{"as_of":"2026-08-14T17:55:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:088acc2b0a03cf12b646b04ed5757e007005d287b41642fdbfecdadd535df724","coverage":[{"denominator":102,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-14T04:19:20.966786Z","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":"2026-08-14T06:32:32.682623+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/2608.10074/citation-record","integrity":"/paper/2608.10074/integrity","json":"/paper/2608.10074/citation-record.json","paper":"/paper/2608.10074"},"outbound":[{"citation":{"cited_paper":{"arxiv_id":"2106.01772","last_updated":"2021-06-03T11:53:11Z","snapshot_observed_at":"2026-08-14T12:22:45.995817Z","submitted_at":"2021-06-03T11:53:11Z","title":"High-redshift Narrow-line Seyfert 1 Galaxies: A Candidate Sample","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2106.01772","snapshot_observed_at":"2026-08-14T04:19:19.011905Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":1,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:19.011905Z"},"links":{"cited_paper":"/paper/2106.01772","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:ea2cbb5d43effaddb04dd5378f9f316ec96bfd759ccbe0685fbfef001339a0d2","observation_id":"01b2c2d5-69dc-4ce6-aea1-c3c97e7673b3","resolution":{"observed_at":"2026-08-14T04:19:19.011905Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2311.13818","last_updated":"2023-11-23T05:58:09Z","snapshot_observed_at":"2026-08-13T05:19:13.967224Z","submitted_at":"2023-11-23T05:58:09Z","title":"Narrow-line Seyfert 1 galaxies in Sloan Digital Sky Survey: a new optical spectroscopic catalogue","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2311.13818","snapshot_observed_at":"2026-08-14T04:19:19.030694Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":2,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:19.030694Z"},"links":{"cited_paper":"/paper/2311.13818","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:414cb8fa40f79ebb131f99f63404058f8cb6790e32d1729de836a4e5cf8f807c","observation_id":"f2acf0ff-9d18-4538-807e-ece53e3410fc","resolution":{"observed_at":"2026-08-14T04:19:19.030694Z","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":"2026-08-14T04:19:19.074750Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":3,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:19.074750Z"},"links":{"citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:adb264add900edb7fa90be491d2c27379609b0849cde536d63ec33e63d83d5d7","observation_id":"af4a071d-2afb-4c0c-a366-e0255e5dea73","resolution":{"observed_at":"2026-08-14T04:19:19.074750Z","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":"2026-08-14T04:19:19.124731Z","title":"Bulletin of the American Astronomical Society , year = 1990, volume =","venue":null,"work_id":null,"year":1990},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":4,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:19.124731Z"},"links":{"citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:bc1cafea81c352d21365f3cd7957bfdef56c85af266b3b2feb120e4fbb821e20","observation_id":"343f70ec-6a2f-41d0-abad-5471c475bad0","resolution":{"observed_at":"2026-08-14T04:19:19.124731Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0603070","last_updated":"2006-03-03T21:23:24Z","snapshot_observed_at":"2026-07-07T00:58:51.013355Z","submitted_at":"2006-03-03T00:48:04Z","title":"A Catalog of Broad Absorption Line Quasars from the Sloan Digital Sky Survey Third Data Release","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0603070","snapshot_observed_at":"2026-08-14T04:19:19.155952Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":5,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:19.155952Z"},"links":{"cited_paper":"/paper/astro-ph/0603070","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:8c37b7430ea570414bf9fde49ce6676a3a28b795a7f2a56d2dd65a406952049e","observation_id":"2d5bbb70-d884-43f9-9914-db5fb570e4c1","resolution":{"observed_at":"2026-08-14T04:19:19.155952Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0704.2882","last_updated":"2007-09-18T15:42:32Z","snapshot_observed_at":"2026-07-06T01:26:33.635105Z","submitted_at":"2007-04-22T13:31:20Z","title":"2MASS Reveals a Large Intrinsic Fraction of BALQSOs","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0704.2882","snapshot_observed_at":"2026-08-14T04:19:19.189828Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":6,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:19.189828Z"},"links":{"cited_paper":"/paper/0704.2882","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:7bb1e7560333243482cb46cc850acb88ea79e66a082d2addbd450c43f088fc09","observation_id":"54b57866-dfd0-429d-8ac0-0d651154175c","resolution":{"observed_at":"2026-08-14T04:19:19.189828Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0808.3668","last_updated":"2008-08-27T10:23:25Z","snapshot_observed_at":"2026-07-06T01:42:46.174353Z","submitted_at":"2008-08-27T10:23:25Z","title":"The FIRST-2MASS Red Quasar Survey II: An anomalously high fraction of LoBALs in searches for dust-reddened quasars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0808.3668","snapshot_observed_at":"2026-08-14T04:19:19.205114Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":7,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:19.205114Z"},"links":{"cited_paper":"/paper/0808.3668","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:fd9b7472a5318a2abd79041dd87191bfe87fd9e21e24368a1f3d4cf2b3e38f82","observation_id":"8693657f-0b80-47ef-ae70-934bb41c4ae9","resolution":{"observed_at":"2026-08-14T04:19:19.205114Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1712.05029","last_updated":"2018-01-14T20:34:21Z","snapshot_observed_at":"2026-08-06T07:06:05.659710Z","submitted_at":"2017-12-13T22:15:56Z","title":"The Sloan Digital Sky Survey Quasar Catalog: Fourteenth Data Release","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1712.05029","snapshot_observed_at":"2026-08-14T04:19:19.210584Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":8,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:19.210584Z"},"links":{"cited_paper":"/paper/1712.05029","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:462fa46add1f70e013420c87434965e4c180ad61754cde7006c503f2ee83c7ae","observation_id":"13220cc1-4fea-41ec-8bd1-20e21d3aac8f","resolution":{"observed_at":"2026-08-14T04:19:19.210584Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0203252","last_updated":"2002-03-15T15:37:09Z","snapshot_observed_at":"2026-08-13T04:09:39.771492Z","submitted_at":"2002-03-15T15:37:09Z","title":"Unusual Broad Absorption Line Quasars from the Sloan Digital Sky Survey","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0203252","snapshot_observed_at":"2026-08-14T04:19:19.219833Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":9,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:19.219833Z"},"links":{"cited_paper":"/paper/astro-ph/0203252","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:19d39dce82937ea1975517d3ba565c94fc78153aa866f6145d16a5285d81879f","observation_id":"1b7b440e-7635-4349-8356-2d25934b759a","resolution":{"observed_at":"2026-08-14T04:19:19.219833Z","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":"2026-08-14T04:19:19.240255Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":10,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:19.240255Z"},"links":{"citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:f1ea1a91bd9253cbcca4b73c82276a46c4bdf1eef5478b923699943ab40bdb1f","observation_id":"22c788f6-3373-4e9e-9eb1-6402c9415a0e","resolution":{"observed_at":"2026-08-14T04:19:19.240255Z","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":"2026-08-14T04:19:19.261903Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":11,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:19.261903Z"},"links":{"citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:ec96294a3b900850268244152f92ceb40d3cbaa4fb61d4eaf16b3254e18b6a5d","observation_id":"096ccb5e-fee1-42b5-a12b-b4a30d789ffc","resolution":{"observed_at":"2026-08-14T04:19:19.261903Z","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":"2026-08-14T04:19:19.278367Z","title":", year = 1994, month = may, volume =","venue":null,"work_id":null,"year":1994},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":12,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:19.278367Z"},"links":{"citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:e01cb9eef84f40b110f5986a5fd18f27e342395ad43a96043e97f8302f54c4f4","observation_id":"e42ecea9-3858-4662-a7bd-cfb021086164","resolution":{"observed_at":"2026-08-14T04:19:19.278367Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9504093","last_updated":"1995-04-26T16:38:03Z","snapshot_observed_at":"2026-07-07T01:11:04.136225Z","submitted_at":"1995-04-26T16:38:03Z","title":"Soft X-ray properties of \"narrow-line\" Seyfert 1 galaxies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9504093","snapshot_observed_at":"2026-08-14T04:19:19.291488Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":13,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:19.291488Z"},"links":{"cited_paper":"/paper/astro-ph/9504093","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:66512f07c16903fe496bcbb58e3af61fac62e415f50f93456711cbf78aa49c44","observation_id":"5b27cf77-d81e-4d08-a3b6-75fc32601dc1","resolution":{"observed_at":"2026-08-14T04:19:19.291488Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9907294","last_updated":"1999-07-21T18:12:23Z","snapshot_observed_at":"2026-07-07T01:27:26.124952Z","submitted_at":"1999-07-21T18:12:23Z","title":"A Comprehensive Spectral and Variability Study of Narrow-Line Seyfert 1 Galaxies Observed by ASCA: I. Observations and Time Series Analysis","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9907294","snapshot_observed_at":"2026-08-14T04:19:19.320419Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":14,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:19.320419Z"},"links":{"cited_paper":"/paper/astro-ph/9907294","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:cae20ab7d2f745ab64202d9fa284bbfc07fdd1af16a6b69c94db22f50bdd5d47","observation_id":"34a741a0-ff39-45ed-b26b-79b4fcc166f1","resolution":{"observed_at":"2026-08-14T04:19:19.320419Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0109317","last_updated":"2001-09-19T17:36:23Z","snapshot_observed_at":"2026-08-11T08:56:17.299519Z","submitted_at":"2001-09-19T17:36:23Z","title":"Black