{"as_of":"2026-08-16T03:27:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:e07591998b236bac09a88b329932af93ab3a426be2f8887287982063db84c9dc","coverage":[{"denominator":295,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-15T14:20:14.050714Z","state":"measured"},{"denominator":100,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":100,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-15T06:32:42.880941+00:00","state":"measured"},{"denominator":0,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"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":[],"links":{"evidence":"/evidence","html":"/paper/2608.11300/citation-record","integrity":"/paper/2608.11300/integrity","json":"/paper/2608.11300/citation-record.json","paper":"/paper/2608.11300"},"outbound":[{"citation":{"cited_paper":{"arxiv_id":"2201.03718","last_updated":"2022-01-11T00:40:50Z","snapshot_observed_at":"2026-08-13T17:01:01.246256Z","submitted_at":"2022-01-11T00:40:50Z","title":"Fitting AGN/galaxy X-ray-to-radio SEDs with CIGALE and improvement of the code","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2201.03718","snapshot_observed_at":"2026-08-15T14:20:13.444928Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":1,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.444928Z"},"links":{"cited_paper":"/paper/2201.03718","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:798504083b335d29ab30a8142a4101fe900446eece40195f5dfce575b9168bc6","observation_id":"4c73e2f1-3d21-4fc6-a972-7a8deb6c4fa2","resolution":{"observed_at":"2026-08-15T14:20:13.444928Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1602.06954","last_updated":"2017-01-12T00:00:57Z","snapshot_observed_at":"2026-08-14T22:09:15.616289Z","submitted_at":"2016-02-22T21:00:09Z","title":"The dust covering factor in active galactic nuclei","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1602.06954","snapshot_observed_at":"2026-08-15T14:20:13.459316Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":3,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.459316Z"},"links":{"cited_paper":"/paper/1602.06954","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:79bfd80b8d19de3c4a2dd5acb64d2f8df571dbe9b4f403fc952ea4594015cd58","observation_id":"746aad7a-8712-47f4-923b-5d5c5e1016e9","resolution":{"observed_at":"2026-08-15T14:20:13.459316Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2006.02258","last_updated":"2020-06-03T13:18:37Z","snapshot_observed_at":"2026-08-16T02:47:18.599352Z","submitted_at":"2020-06-03T13:18:37Z","title":"Compact Radio Emission from Nearby Galaxies with Mid-infrared Nuclear Outbursts","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2006.02258","snapshot_observed_at":"2026-08-15T14:20:13.465693Z","title":", keywords =","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":4,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.465693Z"},"links":{"cited_paper":"/paper/2006.02258","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:157266b662ef56b8650232b2340edc9f6da707f315a45054f9b9719283238baa","observation_id":"0fa1ab5b-e008-45d9-8cfd-36ac24a18807","resolution":{"observed_at":"2026-08-15T14:20:13.465693Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1811.03094","last_updated":"2018-11-07T19:00:00Z","snapshot_observed_at":"2026-08-14T18:02:36.428884Z","submitted_at":"2018-11-07T19:00:00Z","title":"CIGALE: a python Code Investigating GALaxy Emission","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1811.03094","snapshot_observed_at":"2026-08-15T14:20:13.479091Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":6,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.479091Z"},"links":{"cited_paper":"/paper/1811.03094","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:56a7aa3d5e6d7963a3a5a45777cf49e38b90eff829f3206ceabac411b42e3834","observation_id":"7f26a3b3-6c4b-4543-8605-3348fc9bcb15","resolution":{"observed_at":"2026-08-15T14:20:13.479091Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1802.05105","last_updated":"2018-02-14T14:23:29Z","snapshot_observed_at":"2026-08-15T16:00:29.942302Z","submitted_at":"2018-02-14T14:23:29Z","title":"Long-Term Decline of the Mid-Infrared Emission of Normal Galaxies: Dust Echo of Tidal Disruption Flare?","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1802.05105","snapshot_observed_at":"2026-08-15T14:20:13.485187Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":7,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.485187Z"},"links":{"cited_paper":"/paper/1802.05105","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:585d7f79387965f8bea452d38afc5b735c65132e1d07276d73ac6df658923aca","observation_id":"6fdae9f1-4bef-49b9-b5f8-2c4c74657135","resolution":{"observed_at":"2026-08-15T14:20:13.485187Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1512.00020","last_updated":"2015-11-30T21:00:07Z","snapshot_observed_at":"2026-08-15T16:01:47.994217Z","submitted_at":"2015-11-30T21:00:07Z","title":"Infrared emission from tidal disruption events --- probing the pc-scale dust content around galactic nuclei","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1512.00020","snapshot_observed_at":"2026-08-15T14:20:13.491248Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":8,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.491248Z"},"links":{"cited_paper":"/paper/1512.00020","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:6d149cc0c424a3a44c4ac091b85ddba9e6b27301588bce5c860bf0f92af1a0e8","observation_id":"ee6ae94f-a859-4c2d-bdaf-19aa99535ea8","resolution":{"observed_at":"2026-08-15T14:20:13.491248Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1605.05145","last_updated":"2016-12-01T02:28:10Z","snapshot_observed_at":"2026-08-15T15:13:37.803427Z","submitted_at":"2016-05-17T12:59:30Z","title":"Long Fading Mid-Infrared Emission in Transient Coronal Line Emitters: Dust Echo of Tidal Disruption Flare","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1605.05145","snapshot_observed_at":"2026-08-15T14:20:13.497599Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":9,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.497599Z"},"links":{"cited_paper":"/paper/1605.05145","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:02669563eacf612e728aafc436267dd7e3135eba04bc253f1fb7eeea08802ed5","observation_id":"e0ea6a0f-e8c2-4da9-aacf-bc4f0b49909b","resolution":{"observed_at":"2026-08-15T14:20:13.497599Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2111.10465","last_updated":"2021-11-19T22:39:17Z","snapshot_observed_at":"2026-08-16T00:59:08.908477Z","submitted_at":"2021-11-19T22:39:17Z","title":"A novel black-hole mass scaling relation based on coronal gas, and its dependence with the accretion disc","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2111.10465","snapshot_observed_at":"2026-08-15T14:20:13.504520Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":10,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.504520Z"},"links":{"cited_paper":"/paper/2111.10465","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:cacba7aa75aa0ee440360906b55e0ca3d93eeae7c4e12fbc665868485c8989a2","observation_id":"5fbcb3e5-fb0c-4435-9585-6a08c4a3f563","resolution":{"observed_at":"2026-08-15T14:20:13.504520Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2010.12595","last_updated":"2020-10-23T18:03:18Z","snapshot_observed_at":"2026-08-15T11:57:16.054698Z","submitted_at":"2020-10-23T18:03:18Z","title":"Coronal Line Forest AGN I: physical properties of the emission-line regions","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2010.12595","snapshot_observed_at":"2026-08-15T14:20:13.511119Z","title":"Physical properties of the emission-line regions","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":11,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.511119Z"},"links":{"cited_paper":"/paper/2010.12595","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:c2ca12c652abe509bc3fa9aa30d92163ac34fa4bdf5b98283b07764f725392c0","observation_id":"d43f879a-182b-44d9-b679-c7504d289e44","resolution":{"observed_at":"2026-08-15T14:20:13.511119Z","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":"2026-08-15T14:20:13.517521Z","title":"Astronomical Data Analysis Software and Systems II , year = 1993, editor =","venue":null,"work_id":null,"year":1993},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":12,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.517521Z"},"links":{"citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:079c51b882cb60af20754874e908025fd4030cff3326f7150bb91c146ad9ebea","observation_id":"43dabff4-00f4-4cd1-85dc-bb137978a651","resolution":{"observed_at":"2026-08-15T14:20:13.517521Z","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":"2026-08-15T14:20:13.523503Z","title":"Instrumentation in astronomy VI , year = 1986, editor =","venue":null,"work_id":null,"year":1986},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":13,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.523503Z"},"links":{"citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:59e12e0f6d9a91ef3629cfe50dc55a3f70845a55248a52f18ca01e6b807ef0b0","observation_id":"90c37854-c877-45f1-8e91-eb3ba16b7e28","resolution":{"observed_at":"2026-08-15T14:20:13.523503Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2010.10738","last_updated":"2020-10-22T00:57:37Z","snapshot_observed_at":"2026-07-06T10:06:28.380264Z","submitted_at":"2020-10-21T03:18:26Z","title":"TDE Hosts are Green and Centrally Concentrated: Signatures of a