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Paper Citation Record · LEDGER

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics

As of 16 August 2026, this Paper Citation Record lists 100 of 294 outbound references and 0 inbound Pith citation observations for arXiv:2608.12466.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
2608.12466 v1

Coverage vector

measured 100 of 294 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-16T00:12:18.033468Z

measured 100 of 100 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-16T06:30:59.297886+00:00

measured 0 of 0 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links

measured 0 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: cited_works

Reference resolution

100 of 294 outbound references displayed

  • verified exact2
  • verified fuzzy0
  • unresolved98
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

No source-named external measurement is stored.

Outbound references

Observation a034a3cc-a3dc-4194-a675-d7a716889240 · outbound

This paper cites 2010, , 725, 1620, 10.1088/0004-637X/725/2/1620.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics 2010, , 725, 1620, 10.1088/0004-637X/725/2/1620

Reference 1

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no resolver link, observed 2026-08-16T00:12:17.558653Z

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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.558653Z digest=sha256:cfbb0ee3426075d8a2d93aaa76ec4c065dd3a1192553290494129a13259e215c

Observation 4976524b-87e9-48bc-8266-79f572ab6110 · outbound

This paper cites 2025, , 695, A250, 10.1051/0004-6361/202451731.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics 2025, , 695, A250, 10.1051/0004-6361/202451731

Reference 2

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no resolver link, observed 2026-08-16T00:12:17.564025Z

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source=arxiv_source observed=2026-08-16T00:12:17.564025Z digest=sha256:96808a057165ee798379b4bdf05a79214500830f4ff7cd26a4db7548fa57a074

Observation 59265a72-0c18-426d-b82a-dcc99a252274 · outbound

This paper cites Z., Berg , D.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics Z., Berg , D

Reference 3

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no resolver link, observed 2026-08-16T00:12:17.568669Z

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source=arxiv_source observed=2026-08-16T00:12:17.568669Z digest=sha256:8cbfd1e66ab6fdec00c81f79a1e3564b532512153a6bfa23b48e912921785bba

Observation 4ce539a9-126a-4396-8d3f-8c9d891e04ff · outbound

This paper cites L., et al.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics L., et al

Reference 4

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no resolver link, observed 2026-08-16T00:12:17.573253Z

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source=arxiv_source observed=2026-08-16T00:12:17.573253Z digest=sha256:72aa826c49c6ac343ac54fc83316e0ec9975095f90e1f7d0d411e57f3e2fb756

Observation 035e2c0b-846f-4972-a9b4-7fc0acd6921f · outbound

This paper cites P., Tollerud , E.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics P., Tollerud , E

Reference 5

Resolution
unresolved
no resolver link, observed 2026-08-16T00:12:17.577896Z

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source=arxiv_source observed=2026-08-16T00:12:17.577896Z digest=sha256:084b836bc4a61dceb6f0e259391507f4870e4e712306366813b2ad5af64531de

Observation 814ed62d-cacf-47bc-ac45-c110e16efbfd · outbound

This paper cites M., Sip o cz , B.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics M., Sip o cz , B

Reference 6

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no resolver link, observed 2026-08-16T00:12:17.582653Z

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source=arxiv_source observed=2026-08-16T00:12:17.582653Z digest=sha256:5ffb96386f0a271489a1e791ac539c22a0c26c8e8c5e97abebc7ba968e5d23da

Observation 457ade29-b51e-4db7-b9c2-d17b01622f6e · outbound

This paper cites M., Lim , P.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics M., Lim , P

Reference 7

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no resolver link, observed 2026-08-16T00:12:17.587881Z

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source=arxiv_source observed=2026-08-16T00:12:17.587881Z digest=sha256:e86cda44778619293e1a892e960cb2c2fb0b1c3bd97971ff7f855e32600a3cbe

Observation b83c4af2-8390-4574-89ae-6ae641197a05 · outbound

This paper cites A., Chisholm , J., Erb , D.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics A., Chisholm , J., Erb , D

Reference 8

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unresolved
no resolver link, observed 2026-08-16T00:12:17.592489Z

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source=arxiv_source observed=2026-08-16T00:12:17.592489Z digest=sha256:5f1d0f2e7a9de46d5d343e0b6278bdba3e5772bb86f53b7f348c834de7d522ed

Observation e417e79b-d659-49b5-b710-8c3231e029af · outbound

This paper cites A., James , B.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics A., James , B

Reference 9

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no resolver link, observed 2026-08-16T00:12:17.597125Z

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source=arxiv_source observed=2026-08-16T00:12:17.597125Z digest=sha256:e033702bd357440fd5b6c24aa3f1e80bd014fb2d8546a0cc28252f84fb462c5b

Observation a03cac02-3ee0-4bf0-9f11-e5a3132f45aa · outbound

This paper cites A., Naidu , R.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics A., Naidu , R

Reference 10

Resolution
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no resolver link, observed 2026-08-16T00:12:17.601562Z

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source=arxiv_source observed=2026-08-16T00:12:17.601562Z digest=sha256:3561a5f25ac35833ccc776a718fc2a21e61055df7af3e873d1fdd3142a53e27c

Observation dd48944c-dcec-4135-912b-9297f57de47f · outbound

This paper cites 2025, , 983, L30, 10.3847/2041-8213/adc735.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics 2025, , 983, L30, 10.3847/2041-8213/adc735

Reference 11

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no resolver link, observed 2026-08-16T00:12:17.605933Z

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source=arxiv_source observed=2026-08-16T00:12:17.605933Z digest=sha256:409848e00ec27e98d9d2fe1a3916bc09c1f6dd408d8c89e173023c3a7da630f8

Observation 7d5a48fc-84b3-462c-a4f3-93e0a044bf05 · outbound

This paper cites 2025, astropy/photutils: 2.3.0 , 2.3.0, Zenodo, 10.5281/zenodo.17129028.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics 2025, astropy/photutils: 2.3.0 , 2.3.0, Zenodo, 10.5281/zenodo.17129028