Hole Mass and Eddington Ratio as Drivers for the Observable Properties of Radio-Loud and Radio-Quiet QSOs","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0109317","snapshot_observed_at":"2026-08-14T04:19:19.343804Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":15,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:19.343804Z"},"links":{"cited_paper":"/paper/astro-ph/0109317","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:668ad546956c4e7973f71a98395454041d6eada7ef1fb79cd3f939d72a0976f2","observation_id":"72d0fc31-34e0-4665-87f6-a9b83ce235dc","resolution":{"observed_at":"2026-08-14T04:19:19.343804Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0803.0240","last_updated":"2008-03-03T13:41:28Z","snapshot_observed_at":"2026-07-06T01:35:45.551225Z","submitted_at":"2008-03-03T13:41:28Z","title":"On the nature of Seyfert galaxies with high [OIII]5007 blueshifts","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0803.0240","snapshot_observed_at":"2026-08-14T04:19:19.374742Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":16,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:19.374742Z"},"links":{"cited_paper":"/paper/0803.0240","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:d1b8561aaf8c9b5b1b364d17355f79872983d2631662b5902ed7407e273b7242","observation_id":"ad6be892-de09-4085-b20b-ce1bf169bad1","resolution":{"observed_at":"2026-08-14T04:19:19.374742Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1001.3140","last_updated":"2010-02-24T19:13:19Z","snapshot_observed_at":"2026-07-06T02:02:41.083250Z","submitted_at":"2010-01-19T14:55:56Z","title":"The Simultaneous Optical-to-X-ray Spectral Energy Distribution of Soft X-ray Selected AGN observed by Swift","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1001.3140","snapshot_observed_at":"2026-08-14T04:19:19.392171Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":17,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:19.392171Z"},"links":{"cited_paper":"/paper/1001.3140","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:2c54ba35dc18e635fbd1f88a19187d57029cb55ab8b19081de5176b3a02a16fe","observation_id":"f052b635-1a33-4e7f-a5c2-b0d61369623d","resolution":{"observed_at":"2026-08-14T04:19:19.392171Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1201.2810","last_updated":"2012-01-13T11:51:49Z","snapshot_observed_at":"2026-07-06T02:40:51.421431Z","submitted_at":"2012-01-13T11:51:49Z","title":"Correlation Analysis of a Large Sample of Narrow-Line Seyfert 1 Galaxies: Linking Central Engine and Host Properties","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1201.2810","snapshot_observed_at":"2026-08-14T04:19:19.416375Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":18,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:19.416375Z"},"links":{"cited_paper":"/paper/1201.2810","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:20a6454448dcfed4cc50b3c34beeeed6eb6f3bcb8eb9abe15fb9a8262dc5fb59","observation_id":"0cb19293-dff7-48ca-bdac-f3be4d198640","resolution":{"observed_at":"2026-08-14T04:19:19.416375Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0312390","last_updated":"2003-12-15T21:01:25Z","snapshot_observed_at":"2026-07-07T00:39:07.081671Z","submitted_at":"2003-12-15T21:01:25Z","title":"M-BH - sigma relation for a Complete Sample of Soft X-ray Selected AGNs","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0312390","snapshot_observed_at":"2026-08-14T04:19:19.439399Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":19,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:19.439399Z"},"links":{"cited_paper":"/paper/astro-ph/0312390","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:f8580be6009700e99f7ebdf857525fea7dc3c465fbfb34eb68db3d3dc4d3c242","observation_id":"c1a5ea73-3695-410f-ae0b-3e784a94f781","resolution":{"observed_at":"2026-08-14T04:19:19.439399Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0603759","last_updated":"2006-03-28T11:28:58Z","snapshot_observed_at":"2026-07-07T00:59:25.758686Z","submitted_at":"2006-03-28T11:28:58Z","title":"A Comprehensive Study of 2 000 Narrow Line Seyfert 1 Galaxies from the Sloan Digital Sky Survey: I. The Sample","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0603759","snapshot_observed_at":"2026-08-14T04:19:19.465556Z","title":null,"venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":20,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:19.465556Z"},"links":{"cited_paper":"/paper/astro-ph/0603759","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:c8711ed4b9a225833b86774f0de561cefb9e32eb8fe737173bd7e96b2dcf03f9","observation_id":"5c2b0e09-4bd1-44ca-afc9-b485afaedbdc","resolution":{"observed_at":"2026-08-14T04:19:19.465556Z","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":"10.1093/mnras/235.1.261","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:19:21.374736Z","title":", keywords =","venue":null,"work_id":"1adaed30-60c0-47ad-834d-22930ca940b8","year":null},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":21,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:19.472890Z"},"links":{"citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:e258e337fe0420ea48ec46badbd3e81bc25c689e7892d9dd0f3e2e6308064b54","observation_id":"835be8ff-e6b6-495a-8c4d-c855cb52eabe","resolution":{"observed_at":"2026-08-14T04:19:21.394744Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0706.2574","last_updated":"2007-06-18T10:48:21Z","snapshot_observed_at":"2026-07-06T01:28:41.473963Z","submitted_at":"2007-06-18T10:48:21Z","title":"The narrow-line region of narrow-line and broad-line type 1 AGN I. A zone of avoidance in density","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0706.2574","snapshot_observed_at":"2026-08-14T04:19:19.503748Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":22,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:19.503748Z"},"links":{"cited_paper":"/paper/0706.2574","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:0f6734594edd732367fd10ea9c3c247cbe0e40714dd548bc1a4f80ad1fb59623","observation_id":"fd31ca2c-6d8a-4b7c-844a-8f8003049080","resolution":{"observed_at":"2026-08-14T04:19:19.503748Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0201437","last_updated":"2002-04-04T12:05:09Z","snapshot_observed_at":"2026-07-07T00:24:45.735722Z","submitted_at":"2002-01-27T06:57:12Z","title":"Is There a Metallicity--Luminosity Relationship in AGN? The Case of Narrow-Line Seyfert 1 Galaxies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0201437","snapshot_observed_at":"2026-08-14T04:19:19.525630Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":23,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:19.525630Z"},"links":{"cited_paper":"/paper/astro-ph/0201437","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:9ed19d6a536fa5f1e8a773efec3f3bea5792e24f6a1ec84323c91b45b6e88f67","observation_id":"b4743493-6b8b-4a11-8669-0bd722b6e761","resolution":{"observed_at":"2026-08-14T04:19:19.525630Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0204171","last_updated":"2002-04-10T04:30:34Z","snapshot_observed_at":"2026-07-07T00:25:56.846184Z","submitted_at":"2002-04-10T04:30:34Z","title":"Gas Metallicity of Narrow-Line Regions in Narrow-Line Seyfert 1 Galaxies and Broad-Line Seyfert 1 Galaxies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0204171","snapshot_observed_at":"2026-08-14T04:19:19.545687Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":24,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:19.545687Z"},"links":{"cited_paper":"/paper/astro-ph/0204171","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:f4fc067ded67b11329887bec8b1820ec5a5cb8fccd679eeae6755640364deda4","observation_id":"349fb07b-d0a3-4449-b81c-c4e6806ac1ef","resolution":{"observed_at":"2026-08-14T04:19:19.545687Z","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":"2026-08-14T04:19:19.575505Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":25,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:19.575505Z"},"links":{"citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:a287b9013952b32a722a9a21a507362f2c94acf57e58d9be5b318854809f3da2","observation_id":"36308314-1e18-4498-8bc3-2d28135644ec","resolution":{"observed_at":"2026-08-14T04:19:19.575505Z","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":"2026-08-14T04:19:19.592041Z","title":", keywords =","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":26,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:19.592041Z"},"links":{"citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:02e4a169a90f9137627ec21de138141278725cff3093b7b61928ee674dc03d1c","observation_id":"d937a9cd-342c-4f0d-b3a6-7e64bf7746a4","resolution":{"observed_at":"2026-08-14T04:19:19.592041Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1212.1181","last_updated":"2012-12-05T21:20:57Z","snapshot_observed_at":"2026-07-06T03:01:22.904509Z","submitted_at":"2012-12-05T21:20:57Z","title":"Black hole mass estimate for a sample of radio-loud narrow-line Seyfert 1 galaxies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1212.1181","snapshot_observed_at":"2026-08-14T04:19:19.596489Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":27,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:19.596489Z"},"links":{"cited_paper":"/paper/1212.1181","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:e1b61727460998de1853fe498894ba706ab7080d508e0d2dbffdae8cbdb2283e","observation_id":"80fa81fe-3f58-421a-b8ca-ac9404445dfa","resolution":{"observed_at":"2026-08-14T04:19:19.596489Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1602.02783","last_updated":"2016-02-08T21:06:03Z","snapshot_observed_at":"2026-08-10T07:40:32.020121Z","submitted_at":"2016-02-08T21:06:03Z","title":"Radio-loud Narrow Line Seyfert 1 under a different perspective: a revised black hole mass estimate from optical spectropolarimetry","version":1},"cited_work":{"arxiv_id":"1602.02783","doi":null,"metadata_source":"pith","pith_arxiv_id":"1602.02783","snapshot_observed_at":"2026-08-14T04:19:24.957437Z","title":"Radio-loud Narrow Line Seyfert 1 under a different perspective: a revised black hole mass estimate from optical