Post-Merger System","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2010.10738","snapshot_observed_at":"2026-08-15T14:20:13.530809Z","title":", keywords =","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":14,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.530809Z"},"links":{"cited_paper":"/paper/2010.10738","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:c8acf217ca6e0a02611c61c3166f65621da6d847bf8bd2ccc9ed0ec16e425c98","observation_id":"d2097663-6c36-476b-a076-f7711a178aba","resolution":{"observed_at":"2026-08-15T14:20:13.530809Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2104.14580","last_updated":"2021-04-29T18:07:48Z","snapshot_observed_at":"2026-08-15T00:48:39.897278Z","submitted_at":"2021-04-29T18:07:48Z","title":"Tidal Disruption Events","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2104.14580","snapshot_observed_at":"2026-08-15T14:20:13.537451Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":15,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.537451Z"},"links":{"cited_paper":"/paper/2104.14580","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:d24d03804b93b1fc9b9f4cd71f2fbadf6e138070858bf751b61efb70505a054d","observation_id":"6bdfeeba-202c-42fa-b2bf-ef169af39547","resolution":{"observed_at":"2026-08-15T14:20:13.537451Z","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":"2026-08-15T14:20:13.544089Z","title":"Research in Astronomy and Astrophysics , year = 2012, month = sep, volume =","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":16,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.544089Z"},"links":{"citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:55681fcb5154bbd3ef95924038427a360f3f4ef571b702f29193648e6da36569","observation_id":"0a27fac2-bdc8-4995-a0e0-4c0f67d0ddff","resolution":{"observed_at":"2026-08-15T14:20:13.544089Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1611.00036","last_updated":"2016-12-13T15:55:51Z","snapshot_observed_at":"2026-07-29T15:27:21.480241Z","submitted_at":"2016-10-31T20:47:42Z","title":"The DESI Experiment Part I: Science,Targeting, and Survey Design","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1611.00036","snapshot_observed_at":"2026-08-15T14:20:13.549869Z","title":"arXiv e-prints , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":17,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.549869Z"},"links":{"cited_paper":"/paper/1611.00036","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:5a6ebfb00927217c7bec85de8388e49a0ead7b4fc0e8582e6807efeb3c2e09ce","observation_id":"beae0962-02a6-48b2-a282-e312ac6651a5","resolution":{"observed_at":"2026-08-15T14:20:13.549869Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1711.03234","last_updated":"2017-11-09T02:24:05Z","snapshot_observed_at":"2026-08-14T20:15:27.460187Z","submitted_at":"2017-11-09T02:24:05Z","title":"SDSS-V: Pioneering Panoptic Spectroscopy","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1711.03234","snapshot_observed_at":"2026-08-15T14:20:13.556044Z","title":"arXiv e-prints , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":18,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.556044Z"},"links":{"cited_paper":"/paper/1711.03234","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:9fc94fbce280dbde0789069f42a948499b467bfa7ebd29dfc85719fb77e26149","observation_id":"57896b3a-b2ea-4a1e-8b8a-f4769e6a825f","resolution":{"observed_at":"2026-08-15T14:20:13.556044Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1408.3476","last_updated":"2014-08-15T06:59:19Z","snapshot_observed_at":"2026-08-14T23:23:05.382743Z","submitted_at":"2014-08-15T06:59:19Z","title":"HyperLEDA. III. The catalogue of extragalactic distances","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1408.3476","snapshot_observed_at":"2026-08-15T14:20:13.562132Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":19,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.562132Z"},"links":{"cited_paper":"/paper/1408.3476","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:3f1cd79cf0307a7c01cbe405d736ebd4cc7b6cbe7a8af3b2dc4bece45928c20d","observation_id":"51cd4666-066c-47e0-98cb-4834d1aee782","resolution":{"observed_at":"2026-08-15T14:20:13.562132Z","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":"2026-08-15T14:20:13.568003Z","title":", year = 1983, month = sep, volume =","venue":null,"work_id":null,"year":1983},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":20,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.568003Z"},"links":{"citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:759cace718ce7ec77a92c21fedc64e289aeb12af0bf16028586f9bcdeb4588c8","observation_id":"1fc9e5ff-1c37-48d6-a93e-bdb3db7d027c","resolution":{"observed_at":"2026-08-15T14:20:13.568003Z","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":"2026-08-15T14:20:13.573275Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":21,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.573275Z"},"links":{"citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:9e65fb52a07bb0801adb861f96c7fb2b4fe0ace7d41e227c75b06d1309d34f61","observation_id":"0119830c-18d0-4c70-8c3c-f1361aaf262c","resolution":{"observed_at":"2026-08-15T14:20:13.573275Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1707.02686","last_updated":"2017-08-31T04:26:23Z","snapshot_observed_at":"2026-08-14T20:48:44.926627Z","submitted_at":"2017-07-10T03:21:41Z","title":"Mid-infrared variability of changing-look AGN","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1707.02686","snapshot_observed_at":"2026-08-15T14:20:13.579359Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":22,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.579359Z"},"links":{"cited_paper":"/paper/1707.02686","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:370204d2362e87c67149462d973a301100f50c021c6b1ffd8fa640d22833db49","observation_id":"560ab330-4420-4b5b-8acf-3b4c84b2d2e6","resolution":{"observed_at":"2026-08-15T14:20:13.579359Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2108.03245","last_updated":"2024-08-24T01:19:49Z","snapshot_observed_at":"2026-08-13T18:32:51.130915Z","submitted_at":"2021-08-06T18:00:02Z","title":"The Curious Case of ASASSN-20hx: A Slowly-Evolving, UV and X-ray Luminous, Ambiguous Nuclear Transient","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2108.03245","snapshot_observed_at":"2026-08-15T14:20:13.585120Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":23,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.585120Z"},"links":{"cited_paper":"/paper/2108.03245","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:3ad269fcc60e56483483e64249a46c99d5a42b4335406f7ae801656a02be3794","observation_id":"d0fd7c2f-66b3-40d8-9a96-2d291e6a3b89","resolution":{"observed_at":"2026-08-15T14:20:13.585120Z","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":"2026-08-15T14:20:13.590535Z","title":"Monthly Notices of the Royal Astronomical Society , volume =","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":24,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.590535Z"},"links":{"citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:5fb142e4075244005c7420885465c62588e45ce1b05a6ea5432cb2ae69242e9b","observation_id":"50d56fc1-d334-47bb-9b5c-c0cc07cc4bfd","resolution":{"observed_at":"2026-08-15T14:20:13.590535Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2102.08044","last_updated":"2021-02-16T09:43:41Z","snapshot_observed_at":"2026-08-16T01:40:27.200141Z","submitted_at":"2021-02-16T09:43:41Z","title":"Infrared Echoes of Optical Tidal Disruption Events: ~1% Dust Covering Factor or Less at sub-parsec Scale","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2102.08044","snapshot_observed_at":"2026-08-15T14:20:13.596242Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":25,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.596242Z"},"links":{"cited_paper":"/paper/2102.08044","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:b5da6efbd204ee04707bd1137824d659f67cf3f174c8866762e19f781bed5100","observation_id":"a057cec7-ad3e-4740-9b54-c48755e9d59c","resolution":{"observed_at":"2026-08-15T14:20:13.596242Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2012.06806","last_updated":"2020-12-12T12:45:24Z","snapshot_observed_at":"2026-08-13T20:47:19.154758Z","submitted_at":"2020-12-12T12:45:24Z","title":"Mid-InfraRed Outburst in Nearby Galaxies (MIRONG) I: Sample Selection and Characterization","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2012.06806","snapshot_observed_at":"2026-08-15T14:20:13.601421Z","title":null,"venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":26,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.601421Z"},"links":{"cited_paper":"/paper/2012.06806","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:3f187eea006c807eb9cc379d399f334223d79aaed0f3f82f082e6eb3cd1941bb","observation_id":"4a92ba0e-8464-4340-bd1a-a91f8cee8c42","resolution":{"observed_at":"2026-08-15T14:20:13.601421Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1406.6025","last_updated":"2014-06-23T19:01:36Z","snapshot_observed_at":"2026-08-14T23:29:21.634739Z","submitted_at":"2014-06-23T19:01:36Z","title":"Initial Performance of the NEOWISE Reactivation