Reference 12

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no resolver link, observed 2026-08-16T00:12:17.610137Z

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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.610137Z digest=sha256:eaa375caa410280709c9ce012cecb6d9f13e55085f38a233fb9bdcfe92f61797

Observation 5a68b7e6-7976-4c48-812d-3e7716d9b560 · outbound

This paper cites 2023, msaexp: NIRSpec analyis tools , 0.6.17, Zenodo, 10.5281/zenodo.7299500.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics 2023, msaexp: NIRSpec analyis tools , 0.6.17, Zenodo, 10.5281/zenodo.7299500

Reference 13

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unresolved
no resolver link, observed 2026-08-16T00:12:17.614720Z

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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.614720Z digest=sha256:e66e68ba2baa864d27cc62c868655bb1879bb80fdb6444852b69ee3a64f84d0f

Observation bc813014-e614-4452-9f91-559532faf5fc · outbound

This paper cites J., Saxena , A., Cameron , A.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics J., Saxena , A., Cameron , A

Reference 14

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unresolved
no resolver link, observed 2026-08-16T00:12:17.619464Z

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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.619464Z digest=sha256:a067e32251861191faa2a050b608a481b53ee48b5d9cfba5628b5b12283485b4

Observation 465e73fb-7bf9-44ba-a6fe-e08934177034 · outbound

This paper cites 2026, JWST Calibration Pipeline , 2.0.1, Zenodo, 10.5281/zenodo.20058613.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics 2026, JWST Calibration Pipeline , 2.0.1, Zenodo, 10.5281/zenodo.20058613

Reference 15

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no resolver link, observed 2026-08-16T00:12:17.624103Z

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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.624103Z digest=sha256:5f822807834b7c5679cfb5b8d32c003677621a3176a4341250f138f9619547ee

Observation fec16c4b-a551-42d7-afbe-be3760c0dbbc · outbound

This paper cites C., et al.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics C., et al

Reference 16

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unresolved
no resolver link, observed 2026-08-16T00:12:17.629099Z

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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.629099Z digest=sha256:df761e39a89c35da08f371479308392d6c131f0115a9b12e49b268bc95ed1548

Observation ef73e7a4-6503-44a2-9a81-274326b59462 · outbound

This paper cites J., Katz , H., Rey , M.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics J., Katz , H., Rey , M

Reference 17

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unresolved
no resolver link, observed 2026-08-16T00:12:17.634526Z

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source=arxiv_source observed=2026-08-16T00:12:17.634526Z digest=sha256:8ad94f2039c0959349ba983600a89a30d997b0db6a63922ef50da887cdb43026

Observation fc2d76e0-3d96-4fcf-b6d6-bf9409f87c19 · outbound

This paper cites G., Lucatello , S., Bragaglia , A., & Bonifacio , P.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics G., Lucatello , S., Bragaglia , A., & Bonifacio , P

Reference 18

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no resolver link, observed 2026-08-16T00:12:17.639093Z

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source=arxiv_source observed=2026-08-16T00:12:17.639093Z digest=sha256:2f436f3a71af0a757625796a1e3fc0351d5fcc46fea39fdf680079db4aa791bb

Observation 6fe1602c-f28b-4b5a-990a-05b22ccf8460 · outbound

This paper cites H., Kulkarni , V.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics H., Kulkarni , V

Reference 19

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unresolved
no resolver link, observed 2026-08-16T00:12:17.643807Z

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source=arxiv_source observed=2026-08-16T00:12:17.643807Z digest=sha256:fc5b7b9431d1619799512ab670852c42d6855e170306693bb46d876337a5c99f

Observation 4bd84ade-5a49-4257-95a1-7ae5327f2bff · outbound

This paper cites 2024, , 972, 143, 10.3847/1538-4357/ad5f88.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics 2024, , 972, 143, 10.3847/1538-4357/ad5f88

Reference 20

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unresolved
no resolver link, observed 2026-08-16T00:12:17.648494Z

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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.648494Z digest=sha256:dcd650598643229ddb0b5a928e76638e8f473e8f0933b5bb13321b9eca59d581

Observation d2a6f039-db48-4674-b1cb-09e915b94829 · outbound

This paper cites I., Abbott , D.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics I., Abbott , D

Reference 21

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unresolved
no resolver link, observed 2026-08-16T00:12:17.652787Z

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source=arxiv_source observed=2026-08-16T00:12:17.652787Z digest=sha256:d3757e3b72c3a26dc3b484783255391323f3ab6cbfce7a79ab0f0fe06e4095d4

Observation ee23b51f-61f5-49f3-b16d-d418b8b9b874 · outbound

This paper cites 2023, , 673, L7, 10.1051/0004-6361/202346410.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics 2023, , 673, L7, 10.1051/0004-6361/202346410

Reference 22

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no resolver link, observed 2026-08-16T00:12:17.657166Z

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source=arxiv_source observed=2026-08-16T00:12:17.657166Z digest=sha256:efe1e40dec100fc3a15d5aff375ac6edbd94b3b13b2c7f80451d222b73c5a644

Observation 42068bc1-1b94-4015-86e4-739535b7854d · outbound

This paper cites SPURS: Bursty Star Formation in an Extremely Luminous Weak Emission Line Galaxy at $z=9.3$.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics SPURS: Bursty Star Formation in an Extremely Luminous Weak Emission Line Galaxy at $z=9.3$

Reference 23

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unresolved
no resolver link, observed 2026-08-16T00:12:17.662921Z

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source=arxiv_source observed=2026-08-16T00:12:17.662921Z digest=sha256:c1adf09f558b1f3dfe368ed0fad5692d4b32e32b27edf7e1555d28fc2f968c66

Observation 9506dd47-0019-4794-acab-e44d1a1e97df · outbound

This paper cites R., Bayliss , M., et al.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics R., Bayliss , M., et al