spectropolarimetry","venue":"astro-ph.GA","work_id":"ce5508af-cbdb-4671-8424-3aa4aad5ccba","year":2016},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":28,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:19.614756Z"},"links":{"cited_paper":"/paper/1602.02783","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:b1151422a60edc46dc463b14c8a9049322707b5917869a1a7e65f7da1ca4fe5e","observation_id":"f2c326fc-b0d7-4805-9665-b58ad5057676","resolution":{"observed_at":"2026-08-14T04:19:24.962272Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0703452","last_updated":"2007-03-16T18:16:54Z","snapshot_observed_at":"2026-07-07T01:08:10.508068Z","submitted_at":"2007-03-16T18:16:54Z","title":"The origin of the soft excess in high L/L_Edd AGN","version":1},"cited_work":{"arxiv_id":"astro-ph/0703452","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0703452","snapshot_observed_at":"2026-08-14T04:19:24.934033Z","title":"The origin of the soft excess in high L/L_Edd AGN","venue":"astro-ph","work_id":"211156ff-df6b-40f8-9533-73b7715c75e5","year":2007},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":29,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:19.637014Z"},"links":{"cited_paper":"/paper/astro-ph/0703452","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:d074af29730e468939a3aa076bd11ee4b790760b1b6bdc1e5c3d72c389263448","observation_id":"1b50c904-02eb-4aaf-9fed-18622eb6ed28","resolution":{"observed_at":"2026-08-14T04:19:24.940808Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1910.10395","last_updated":"2020-06-02T07:48:04Z","snapshot_observed_at":"2026-08-04T08:10:50.354039Z","submitted_at":"2019-10-23T07:53:11Z","title":"Spectral properties of quasars from Sloan Digital Sky Survey data release 14: The catalog","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1910.10395","snapshot_observed_at":"2026-08-14T04:19:19.653166Z","title":", keywords =","venue":null,"work_id":null,"year":1910},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":30,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:19.653166Z"},"links":{"cited_paper":"/paper/1910.10395","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:3923d7ced10b395db3badfa9124231617a1e5b67aa4ee38187fca23f623a4347","observation_id":"d9accd35-d084-4db0-aa66-cab17408652b","resolution":{"observed_at":"2026-08-14T04:19:19.653166Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1706.05785","last_updated":"2017-06-19T04:53:18Z","snapshot_observed_at":"2026-07-06T05:47:20.889388Z","submitted_at":"2017-06-19T04:53:18Z","title":"Discovery of a very Lyman-$\\alpha$-luminous quasar at z=6.62","version":1},"cited_work":{"arxiv_id":"1706.05785","doi":null,"metadata_source":"pith","pith_arxiv_id":"1706.05785","snapshot_observed_at":"2026-08-14T04:19:24.850978Z","title":"Discovery of a very Lyman-$\\alpha$-luminous quasar at z=6.62","venue":"astro-ph.GA","work_id":"9ce5699b-40d7-4170-bbff-41a6d78f870f","year":2017},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":31,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:19.682253Z"},"links":{"cited_paper":"/paper/1706.05785","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:3a6f0b0b92521a6f4a63339fbf4620160c81c8188246070db751e1910d0125fe","observation_id":"63bf186c-2827-41cb-a662-ea11682becfc","resolution":{"observed_at":"2026-08-14T04:19:24.856445Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1603.02281","last_updated":"2016-09-05T00:24:30Z","snapshot_observed_at":"2026-08-02T01:02:00.491757Z","submitted_at":"2016-03-07T21:00:08Z","title":"Subaru high-z exploration of low-luminosity quasars (SHELLQs). I. Discovery of 15 quasars and bright galaxies at 5.7 < z < 6.9","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1603.02281","snapshot_observed_at":"2026-08-14T04:19:19.705822Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":32,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:19.705822Z"},"links":{"cited_paper":"/paper/1603.02281","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:e9a2f1c96e7e4583eeb75559b9f23b2021f707b920bd9518b222e3bfcd579a77","observation_id":"94a3a379-a02a-4f15-9696-13140ccfc090","resolution":{"observed_at":"2026-08-14T04:19:19.705822Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1904.07278","last_updated":"2019-07-12T11:00:49Z","snapshot_observed_at":"2026-08-14T16:46:12.447524Z","submitted_at":"2019-04-15T18:27:25Z","title":"Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). VI. Black Hole Mass Measurements of Six Quasars at 6.1<z<6.7","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1904.07278","snapshot_observed_at":"2026-08-14T04:19:19.726772Z","title":null,"venue":null,"work_id":null,"year":1904},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":33,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:19.726772Z"},"links":{"cited_paper":"/paper/1904.07278","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:7cc8489ac9a1dbdc6628d8479809f7a5ac4402a2f21c46619d77612123db9dfc","observation_id":"81d62287-8d0c-4ca1-8ad3-d9fbfe09caf2","resolution":{"observed_at":"2026-08-14T04:19:19.726772Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2310.12222","last_updated":"2023-10-18T18:01:07Z","snapshot_observed_at":"2026-08-13T05:45:58.689089Z","submitted_at":"2023-10-18T18:01:07Z","title":"Subaru High-$z$ Exploration of Low-luminosity Quasars (SHELLQs). XVII. Black Hole Mass Distribution at $z \\sim 6$ Estimated via Spectral Comparison with Low-$z$ Quasars","version":1},"cited_work":{"arxiv_id":"2310.12222","doi":null,"metadata_source":"pith","pith_arxiv_id":"2310.12222","snapshot_observed_at":"2026-08-14T04:19:24.748130Z","title":"Subaru High-$z$ Exploration of Low-luminosity Quasars (SHELLQs). XVII. Black Hole Mass Distribution at $z \\sim 6$ Estimated via Spectral Comparison with Low-$z$ Quasars","venue":"astro-ph.GA","work_id":"d589d5d2-6fa7-484e-a054-055ecf191f3d","year":2023},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":34,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:19.747791Z"},"links":{"cited_paper":"/paper/2310.12222","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:45d2a130508deac36771213a578b0307905d355effcc1b61208f7bf56217188c","observation_id":"2262363a-90b5-4139-b330-35bc7e99e4cf","resolution":{"observed_at":"2026-08-14T04:19:24.766141Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1608.01075","last_updated":"2016-08-03T05:28:37Z","snapshot_observed_at":"2026-08-03T07:39:07.066384Z","submitted_at":"2016-08-03T05:28:37Z","title":"Prime Focus Spectrograph (PFS) for the Subaru Telescope: Overview, recent progress, and future perspectives","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1608.01075","snapshot_observed_at":"2026-08-14T04:19:19.751867Z","title":"Ground-based and Airborne Instrumentation for Astronomy VI , year = 2016, editor =","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":35,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:19.751867Z"},"links":{"cited_paper":"/paper/1608.01075","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:2623e9b3d80c3739986ba994b026e5daedc53f6269541600a5435e738a988de3","observation_id":"c40efda2-27d7-4839-aa42-25a094420a58","resolution":{"observed_at":"2026-08-14T04:19:19.751867Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1206.0737","last_updated":"2013-07-30T05:39:14Z","snapshot_observed_at":"2026-08-02T07:32:31.012838Z","submitted_at":"2012-06-04T20:00:02Z","title":"Extragalactic Science, Cosmology and Galactic Archaeology with the Subaru Prime Focus Spectrograph (PFS)","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1206.0737","snapshot_observed_at":"2026-08-14T04:19:19.774838Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":36,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:19.774838Z"},"links":{"cited_paper":"/paper/1206.0737","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:d321d71e205d4079180e415fa860f9a8be5c47a99db6532bdd85bbd6165e99a1","observation_id":"2f0c0fc2-8446-439c-99c9-32f395fff652","resolution":{"observed_at":"2026-08-14T04:19:19.774838Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2206.14908","last_updated":"2022-06-29T20:51:22Z","snapshot_observed_at":"2026-08-13T15:13:54.878612Z","submitted_at":"2022-06-29T20:51:22Z","title":"The Prime Focus Spectrograph Galaxy Evolution Survey","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2206.14908","snapshot_observed_at":"2026-08-14T04:19:19.786794Z","title":"arXiv e-prints , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":37,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:19.786794Z"},"links":{"cited_paper":"/paper/2206.14908","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:55f4f001bf8a02d613b9987638c7d1f41729cb494ff45cdea6ecfedf0b969fe6","observation_id":"17e3c5da-54d6-4c26-b6f1-febee7e7b443","resolution":{"observed_at":"2026-08-14T04:19:19.786794Z","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":"2026-08-14T04:19:19.813045Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":38,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:19.813045Z"},"links":{"citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:b35f106f72b045ad35becf149e61342d675b90a0a366bc73ec095115ec32f8ba","observation_id":"518a98d1-d326-4992-81a1-6a6190bf3bfa","resolution":{"observed_at":"2026-08-14T04:19:19.813045Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9710327","last_updated":"1998-02-10T18:16:10Z","snapshot_observed_at":"2026-07-07T01:18:46.850516Z","submitted_at":"1997-10-28T22:41:39Z","title":"Maps of Dust IR Emission for Use in Estimation of Reddening and CMBR Foregrounds","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9710327","snapshot_observed_at":"2026-08-14T04:19:19.836142Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":39,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:19.836142Z"},"links":{"cited_paper":"/paper/astro-ph/9710327","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:2c81ec1d5f6a645cd1ba2f4238fba1aaddc15000a6df649030cab733b3dca768","observation_id":"4dd5ee19-6fd2-47dc-a867-7a35e0aa1ec8","resolution":{"observed_at":"2026-08-14T04:19:19.836142Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9809387","last_updated":"1998-09-29T20:55:43Z","snapshot_observed_at":"2026-07-07T01:22:24.532532Z","submitted_at":"1998-09-29T20:55:43Z","title":"Correcting for the Effects of Interstellar