Mission","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1406.6025","snapshot_observed_at":"2026-08-15T14:20:13.606622Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":27,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.606622Z"},"links":{"cited_paper":"/paper/1406.6025","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:f41ad7627f1cc5a34d49cdf75c4a89f73d79188e3df6625b3b9ef1f443b28c03","observation_id":"0c6f089b-3a35-450b-b979-5b8c498ddf2b","resolution":{"observed_at":"2026-08-15T14:20:13.606622Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1102.1996","last_updated":"2011-02-09T22:14:19Z","snapshot_observed_at":"2026-08-15T04:55:05.146380Z","submitted_at":"2011-02-09T22:14:19Z","title":"Preliminary Results from NEOWISE: An Enhancement to the Wide-field Infrared Survey Explorer for Solar System Science","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1102.1996","snapshot_observed_at":"2026-08-15T14:20:13.611749Z","title":", keywords =","venue":null,"work_id":null,"year":1996},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":28,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.611749Z"},"links":{"cited_paper":"/paper/1102.1996","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:cc71c3a4b59a91311bdae782a8adc986b36a5127db42781dd711fd0a9352c7ee","observation_id":"72c45c35-c42b-4318-8025-5e7f02d2a174","resolution":{"observed_at":"2026-08-15T14:20:13.611749Z","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":"2026-08-15T14:20:13.616917Z","title":"Transient Name Server Classification Report , keywords =","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":29,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.616917Z"},"links":{"citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:eeed04f3fc8d113ba0b68b35c927571e41d2f43aaed5f8b6f238125c1f2d7f0e","observation_id":"9bd1f98f-68f4-4b78-8f5f-63098d25ffc5","resolution":{"observed_at":"2026-08-15T14:20:13.616917Z","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":"2026-08-15T14:20:13.622181Z","title":"Transient Name Server Classification Report , keywords =","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":30,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.622181Z"},"links":{"citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:510a731701bad580aac4c5f5f8b1ba2ce0a2d9d3bfc29a22923a5215f8fc3463","observation_id":"61e8ca2b-de1c-4898-978e-58938e2ed578","resolution":{"observed_at":"2026-08-15T14:20:13.622181Z","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":"2026-08-15T14:20:13.627282Z","title":"Transient Name Server Discovery Report , keywords =","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":31,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.627282Z"},"links":{"citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:a06d37a87725c42e2cc098fa35af765503e76934ebc6aeab36194c17b2c75195","observation_id":"cbdb7b1c-9686-49cf-90de-efc7adca45ff","resolution":{"observed_at":"2026-08-15T14:20:13.627282Z","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":"2026-08-15T14:20:13.632217Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":32,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.632217Z"},"links":{"citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:1a9ee50a3bcda539820855628cf87082ceaa9110ad761202f67b3335c5bc3f0c","observation_id":"c0532e0d-758e-4ef1-800c-00196db4bab9","resolution":{"observed_at":"2026-08-15T14:20:13.632217Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2204.05461","last_updated":"2022-05-16T14:44:01Z","snapshot_observed_at":"2026-08-13T16:04:04.174441Z","submitted_at":"2022-04-12T01:23:17Z","title":"Discovery of ATLAS17jrp as an Optical, X-ray and Infrared Bright TDE in a Star-forming Galaxy","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2204.05461","snapshot_observed_at":"2026-08-15T14:20:13.638102Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":33,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.638102Z"},"links":{"cited_paper":"/paper/2204.05461","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:64ea46cb7e34542eb8596eb4ce01a76b51769ae7d6702bee69f7713d95039e56","observation_id":"42c92714-2cde-4441-92fd-de9146ce075c","resolution":{"observed_at":"2026-08-15T14:20:13.638102Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2111.12729","last_updated":"2021-11-24T19:00:05Z","snapshot_observed_at":"2026-08-13T17:28:11.644721Z","submitted_at":"2021-11-24T19:00:05Z","title":"Mid-InfraRed Outbursts in Nearby Galaxies (MIRONG). II. Optical Spectroscopic Follow-up","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2111.12729","snapshot_observed_at":"2026-08-15T14:20:13.644081Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":34,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.644081Z"},"links":{"cited_paper":"/paper/2111.12729","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:6495393247902f1589bb8e95c52398501197a98b888bb17900a09a421eaeb699","observation_id":"29e8b27f-ae4a-4478-9069-fda5bbaae4be","resolution":{"observed_at":"2026-08-15T14:20:13.644081Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1512.08614","last_updated":"2015-12-29T08:13:11Z","snapshot_observed_at":"2026-08-14T22:16:42.173877Z","submitted_at":"2015-12-29T08:13:11Z","title":"Revealing the Nature of Extreme Coronal-line Emitter SDSS J095209.56+214313.3","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1512.08614","snapshot_observed_at":"2026-08-15T14:20:13.649034Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":35,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.649034Z"},"links":{"cited_paper":"/paper/1512.08614","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:f74672a98bc969f1eaf286095746ab778b6cb4895fb6431339abd88b61dc2a54","observation_id":"62f5200f-41cc-45aa-9577-f7f8448588a3","resolution":{"observed_at":"2026-08-15T14:20:13.649034Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0902.3248","last_updated":"2009-07-06T18:17:17Z","snapshot_observed_at":"2026-08-15T05:54:38.840732Z","submitted_at":"2009-02-19T14:01:51Z","title":"NTT, Spitzer and Chandra spectroscopy of SDSSJ095209.56+214313.3: the most luminous coronal-line supernova ever observed, or a stellar tidal disruption event ?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0902.3248","snapshot_observed_at":"2026-08-15T14:20:13.654408Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":36,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.654408Z"},"links":{"cited_paper":"/paper/0902.3248","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:f8163911b2555cb2b23da5317ae12dc07ff9696b572c1e0d2beb3a8e7b598e96","observation_id":"c0fd0d69-513c-4fad-b667-1a6c0a5f5471","resolution":{"observed_at":"2026-08-15T14:20:13.654408Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2206.00049","last_updated":"2022-09-09T10:42:31Z","snapshot_observed_at":"2026-08-13T15:32:52.895257Z","submitted_at":"2022-05-31T18:32:08Z","title":"The nuclear transient AT 2017gge: a tidal disruption event in a dusty and gas-rich environment and the awakening of a dormant SMBH","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2206.00049","snapshot_observed_at":"2026-08-15T14:20:13.659750Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":37,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.659750Z"},"links":{"cited_paper":"/paper/2206.00049","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:f7e15fd0b63891e1ad14ccbe16892ced0e15b72c362474075808bad1eb46fae7","observation_id":"eea08d32-bdc8-4989-a5e1-18a4df93bb2a","resolution":{"observed_at":"2026-08-15T14:20:13.659750Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0804.2670","last_updated":"2008-04-16T19:56:26Z","snapshot_observed_at":"2026-08-15T10:17:26.094908Z","submitted_at":"2008-04-16T19:56:26Z","title":"Discovery of superstrong, fading, iron line emission and double-peaked Balmer lines of the galaxy SDSSJ0952+2143 - the light echo of a huge flare","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0804.2670","snapshot_observed_at":"2026-08-15T14:20:13.665605Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":38,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.665605Z"},"links":{"cited_paper":"/paper/0804.2670","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:a66cd5452b9b856c574c56be92eed65c252a3a74e33a72ee6896b6d54f7df179","observation_id":"4ea0e5dc-ceb7-4e40-93aa-e8a26ee7a0ca","resolution":{"observed_at":"2026-08-15T14:20:13.665605Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2203.01461","last_updated":"2022-11-28T17:00:55Z","snapshot_observed_at":"2026-08-13T16:30:29.171702Z","submitted_at":"2022-03-03T00:06:36Z","title":"The Final Season Reimagined: 30 Tidal Disruption Events from the ZTF-I Survey","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2203.01461","snapshot_observed_at":"2026-08-15T14:20:13.671343Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":39,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.671343Z"},"links":{"cited_paper":"/paper/2203.01461","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:f371c356da5f458fc233b9aa6fc849346c69d88c243543fcdcab5817e75197a2","observation_id":"8762f088-1ae1-408e-a4fa-88069519d24e","resolution":{"observed_at":"2026-08-15T14:20:13.671343Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2110.03013","last_updated":"2022-02-23T02:00:47Z","snapshot_observed_at":"2026-08-13T07:46:16.967053Z","submitted_at":"2021-10-06T18:51:39Z","title":"Evidence for the preferential disruption of moderately massive stars by supermassive black