Reference 24

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no resolver link, observed 2026-08-16T00:12:17.668512Z

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source=arxiv_source observed=2026-08-16T00:12:17.668512Z digest=sha256:bf954bde1bdcd687d99eb4d0c3954f28606b2640e8e6ed92ec6bb279ebafd38c

Observation f5d2579a-03d4-40a0-a2cf-bb9580d093b0 · outbound

This paper cites 2021, , 508, 4175, 10.1093/mnras/stab2497.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics 2021, , 508, 4175, 10.1093/mnras/stab2497

Reference 25

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no resolver link, observed 2026-08-16T00:12:17.673156Z

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source=arxiv_source observed=2026-08-16T00:12:17.673156Z digest=sha256:60fa56338793d1701113a217760a006de51b185c7e4e016b1ad66c70b6e12c20

Observation 1fc8ba49-3dcd-4629-b058-503d9287fcdb · outbound

This paper cites G., et al.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics G., et al

Reference 26

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unresolved
no resolver link, observed 2026-08-16T00:12:17.677587Z

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source=arxiv_source observed=2026-08-16T00:12:17.677587Z digest=sha256:cabff3e2548089841ea616f8f6150414443dce6d2eb02b5e38604335449feb4b

Observation 4125c69d-695f-43ce-932d-a8226e5c6bc0 · outbound

This paper cites 2026, , 710, A18, 10.1051/0004-6361/202558145.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics 2026, , 710, A18, 10.1051/0004-6361/202558145

Reference 27

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unresolved
no resolver link, observed 2026-08-16T00:12:17.682019Z

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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.682019Z digest=sha256:9dcf8f279fc378b15b2f0a1db126a3560b715c6d225f688060f91242669a45ff

Observation c416d188-d4a8-4d8b-accd-c75944f6a12d · outbound

This paper cites 2023, Nature Astronomy, 7, 622, 10.1038/s41550-023-01918-w.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics 2023, Nature Astronomy, 7, 622, 10.1038/s41550-023-01918-w

Reference 28

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unresolved
no resolver link, observed 2026-08-16T00:12:17.686341Z

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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.686341Z digest=sha256:93bd5d3aee8eab370be42f656b474f9102b0e8036d6601ac039d216f5a92bcf1

Observation 1de0416d-6e21-4130-af94-5dc574570ffb · outbound

This paper cites 2024, , 684, A87, 10.1051/0004-6361/202347755.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics 2024, , 684, A87, 10.1051/0004-6361/202347755

Reference 29

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unresolved
no resolver link, observed 2026-08-16T00:12:17.690539Z

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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.690539Z digest=sha256:ea5fe32323b1dd255d097338d5185b6678f766fdc13c4d307e265317d8dd9872

Observation 30d2489a-289e-45e7-a997-e63dcd409285 · outbound

This paper cites C., Birnboim , Y., Mandelker , N., & Li , Z.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics C., Birnboim , Y., Mandelker , N., & Li , Z

Reference 30

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unresolved
no resolver link, observed 2026-08-16T00:12:17.694985Z

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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.694985Z digest=sha256:a1259c45c03f39e9f35526f04b2e128aebf1f68209bbecea9a9cc89294399023

Observation 90f33ab5-900b-4745-b0e9-4fa047d53781 · outbound

This paper cites 2026, , 547, stag401, 10.1093/mnras/stag401.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics 2026, , 547, stag401, 10.1093/mnras/stag401

Reference 31

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no resolver link, observed 2026-08-16T00:12:17.699434Z

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source=arxiv_source observed=2026-08-16T00:12:17.699434Z digest=sha256:7ea257e93c6c5cb78bb1ade0b870e2bb3177d3d8633420e0ce9a2cefaee1cd7b

Observation c125daeb-eabe-4713-9406-f82d5d3c293c · outbound

This paper cites T., McLeod , D.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics T., McLeod , D

Reference 32

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unresolved
no resolver link, observed 2026-08-16T00:12:17.703609Z

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source=arxiv_source observed=2026-08-16T00:12:17.703609Z digest=sha256:537aa7a5344cc8c7cf423fecfe04a0ccadeb4e287a1fe336d9668e56579d8098

Observation b62259fe-eb55-4005-977b-cc1a32a66a55 · outbound

This paper cites 2026, , 710, A239, 10.1051/0004-6361/202558704.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics 2026, , 710, A239, 10.1051/0004-6361/202558704

Reference 33

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unresolved
no resolver link, observed 2026-08-16T00:12:17.708651Z

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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.708651Z digest=sha256:74f65a1b1bcd4ddb3ec3b647dbfd525465928dbcfb923c72cb91408d1bac7838

Observation 8b8b60e7-5fcd-4a3a-829f-f951a866be3c · outbound

This paper cites 2026, , 283, 6, 10.3847/1538-4365/ae3163.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics 2026, , 283, 6, 10.3847/1538-4365/ae3163

Reference 35

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unresolved
no resolver link, observed 2026-08-16T00:12:17.718880Z

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source=arxiv_source observed=2026-08-16T00:12:17.718880Z digest=sha256:3a24e8db6c4b3471e10a0db5df03a4b89ef6db41846dae20edde58017a85d86b

Observation 56392dfa-cdeb-4cb5-8338-4e5847653bb1 · outbound

This paper cites J., Stanway , E.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics J., Stanway , E

Reference 36

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unresolved
no resolver link, observed 2026-08-16T00:12:17.723444Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.723444Z digest=sha256:f99d10f2f06d40ecb440759bc6d044112ec5f6b0c0c9131c202de6927228840d

Observation 5b714550-0ef1-47c3-8ec6-10e3185b0fc5 · outbound

This paper cites 2024, , 684, A207, 10.1051/0004-6361/202348321.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics 2024, , 684, A207, 10.1051/0004-6361/202348321