Extinction","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9809387","snapshot_observed_at":"2026-08-14T04:19:19.865057Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":40,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:19.865057Z"},"links":{"cited_paper":"/paper/astro-ph/9809387","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:a557e3b625f25d28fbc0331217156a3987ff3d571d359a182a2d5445a25530ac","observation_id":"a706e7f7-a9dc-4be6-8aa7-5a688297b380","resolution":{"observed_at":"2026-08-14T04:19:19.865057Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0105231","last_updated":"2001-05-14T17:29:00Z","snapshot_observed_at":"2026-07-07T00:18:25.513971Z","submitted_at":"2001-05-14T17:29:00Z","title":"Composite Quasar Spectra From the Sloan Digital Sky Survey","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0105231","snapshot_observed_at":"2026-08-14T04:19:19.895187Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":41,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:19.895187Z"},"links":{"cited_paper":"/paper/astro-ph/0105231","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:ecf0cc429932eadbda4f5448a2f4592c9a42806dc5328ed98d115a9111eb6f56","observation_id":"0ce7ffcd-ce0d-4c41-8357-92383246b1f8","resolution":{"observed_at":"2026-08-14T04:19:19.895187Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0504484","last_updated":"2005-04-21T20:18:19Z","snapshot_observed_at":"2026-08-04T18:47:34.507508Z","submitted_at":"2005-04-21T20:18:19Z","title":"The Relationship Between Luminosity and Broad-Line Region Size in Active Galactic Nuclei","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0504484","snapshot_observed_at":"2026-08-14T04:19:19.905448Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":42,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:19.905448Z"},"links":{"cited_paper":"/paper/astro-ph/0504484","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:86d05aac152c2f78f5970ecc90478a1f0fcd6b6dcfc8352601595458317634c8","observation_id":"8d129b21-5c37-419e-a239-6ac45e14c57e","resolution":{"observed_at":"2026-08-14T04:19:19.905448Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0601303","last_updated":"2006-01-13T21:00:02Z","snapshot_observed_at":"2026-07-07T00:57:33.572041Z","submitted_at":"2006-01-13T21:00:02Z","title":"Determining Central Black Hole Masses in Distant Active Galaxies and Quasars. II. Improved Optical and UV Scaling Relationships","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0601303","snapshot_observed_at":"2026-08-14T04:19:19.921169Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":43,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:19.921169Z"},"links":{"cited_paper":"/paper/astro-ph/0601303","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:760a2771f2af8fdd874ad30905a2be90f86608fe9be3d8b5bea647601e4178a5","observation_id":"8e2fd93e-6507-4783-8ca4-f0bccc591a99","resolution":{"observed_at":"2026-08-14T04:19:19.921169Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0601434","last_updated":"2006-02-22T16:22:10Z","snapshot_observed_at":"2026-08-12T16:54:44.891883Z","submitted_at":"2006-01-19T15:20:26Z","title":"The SDSS Quasar Survey: Quasar Luminosity Function from Data Release Three","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0601434","snapshot_observed_at":"2026-08-14T04:19:19.964749Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":44,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:19.964749Z"},"links":{"cited_paper":"/paper/astro-ph/0601434","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:c78b2c16bee16c46f07110ed8868771c5aebd09ef0a3249d8d6365a8d79e7a8f","observation_id":"5dec1e5f-81ec-4727-9275-d48297e5eafd","resolution":{"observed_at":"2026-08-14T04:19:19.964749Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0005140","last_updated":"2000-05-08T14:03:30Z","snapshot_observed_at":"2026-08-08T08:17:05.948471Z","submitted_at":"2000-05-08T14:03:30Z","title":"Observational Similarities and Potential Connections Between Luminous Ultrasoft NLS1s and BALQSOs","version":1},"cited_work":{"arxiv_id":"astro-ph/0005140","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0005140","snapshot_observed_at":"2026-08-14T04:19:24.452511Z","title":"Observational Similarities and Potential Connections Between Luminous Ultrasoft NLS1s and BALQSOs","venue":"astro-ph","work_id":"13504da7-3ecb-4630-a4ac-80e99b8c9c2b","year":2000},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":45,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:20.004755Z"},"links":{"cited_paper":"/paper/astro-ph/0005140","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:4d5995ed96128b321b08df18873e01a543d4b5e035a97e541bc55c827bc2df65","observation_id":"fcf1c2b1-294c-4f0a-90dd-1b3ae9ee6f46","resolution":{"observed_at":"2026-08-14T04:19:24.466809Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1412.8256","last_updated":"2014-12-29T04:54:57Z","snapshot_observed_at":"2026-07-06T04:04:51.733674Z","submitted_at":"2014-12-29T04:54:57Z","title":"Is there a connection between Broad Absorption Line Quasars and Narrow Line Seyfert 1 galaxies?","version":1},"cited_work":{"arxiv_id":"1412.8256","doi":null,"metadata_source":"pith","pith_arxiv_id":"1412.8256","snapshot_observed_at":"2026-08-14T04:19:24.409249Z","title":"Is there a connection between Broad Absorption Line Quasars and Narrow Line Seyfert 1 galaxies?","venue":"astro-ph.GA","work_id":"af85fd04-bbce-4278-bdf7-e8c0070be524","year":2014},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":46,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:20.044755Z"},"links":{"cited_paper":"/paper/1412.8256","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:80129d758f4432b324146bceaa89e6c20882a200953960de9434dd5cef6d3f5d","observation_id":"a6656a6d-dda9-4281-8705-413e67e6d965","resolution":{"observed_at":"2026-08-14T04:19:24.420846Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0906.2149","last_updated":"2009-06-11T16:19:11Z","snapshot_observed_at":"2026-07-06T01:57:42.710730Z","submitted_at":"2009-06-11T16:19:11Z","title":"Emergence of a Broad-Absorption-Line Outflow in the Narrow-line Seyfert 1 Galaxy WPVS 007","version":1},"cited_work":{"arxiv_id":"0906.2149","doi":null,"metadata_source":"pith","pith_arxiv_id":"0906.2149","snapshot_observed_at":"2026-08-14T04:19:24.290623Z","title":"Emergence of a Broad-Absorption-Line Outflow in the Narrow-line Seyfert 1 Galaxy WPVS 007","venue":"astro-ph.CO","work_id":"f324b420-68d1-4ce2-85f3-bfec0e99fb56","year":2009},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":47,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:20.091166Z"},"links":{"cited_paper":"/paper/0906.2149","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:3eed653f80824b61c13e1cd24bfda5d7f338cc7de4c3747aa488eb7233ddba50","observation_id":"a70d43fb-2b29-45e3-9340-d5cd865d9dc6","resolution":{"observed_at":"2026-08-14T04:19:24.312208Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2301.09731","last_updated":"2023-04-18T18:17:32Z","snapshot_observed_at":"2026-08-14T08:13:23.862002Z","submitted_at":"2023-01-23T21:48:13Z","title":"The fraction and kinematics of broad absorption line quasars across cosmic time","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2301.09731","snapshot_observed_at":"2026-08-14T04:19:20.131133Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":48,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:20.131133Z"},"links":{"cited_paper":"/paper/2301.09731","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:a66ba03ed6d1946f3b902a29141379ed2756a0ffc2d0237a44f747a5599344e5","observation_id":"d91261bb-61ee-49e5-8e11-19b2858380ff","resolution":{"observed_at":"2026-08-14T04:19:20.131133Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0006376","last_updated":"2000-08-17T06:04:53Z","snapshot_observed_at":"2026-08-11T07:25:59.346913Z","submitted_at":"2000-06-27T19:41:01Z","title":"Quasar Str\\\"omgren Spheres Before Cosmological Reionization","version":2},"cited_work":{"arxiv_id":"astro-ph/0006376","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0006376","snapshot_observed_at":"2026-08-14T04:19:24.164735Z","title":"Quasar Str\\\"omgren Spheres Before Cosmological Reionization","venue":"astro-ph","work_id":"cbab1c40-7f06-4ca1-af52-2d29ecf402b1","year":2000},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":49,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:20.153395Z"},"links":{"cited_paper":"/paper/astro-ph/0006376","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:232996b985d04a32cb432f605f2d8b9e3f0ece67acbc555c2b239a3842fe3cdc","observation_id":"82d5be61-1f9d-4a01-b59f-91851337c7cd","resolution":{"observed_at":"2026-08-14T04:19:24.204756Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0006271","last_updated":"2000-08-18T09:00:44Z","snapshot_observed_at":"2026-08-12T04:01:51.951411Z","submitted_at":"2000-06-20T09:24:36Z","title":"The Earliest Luminous Sources and the Damping Wing of the Gunn-Peterson Trough","version":2},"cited_work":{"arxiv_id":"astro-ph/0006271","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0006271","snapshot_observed_at":"2026-08-14T04:19:24.083523Z","title":"The Earliest Luminous Sources and the Damping Wing of the Gunn-Peterson Trough","venue":"astro-ph","work_id":"8ff7a222-240f-44f7-8f05-0327ae5baf9c","year":2000},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":50,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:20.164932Z"},"links":{"cited_paper":"/paper/astro-ph/0006271","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:cdbef10681662498002151f2cb40741c54026bec16cdd3ae6cc155d57542bd4e","observation_id":"e4e77a13-a9df-4b7c-915d-a42f61091da4","resolution":{"observed_at":"2026-08-14T04:19:24.094800Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0205410","last_updated":"2002-05-23T20:02:00Z","snapshot_observed_at":"2026-07-07T00:26:35.863418Z","submitted_at":"2002-05-23T20:02:00Z","title":"The Detectability of High Redshift Lyman Alpha Emission Lines Prior to the Reionization of the Universe","version":1},"cited_work":{"arxiv_id":"astro-ph/0205410","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0205410","snapshot_observed_at":"2026-08-14T04:19:24.054058Z","title":"The Detectability of High Redshift Lyman Alpha Emission Lines Prior to the Reionization of the Universe","venue":"astro-ph","work_id":"e87be417-76c7-4a37-b401-0d4f5d8766b2","year":2002},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":51,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:20.190939Z"},"links":{"cited_paper":"/paper/astro-ph/0205410","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:727194e8cc5d38094f66fd1e151ae1d0a8e7011f07e35ae6ce2fc07b267a8208","observation_id":"4b1bb0d8-37dd-44e4-b00e-7a6ab39d685c","resolution":{"observed_at":"2026-08-14T04:19:24.066426Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0512082","last_updated":"2006-03-19T04:20:18Z","snapshot_observed_at":"2026-08-05T23:28:57.001095Z","submitted_at":"2005-12-04T17:04:02Z","title":"Constraining