D\\'iaz-Santos, T. Izumi, T. Shimizu","submitted_at":"2024-07-22T17:20:31Z","abstract_excerpt":"We present observations of the type-2 Seyfert NGC7172 obtained with the medium-resolution spectrometer (MRS) of the Mid-Infrared Instrument (MIRI) on board of the JWST. This galaxy hosts one of the lowest ionised gas mass outflow rates (Mout~0.005 M/yr) in a sample of six AGN with similar bolometric luminosities (log Lbol~44erg/s) within the Galactic Activity, Torus and Outflow Survey (GATOS). We aim to understand the properties of the ionised gas outflow, mainly using the emission lines from the neon transitions, that cover a broad range of ionisation potentials (IP) from ~20 eV to ~130 eV. W"},"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":"2407.15807","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2024-07-22T17:20:31Z","cross_cats_sorted":[],"title_canon_sha256":"11bca313b80db419dc8813a8c1b5d9ecbff1f70e66611197666bd06f04da8e66","abstract_canon_sha256":"6435b84eedf4f317345abaf6a37a5497308188eed2e22dca8cfa25e4356072ed"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T09:23:55.111393Z","signature_b64":"Cb9ZFU48Dpcu3sglBhtG7sNcjE5xZ/cVvX8lPo2k5flwA6wc+LNQPQIEDyYhkniDnhJc6afuqjQsIpLsRpSfDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e51ce19ab43779d28c21662df2de56e153d68d142f87ab67f8e4bf412780d36d","last_reissued_at":"2026-07-05T09:23:55.110891Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T09:23:55.110891Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A biconical ionised gas outflow and evidence for positive feedback in NGC 7172 uncovered by MIRI/JWST","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Alonso-Herrero, A. Audibert, A. J. Bunker, A. Labiano, B. Garc\\'ia-Lorenzo, C. Packham, C. Ramos Almeida, C. Ricci, D. Esparza-Arredondo, D. Rigopoulou, D. Rosario, D. Rouan, E. Bellocchi, E. K. S. Hicks, E. L\\'opez-Rodr\\'iguez, F. Combes, H. Haidar, I. Garc\\'ia-Bernete, L. Fuller, L. Hermosa Mu\\~noz, L. Zhang, M. Imanishi, M.J. Ward, M. Leist, M. Pereira-Santaella, M. Stalevski, M. Villar-Mart\\'in, N.A. Levenson, O. Gonz\\'alez-Mart\\'in, P. Boorman, P. Gandhi, R. Davies, S. Campbell, S. Garc\\'ia-Burillo, S. H\\\"onig, T. D\\'iaz-Santos, T. Izumi, T. Shimizu","submitted_at":"2024-07-22T17:20:31Z","abstract_excerpt":"We present observations of the type-2 Seyfert NGC7172 obtained with the medium-resolution spectrometer (MRS) of the Mid-Infrared Instrument (MIRI) on board of the JWST. This galaxy hosts one of the lowest ionised gas mass outflow rates (Mout~0.005 M/yr) in a sample of six AGN with similar bolometric luminosities (log Lbol~44erg/s) within the Galactic Activity, Torus and Outflow Survey (GATOS). We aim to understand the properties of the ionised gas outflow, mainly using the emission lines from the neon transitions, that cover a broad range of ionisation potentials (IP) from ~20 eV to ~130 eV. W"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2407.15807","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/2407.15807/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":"2407.15807","created_at":"2026-07-05T09:23:55.110951+00:00"},{"alias_kind":"arxiv_version","alias_value":"2407.15807v1","created_at":"2026-07-05T09:23:55.110951+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2407.15807","created_at":"2026-07-05T09:23:55.110951+00:00"},{"alias_kind":"pith_short_12","alias_value":"4UOODGVUG545","created_at":"2026-07-05T09:23:55.110951+00:00"},{"alias_kind":"pith_short_16","alias_value":"4UOODGVUG545FDBB","created_at":"2026-07-05T09:23:55.110951+00:00"},{"alias_kind":"pith_short_8","alias_value":"4UOODGVU","created_at":"2026-07-05T09:23:55.110951+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/4UOODGVUG545FDBBMYW7FXSW4F","json":"https://pith.science/pith/4UOODGVUG545FDBBMYW7FXSW4F.json","graph_json":"https://pith.science/api/pith-number/4UOODGVUG545FDBBMYW7FXSW4F/graph.json","events_json":"https://pith.science/api/pith-number/4UOODGVUG545FDBBMYW7FXSW4F/events.json","paper":"https://pith.science/paper/4UOODGVU"},"agent_actions":{"view_html":"https://pith.science/pith/4UOODGVUG545FDBBMYW7FXSW4F","download_json":"https://pith.science/pith/4UOODGVUG545FDBBMYW7FXSW4F.json","view_paper":"https://pith.science/paper/4UOODGVU","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2407.15807&json=true","fetch_graph":"https://pith.science/api/pith-number/4UOODGVUG545FDBBMYW7FXSW4F/graph.json","fetch_events":"https://pith.science/api/pith-number/4UOODGVUG545FDBBMYW7FXSW4F/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/4UOODGVUG545FDBBMYW7FXSW4F/action/timestamp_anchor","attest_storage":"https://pith.science/pith/4UOODGVUG545FDBBMYW7FXSW4F/action/storage_attestation","attest_author":"https://pith.science/pith/4UOODGVUG545FDBBMYW7FXSW4F/action/author_attestation","sign_citation":"https://pith.science/pith/4UOODGVUG545FDBBMYW7FXSW4F/action/citation_signature","submit_replication":"https://pith.science/pith/4UOODGVUG545FDBBMYW7FXSW4F/action/replication_record"}},"created_at":"2026-07-05T09:23:55.110951+00:00","updated_at":"2026-07-05T09:23:55.110951+00:00"}