holes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2110.03013","snapshot_observed_at":"2026-08-15T14:20:13.677906Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":40,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.677906Z"},"links":{"cited_paper":"/paper/2110.03013","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:f61c0ef659da914ac1ca7702b6a24f1f2db2473014d89e3611018abed55c53d4","observation_id":"29f28fe1-66a1-4abb-88b9-4929e82b72b8","resolution":{"observed_at":"2026-08-15T14:20:13.677906Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1604.02056","last_updated":"2016-12-29T03:42:22Z","snapshot_observed_at":"2026-08-14T22:02:38.912532Z","submitted_at":"2016-04-07T16:11:33Z","title":"An enhanced rate of tidal disruptions in the centrally overdense E+A galaxy NGC 3156","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1604.02056","snapshot_observed_at":"2026-08-15T14:20:13.683270Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":41,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.683270Z"},"links":{"cited_paper":"/paper/1604.02056","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:39623f6d079ea6b51fa9af54762199312001f27841f7bd9bdde721dda8ce1382","observation_id":"0bc9f112-29ba-4e05-a6a0-5d22a4ee7468","resolution":{"observed_at":"2026-08-15T14:20:13.683270Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2106.05982","last_updated":"2021-06-10T18:00:10Z","snapshot_observed_at":"2026-08-13T19:05:37.320097Z","submitted_at":"2021-06-10T18:00:10Z","title":"Evolution Through the Post-Starburst Phase: Using Post-Starburst Galaxies as Laboratories for Understanding the Processes that Drive Galaxy Evolution","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2106.05982","snapshot_observed_at":"2026-08-15T14:20:13.688537Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":42,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.688537Z"},"links":{"cited_paper":"/paper/2106.05982","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:2694151b3c4d4eb2ee00cf7bc102c95e13e62c4d6a2539cc280eac5b46b98c31","observation_id":"ea23c92d-dc72-4b47-aa0b-f141c423dae6","resolution":{"observed_at":"2026-08-15T14:20:13.688537Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1806.05717","last_updated":"2018-06-14T19:42:26Z","snapshot_observed_at":"2026-08-14T19:03:31.196627Z","submitted_at":"2018-06-14T19:42:26Z","title":"A dust-enshrouded tidal disruption event with a resolved radio jet in a galaxy merger","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1806.05717","snapshot_observed_at":"2026-08-15T14:20:13.694181Z","title":"Science , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":43,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.694181Z"},"links":{"cited_paper":"/paper/1806.05717","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:efb81e545c63cc4f41e5e0a36b5bb391265712f3e1c78ede2131b37bfea44f3f","observation_id":"2af2540a-c213-4d17-a069-e1d41e7b7d24","resolution":{"observed_at":"2026-08-15T14:20:13.694181Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1702.02573","last_updated":"2017-02-08T19:00:05Z","snapshot_observed_at":"2026-08-14T21:17:21.732185Z","submitted_at":"2017-02-08T19:00:05Z","title":"A tidal disruption event in the nearby ultra-luminous infrared galaxy F01004-2237","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1702.02573","snapshot_observed_at":"2026-08-15T14:20:13.699974Z","title":"Nature Astronomy , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":44,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.699974Z"},"links":{"cited_paper":"/paper/1702.02573","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:792a0cf7a53c03cbff55b14dc031d96eb2a493f14d9b10a6f8e6f63a52c75c61","observation_id":"18770060-5cbb-42ac-bff9-f576fac51247","resolution":{"observed_at":"2026-08-15T14:20:13.699974Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2006.01518","last_updated":"2020-08-04T14:35:34Z","snapshot_observed_at":"2026-07-06T09:25:19.117559Z","submitted_at":"2020-06-02T11:00:21Z","title":"AT 2017gbl: a dust obscured TDE candidate in a luminous infrared galaxy","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2006.01518","snapshot_observed_at":"2026-08-15T14:20:13.708183Z","title":", keywords =","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":45,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.708183Z"},"links":{"cited_paper":"/paper/2006.01518","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:707bebbb96fbbf79b70ed54fce2db43bca0c7a1b8b6fb6b6ba7e1b8dc4857a49","observation_id":"20585315-f247-4088-afeb-bae5872212ad","resolution":{"observed_at":"2026-08-15T14:20:13.708183Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0305029","last_updated":"2003-09-26T17:07:51Z","snapshot_observed_at":"2026-08-11T08:50:17.961904Z","submitted_at":"2003-05-01T22:12:18Z","title":"Magnetically Arrested Disk: An Energetically Efficient Accretion Flow","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0305029","snapshot_observed_at":"2026-08-15T14:20:13.714437Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":46,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.714437Z"},"links":{"cited_paper":"/paper/astro-ph/0305029","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:e98e3d5ad9fbca7d25b63f33a83f90a51ee9c797b4c9a8358729e3a353f57bcf","observation_id":"a652d28b-9d01-4730-9120-72db4fdd36e1","resolution":{"observed_at":"2026-08-15T14:20:13.714437Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2208.01797","last_updated":"2022-08-03T00:53:56Z","snapshot_observed_at":"2026-08-13T14:52:11.568953Z","submitted_at":"2022-08-03T00:53:56Z","title":"The Host Galaxy and Rapidly Evolving Broad-line Region in the Changing-look Active Galactic Nucleus 1ES 1927+654","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2208.01797","snapshot_observed_at":"2026-08-15T14:20:13.720445Z","title":", keywords =","venue":null,"work_id":null,"year":1927},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":47,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.720445Z"},"links":{"cited_paper":"/paper/2208.01797","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:4c005341877a5f7471d78ac90fb048d11147e658ae2dac3439926f8992f4f7a0","observation_id":"9fe23c6e-0350-4c5e-899c-991c4c9c6771","resolution":{"observed_at":"2026-08-15T14:20:13.720445Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2206.05140","last_updated":"2022-06-10T14:25:12Z","snapshot_observed_at":"2026-08-13T15:26:01.524746Z","submitted_at":"2022-06-10T14:25:12Z","title":"Evolution of a Relativistic Outflow and X-ray Corona in the Extreme Changing-Look AGN 1ES 1927+654","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2206.05140","snapshot_observed_at":"2026-08-15T14:20:13.726732Z","title":", keywords =","venue":null,"work_id":null,"year":1927},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":48,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.726732Z"},"links":{"cited_paper":"/paper/2206.05140","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:79aa4e20435deab09fad1a0e805a88f0841d07c87d280719656be76dcbb46bbc","observation_id":"38ef3770-efda-4a2d-9af1-d45156c60838","resolution":{"observed_at":"2026-08-15T14:20:13.726732Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2211.03801","last_updated":"2023-03-27T22:42:53Z","snapshot_observed_at":"2026-08-13T13:47:55.962172Z","submitted_at":"2022-11-07T19:00:02Z","title":"Multiple Flares in the Changing-Look AGN NGC 5273","version":2},"cited_work":{"arxiv_id":"2211.03801","doi":"10.48550/arxiv.2211.03801","metadata_source":"pith","pith_arxiv_id":"2211.03801","snapshot_observed_at":"2026-08-15T18:16:14.067578Z","title":"Multiple Flares in the Changing-Look AGN NGC 5273","venue":"astro-ph.HE","work_id":"76e86aa0-346c-44f7-aa76-b650d9ffb61e","year":2022},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":49,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.733161Z"},"links":{"cited_paper":"/paper/2211.03801","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:ce67a929584f481fd639804ca3a41e0ba31469df545b6e83e6e56413c5932422","observation_id":"f2d3d991-2a69-4acb-94a0-a1651b7e9b70","resolution":{"observed_at":"2026-08-15T14:20:16.046914Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2209.07538","last_updated":"2022-11-07T23:03:48Z","snapshot_observed_at":"2026-08-13T14:25:33.604848Z","submitted_at":"2022-09-15T18:00:02Z","title":"Live to die another day: the rebrightening of AT2018fyk as a repeating partial tidal disruption event","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2209.07538","snapshot_observed_at":"2026-08-15T14:20:13.738669Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":50,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.738669Z"},"links":{"cited_paper":"/paper/2209.07538","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:ba2afde0f1f4762b89b32b9bd8e7efe29f1a2fe0e4d1b35527c51621b7fa6371","observation_id":"8ff0cb16-2e58-4567-a11a-53ece20d5d66","resolution":{"observed_at":"2026-08-15T14:20:13.738669Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2301.05501","last_updated":"2023-01-13T12:04:24Z","snapshot_observed_at":"2026-08-13T13:04:49.165291Z","submitted_at":"2023-01-13T12:04:24Z","title":"The rebrightening of a ROSAT-selected tidal disruption event: repeated weak partial disruption flares from a quiescent galaxy?","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2301.05501","snapshot_observed_at":"2026-08-15T14:20:13.744436Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":51,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.744436Z"},"links":{"cited_paper":"/paper/2301.05501","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:444bb2cf4ea49c5586d1a5241aa4deed311548de940aa62eaac5b16d907a4259","observation_id":"efd337f6-cbf1-46af-9842-d7fc1ea4c1bf","resolution":{"observed_at":"2026-08-15T14:20:13.744436Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0310336","last_updated":"2003-10-13T20:08:29Z","snapshot_observed_at":"2026-07-07T00:37:16.792675Z","submitted_at":"2003-10-13T20:08:29Z","title":"The