Reference 38

Resolution
unresolved
no resolver link, observed 2026-08-16T00:12:17.732117Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.732117Z digest=sha256:66d2ee184dcb12c9deb0aac4211f84fe75aeacab3b27c59d4bf6917884b52d5e

Observation 456d7bc1-b7ea-4134-ab95-b1eb8daf6a7e · outbound

This paper cites 2023, , 522, 3986, 10.1093/mnras/stad1095.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics 2023, , 522, 3986, 10.1093/mnras/stad1095

Reference 39

Resolution
unresolved
no resolver link, observed 2026-08-16T00:12:17.736462Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.736462Z digest=sha256:62976713545f47b867e8660ca9fbf6e2a310899859370a53f49db085414e2384

Observation 3d7b31d5-95e9-4a4d-9f87-89996bef62f4 · outbound

This paper cites L., Bagley , M.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics L., Bagley , M

Reference 40

Resolution
unresolved
no resolver link, observed 2026-08-16T00:12:17.740794Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.740794Z digest=sha256:f17a8c85e554eadc65d22c0982ed9c1f3d95823ce6acc84a85ae93b2558a2d40

Observation 1f726756-bad1-4c84-8643-adbb460189f3 · outbound

This paper cites W., Lang , D., & Goodman , J.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics W., Lang , D., & Goodman , J

Reference 41

Resolution
unresolved
no resolver link, observed 2026-08-16T00:12:17.745098Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.745098Z digest=sha256:560d70d32df726a46597db0dd89f4f8ec6bc4f7b054fa42f2ca404aae3554d5c

Observation c9dbcd24-5275-407e-a80f-e4ffddb6d406 · outbound

This paper cites R., et al.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics R., et al

Reference 42

Resolution
unresolved
no resolver link, observed 2026-08-16T00:12:17.749560Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.749560Z digest=sha256:656fe7eee0e9157568dea5711f358896481119e482d0d9eec712067b0bafaed6

Observation 99f9a38e-a04a-4bcd-8ec5-1b92ab1f4c14 · outbound

This paper cites 2021, , 506, 5512, 10.1093/mnras/stab2099.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics 2021, , 506, 5512, 10.1093/mnras/stab2099

Reference 43

Resolution
unresolved
no resolver link, observed 2026-08-16T00:12:17.754059Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.754059Z digest=sha256:e2d8e1acebdb7424802187684dfc8679d4aa6cd439415c364e3134d0c32d1cca

Observation 211b4957-57a9-4c89-8b1e-646f18657efa · outbound

This paper cites 2024, , 76, 1122, 10.1093/pasj/psae074.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics 2024, , 76, 1122, 10.1093/pasj/psae074

Reference 44

Resolution
unresolved
no resolver link, observed 2026-08-16T00:12:17.758335Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.758335Z digest=sha256:47900a087649e48e51a6ab5d237b2aac7903f832745ce1c243d6e2f029e4c1c3

Observation 49cb2117-6013-4333-9d40-22bc94d528f5 · outbound

This paper cites 2007, , 670, 457, 10.1086/521871.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics 2007, , 670, 457, 10.1086/521871

Reference 45

Resolution
unresolved
no resolver link, observed 2026-08-16T00:12:17.762656Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.762656Z digest=sha256:7b0b15db8df6c4c649f07e02b6e461613c9f242a3741acdff9990c657547256d

Observation 5757bfdf-4866-497d-9a35-c2b2e8e89341 · outbound

This paper cites J., et al.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics J., et al

Reference 46

Resolution
verified exact
doi, observed 2026-08-16T00:13:35.291384Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

source=arxiv_source observed=2026-08-16T00:12:17.766923Z digest=sha256:ca470e7580909a634b20772b842131a053f093c92ac937e868522fbe293e3680

Observation 14961a48-c699-44f2-a5ea-e80eca23a5a9 · outbound

This paper cites E., & Ho , L.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics E., & Ho , L

Reference 47

Resolution
unresolved
no resolver link, observed 2026-08-16T00:12:17.771401Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.771401Z digest=sha256:fa40cf3d936e7361da0ff950cc7167df78f52352d6f1107e05c1045db1f0a76b

Observation 55ede41b-a92c-4e17-a523-b8c7d24c78b0 · outbound

This paper cites M., van Hoof , P.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics M., van Hoof , P

Reference 48

Resolution
unresolved
no resolver link, observed 2026-08-16T00:12:17.775501Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.775501Z digest=sha256:2bf93599e3b7e1bebe7385a099ca23d312e6b005659c727f1ae4e6c9933fcab8

Observation fd424851-3a73-467d-92d2-99ec93d643e0 · outbound

This paper cites an unresolved cited work.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics Unresolved cited work

Reference 49

Resolution
verified exact
doi, observed 2026-08-16T00:13:35.142022Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

source=arxiv_source observed=2026-08-16T00:12:17.779883Z digest=sha256:c278a44e366c5e18de7c503d808633a1dd3aea47c8581a066adb9a850bd321c0

Observation d129f82d-1369-4e87-8616-8d5ac224c5a4 · outbound

This paper cites J., & Crowther , P.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics J., & Crowther , P

Reference 50

Resolution
unresolved
no resolver link, observed 2026-08-16T00:12:17.784098Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.784098Z digest=sha256:fcc889589a9e7cb0526ddc68af4597412d105f1140b9bbceead5dc68acc54f5e

Observation 4fdf2084-2f6b-4315-b504-71864ae5168b · outbound

This paper cites 2006, , 457, 1015, 10.1051/0004-6361:20065052.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics 2006, , 457, 1015, 10.1051/0004-6361:20065052

Reference 51

Resolution
unresolved
no resolver link, observed 2026-08-16T00:12:17.788981Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.788981Z digest=sha256:c2aeb5e52cd11fd18b295c3d5f20477c1f53495d759093212663cda02f129346