the Evolution of the Ionizing Background and the Epoch of Reionization with z ~ 6 Quasars II: A Sample of 19 Quasars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0512082","snapshot_observed_at":"2026-08-14T04:19:20.211045Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":52,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:20.211045Z"},"links":{"cited_paper":"/paper/astro-ph/0512082","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:7821cb267d42f58b2b5a607ac677665d96c06a62ae88ff039315d2be413999f6","observation_id":"c034ac9a-d602-4fdd-890e-82644325ce75","resolution":{"observed_at":"2026-08-14T04:19:20.211045Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1703.02539","last_updated":"2017-05-10T13:33:39Z","snapshot_observed_at":"2026-07-06T05:32:45.187702Z","submitted_at":"2017-03-07T19:00:00Z","title":"Implications of $z \\sim 6$ Quasar Proximity Zones for the Epoch of Reionization and Quasar Lifetimes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1703.02539","snapshot_observed_at":"2026-08-14T04:19:20.253704Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":53,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:20.253704Z"},"links":{"cited_paper":"/paper/1703.02539","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:b2b800e49fceac04f7185d955bf20662d60cf5830e21c2a7f8722008046bfa4d","observation_id":"d5da498a-c2de-44cc-b4ed-9e1e4e8386bb","resolution":{"observed_at":"2026-08-14T04:19:20.253704Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2009.06648","last_updated":"2020-09-14T18:00:03Z","snapshot_observed_at":"2026-07-06T09:55:31.575678Z","submitted_at":"2020-09-14T18:00:03Z","title":"Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). XI. Proximity Zone Analysis for Faint Quasar Spectra at z~6","version":1},"cited_work":{"arxiv_id":"2009.06648","doi":null,"metadata_source":"pith","pith_arxiv_id":"2009.06648","snapshot_observed_at":"2026-08-14T04:19:23.958484Z","title":"Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). XI. Proximity Zone Analysis for Faint Quasar Spectra at z~6","venue":"astro-ph.GA","work_id":"3ed98535-9864-4d03-81b9-9d0d91e7f2ae","year":2020},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":54,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:20.269095Z"},"links":{"cited_paper":"/paper/2009.06648","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:09a6160fb6634b1153fd942fbf096dc9394694f941659e2f0f6ac2398ce0921a","observation_id":"558a4df4-52cc-4747-a9c3-a45a7dea200b","resolution":{"observed_at":"2026-08-14T04:19:23.965935Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2305.00998","last_updated":"2023-05-01T18:00:01Z","snapshot_observed_at":"2026-08-13T11:51:53.084322Z","submitted_at":"2023-05-01T18:00:01Z","title":"New quasar proximity zone size measurements at $z\\sim 6$ using the enlarged XQR-30 sample","version":1},"cited_work":{"arxiv_id":"2305.00998","doi":null,"metadata_source":"pith","pith_arxiv_id":"2305.00998","snapshot_observed_at":"2026-08-14T04:19:23.922813Z","title":"New quasar proximity zone size measurements at $z\\sim 6$ using the enlarged XQR-30 sample","venue":"astro-ph.GA","work_id":"e9bd84cd-da6a-48c1-99d0-81b62087b91a","year":2023},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":55,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:20.273710Z"},"links":{"cited_paper":"/paper/2305.00998","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:f5b22186c3f276d32a059399a4129d483baf8f2815ba421fa2bd2247b42d02cb","observation_id":"21a29484-9def-4324-8eba-c638aa9fac6b","resolution":{"observed_at":"2026-08-14T04:19:23.932769Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1903.12346","last_updated":"2019-03-29T03:50:18Z","snapshot_observed_at":"2026-08-14T16:54:58.744756Z","submitted_at":"2019-03-29T03:50:18Z","title":"Time-dependent behaviour of quasar proximity zones at $z \\sim 6$","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1903.12346","snapshot_observed_at":"2026-08-14T04:19:20.294746Z","title":", keywords =","venue":null,"work_id":null,"year":1903},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":56,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:20.294746Z"},"links":{"cited_paper":"/paper/1903.12346","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:9f6d445ee937bddb677199ee704928181f17d4969b5585f04978d73ca6b0294d","observation_id":"3ef6b44e-fb42-4d98-a843-188bd536959b","resolution":{"observed_at":"2026-08-14T04:19:20.294746Z","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":"2026-08-14T04:19:20.333228Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":57,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:20.333228Z"},"links":{"citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:beffa3513dc87a405ffcc9e67d77a4db9a88e04836816c6128094e291b5e54ed","observation_id":"62fdcab9-6b1e-4e2e-89c1-e1ecf4ca9b99","resolution":{"observed_at":"2026-08-14T04:19:20.333228Z","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":"2026-08-14T04:19:20.348293Z","title":", year = 2013, month = nov, volume =","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":58,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:20.348293Z"},"links":{"citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:5d505634fe868d3a1b524983f1568eaafc11641cba58424c8fc320c0a81b8185","observation_id":"6fc473d7-5d8e-4486-9393-488a06bcc2ea","resolution":{"observed_at":"2026-08-14T04:19:20.348293Z","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":"2026-08-14T04:19:20.371313Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":59,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:20.371313Z"},"links":{"citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:38f02f5a033306710036df7710136fd3c77d3c754b05be46c1920b6c205fe446","observation_id":"db100bb4-3445-4d2e-960a-0ea63c663bdc","resolution":{"observed_at":"2026-08-14T04:19:20.371313Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1612.06148","last_updated":"2019-01-17T03:47:06Z","snapshot_observed_at":"2026-07-06T05:23:17.257288Z","submitted_at":"2016-12-19T12:12:10Z","title":"A Quasar Discovered at redshift 6.6 from Pan-STARRS1","version":2},"cited_work":{"arxiv_id":"1612.06148","doi":null,"metadata_source":"pith","pith_arxiv_id":"1612.06148","snapshot_observed_at":"2026-08-14T04:19:23.762729Z","title":"A Quasar Discovered at redshift 6.6 from Pan-STARRS1","venue":"astro-ph.GA","work_id":"069396d4-1454-407c-bf64-4abb77ce6fad","year":2016},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":60,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:20.379066Z"},"links":{"cited_paper":"/paper/1612.06148","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:68ed9dc5e4515ca75c834b212e32a36ed077968bbb159450333280f00686512c","observation_id":"219eb212-051f-445b-ba5f-f3dbf07b4de7","resolution":{"observed_at":"2026-08-14T04:19:23.774884Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1810.01447","last_updated":"2019-04-11T19:19:51Z","snapshot_observed_at":"2026-08-14T07:26:16.372513Z","submitted_at":"2018-10-02T18:31:42Z","title":"The Sloan Digital Sky Survey Reverberation Mapping Project: Sample Characterization","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1810.01447","snapshot_observed_at":"2026-08-14T04:19:20.388483Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":61,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:20.388483Z"},"links":{"cited_paper":"/paper/1810.01447","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:19a275bb1214434568a7c844261ba6c76eee4d7a4610dbe3a270bed153937ba9","observation_id":"591ed52c-50d7-4b1a-8880-fdbade44a134","resolution":{"observed_at":"2026-08-14T04:19:20.388483Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0104320","last_updated":"2001-04-19T16:20:14Z","snapshot_observed_at":"2026-08-08T21:01:19.115833Z","submitted_at":"2001-04-19T16:20:14Z","title":"An Empirical Ultraviolet Template for Iron Emission in Quasars as Derived from I Zw 1","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0104320","snapshot_observed_at":"2026-08-14T04:19:20.404947Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":62,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:20.404947Z"},"links":{"cited_paper":"/paper/astro-ph/0104320","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:2adf6376b9ff7a8af299acd9e2664cb45bd2d836021f07df23f5af549751d93a","observation_id":"df1b99f5-d53f-49e4-982b-9e856a6c2b98","resolution":{"observed_at":"2026-08-14T04:19:20.404947Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0612568","last_updated":"2006-12-20T02:37:21Z","snapshot_observed_at":"2026-07-07T01:05:37.020605Z","submitted_at":"2006-12-20T02:37:21Z","title":"The Black Hole Mass - Galaxy Bulge Relationship for QSOs in the SDSS DR3","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0612568","snapshot_observed_at":"2026-08-14T04:19:20.427786Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":63,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:20.427786Z"},"links":{"cited_paper":"/paper/astro-ph/0612568","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:8a9cb15bca83e6de99dd81ac5e584b06a3d87ae78660db437b2c76f9cb1b303b","observation_id":"d7164338-1f3f-4f20-9cce-948aa013209d","resolution":{"observed_at":"2026-08-14T04:19:20.427786Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0606040","last_updated":"2006-06-02T04:18:52Z","snapshot_observed_at":"2026-07-07T01:00:49.053341Z","submitted_at":"2006-06-02T04:18:52Z","title":"Fe II Emission in 14 Low-Redshift Quasars: I - Observations","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0606040","snapshot_observed_at":"2026-08-14T04:19:20.433330Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":64,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:20.433330Z"},"links":{"cited_paper":"/paper/astro-ph/0606040","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:ea083aae493a1bdfc4d8f570dcc7c86e0774a94cff9d9960a2abd7017224b43e","observation_id":"5cb625f5-dca0-4e53-9fe0-9696d8b9fafd","resolution":{"observed_at":"2026-08-14T04:19:20.433330Z","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":"2026-08-14T04:19:20.439858Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":65,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:20.439858Z"},"links":{"citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:addee5e00b88f30397635d3b63721d1a83d5650f7944cd1a7233b16ea7ea81a9","observation_id":"3aa0fbae-7831-499d-9c42-53414888b421","resolution":{"observed_at":"2026-08-14T04:19:20.439858Z","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":"10.48550/arxiv.2606.14012","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:19:21.110107Z","title":"arXiv