Ensemble Photometric Variability of ~25000 Quasars in the Sloan Digital Sky Survey","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0310336","snapshot_observed_at":"2026-08-15T14:20:13.749963Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":52,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.749963Z"},"links":{"cited_paper":"/paper/astro-ph/0310336","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:5718695483c5ff9522698bacd8843a28e42860095eab15301327b04180a975ee","observation_id":"2ee2325f-0012-4e6c-8d50-592fd89c5545","resolution":{"observed_at":"2026-08-15T14:20:13.749963Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2012.14452","last_updated":"2020-12-28T19:16:46Z","snapshot_observed_at":"2026-08-09T13:54:13.330717Z","submitted_at":"2020-12-28T19:16:46Z","title":"Properties of a Previously Unidentified Instrumental Signature in $\\textit{Kepler/K2}$ that was Confused for AGN Variability","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2012.14452","snapshot_observed_at":"2026-08-15T14:20:13.761360Z","title":", keywords =","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":54,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.761360Z"},"links":{"cited_paper":"/paper/2012.14452","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:287b97fc45280e7b653514ffe098377009642efce28d56b7144a69727337490d","observation_id":"60b4e2f1-e692-447a-8e23-37f633050add","resolution":{"observed_at":"2026-08-15T14:20:13.761360Z","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":"2026-08-15T14:20:13.767278Z","title":"arXiv e-prints , keywords =","venue":null,"work_id":null,"year":1927},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":55,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.767278Z"},"links":{"citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:61406934bdf2c1d9c0cdfd496a39eb2beec4dbf5319a5f9ee88f600b1d9fceaa","observation_id":"210f974f-b25d-4a1e-9d03-ba437cc71fda","resolution":{"observed_at":"2026-08-15T14:20:13.767278Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1809.09157","last_updated":"2018-09-24T18:40:20Z","snapshot_observed_at":"2026-08-14T18:24:10.743728Z","submitted_at":"2018-09-24T18:40:20Z","title":"The ATLAS All-Sky Stellar Reference Catalog","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1809.09157","snapshot_observed_at":"2026-08-15T14:20:13.772633Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":56,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.772633Z"},"links":{"cited_paper":"/paper/1809.09157","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:bf914c6bd1f04391d50da49b69cfaab6eeab34291364bc725f12eb3d64ce308f","observation_id":"83802b1f-77ff-48b9-b4da-f9519c5b2757","resolution":{"observed_at":"2026-08-15T14:20:13.772633Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1709.05353","last_updated":"2017-09-15T18:00:31Z","snapshot_observed_at":"2026-08-14T20:32:43.387243Z","submitted_at":"2017-09-15T18:00:31Z","title":"The DEdicated MONitor of EXotransits and Transients (DEMONEXT): System Overview and Year One Results from a Low-Cost Robotic Telescope for Follow-Up of Exoplanetary Transits and Transients","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1709.05353","snapshot_observed_at":"2026-08-15T14:20:13.777925Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":57,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.777925Z"},"links":{"cited_paper":"/paper/1709.05353","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:fecca2bce5d570f382f2bb549a199845332f12b62b03eb41a6307167bee5ff1e","observation_id":"d15bf064-506a-4a24-b004-6dde1be738e4","resolution":{"observed_at":"2026-08-15T14:20:13.777925Z","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":"2026-08-15T14:20:13.783186Z","title":"Ground-based and Airborne Telescopes VI , year = 2016, editor =","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":58,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.783186Z"},"links":{"citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:218917f1945bcb85aaf586e30a2f771fbc6677cb1d163f25a8c608b3d7db4983","observation_id":"de56dd86-5fbc-4427-8579-a534e5ddfaa1","resolution":{"observed_at":"2026-08-15T14:20:13.783186Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0609593","last_updated":"2006-10-10T23:22:20Z","snapshot_observed_at":"2026-08-15T11:02:48.492634Z","submitted_at":"2006-09-20T21:48:47Z","title":"A Cosmology Calculator for the World Wide Web","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0609593","snapshot_observed_at":"2026-08-15T14:20:13.788419Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":59,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.788419Z"},"links":{"cited_paper":"/paper/astro-ph/0609593","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:024e24e55447bb3353df81a74f8995e1c6a2a786f3e2a1113c9fe3bd501fb757","observation_id":"7d856533-8e76-4c97-8c17-462810cd4ce3","resolution":{"observed_at":"2026-08-15T14:20:13.788419Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1803.06436","last_updated":"2018-06-25T23:06:04Z","snapshot_observed_at":"2026-08-14T19:35:16.522093Z","submitted_at":"2018-03-17T00:54:06Z","title":"The Kepler Light Curves of AGN: A Detailed Analysis","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1803.06436","snapshot_observed_at":"2026-08-15T14:20:13.794230Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":60,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.794230Z"},"links":{"cited_paper":"/paper/1803.06436","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:6f352733728b5203395e3e816ec40ef6121794087cdbd9d5937000010e333f5a","observation_id":"6bb9ae71-23d2-4d39-afc9-433f0d9a9f47","resolution":{"observed_at":"2026-08-15T14:20:13.794230Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1406.1718","last_updated":"2014-10-13T18:38:20Z","snapshot_observed_at":"2026-08-14T23:31:17.329382Z","submitted_at":"2014-06-06T15:54:56Z","title":"The 1% Concordance Hubble Constant","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1406.1718","snapshot_observed_at":"2026-08-15T14:20:13.800527Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":61,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.800527Z"},"links":{"cited_paper":"/paper/1406.1718","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:e17e5970e4cfb858d81a6c9b73ac597b362927384ed2a400da198f2a9b7ca11b","observation_id":"583ae663-aca1-4fcd-b606-33ffe2512725","resolution":{"observed_at":"2026-08-15T14:20:13.800527Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2006.08645","last_updated":"2020-12-21T17:36:20Z","snapshot_observed_at":"2026-07-06T09:29:21.603604Z","submitted_at":"2020-06-15T18:00:23Z","title":"High-redshift Extreme Variability Quasars from Sloan Digital Sky Survey Multi-Epoch Spectroscopy","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2006.08645","snapshot_observed_at":"2026-08-15T14:20:13.806461Z","title":", keywords =","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":62,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.806461Z"},"links":{"cited_paper":"/paper/2006.08645","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:2eaa91719dc451b7e174d2682a04604921b320a919b8956aa193fb8d76b304ac","observation_id":"461665fa-bd1e-4562-bdfa-a020d44a3096","resolution":{"observed_at":"2026-08-15T14:20:13.806461Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2011.01954","last_updated":"2020-11-03T19:00:33Z","snapshot_observed_at":"2026-08-13T21:08:25.150994Z","submitted_at":"2020-11-03T19:00:33Z","title":"Magnetic flux inversion in a peculiar changing look AGN","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2011.01954","snapshot_observed_at":"2026-08-15T14:20:13.812666Z","title":", keywords =","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":63,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.812666Z"},"links":{"cited_paper":"/paper/2011.01954","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:250d1ea90d81181183f099e5706845d8767d5de4197a2d64224827765954c558","observation_id":"4a1c82bb-4d4a-4140-9a7e-d3af3510fa32","resolution":{"observed_at":"2026-08-15T14:20:13.812666Z","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":"2026-08-15T14:20:13.818205Z","title":"Analytical Chemistry , year = 1964, month = jan, volume =","venue":null,"work_id":null,"year":1964},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":64,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.818205Z"},"links":{"citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:c37a7c858a4741bc99aea79cf0855236290dc8bdd32f22d26232d13fb80586cd","observation_id":"35539f77-37af-4537-add1-9076ff3a7df2","resolution":{"observed_at":"2026-08-15T14:20:13.818205Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1906.12236","last_updated":"2019-12-24T08:10:57Z","snapshot_observed_at":"2026-08-14T16:10:31.600555Z","submitted_at":"2019-06-28T14:19:59Z","title":"Implications from Late-Time X-ray Detections of Optically Selected Tidal Disruption Events: State Changes, Unification, and Detection Rates","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1906.12236","snapshot_observed_at":"2026-08-15T14:20:13.823402Z","title":", keywords =","venue":null,"work_id":null,"year":1906},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":65,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.823402Z"},"links":{"cited_paper":"/paper/1906.12236","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:76acbfe3d56e9b382da43145af963fecee5a18b490296542575c9aa7f54db897","observation_id":"862bcda6-6bf6-4ff6-9cb6-fc6a9e6f16aa","resolution":{"observed_at":"2026-08-15T14:20:13.823402Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1809.02146","last_updated":"2018-09-06T18:01:46Z","snapshot_observed_at":"2026-08-15T06:23:31.936949Z","submitted_at":"2018-09-06T18:01:46Z","title":"The evolution of Kerr discs and late-time tidal disruption event light curves","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1809.02146","snapshot_observed_at":"2026-08-15T14:20:13.828844Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":66,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.828844Z"},"links":{"cited_paper":"/paper/1809.02146","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:e5682ad081d9d1a1004ed92b765690e2a144f74b6f62e4cd2c091a76b40a7653","observation_id":"dee951cb-4e54-4403-b571-9763bebbfc2f","resolution":{"observed_at":"2026-08-15T14:20:13.828844Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1809.00003","last_updated":"2019-07-26T01:28:57Z","snapshot_observed_at":"2026-08-14T18:34:25.536701Z","submitted_at":"2018-08-31T18:00:00Z","title":"Late-time UV observations of tidal disruption flares reveal unobscured, compact accretion disks","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1809.00003","snapshot_observed_at":"2026-08-15T14:20:13.833979Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":67,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.833979Z"},"links":{"cited_paper":"/paper/1809.00003","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:864352fd7cf92ceebe7837e5391898fa5051a4df12d64911b39936fd81bdd0b3","observation_id":"81b6af96-623e-49f3-b05f-14d58e35b15c","resolution":{"observed_at":"2026-08-15T14:20:13.833979Z","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":"2026-08-15T14:20:13.839427Z","title":"The Astronomer's Telegram , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":68,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.839427Z"},"links":{"citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:f9d52fc75416b3d2ff32ecf6259f93bcd658779a510ce2043c7ebcc802a2935a","observation_id":"feae5840-a669-4979-86cf-0a8dd43cd885","resolution":{"observed_at":"2026-08-15T14:20:13.839427Z","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":"2026-08-15T14:20:13.844337Z","title":"arXiv e-prints , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":69,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.844337Z"},"links":{"citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:0bd7b7bc7b4390801f9703c4e066fc91267fa228dee40bfcdd0cac86ea802a8e","observation_id":"cecea686-2a81-447b-94e3-bea3853f2047","resolution":{"observed_at":"2026-08-15T14:20:13.844337Z","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":"2026-08-15T14:20:13.849554Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":70,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.849554Z"},"links":{"citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:3864e92edbedd0dd297aa9dcad770c22868d9df1509c663a36119cd06ee8b424","observation_id":"7cf2f6b1-5f15-46a1-ba03-ea03d0a51c6b","resolution":{"observed_at":"2026-08-15T14:20:13.849554Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1412.2136","last_updated":"2015-01-20T16:29:52Z","snapshot_observed_at":"2026-08-14T23:08:44.639723Z","submitted_at":"2014-12-05T21:00:08Z","title":"The Discovery of the First \"Changing Look\" Quasar: New Insights into the Physics & Phenomenology of AGN","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1412.2136","snapshot_observed_at":"2026-08-15T14:20:13.855087Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":71,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.855087Z"},"links":{"cited_paper":"/paper/1412.2136","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:0f71de6b4b22647f7b73813645e752938601ce307bc75d6c647ac09393d9902e","observation_id":"074b4a1e-00a3-4791-a58c-ef606c8c6cba","resolution":{"observed_at":"2026-08-15T14:20:13.855087Z","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":"2026-08-15T14:20:13.860830Z","title":"arXiv e-prints , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":72,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.860830Z"},"links":{"citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:4d7ce7e6ffc826227bd06e18237d61409c6a04be6c6a48f04a15c1b130514416","observation_id":"b972eee3-2c9e-46d1-acbe-1e902393d20e","resolution":{"observed_at":"2026-08-15T14:20:13.860830Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0308312","last_updated":"2003-08-18T22:00:41Z","snapshot_observed_at":"2026-07-07T00:35:34.188129Z","submitted_at":"2003-08-18T22:00:41Z","title":"Long-Term X-ray Spectral Variability in Seyfert 1 Galaxies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0308312","snapshot_observed_at":"2026-08-15T14:20:13.866145Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":73,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.866145Z"},"links":{"cited_paper":"/paper/astro-ph/0308312","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:347f98b5356d7d8c86b0d973c34ca0ee51e2b7df06f178fd0eecbb64ff4a1fd9","observation_id":"a688b134-4101-41c5-9f09-a2f422865aea","resolution":{"observed_at":"2026-08-15T14:20:13.866145Z","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":"2026-08-15T14:20:13.871474Z","title":", keywords =","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":74,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.871474Z"},"links":{"citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:2d206a8ad330da710643b449c0d0d4c102a37b4b7299dd9c4baa308f828745c8","observation_id":"b0b5ebfa-c4ae-4db5-993c-e4edbbc6675a","resolution":{"observed_at":"2026-08-15T14:20:13.871474Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9810481","last_updated":"1998-10-29T18:11:26Z","snapshot_observed_at":"2026-07-07T01:22:49.329106Z","submitted_at":"1998-10-29T18:11:26Z","title":"A Cutoff in the X-ray Fluctuation Power Density Spectrum of the Seyfert 1 Galaxy NGC 3516","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9810481","snapshot_observed_at":"2026-08-15T14:20:13.876821Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":75,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.876821Z"},"links":{"cited_paper":"/paper/astro-ph/9810481","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:627a2699f1defa8adabe86eee818e2062160d7d23044a0d770b28c04702ef910","observation_id":"2f92e960-e06e-4179-82bb-d401604b6ff1","resolution":{"observed_at":"2026-08-15T14:20:13.876821Z","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":"2026-08-15T14:20:13.882774Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":76,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.882774Z"},"links":{"citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:2f468240e71895f0fb60580eb95ed6df5b777f5dffe3063a9d9d90a012a246b1","observation_id":"09a82407-3578-4c88-8b6a-4d0b197b2fde","resolution":{"observed_at":"2026-08-15T14:20:13.882774Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1004.0276","last_updated":"2010-08-21T18:12:12Z","snapshot_observed_at":"2026-08-15T05:22:39.757031Z","submitted_at":"2010-04-02T02:43:45Z","title":"Modeling the Time Variability of SDSS Stripe 82 Quasars as a Damped Random Walk","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1004.0276","snapshot_observed_at":"2026-08-15T14:20:13.888131Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":77,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.888131Z"},"links":{"cited_paper":"/paper/1004.0276","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:101b4e6ab1fb22aa43198569dc302ff0c75d81feb6eec89b420585d08ddfb76c","observation_id":"607d9813-1e2c-4d9c-a340-56feeb28bf50","resolution":{"observed_at":"2026-08-15T14:20:13.888131Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1611.08248","last_updated":"2016-11-24T16:51:03Z","snapshot_observed_at":"2026-08-14T21:28:46.404300Z","submitted_at":"2016-11-24T16:51:03Z","title":"Limitations on the recovery of the true AGN variability parameters using Damped Random Walk modeling","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1611.08248","snapshot_observed_at":"2026-08-15T14:20:13.893967Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":78,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.893967Z"},"links":{"cited_paper":"/paper/1611.08248","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:3455dd2345b69805adee3b68b7f4c9baa122093577b83631ced9df1cb41d13d5","observation_id":"3d08591d-8460-410f-95e5-6c843594a8d5","resolution":{"observed_at":"2026-08-15T14:20:13.893967Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2108.05389","last_updated":"2021-08-11T18:09:22Z","snapshot_observed_at":"2026-08-13T18:29:58.905107Z","submitted_at":"2021-08-11T18:09:22Z","title":"A characteristic optical variability timescale in astrophysical accretion disks","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2108.05389","snapshot_observed_at":"2026-08-15T14:20:13.899669Z","title":"Science , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":79,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.899669Z"},"links":{"cited_paper":"/paper/2108.05389","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:67aaf2758d01ed41948e739b15cc189a73cf5d61495331d6f408e6bc77591d41","observation_id":"6d107cab-1b5c-44ba-a6c3-6db820822d3e","resolution":{"observed_at":"2026-08-15T14:20:13.899669Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1111.0672","last_updated":"2011-11-02T21:46:49Z","snapshot_observed_at":"2026-08-15T04:30:07.587127Z","submitted_at":"2011-11-02T21:46:49Z","title":"Kepler Observations of Rapid Optical Variability in Active Galactic Nuclei","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1111.0672","snapshot_observed_at":"2026-08-15T14:20:13.905090Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":80,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.905090Z"},"links":{"cited_paper":"/paper/1111.0672","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:44a5b683691969a5717dab450e1bb1f2abff662caa370833b26a4a474b380145","observation_id":"eabcb3b7-128c-406d-8b2b-a12113d56017","resolution":{"observed_at":"2026-08-15T14:20:13.905090Z","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":"2026-08-15T14:20:13.910707Z","title":"arXiv e-prints , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":81,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.910707Z"},"links":{"citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:33bb4620bc89ef94ae844bd8c03bd4d9962813436f977265abdce0093907b861","observation_id":"3c54d685-d88d-4c2d-92c4-7bd6068f335a","resolution":{"observed_at":"2026-08-15T14:20:13.910707Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0909.1326","last_updated":"2009-11-30T16:26:11Z","snapshot_observed_at":"2026-08-15T05:39:39.882092Z","submitted_at":"2009-09-07T20:05:17Z","title":"Quantifying Quasar Variability As Part of a General Approach To Classifying Continuously Varying Sources","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0909.1326","snapshot_observed_at":"2026-08-15T14:20:13.916204Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":82,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.916204Z"},"links":{"cited_paper":"/paper/0909.1326","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:e9c9731a8af577927c514e52aa15ad520c533bbb4e20c98de785c3b201b0a27f","observation_id":"2abfefe4-a0ec-4fb4-8da6-0790246a8590","resolution":{"observed_at":"2026-08-15T14:20:13.916204Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2005.04491","last_updated":"2020-08-24T16:57:22Z","snapshot_observed_at":"2026-07-06T09:19:02.177410Z","submitted_at":"2020-05-09T18:37:16Z","title":"Optical Variability of the Dwarf AGN NGC 4395 from the Transiting Exoplanet Survey Satellite","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2005.04491","snapshot_observed_at":"2026-08-15T14:20:13.921709Z","title":", keywords =","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":83,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.921709Z"},"links":{"cited_paper":"/paper/2005.04491","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:b81fad19c279249342b5b8676ad89d16693835a20c6ab13096df5d0f77cf1a0d","observation_id":"793a96d8-f584-4e52-8c4a-98cf9794ebe1","resolution":{"observed_at":"2026-08-15T14:20:13.921709Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0705.2774","last_updated":"2007-05-18T20:27:02Z","snapshot_observed_at":"2026-08-15T10:40:30.473656Z","submitted_at":"2007-05-18T20:27:02Z","title":"Some Aspects of Measurement Error in Linear Regression of Astronomical Data","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0705.2774","snapshot_observed_at":"2026-08-15T14:20:13.927353Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":84,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.927353Z"},"links":{"cited_paper":"/paper/0705.2774","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:3ce75c5c646355fac84eda1772e7c0393a3ec2338c5ad2422b85b4841e6897cb","observation_id":"60255945-bcaf-4380-84ce-aa2cfcd66900","resolution":{"observed_at":"2026-08-15T14:20:13.927353Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0903.5315","last_updated":"2009-03-30T20:27:55Z","snapshot_observed_at":"2026-08-15T05:51:46.911927Z","submitted_at":"2009-03-30T20:27:55Z","title":"Are the Variations in Quasar Optical Flux Driven by Thermal Fluctuations?","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0903.5315","snapshot_observed_at":"2026-08-15T14:20:13.932816Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":85,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.932816Z"},"links":{"cited_paper":"/paper/0903.5315","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:e2236c35af1f51a1ea5de960b771fb5125298fe8c18f1991078a1cb08d34f07e","observation_id":"7ce8242f-fef5-40b5-af01-7c3cf87dc8a6","resolution":{"observed_at":"2026-08-15T14:20:13.932816Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1008.0641","last_updated":"2011-05-02T03:22:06Z","snapshot_observed_at":"2026-08-15T05:12:14.648637Z","submitted_at":"2010-08-03T20:00:07Z","title":"An Alternative Approach To Measuring Reverberation Lags in Active Galactic Nuclei","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1008.0641","snapshot_observed_at":"2026-08-15T14:20:13.938776Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":86,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.938776Z"},"links":{"cited_paper":"/paper/1008.0641","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:0a2a673fb6d8c3f2da4244435317cffd4404a9949a1727c7f696e08474997a10","observation_id":"1046f238-6784-4a96-809e-6cfbb5fc676b","resolution":{"observed_at":"2026-08-15T14:20:13.938776Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1202.3783","last_updated":"2013-02-22T02:08:16Z","snapshot_observed_at":"2026-08-15T04:19:02.634539Z","submitted_at":"2012-02-16T21:00:00Z","title":"Is Quasar Optical Variability a Damped Random Walk?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1202.3783","snapshot_observed_at":"2026-08-15T14:20:13.944896Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":87,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.944896Z"},"links":{"cited_paper":"/paper/1202.3783","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:57482fc5944c40a8bd0a69051ba692142e8ba674a41b0c14fb8128e40a0db65a","observation_id":"8bd3c9b5-6224-4cbe-b2a2-fa86ec29352e","resolution":{"observed_at":"2026-08-15T14:20:13.944896Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2102.05666","last_updated":"2021-02-10T19:00:00Z","snapshot_observed_at":"2026-08-13T20:16:42.755873Z","submitted_at":"2021-02-10T19:00:00Z","title":"The 450 days X-ray monitoring of the changing-look AGN 1ES 1927+654","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2102.05666","snapshot_observed_at":"2026-08-15T14:20:13.950283Z","title":", keywords =","venue":null,"work_id":null,"year":1927},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":88,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.950283Z"},"links":{"cited_paper":"/paper/2102.05666","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:6d5cd407520a419411b9912d6cae22f1db31e39a9ff138e7c521a2a5c0b8262c","observation_id":"3a90c318-43ff-4444-81d0-631d80d82361","resolution":{"observed_at":"2026-08-15T14:20:13.950283Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1012.1865","last_updated":"2010-12-17T22:58:43Z","snapshot_observed_at":"2026-08-15T05:00:32.721221Z","submitted_at":"2010-12-08T21:04:47Z","title":"Indecent Exposure in Seyfert 2 Galaxies: A Close Look","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1012.1865","snapshot_observed_at":"2026-08-15T14:20:13.955409Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":89,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.955409Z"},"links":{"cited_paper":"/paper/1012.1865","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:dbf03d078c49669b3d605cb519fe25ae8f8717d94909eeaa96a910b79009707a","observation_id":"b11e1303-a049-41a7-865b-0a07f3534275","resolution":{"observed_at":"2026-08-15T14:20:13.955409Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0210369","last_updated":"2002-10-16T16:12:51Z","snapshot_observed_at":"2026-08-12T14:43:16.756970Z","submitted_at":"2002-10-16T16:12:51Z","title":"1ES 1927+654: Persistent and rapid X-ray variability in an AGN with low intrinsic neutral X-ray absorption and narrow optical emission lines","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0210369","snapshot_observed_at":"2026-08-15T14:20:13.961243Z","title":", keywords =","venue":null,"work_id":null,"year":1927},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":90,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.961243Z"},"links":{"cited_paper":"/paper/astro-ph/0210369","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:cf742044b6db0e7dce710aace8872accd72c7f9e5af250c37e2593172adf6ff1","observation_id":"709503eb-e118-453b-9848-a6242a1e1ff7","resolution":{"observed_at":"2026-08-15T14:20:13.961243Z","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":"2026-08-15T14:20:13.966428Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":91,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.966428Z"},"links":{"citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:0e09bd8fb39225e7126f5848b8e60b26d8156f7ab46262abbfa41d3aec065157","observation_id":"150c8f04-8b39-4378-b0e5-ca050e5e7466","resolution":{"observed_at":"2026-08-15T14:20:13.966428Z","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":"2026-08-15T14:20:13.971833Z","title":", year = 1997, month = jan, volume =","venue":null,"work_id":null,"year":1997},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":92,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.971833Z"},"links":{"citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:8cb0c4c199375f97fedaa59a6720ed53c4a4b8fd802a10471376f6eb26e83c67","observation_id":"49f6138d-f0f4-4c0d-bc8a-f8bc49a701a7","resolution":{"observed_at":"2026-08-15T14:20:13.971833Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1004.2077","last_updated":"2010-04-12T22:55:35Z","snapshot_observed_at":"2026-08-15T05:21:52.773972Z","submitted_at":"2010-04-12T22:55:35Z","title":"Unobscured Type 2 AGNs","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1004.2077","snapshot_observed_at":"2026-08-15T14:20:13.977245Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":93,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.977245Z"},"links":{"cited_paper":"/paper/1004.2077","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:f15a6a2321c22355471c9e0d6b40418bc8f882fce3cb21dd97b487e75c74c0c2","observation_id":"11f3e79e-36ca-442b-9520-a4b3cdca133a","resolution":{"observed_at":"2026-08-15T14:20:13.977245Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1404.5211","last_updated":"2014-04-21T14:30:21Z","snapshot_observed_at":"2026-08-14T23:36:52.738166Z","submitted_at":"2014-04-21T14:30:21Z","title":"Optical spectroscopic observations of gamma-ray blazars candidates I: preliminary results","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1404.5211","snapshot_observed_at":"2026-08-15T14:20:13.989057Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":95,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.989057Z"},"links":{"cited_paper":"/paper/1404.5211","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:8a75a6eee019582299ae7f306f85c21b0baee8746df7346d24a47a339be5fd7c","observation_id":"96f23d87-b398-4a50-b6ea-cd874694cb61","resolution":{"observed_at":"2026-08-15T14:20:13.989057Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1401.5242","last_updated":"2014-01-21T09:51:38Z","snapshot_observed_at":"2026-08-14T23:47:35.947631Z","submitted_at":"2014-01-21T09:51:38Z","title":"The HST view of the broad line region in low luminosity AGN","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1401.5242","snapshot_observed_at":"2026-08-15T14:20:13.995661Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":96,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:13.995661Z"},"links":{"cited_paper":"/paper/1401.5242","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:66b4b4625cc7f47f1984aa6ebd2343caee54800de922191fcc9cbf9d7b185be8","observation_id":"eabcf033-1e05-48e5-8f18-53e95d53f42c","resolution":{"observed_at":"2026-08-15T14:20:13.995661Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2103.10543","last_updated":"2021-03-18T22:00:26Z","snapshot_observed_at":"2026-08-13T17:07:54.168010Z","submitted_at":"2021-03-18T22:00:26Z","title":"BAT AGN Spectroscopic Survey XXVII: Scattered X-Ray Radiation in Obscured Active Galactic Nuclei","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2103.10543","snapshot_observed_at":"2026-08-15T14:20:14.001322Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":97,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:14.001322Z"},"links":{"cited_paper":"/paper/2103.10543","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:27abda451f3abc91e0f258e41982d2bbf1bb9ab187814e685bc9e3047c731a5d","observation_id":"e03230f3-6c50-47cc-a340-192e8cb5dea0","resolution":{"observed_at":"2026-08-15T14:20:14.001322Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1903.08665","last_updated":"2020-01-17T18:45:58Z","snapshot_observed_at":"2026-08-14T16:59:15.421303Z","submitted_at":"2019-03-20T18:00:09Z","title":"ASASSN-18tb: A Most Unusual Type Ia Supernova Observed by TESS and SALT","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1903.08665","snapshot_observed_at":"2026-08-15T14:20:14.009342Z","title":", keywords =","venue":null,"work_id":null,"year":1903},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":98,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:14.009342Z"},"links":{"cited_paper":"/paper/1903.08665","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:f7a1f9ce1fddfd0bcad61a00e203b5bb124db978119fcc0ad29a055cdea39f45","observation_id":"e46b4eb5-8981-4feb-9d82-ed488d628346","resolution":{"observed_at":"2026-08-15T14:20:14.009342Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1905.02904","last_updated":"2019-05-08T04:24:09Z","snapshot_observed_at":"2026-08-14T16:35:43.179975Z","submitted_at":"2019-05-08T04:24:09Z","title":"Initial results from a systematic search for changing-look active galactic nuclei selected via mid-infrared variability","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1905.02904","snapshot_observed_at":"2026-08-15T14:20:14.016878Z","title":", keywords =","venue":null,"work_id":null,"year":1905},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":99,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:14.016878Z"},"links":{"cited_paper":"/paper/1905.02904","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:08dd58b4ab7a82037394f37f8f63522b1917987509efbe78eb21380d1a290764","observation_id":"c3fd7fb2-041a-441f-b945-bf9096b199fe","resolution":{"observed_at":"2026-08-15T14:20:14.016878Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0909.3849","last_updated":"2010-03-09T19:26:07Z","snapshot_observed_at":"2026-08-15T05:38:36.156809Z","submitted_at":"2009-09-21T20:00:34Z","title":"Low Resolution Spectral Templates For AGNs and Galaxies From 0.03 -- 30 microns","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0909.3849","snapshot_observed_at":"2026-08-15T14:20:14.023369Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":100,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:14.023369Z"},"links":{"cited_paper":"/paper/0909.3849","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:c6ad2ce0ad69bb3b257c9d5243f5afa1fbf9c16579d499e884f0f683fb19ea28","observation_id":"8eb8f323-05af-4027-9a22-0383fd42fb31","resolution":{"observed_at":"2026-08-15T14:20:14.023369Z","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":"2026-08-15T14:20:14.030205Z","title":"arXiv e-prints , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":101,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:14.030205Z"},"links":{"citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:2fd1150280dda7693fbb6d72a81bfcb04fda9638ffeca999eb69d35085b5e9e2","observation_id":"d7edd67b-81f4-4677-9c2c-d81cbe3d34c9","resolution":{"observed_at":"2026-08-15T14:20:14.030205Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1904.02171","last_updated":"2020-12-21T18:29:07Z","snapshot_observed_at":"2026-08-15T05:49:34.142619Z","submitted_at":"2019-04-03T18:00:07Z","title":"Early Time Light Curves of Type Ia Supernovae Observed with TESS","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1904.02171","snapshot_observed_at":"2026-08-15T14:20:14.036907Z","title":", keywords =","venue":null,"work_id":null,"year":1904},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":102,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:14.036907Z"},"links":{"cited_paper":"/paper/1904.02171","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:ad0800ca3a8a522c14f99cc122afa8ecf5137be3da371b2d43c73ec2800fc9a6","observation_id":"fe56b36f-4797-4005-a7b0-a81312931dc9","resolution":{"observed_at":"2026-08-15T14:20:14.036907Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2010.06596","last_updated":"2020-10-13T18:00:03Z","snapshot_observed_at":"2026-08-09T01:39:09.333078Z","submitted_at":"2020-10-13T18:00:03Z","title":"High-Cadence, Early-Time Observations of Core-Collapse Supernovae From the TESS Prime Mission","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2010.06596","snapshot_observed_at":"2026-08-15T14:20:14.043877Z","title":", keywords =","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":103,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:14.043877Z"},"links":{"cited_paper":"/paper/2010.06596","citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:8556dc8c97a5b9a95f7f58b7aa381f6d2dfb8f455c65c03782765584fa1f03df","observation_id":"38407d34-9034-4860-b665-fb44ebcc806b","resolution":{"observed_at":"2026-08-15T14:20:14.043877Z","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":"2026-08-15T14:20:14.050714Z","title":"The Astronomer's Telegram , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo","version":1},"reference_index":104,"source":"arxiv_source","source_observed_at":"2026-08-15T14:20:14.050714Z"},"links":{"citing_paper":"/paper/2608.11300"},"observation_digest":"sha256:5b5edb5b85abb68280f5a5d7e9e3660624140b1b409c4489667a667e57838d91","observation_id":"4091f627-9fa8-48e5-ac85-aaef56faf32c","resolution":{"observed_at":"2026-08-15T14:20:14.050714Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2608.11300","last_updated":"2026-08-11T18:00:01Z","latest_version":1,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-15T23:09:56.956340Z","submitted_at":"2026-08-11T18:00:01Z","title":"ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":0,"metadata_mismatch":1,"parse_uncertain":0,"unresolved":99,"verified_exact":0,"verified_fuzzy":0},"total_outbound_references":295},"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":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"thesis":"As of 16 August 2026, this Paper Citation Record lists 100 of 295 outbound references and 0 inbound Pith citation observations for arXiv:2608.11300."}