Observation d2baf0cc-9f99-42b3-a512-ada3db08e6f0 · outbound

This paper cites 2024, , 960, 56, 10.3847/1538-4357/ad0b7e.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics 2024, , 960, 56, 10.3847/1538-4357/ad0b7e

Reference 52

Resolution
unresolved
no resolver link, observed 2026-08-16T00:12:17.793662Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.793662Z digest=sha256:57dd597914f057afd853737b4395d5eef378fc1dd0ee24f339fd6599b214d561

Observation 3554afeb-905d-40ee-9df0-f69e339fbb5c · outbound

This paper cites 2023, , 959, 39, 10.3847/1538-4357/ad029e.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics 2023, , 959, 39, 10.3847/1538-4357/ad029e

Reference 53

Resolution
unresolved
no resolver link, observed 2026-08-16T00:12:17.798070Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.798070Z digest=sha256:2ae4cf16b564435fc3428b7a8116b81f4511dbd90796da331e7c8bea644b4d2f

Observation 4e58c00a-721d-4d8d-a282-f9e60e58e74b · outbound

This paper cites K., Ellis , R.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics K., Ellis , R

Reference 54

Resolution
unresolved
no resolver link, observed 2026-08-16T00:12:17.803139Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.803139Z digest=sha256:a5b848dacb349882a4fddbd0b8a5a178cc8c68fc63d4041c5d89e5db832dd4d5

Observation 831413ef-3195-4c19-9dbd-3b1fae28305d · outbound

This paper cites G., Alvarez-Marquez , J., et al.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics G., Alvarez-Marquez , J., et al

Reference 55

Resolution
unresolved
no resolver link, observed 2026-08-16T00:12:17.808419Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.808419Z digest=sha256:330fd1caa9fc8d20e4feead07c4e450716381395861bafb1c13f1b5fc001cfde

Observation 25c1cb7e-1a3d-4f2f-9573-ee9c4ddba04f · outbound

This paper cites 2024, , 688, A105, 10.1051/0004-6361/202245588.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics 2024, , 688, A105, 10.1051/0004-6361/202245588

Reference 57

Resolution
unresolved
no resolver link, observed 2026-08-16T00:12:17.816960Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.816960Z digest=sha256:de9ae4170cd927232493bc975ae67c36e63192cc57af2a0312e33cfc0c7ec368

Observation 761b23e6-fe83-4a37-955e-a06e383eb265 · outbound

This paper cites M., & Furlanetto , S.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics M., & Furlanetto , S

Reference 58

Resolution
unresolved
no resolver link, observed 2026-08-16T00:12:17.821183Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.821183Z digest=sha256:7659d9ee189b78b8e5753088267f2fcb308cf22eff290860f97ba6f0b037dc8e

Observation eec2753c-a11c-48ef-8d7a-7bbbbdbbc494 · outbound

This paper cites E., Brammer , G.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics E., Brammer , G

Reference 59

Resolution
unresolved
no resolver link, observed 2026-08-16T00:12:17.825916Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.825916Z digest=sha256:38371e2f1041085f03ad4fb79010bb06942dd94d21776586f79669da98781cb1

Observation 5c99fb32-8c42-480b-837a-55e468d1fbaf · outbound

This paper cites J., Koenigsberger , G., Naz \'e , Y., et al.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics J., Koenigsberger , G., Naz \'e , Y., et al

Reference 60

Resolution
unresolved
no resolver link, observed 2026-08-16T00:12:17.830204Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.830204Z digest=sha256:034c8ff422ccc514d4e6053363d72a4b64a7bda314dc0ebddd7bfdc3635b51cc

Observation f85c0e92-9527-4118-b663-be12d3404e52 · outbound

This paper cites C., Feigelson , E.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics C., Feigelson , E

Reference 61

Resolution
unresolved
no resolver link, observed 2026-08-16T00:12:17.834547Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.834547Z digest=sha256:645892586effcf07923aba8335f80280753efea01215ecab6c489a1e079a217a

Observation 9c799e8d-196d-4516-b5c2-069b5ed654fd · outbound

This paper cites 1986, , 98, 609, 10.1086/131801.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics 1986, , 98, 609, 10.1086/131801

Reference 62

Resolution
unresolved
no resolver link, observed 2026-08-16T00:12:17.838733Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.838733Z digest=sha256:8ee813862d70b82867480ff81c700fcef6b2e4fdde7fafd04cb17c44711c3297

Observation 639cf488-02b0-4d92-b581-0b8f7139e3f4 · outbound

This paper cites an unresolved cited work.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics Unresolved cited work

Reference 63

Resolution
unresolved
no resolver link, observed 2026-08-16T00:12:17.843374Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.843374Z digest=sha256:3a0039d155cfd5866cb8916ee1fb922be716b5629351fa56a0cc54cbdd4661e5

Observation acae43b0-6dd0-4d7f-ad31-ff5ae5ba1b15 · outbound

This paper cites K., Shimizu , I., Iwata , I., & Tanaka , M.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics K., Shimizu , I., Iwata , I., & Tanaka , M

Reference 64

Resolution
unresolved
no resolver link, observed 2026-08-16T00:12:17.848120Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.848120Z digest=sha256:18a8d65572cbcbd0ae55965e18882e7872dc3e64cff1318b9b9ca97520a7260c

Observation efd94376-31c5-4cda-913b-89040b85509c · outbound

This paper cites 2023 a , , 956, 139, 10.3847/1538-4357/acf376.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics 2023 a , , 956, 139, 10.3847/1538-4357/acf376

Reference 65

Resolution
unresolved
no resolver link, observed 2026-08-16T00:12:17.852875Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.852875Z digest=sha256:5002822094bb898670ccd94f51a0620aaf81bc80e3993590fb443952c1f00990

Observation d402fd58-5b5a-489c-b9ff-8049eafa566d · outbound

This paper cites 2023 b , , 959, 100, 10.3847/1538-4357/ad09be.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics 2023 b , , 959, 100, 10.3847/1538-4357/ad09be