e-prints , keywords =","venue":null,"work_id":"17bb971c-7b7e-493c-9375-44b2c86bfdb0","year":null},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":66,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:20.443846Z"},"links":{"citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:ba478b2d7128c411fda0368bdb933a6d1f993dba82025fc06b77be629e76b43b","observation_id":"70466d66-ec7c-4e02-a866-fb65b83e968e","resolution":{"observed_at":"2026-08-14T04:19:21.134743Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2209.03987","last_updated":"2022-09-08T18:12:32Z","snapshot_observed_at":"2026-08-13T14:30:06.776929Z","submitted_at":"2022-09-08T18:12:32Z","title":"A Catalog of Quasar Properties from Sloan Digital Sky Survey Data Release 16","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2209.03987","snapshot_observed_at":"2026-08-14T04:19:20.458343Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":67,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:20.458343Z"},"links":{"cited_paper":"/paper/2209.03987","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:09191a240f5ff4deb34e43a9e6fe18ea30dd3b72dc0e9dbc80d4110a97c866cd","observation_id":"4a1941c5-f8e8-4b02-abe2-8a2584730d16","resolution":{"observed_at":"2026-08-14T04:19:20.458343Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2108.13045","last_updated":"2021-08-30T08:10:14Z","snapshot_observed_at":"2026-08-05T11:50:30.862426Z","submitted_at":"2021-08-30T08:10:14Z","title":"Third Data Release of the Hyper Suprime-Cam Subaru Strategic Program","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2108.13045","snapshot_observed_at":"2026-08-14T04:19:20.493276Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":68,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:20.493276Z"},"links":{"cited_paper":"/paper/2108.13045","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:1d8f0ba9314db478cd2fca018c1275b64436b6cd810b8c9059012aeb8001f2e0","observation_id":"85c69f38-7124-4acb-a3fd-78f9627b3bcc","resolution":{"observed_at":"2026-08-14T04:19:20.493276Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1909.05898","last_updated":"2019-09-12T18:34:03Z","snapshot_observed_at":"2026-08-09T16:16:18.781258Z","submitted_at":"2019-09-12T18:34:03Z","title":"The CFHT Large Area U-band Deep Survey (CLAUDS)","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1909.05898","snapshot_observed_at":"2026-08-14T04:19:20.511023Z","title":", keywords =","venue":null,"work_id":null,"year":1909},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":69,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:20.511023Z"},"links":{"cited_paper":"/paper/1909.05898","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:99c751e341498d48bfe42b7412bf818709567456d94e9d313889c628418f554c","observation_id":"bf1c4373-506d-4e3a-8c6e-ca7677d4ea02","resolution":{"observed_at":"2026-08-14T04:19:20.511023Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2308.01230","last_updated":"2024-08-23T14:17:24Z","snapshot_observed_at":"2026-08-13T10:42:28.528320Z","submitted_at":"2023-08-02T15:38:52Z","title":"JADES. The diverse population of infant Black Holes at 4<z<11: merging, tiny, poor, but mighty","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2308.01230","snapshot_observed_at":"2026-08-14T04:19:20.536693Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":70,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:20.536693Z"},"links":{"cited_paper":"/paper/2308.01230","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:d6a60929cdf0dfe6a8bbcbdd461a0b42f31849ac31e9ab422cfa00be0c440cd0","observation_id":"40a3b7a8-566b-42eb-b174-127407f741fd","resolution":{"observed_at":"2026-08-14T04:19:20.536693Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2302.06647","last_updated":"2023-06-21T16:03:09Z","snapshot_observed_at":"2026-08-13T12:45:12.075441Z","submitted_at":"2023-02-13T19:20:16Z","title":"GA-NIFS: A massive black hole in a low-metallicity AGN at $z\\sim5.55$ revealed by JWST/NIRSpec IFS","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2302.06647","snapshot_observed_at":"2026-08-14T04:19:20.549534Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":71,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:20.549534Z"},"links":{"cited_paper":"/paper/2302.06647","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:c172e4d524d899fa7b25969367159b811c09f30e469e7d106b611a4698e34e20","observation_id":"6f622e79-07a7-4609-a7b7-6155c61a1bd6","resolution":{"observed_at":"2026-08-14T04:19:20.549534Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2308.05735","last_updated":"2024-08-15T07:48:45Z","snapshot_observed_at":"2026-08-13T10:37:02.964951Z","submitted_at":"2023-08-10T17:56:31Z","title":"A high black hole to host mass ratio in a lensed AGN in the early Universe","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2308.05735","snapshot_observed_at":"2026-08-14T04:19:20.574820Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":72,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:20.574820Z"},"links":{"cited_paper":"/paper/2308.05735","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:c5dd38e31fa0db9cda9df6ca0a8963b237cc576633fef0d59aedd5129f9af255","observation_id":"1002d276-7b2f-429b-b742-7ebea948e1c6","resolution":{"observed_at":"2026-08-14T04:19:20.574820Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2303.11946","last_updated":"2023-10-29T05:22:53Z","snapshot_observed_at":"2026-08-14T12:19:46.555795Z","submitted_at":"2023-03-21T15:40:30Z","title":"A JWST/NIRSpec First Census of Broad-Line AGNs at z=4-7: Detection of 10 Faint AGNs with M_BH~10^6-10^8 M_sun and Their Host Galaxy Properties","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2303.11946","snapshot_observed_at":"2026-08-14T04:19:20.596106Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":73,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:20.596106Z"},"links":{"cited_paper":"/paper/2303.11946","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:ec4e0d2ea3737b178f1a9148ee321632f17b937a8cb3aeb3afbd406c2d8c0a46","observation_id":"e04e0895-38f3-4810-9a98-b7197c0fc6b3","resolution":{"observed_at":"2026-08-14T04:19:20.596106Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2302.00012","last_updated":"2023-01-31T19:00:00Z","snapshot_observed_at":"2026-08-13T12:54:01.359791Z","submitted_at":"2023-01-31T19:00:00Z","title":"Hidden Little Monsters: Spectroscopic Identification of Low-Mass, Broad-Line AGN at $z>5$ with CEERS","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2302.00012","snapshot_observed_at":"2026-08-14T04:19:20.618113Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":74,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:20.618113Z"},"links":{"cited_paper":"/paper/2302.00012","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:9e3d8f7b565ed0e891ea11650f4ea63b8507d84ee3691f3c2a5fd8e3bab2d111","observation_id":"f148aa61-9d4c-4800-821f-8a617cbe4a89","resolution":{"observed_at":"2026-08-14T04:19:20.618113Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2310.18395","last_updated":"2024-02-05T20:16:43Z","snapshot_observed_at":"2026-08-13T05:38:52.669830Z","submitted_at":"2023-10-27T18:00:01Z","title":"Undermassive Host Galaxies of Five z~6 Luminous Quasars Detected with JWST","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2310.18395","snapshot_observed_at":"2026-08-14T04:19:20.639658Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":75,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:20.639658Z"},"links":{"cited_paper":"/paper/2310.18395","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:c674bc7ddd1a30ba510e8d16fcc0632cd60e65e8c108b778c69e7246c9929305","observation_id":"b3ef058f-4c74-44f5-828b-41d1d3aaaa9f","resolution":{"observed_at":"2026-08-14T04:19:20.639658Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2309.04614","last_updated":"2024-03-28T23:40:11Z","snapshot_observed_at":"2026-08-13T10:17:37.564662Z","submitted_at":"2023-09-08T22:08:51Z","title":"EIGER V. Characterizing the Host Galaxies of Luminous Quasars at $z\\gtrsim6$","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2309.04614","snapshot_observed_at":"2026-08-14T04:19:20.656180Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":76,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:20.656180Z"},"links":{"cited_paper":"/paper/2309.04614","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:351d6993ae8cfc8a081ef527e8f9964aaa5a8ec592d031ae25e7ff66aff63404","observation_id":"00b5f6f3-7c0d-4626-a598-6c12ff719697","resolution":{"observed_at":"2026-08-14T04:19:20.656180Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2308.12331","last_updated":"2023-10-09T15:54:33Z","snapshot_observed_at":"2026-08-13T17:16:18.420580Z","submitted_at":"2023-08-23T18:00:00Z","title":"JWST CEERS & JADES Active Galaxies at z = 4-7 Violate the Local $M_\\bullet-M_\\star$ Relation at $>3\\sigma$: Implications for Low-Mass Black Holes and Seeding Models","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2308.12331","snapshot_observed_at":"2026-08-14T04:19:20.669512Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":77,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:20.669512Z"},"links":{"cited_paper":"/paper/2308.12331","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:535ad13bbef2ef97ddf9ccfbc12e582487be75866a2aba7ee90d91aaa0a02029","observation_id":"56a257c7-c106-412f-9608-13f9f64bb96a","resolution":{"observed_at":"2026-08-14T04:19:20.669512Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2303.08918","last_updated":"2023-08-29T19:36:47Z","snapshot_observed_at":"2026-08-14T16:16:45.640893Z","submitted_at":"2023-03-15T20:22:38Z","title":"A CEERS Discovery of an Accreting Supermassive Black Hole 570 Myr after the Big Bang: Identifying a Progenitor of Massive z > 6 