Reference 66

Resolution
unresolved
no resolver link, observed 2026-08-16T00:12:17.857121Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.857121Z digest=sha256:9659984ae8c4bbeffa029626eedcb00c6dc6ea9519be06ed00e16d8256e94ec8

Observation a8ab01f4-63be-4d30-bd96-bea2dd1c3051 · outbound

This paper cites 2026, , 547, stag123, 10.1093/mnras/stag123.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics 2026, , 547, stag123, 10.1093/mnras/stag123

Reference 67

Resolution
unresolved
no resolver link, observed 2026-08-16T00:12:17.861244Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.861244Z digest=sha256:e117179c9635ff6a54aca688a574ecf2451ef6e31c981ab267b68eed57002c65

Observation 200ac07b-c2f2-4399-b5ad-229fac6f447b · outbound

This paper cites I., Stasi \'n ska , G., Meynet , G., Guseva , N.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics I., Stasi \'n ska , G., Meynet , G., Guseva , N

Reference 68

Resolution
unresolved
no resolver link, observed 2026-08-16T00:12:17.865293Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.865293Z digest=sha256:96d1ad884857a4803c7b4add1a7b7f599b348ebc3f0ea2c53af38d78b5699fc6

Observation fd013436-cb63-4633-85cd-b46cd57dba6e · outbound

This paper cites L., Tsamis , Y.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics L., Tsamis , Y

Reference 69

Resolution
unresolved
no resolver link, observed 2026-08-16T00:12:17.869403Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.869403Z digest=sha256:755c7cd7a586a4a19767e19f460e8a6b2e836aecafd1c2c9ff8f3eb86d2f542f

Observation 68249aca-3046-4f98-b067-a0b2ae05c5b1 · outbound

This paper cites L., Abril-Melgarejo , V., Arellano-C \'o rdova , K.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics L., Abril-Melgarejo , V., Arellano-C \'o rdova , K

Reference 70

Resolution
unresolved
no resolver link, observed 2026-08-16T00:12:17.873697Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.873697Z digest=sha256:b36155ff3dd5788daadc746ec77d7d0e0e44c02d0216332ff6ae90e901135402

Observation 7ad8d26a-be4a-44a0-ae7e-002ce1386137 · outbound

This paper cites 2026, , 545, staf2110, 10.1093/mnras/staf2110.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics 2026, , 545, staf2110, 10.1093/mnras/staf2110

Reference 71

Resolution
unresolved
no resolver link, observed 2026-08-16T00:12:17.877966Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.877966Z digest=sha256:e897d90032757dd4baaba5416fcea64d1b33ab4494e9a71f54758bf53109bb4e

Observation b83c4a66-8d4a-471c-97af-a08dfdb770fd · outbound

This paper cites 2024, , 10.1093/mnras/stae2375.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics 2024, , 10.1093/mnras/stae2375

Reference 72

Resolution
unresolved
no resolver link, observed 2026-08-16T00:12:17.882111Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.882111Z digest=sha256:9b46972a3b787512f1b8119d44cd8d529264e2eb41278b9812fb57e05080490e

Observation 209109e8-ad3f-41f3-9d36-01463ef00287 · outbound

This paper cites 2008, , 679, 962, 10.1086/587868.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics 2008, , 679, 962, 10.1086/587868

Reference 73

Resolution
unresolved
no resolver link, observed 2026-08-16T00:12:17.886255Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.886255Z digest=sha256:11ab15edf529dffbaf3f99902ab5d8dd0f3fe59568c20f40d1941f0d3e9923a1

Observation 8fb5c549-7243-4b98-8c63-69225485b4d5 · outbound

This paper cites 2012, , 422, 3268, 10.1111/j.1365-2966.2012.20847.x.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics 2012, , 422, 3268, 10.1111/j.1365-2966.2012.20847.x

Reference 74

Resolution
unresolved
no resolver link, observed 2026-08-16T00:12:17.891297Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.891297Z digest=sha256:4adb389398d1f2cf6c93884f5e32980dc0df3b992fb4a3eefd355b0ff283df28

Observation b838c730-4df9-4ea3-bd73-2e817ca8ab48 · outbound

This paper cites A., Ellis , R.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics A., Ellis , R

Reference 75

Resolution
unresolved
no resolver link, observed 2026-08-16T00:12:17.896484Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.896484Z digest=sha256:dd0f3f1d73a062f8c58d877698b542b67710daf876dec21d6ccaba5972396d8f

Observation dc6083a7-f524-4d38-a44a-92b0a1adbbee · outbound

This paper cites 2025, , 278, 33, 10.3847/1538-4365/adc690.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics 2025, , 278, 33, 10.3847/1538-4365/adc690

Reference 76

Resolution
unresolved
no resolver link, observed 2026-08-16T00:12:17.900718Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.900718Z digest=sha256:352253afc282f35edaba53c52ad8d298afd152babe580674c00342a4a1874e44

Observation 6a353180-e0a6-4d87-bc86-f4c2683dda8e · outbound

This paper cites 2025, , 995, 150, 10.3847/1538-4357/ae1cc3.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics 2025, , 995, 150, 10.3847/1538-4357/ae1cc3

Reference 77

Resolution
unresolved
no resolver link, observed 2026-08-16T00:12:17.904990Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.904990Z digest=sha256:384ce54c526b4ad04b860697f8397c88795c0b19ce252445c68de8d975ebe86e

Observation c12d9fbf-bcec-423b-aea4-c4c3c1481a1e · outbound

This paper cites 2024 b , , 962, L6, 10.3847/2041-8213/ad1de1.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics 2024 b , , 962, L6, 10.3847/2041-8213/ad1de1

Reference 79

Resolution
unresolved
no resolver link, observed 2026-08-16T00:12:17.914733Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.914733Z digest=sha256:7bced372997c4358b00ce61565437c6f184545a27ec03f382e48ae8529b9a4ef