Quasars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2303.08918","snapshot_observed_at":"2026-08-14T04:19:20.673560Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":78,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:20.673560Z"},"links":{"cited_paper":"/paper/2303.08918","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:b07a3eefeeb162e07e2c818de0aa1d440b6f9baf1f5f65e676a53779a2305569","observation_id":"55d2549a-44b4-4cb8-ade5-527c2723a5c1","resolution":{"observed_at":"2026-08-14T04:19:20.673560Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0603680","last_updated":"2006-03-24T18:12:59Z","snapshot_observed_at":"2026-07-07T00:59:21.520135Z","submitted_at":"2006-03-24T18:12:59Z","title":"Radio-loud Narrow-Line Type 1 Quasars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0603680","snapshot_observed_at":"2026-08-14T04:19:20.677851Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":79,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:20.677851Z"},"links":{"cited_paper":"/paper/astro-ph/0603680","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:3d5ab2dd86d7f4c6f914fde555902b8eeaf978d1ecbcb51773aab225a27981af","observation_id":"961fa830-8565-4701-b14c-91a5810fa245","resolution":{"observed_at":"2026-08-14T04:19:20.677851Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1412.2881","last_updated":"2014-12-09T08:06:08Z","snapshot_observed_at":"2026-07-06T04:03:02.362934Z","submitted_at":"2014-12-09T08:06:08Z","title":"Unshifted Metastable He I* Mini-Broad Absorption Line System in the Narrow Line Type 1 Quasar SDSS J080248.18$+$551328.9","version":1},"cited_work":{"arxiv_id":"1412.2881","doi":null,"metadata_source":"pith","pith_arxiv_id":"1412.2881","snapshot_observed_at":"2026-08-14T04:19:23.097955Z","title":"Unshifted Metastable He I* Mini-Broad Absorption Line System in the Narrow Line Type 1 Quasar SDSS J080248.18$+$551328.9","venue":"astro-ph.GA","work_id":"8291cd4e-cf36-44ed-b090-1959c4fe6eac","year":2014},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":80,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:20.682638Z"},"links":{"cited_paper":"/paper/1412.2881","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:7b75608ca2017d55f8c1f269d26acf73552ba4263d36e037ef4d09835edb57c9","observation_id":"5f4b8ed0-0244-4750-a256-1f6d92817245","resolution":{"observed_at":"2026-08-14T04:19:23.108303Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2401.04159","last_updated":"2024-03-03T15:45:20Z","snapshot_observed_at":"2026-08-13T04:47:04.800836Z","submitted_at":"2024-01-08T19:00:00Z","title":"The Redshift Evolution of the $M_\\bullet-M_\\star$ Relation for JWST's Supermassive Black Holes at $z > 4$","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2401.04159","snapshot_observed_at":"2026-08-14T04:19:20.699883Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":81,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:20.699883Z"},"links":{"cited_paper":"/paper/2401.04159","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:fea66dfbdeccacd8388f81f76a66d2727541f0bda10ad3c98672b251044fc91b","observation_id":"e878a109-4554-4e1e-8fd8-f0644ee778ba","resolution":{"observed_at":"2026-08-14T04:19:20.699883Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9812265","last_updated":"1998-12-14T14:56:16Z","snapshot_observed_at":"2026-08-05T00:14:49.701550Z","submitted_at":"1998-12-14T14:56:16Z","title":"Intrinsic Absorption Lines in Seyfert 1 Galaxies. I. Ultraviolet Spectra from the Hubble Space Telescope","version":1},"cited_work":{"arxiv_id":"astro-ph/9812265","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/9812265","snapshot_observed_at":"2026-08-14T04:19:22.957316Z","title":"Intrinsic Absorption Lines in Seyfert 1 Galaxies. I. Ultraviolet Spectra from the Hubble Space Telescope","venue":"astro-ph","work_id":"200ae7be-a478-4d0c-89e5-ab74d7aa1bf0","year":1998},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":82,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:20.724358Z"},"links":{"cited_paper":"/paper/astro-ph/9812265","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:9affe2bf432c9e7d59cfce5b2719ecfd6dedd35facde8c8319f845f1b539c7d9","observation_id":"1f79d968-3654-4f93-94fd-ee8e8d96fdd4","resolution":{"observed_at":"2026-08-14T04:19:22.970239Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0409546","last_updated":"2004-09-22T19:34:12Z","snapshot_observed_at":"2026-07-07T00:44:53.460945Z","submitted_at":"2004-09-22T19:34:12Z","title":"The Largest Blueshifts of [O III] emission line in Two Narrow-Line Quasars","version":1},"cited_work":{"arxiv_id":"astro-ph/0409546","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0409546","snapshot_observed_at":"2026-08-14T04:19:22.931343Z","title":"The Largest Blueshifts of [O III] emission line in Two Narrow-Line Quasars","venue":"astro-ph","work_id":"5d40bb41-5861-44b7-86da-a6d3040b4950","year":2004},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":83,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:20.736776Z"},"links":{"cited_paper":"/paper/astro-ph/0409546","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:db0d38e1b57a75dce696b846aeca2389ce73a0b216712f58cebe00587d53f4cd","observation_id":"685fc7d5-a019-4f45-9cfc-df14291fb4a5","resolution":{"observed_at":"2026-08-14T04:19:22.938184Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:19:20.752728Z","title":", keywords =","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":84,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:20.752728Z"},"links":{"citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:1a1e5601e8d43dbe323644f4edba64fdd584049c2cbfa3a8c3c190ec1b113e45","observation_id":"ed6c9dab-cf34-45c1-bc53-750b1ed5c7f0","resolution":{"observed_at":"2026-08-14T04:19:20.752728Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0304373","last_updated":"2003-06-30T00:06:28Z","snapshot_observed_at":"2026-07-07T00:32:49.202517Z","submitted_at":"2003-04-22T01:13:49Z","title":"Comptonization in Super-Eddington Accretion Flow and Growth Timescale of Supermassive Black Holes","version":2},"cited_work":{"arxiv_id":"astro-ph/0304373","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0304373","snapshot_observed_at":"2026-08-14T04:19:22.691197Z","title":"Comptonization in Super-Eddington Accretion Flow and Growth Timescale of Supermassive Black Holes","venue":"astro-ph","work_id":"814fc83a-7bec-4fce-836b-cae2326129d8","year":2003},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":85,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:20.764951Z"},"links":{"cited_paper":"/paper/astro-ph/0304373","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:83e7e8df96a9a8e92036b120c1544233478eb0725f5d932c80427e3be3d4ee85","observation_id":"78004880-eab0-4b98-9646-e0e2127fcf22","resolution":{"observed_at":"2026-08-14T04:19:22.722238Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0306404","last_updated":"2003-06-19T20:27:46Z","snapshot_observed_at":"2026-08-12T22:56:22.966830Z","submitted_at":"2003-06-19T20:27:46Z","title":"The Host Galaxies of Narrow-Line Seyfert 1s: Evidence for Bar-Driven Fueling","version":1},"cited_work":{"arxiv_id":"astro-ph/0306404","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0306404","snapshot_observed_at":"2026-08-14T04:19:22.554740Z","title":"The Host Galaxies of Narrow-Line Seyfert 1s: Evidence for Bar-Driven Fueling","venue":"astro-ph","work_id":"ef4e4e15-619e-409a-a6eb-63a76e46fa74","year":2003},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":86,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:20.769977Z"},"links":{"cited_paper":"/paper/astro-ph/0306404","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:a542ce1551847bd66b3b369754e8ead2abd0a93b4026676e7824436a44b29d74","observation_id":"3d2dc00b-63ad-4c37-96d4-5999df34713a","resolution":{"observed_at":"2026-08-14T04:19:22.575831Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0610355","last_updated":"2006-10-12T09:34:28Z","snapshot_observed_at":"2026-07-07T01:03:44.349244Z","submitted_at":"2006-10-12T09:34:28Z","title":"A Bar Fuels a Super-Massive Black Hole?: Host Galaxies of Narrow-Line Seyfert 1 Galaxies","version":1},"cited_work":{"arxiv_id":"astro-ph/0610355","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0610355","snapshot_observed_at":"2026-08-14T04:19:22.485201Z","title":"A Bar Fuels a Super-Massive Black Hole?: Host Galaxies of Narrow-Line Seyfert 1 Galaxies","venue":"astro-ph","work_id":"b15e8b38-23dc-4671-94e2-6e1c838a9845","year":2006},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":87,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:20.774546Z"},"links":{"cited_paper":"/paper/astro-ph/0610355","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:04ca295d4aec1ea2d6297ab25e56aa746ad093b7487152fc3ee46febf123d259","observation_id":"ec962a76-f371-4651-82b7-2b12445f9a78","resolution":{"observed_at":"2026-08-14T04:19:22.520407Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2006.02436","last_updated":"2020-06-03T18:00:00Z","snapshot_observed_at":"2026-08-01T17:30:25.635068Z","submitted_at":"2020-06-03T18:00:00Z","title":"Revisiting Soltan's argument based on a semi-analytical model for galaxy and black hole evolution","version":1},"cited_work":{"arxiv_id":"2006.02436","doi":null,"metadata_source":"pith","pith_arxiv_id":"2006.02436","snapshot_observed_at":"2026-08-14T04:19:22.467296Z","title":"Revisiting Soltan's argument based on a semi-analytical model for galaxy and black hole evolution","venue":"astro-ph.GA","work_id":"94bbd004-b1f3-43c8-abbf-bc5a339ca22c","year":2020},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":88,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:20.791041Z"},"links":{"cited_paper":"/paper/2006.02436","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:44ce31ddb1cca4e7fd94fa3cd20dd329c5abdfd372c2783da7e4ddfdf9ecc48d","observation_id":"2a512651-8d7e-42b7-adde-f0580d9b2cee","resolution":{"observed_at":"2026-08-14T04:19:22.472363Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0405024","last_updated":"2004-05-05T09:25:07Z","snapshot_observed_at":"2026-08-11T18:37:19.845462Z","submitted_at":"2004-05-03T13:35:03Z","title":"Growth of massive black holes by super-Eddington accretion","version":2},"cited_work":{"arxiv_id":"astro-ph/0405024","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0405024","snapshot_observed_at":"2026-08-14T04:19:22.428665Z","title":"Growth of massive black holes by super-Eddington accretion","venue":"astro-ph","work_id":"58cffe39-58eb-4b31-a907-54eff0138e4b","year":2004},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":89,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:20.804737Z"},"links":{"cited_paper":"/paper/astro-ph/0405024","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:d509d407cf390534404c00e7962bb2a1de6fc1d9cfed893c5ec557664ead0ec6","observation_id":"94f986df-8f36-4de5-8cd9-bd32277f86e8","resolution":{"observed_at":"2026-08-14T04:19:22.439101Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1712.01860","last_updated":"2018-07-06T17:30:48Z","snapshot_observed_at":"2026-07-06T06:12:55.877365Z","submitted_at":"2017-12-05T19:00:21Z","title":"An 800-million-solar-mass black hole in a significantly neutral Universe at redshift 7.5","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1712.01860","snapshot_observed_at":"2026-08-14T04:19:20.824817Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":90,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:20.824817Z"},"links":{"cited_paper":"/paper/1712.01860","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:6bc867bfe5683468e1852b35607ba5d9fcb9f1c6d13dcafe418177c99cf616b9","observation_id":"b53e19ff-d507-4595-a29b-3526e2743043","resolution":{"observed_at":"2026-08-14T04:19:20.824817Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2109.13942","last_updated":"2021-09-28T18:00:02Z","snapshot_observed_at":"2026-08-13T18:03:25.690166Z","submitted_at":"2021-09-28T18:00:02Z","title":"Probing Early Super-massive Black Hole Growth and Quasar Evolution with Near-infrared Spectroscopy of 37 Reionization-era Quasars at 6.3 < z <= 7.64","version":1},"cited_work":{"arxiv_id":"2109.13942","doi":null,"metadata_source":"pith","pith_arxiv_id":"2109.13942","snapshot_observed_at":"2026-08-14T04:19:22.393009Z","title":"Probing Early Super-massive Black Hole Growth and Quasar Evolution with Near-infrared Spectroscopy of 37 Reionization-era Quasars at 6.3 < z <= 7.64","venue":"astro-ph.GA","work_id":"9783c838-e0a9-4697-9626-b4c108c834fd","year":2021},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":91,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:20.841929Z"},"links":{"cited_paper":"/paper/2109.13942","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:43b483cc3082da94b6a29581796ad16af20439e1c8d6f0d2d8ac05f46572009c","observation_id":"4c6804dd-bff6-4f2e-be9b-4748de21f072","resolution":{"observed_at":"2026-08-14T04:19:22.398802Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2101.03179","last_updated":"2021-01-08T19:00:12Z","snapshot_observed_at":"2026-07-06T10:31:05.724797Z","submitted_at":"2021-01-08T19:00:12Z","title":"A Luminous Quasar at Redshift 7.642","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2101.03179","snapshot_observed_at":"2026-08-14T04:19:20.874743Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":92,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:20.874743Z"},"links":{"cited_paper":"/paper/2101.03179","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:9339c1f11e06e8d608437ef4bda944771972820dd66ac1ef28a642400957a313","observation_id":"9f41d3c8-1577-4c97-bbf0-3b8f9f45a3a9","resolution":{"observed_at":"2026-08-14T04:19:20.874743Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1106.6088","last_updated":"2011-06-30T00:06:43Z","snapshot_observed_at":"2026-08-10T10:52:04.754427Z","submitted_at":"2011-06-30T00:06:43Z","title":"A luminous quasar at a redshift of z = 7.085","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1106.6088","snapshot_observed_at":"2026-08-14T04:19:20.885117Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":93,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:20.885117Z"},"links":{"cited_paper":"/paper/1106.6088","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:f453e501dd8dc1621713ba21dc6869ca151f9187bec48f7761775b1ad5904b7f","observation_id":"4358595a-42eb-44bf-b28e-74f4f1ab6b84","resolution":{"observed_at":"2026-08-14T04:19:20.885117Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1502.07418","last_updated":"2015-02-28T07:04:32Z","snapshot_observed_at":"2026-08-14T13:24:07.795422Z","submitted_at":"2015-02-26T03:25:37Z","title":"An ultra-luminous quasar with a twelve-billion-solar-mass black hole at redshift 6.30","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1502.07418","snapshot_observed_at":"2026-08-14T04:19:20.895568Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":94,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:20.895568Z"},"links":{"cited_paper":"/paper/1502.07418","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:d04bd6cdf8c15e69d1e34ca9fe2893b05126bdc0abefcd645cccf76aa400abfd","observation_id":"c1928e8e-f897-424a-a009-66ba15a8d238","resolution":{"observed_at":"2026-08-14T04:19:20.895568Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0506040","last_updated":"2005-07-26T12:47:15Z","snapshot_observed_at":"2026-08-14T10:48:32.496551Z","submitted_at":"2005-06-02T14:38:08Z","title":"Rapid growth of high redshift black holes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0506040","snapshot_observed_at":"2026-08-14T04:19:20.911436Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":95,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:20.911436Z"},"links":{"cited_paper":"/paper/astro-ph/0506040","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:69faf630b88309da797d05b5f3120b1139de396a136b369036028d6d0bdd903e","observation_id":"ff72f4c1-2d80-4597-82d9-73e2f6f132e2","resolution":{"observed_at":"2026-08-14T04:19:20.911436Z","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":"2026-08-14T04:19:20.932266Z","title":", keywords =","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":96,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:20.932266Z"},"links":{"citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:bbf3269721302e748eeb166e4dc608c12f8b0c2c5fa9cccb6a13e3852d08fb14","observation_id":"39ec17af-f41a-4f85-913e-bae6739594d6","resolution":{"observed_at":"2026-08-14T04:19:20.932266Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1402.6995","last_updated":"2014-03-12T18:09:05Z","snapshot_observed_at":"2026-07-06T03:37:10.050973Z","submitted_at":"2014-02-27T18:08:14Z","title":"Super-Critical Growth of Massive Black Holes from Stellar-Mass Seeds","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1402.6995","snapshot_observed_at":"2026-08-14T04:19:20.936513Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":97,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:20.936513Z"},"links":{"cited_paper":"/paper/1402.6995","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:14b48a43b336aeb39aec4d18125d121c8ea4df695aec4e485789d4e267c082ac","observation_id":"fd18d74c-a62c-4e88-b8b8-e556549fcbb1","resolution":{"observed_at":"2026-08-14T04:19:20.936513Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1408.1718","last_updated":"2014-10-05T18:51:54Z","snapshot_observed_at":"2026-07-06T03:51:11.258651Z","submitted_at":"2014-08-07T21:38:23Z","title":"Rapid growth of seed black holes in the early universe by supra-exponential accretion","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1408.1718","snapshot_observed_at":"2026-08-14T04:19:20.951814Z","title":"Science , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":98,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:20.951814Z"},"links":{"cited_paper":"/paper/1408.1718","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:7ed200d202be6910f635ec2868439891d7af91a16ff7bb3f91271d39e3715ffb","observation_id":"3b5aaa96-38de-4882-b88f-1319b140ad0f","resolution":{"observed_at":"2026-08-14T04:19:20.951814Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1905.00617","last_updated":"2019-05-02T08:33:07Z","snapshot_observed_at":"2026-08-14T16:38:24.520422Z","submitted_at":"2019-05-02T08:33:07Z","title":"Black hole mass estimates in quasars - A comparative analysis of high- and low-ionization lines","version":1},"cited_work":{"arxiv_id":"1905.00617","doi":null,"metadata_source":"pith","pith_arxiv_id":"1905.00617","snapshot_observed_at":"2026-08-14T04:19:22.152256Z","title":"Black hole mass estimates in quasars - A comparative analysis of high- and low-ionization lines","venue":"astro-ph.GA","work_id":"92d33e4c-847f-4e5e-9ca8-49742358d3a0","year":2019},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":99,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:20.959577Z"},"links":{"cited_paper":"/paper/1905.00617","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:4f83553e13d99cfcb78e6dda1fa903359510ea281bd9ba4ed89699eec624d84b","observation_id":"86ec3284-7706-4281-8306-ed05fdaac1ed","resolution":{"observed_at":"2026-08-14T04:19:22.165038Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0712.1831","last_updated":"2007-12-11T21:22:39Z","snapshot_observed_at":"2026-07-06T01:36:35.924821Z","submitted_at":"2007-12-11T21:22:39Z","title":"Quasar Broad Absorption Line Variability on Multi-Year Time Scales","version":1},"cited_work":{"arxiv_id":"0712.1831","doi":null,"metadata_source":"pith","pith_arxiv_id":"0712.1831","snapshot_observed_at":"2026-08-14T04:19:22.044751Z","title":"Quasar Broad Absorption Line Variability on Multi-Year Time Scales","venue":"astro-ph","work_id":"dff002f6-3c42-4eba-8436-dc395c0d2ffe","year":2007},"citing_paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP","version":1},"reference_index":100,"source":"arxiv_source","source_observed_at":"2026-08-14T04:19:20.966786Z"},"links":{"cited_paper":"/paper/0712.1831","citing_paper":"/paper/2608.10074"},"observation_digest":"sha256:041c367c91143d4e17976bb083d4e32d951ef19a54cba6eee112935d57c6ec57","observation_id":"a8748608-2759-4891-ae15-d5bb9fef5ba4","resolution":{"observed_at":"2026-08-14T04:19:22.062209Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2608.10074","last_updated":"2026-08-10T18:00:02Z","latest_version":1,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-08-14T17:10:49.105024Z","submitted_at":"2026-08-10T18:00:02Z","title":"Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":0,"metadata_mismatch":2,"parse_uncertain":0,"unresolved":74,"verified_exact":24,"verified_fuzzy":0},"total_outbound_references":102},"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":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"thesis":"As of 14 August 2026, this Paper Citation Record lists 100 of 102 outbound references and 0 inbound Pith citation observations for arXiv:2608.10074."}