Observation 70b567c7-7bf2-4ac4-ab3c-884285f93c93 · outbound

This paper cites C., Kim , J.-G., & Kim , C.-G.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics C., Kim , J.-G., & Kim , C.-G

Reference 80

Resolution
unresolved
no resolver link, observed 2026-08-16T00:12:17.919665Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.919665Z digest=sha256:295cb5502f92e915521f312e45d7db140d77bf9e850908ef0915b7156a4ab76b

Observation 10a7cc8d-d631-481f-8711-a290c57c9c73 · outbound

This paper cites L., Finkelstein , S.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics L., Finkelstein , S

Reference 81

Resolution
unresolved
no resolver link, observed 2026-08-16T00:12:17.924931Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.924931Z digest=sha256:b34c8a7b36a417910f5df3ac7c2c4fa48cec0ad7abb1689831c8e6b5ea3b5995

Observation 08b10bc7-5470-4b90-9c51-455162bf4e5b · outbound

This paper cites 1992, , 401, 596, 10.1086/172089.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics 1992, , 401, 596, 10.1086/172089

Reference 82

Resolution
unresolved
no resolver link, observed 2026-08-16T00:12:17.929273Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.929273Z digest=sha256:db7663161ee2c0ceafeff0878f395d1d1529fdf388dc9fd163b46b5b95426b4d

Observation d6e8d158-1028-4364-9323-8e2e2e9f07c9 · outbound

This paper cites A., Heckman , T.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics A., Heckman , T

Reference 83

Resolution
unresolved
no resolver link, observed 2026-08-16T00:12:17.933536Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.933536Z digest=sha256:2cbd953bad1ef93ac96d0532d9eb01e29bca5c515fe2295814f70518a7033ec7

Observation 6951198d-0311-42ac-b1a9-fc947e3896c9 · outbound

This paper cites an unresolved cited work.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics Unresolved cited work

Reference 84

Resolution
unresolved
no resolver link, observed 2026-08-16T00:12:17.937838Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.937838Z digest=sha256:b30f8cc14e5e03a6629309de642dc6eb26008f99f5af34e59955d2c7d24cbb71

Observation 65c61aa2-a8b1-493a-8b0a-d573bec371cd · outbound

This paper cites 2024, , 627, 59, 10.1038/s41586-024-07052-5.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics 2024, , 627, 59, 10.1038/s41586-024-07052-5

Reference 85

Resolution
unresolved
no resolver link, observed 2026-08-16T00:12:17.942849Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.942849Z digest=sha256:0141261a6f89cc539ed3ab215ff95de66a14b553c4c82c8f03b1107237a2c1b2

Observation acf3464f-26a2-4295-8dae-6a641b6fe624 · outbound

This paper cites The search for Population III: Confirmation of a HeII emitter with no metal lines at z=10.6.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics The search for Population III: Confirmation of a HeII emitter with no metal lines at z=10.6

Reference 86

Resolution
unresolved
no resolver link, observed 2026-08-16T00:12:17.947009Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.947009Z digest=sha256:1d985063b33e59eb8d9f6499125dfa1332b79fe512127a47e52a55cc12e2ff23

Observation 1f4e3282-ffd4-43bb-a5a9-84a791751dc9 · outbound

This paper cites Signatures of Very Massive Stars in the Epoch of Reionization.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics Signatures of Very Massive Stars in the Epoch of Reionization

Reference 87

Resolution
unresolved
no resolver link, observed 2026-08-16T00:12:17.952644Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.952644Z digest=sha256:40dbf22329b46ce725509ab3e526b9c0cab102f2b3e99092251be20b33582571

Observation e0e9a8eb-c5ba-42e1-a473-b041cdfc6bc0 · outbound

This paper cites 1995, , 298, 767.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics 1995, , 298, 767

Reference 88

Resolution
unresolved
no resolver link, observed 2026-08-16T00:12:17.956975Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.956975Z digest=sha256:86a8a178acf62c20128cc10e8d2302b2bacc752617cfcbc3643692642650c7d8

Observation d879cd56-2e48-4286-a706-02e895f9313b · outbound

This paper cites L., Arellano-C \'o rdova , K.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics L., Arellano-C \'o rdova , K

Reference 89

Resolution
unresolved
no resolver link, observed 2026-08-16T00:12:17.961097Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.961097Z digest=sha256:66a17c462cac9ebdd16ec18c4d609b0a18d894d34a90553f373d724067f6d0b8

Observation 4592f54a-ef2f-4fea-8621-ae50b5d4f51f · outbound

This paper cites B., Mirocha , J., Furlanetto , S., & Sabti , N.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics B., Mirocha , J., Furlanetto , S., & Sabti , N

Reference 90

Resolution
unresolved
no resolver link, observed 2026-08-16T00:12:17.965463Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.965463Z digest=sha256:ab4c1850bb35a11113be9f4344a3f1ea9e9284dc1e4f9f23a0756b37a0f99f13

Observation 94964076-2eee-491c-8f7d-8c1656a01b7d · outbound

This paper cites 2023, , 949, L16, 10.3847/2041-8213/acd550.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics 2023, , 949, L16, 10.3847/2041-8213/acd550

Reference 91

Resolution
unresolved
no resolver link, observed 2026-08-16T00:12:17.969758Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.969758Z digest=sha256:0937ebbcefbcaa152e59d1bbd68043da981cb63d3495136b3c447df97fa973ff

Observation 4601906c-c0d7-4970-878a-0d5e0178bded · outbound

This paper cites P., Oesch , P.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics P., Oesch , P

Reference 92

Resolution
unresolved
no resolver link, observed 2026-08-16T00:12:17.974174Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.974174Z digest=sha256:17d0934e0af8533e5716216bfd6ea191e17806a4d3a7292a617e4e1bd3323ef0

Observation e05f1942-b0ec-4860-909e-536f971b4f09 · outbound

This paper cites JWST Absorption-Line Analysis of UV-Bright Galaxies at $z=7.2-10.6$: Early Chemical Enrichment Traced by C, O, Mg, Al, Si, and Fe.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics JWST Absorption-Line Analysis of UV-Bright Galaxies at $z=7.2-10.6$: Early Chemical Enrichment Traced by C, O, Mg, Al, Si, and Fe

Reference 93

Resolution
unresolved
no resolver link, observed 2026-08-16T00:12:17.978421Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.978421Z digest=sha256:cd9f867b81be40d84233b58b347c7088b20b091d7fd4db222375849f7c8d75c4

Observation 51c28898-7b0a-48f2-b8ed-98fdaa5d2ed6 · outbound

This paper cites 2024 a , , 976, 122, 10.3847/1538-4357/ad84e810.1134/S1063773708080045.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics 2024 a , , 976, 122, 10.3847/1538-4357/ad84e810.1134/S1063773708080045

Reference 94

Resolution
unresolved
no resolver link, observed 2026-08-16T00:12:17.982933Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.982933Z digest=sha256:8cfbf1b696ef23dafa1c459b9f6d2e33d277c49a730f86a707b60d2ef220b58d

Observation cc93536b-9af7-4129-a806-a7743c0f143f · outbound

This paper cites 2024 b , , 967, 28, 10.3847/1538-4357/ad38c2.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics 2024 b , , 967, 28, 10.3847/1538-4357/ad38c2

Reference 95

Resolution
unresolved
no resolver link, observed 2026-08-16T00:12:17.987717Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.987717Z digest=sha256:d94f82772ccc00eb350b01501a23ed3f17fe1c68ff68b17d69b952c6c024ab8e

Observation adee739d-c5a2-495b-81ae-01c902281840 · outbound

This paper cites 2025, , 994, 65, 10.3847/1538-4357/ae04e6.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics 2025, , 994, 65, 10.3847/1538-4357/ae04e6

Reference 96

Resolution
unresolved
no resolver link, observed 2026-08-16T00:12:17.992421Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.992421Z digest=sha256:60a0004a767366d76b7ed3ec955acd9134f20dc3094a352336e3bc6707dabf0e

Observation 59f0b128-bce5-4753-8d89-d3f6b8960dba · outbound

This paper cites J., Latif , M.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics J., Latif , M

Reference 97

Resolution
unresolved
no resolver link, observed 2026-08-16T00:12:17.997523Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.997523Z digest=sha256:8c5b56ca535f883630954286b6498896931d0a31133d76a4326449ed88b50bc7

Observation d951b26a-ef93-4850-a8dd-25d5c18ed4fc · outbound

This paper cites 2025, , 693, A50, 10.1051/0004-6361/202452090.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics 2025, , 693, A50, 10.1051/0004-6361/202452090

Reference 98

Resolution
unresolved
no resolver link, observed 2026-08-16T00:12:18.002565Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:18.002565Z digest=sha256:661820b2350879ea6c5b1ae26625812d05712b7d0d233bfb6ac3a473310276b6

Observation b14a1155-8e69-4136-bdc6-6b76c6445cbd · outbound

This paper cites I., Iani , E., et al.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics I., Iani , E., et al

Reference 99

Resolution
unresolved
no resolver link, observed 2026-08-16T00:12:18.006961Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:18.006961Z digest=sha256:3c92595ff1f72116772cf1d3b5f4bd5b044e3b2be9d32d0a1ee7235a39d1e21a

Observation a843fc63-7131-4d54-a0b2-3697a8c5e734 · outbound

This paper cites A., Brammer , G., van Dokkum , P.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics A., Brammer , G., van Dokkum , P

Reference 100

Resolution
unresolved
no resolver link, observed 2026-08-16T00:12:18.011093Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:18.011093Z digest=sha256:85ff3343e2283113d29060b5e19a4c8035e942bdbfc6e36423321d9fceb602ef

Observation a5b73403-2f5b-4863-8e5f-9332d78b3c89 · outbound

This paper cites 2005, , 626, 627, 10.1086/429955.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics 2005, , 626, 627, 10.1086/429955

Reference 102

Resolution
unresolved
no resolver link, observed 2026-08-16T00:12:18.020157Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:18.020157Z digest=sha256:c242d4e4592e75482e1cf3163299014b737eb0215a7bb40c8a7f73766364913c

Observation fa9046d1-4a56-4449-b916-7ac14e00c6f6 · outbound

This paper cites 2020, , 58, 617, 10.1146/annurev-astro-032620-021859.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics 2020, , 58, 617, 10.1146/annurev-astro-032620-021859

Reference 103

Resolution
unresolved
no resolver link, observed 2026-08-16T00:12:18.024798Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:18.024798Z digest=sha256:bb7de9a2fc6eb67326a4bba6e9fb2e2099651398c503f83c93d4c9560d02c7f9

Observation 4719ff45-7662-4caf-b0c4-b6fa93967c51 · outbound

This paper cites 2023, , 679, A89, 10.1051/0004-6361/202346649.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics 2023, , 679, A89, 10.1051/0004-6361/202346649

Reference 104

Resolution
unresolved
no resolver link, observed 2026-08-16T00:12:18.029120Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:18.029120Z digest=sha256:c7e468657624eccc28b8d7b9be983daf519795143af42815820868a0618a0f9d

Observation ca0c1e3a-1430-4cc2-9dc1-a838abb221d1 · outbound

This paper cites 2025, STPSF , 2.1.0, Zenodo, 10.5281/zenodo.15747364.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics 2025, STPSF , 2.1.0, Zenodo, 10.5281/zenodo.15747364

Reference 105

Resolution
unresolved
no resolver link, observed 2026-08-16T00:12:18.033468Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:18.033468Z digest=sha256:7f941089bf273137810fd0d5ab8d6b414d2100fdeb0871dd330641ce8bc1c011

Pith citing papers

No inbound Pith citation observations are available.