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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

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  • 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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source=arxiv_source observed=2026-08-16T00:12:17.558653Z digest=sha256:e8b6348b649f8fd600cfd16c187705cca816bac209da1aa05d2eb0b600f73d2d

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:ca292e7d33fcca00db0f11e0105a9a5442260b87b17ceec330f9acd22513e069

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:fa0f34c2e0fa1ca691e9a78c7b128ff5d270773670a969cb4ce0fd4440f05ed3

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=sha256:85ffb9102a2ad2ba122daca8a8f9d635e930a64c0b7a4f051499348de8a4fe10

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=sha256:1df0902deb4d675c22fafc164e7dbd9d443c82684a3c3632c06fc448327fbc34

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:b27fc0b9cdd11c3b64df32d0e63350a8ed5a667c543cd29a76a4d91fcb9611c7

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:c74e8228103694f825b55003b26c88143847918b58342468da0c750d6738c4d2

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

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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.592489Z digest=sha256:24913aa20cb196a048f0c133d3f3b9c617a5b56cd5a64558a6b6390e14d00d9f

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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unresolved
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=sha256:7dde3ccd1529b64a1458c6ca91edaa7ab72d623c3690860c6d122e53f4ac2b98

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

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unresolved
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=sha256:76f191beee47edeed124297891ae17f45c6c1a81d883cb1c5305a1cace43e285

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=sha256:0132e9fbf5a803acb5a626e20c961c614de5919bd8002188b31a17db600ce299

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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source=arxiv_source observed=2026-08-16T00:12:17.610137Z digest=sha256:f06e2524939127be3ce78241de18166dbe87f36974560121eebee1ac81668cac

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:bd6f42df70c56ee6e91f22b85f010991caff3b3da2cab631e4fe8f0b389effc8

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:bfea0c4dfd8dc74340ef9964b924a71e9099de86c0bb5568a9e80a4a334cc0ef

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:e8e4d84fc2baf976f1f2516145f0f2ee7fea3d58799ac465f525645e2a19302b

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=sha256:047c55152c2fed93f80d50dab5fed80a7dcc7f84b8411f9ea92470a0de8196aa

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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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=sha256:11438428feb35257dbff2bdd9a932669f70c0b3acc7688c33e606fc56b779fad

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=sha256:8166496e13243494eedfed2567722a412ac7f03b7f80afdb2e902c12ca294589

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:cfad2a95f37909d8c7b682e48ef818c96b690b5b58e81f89d5538ce8303c7487

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=sha256:154f4fb4b9e3d8d0f7db6194abddb4cf7dea56776b7142a78b0bbe37491fd769

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=sha256:1dc014b263eb19f7e02e9abc6c5b76cdd9474fb04be11ecded4d26d2ba249c28

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:c04e33c498fb0f0c5a5b4dbe6e05dcde2af7e2a1790a1af3b03caea1a0774b7f

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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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:a63d65d8808f1b9c009b061cacf55cebc21b642b01cfd9c5a2cefb06b98bd7dc

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:c97924a0b37de0ad565740db48a9b603e02fba5c35060f6a25e8bde22c6a1b89

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=sha256:27a893ac4da81399677af512b725c013c7251eeaf2152208f3bc72fcbe594987

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=sha256:6f93b046af647e7af29556801e44cd4e174cded4257e78fe96cb3aa6a77fa25e

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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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=sha256:6c6c90a749171f9ce9ef9c9308c2ba7993c6bb0c57957712956910e0bb8da0d8

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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source=arxiv_source observed=2026-08-16T00:12:17.686341Z digest=sha256:f86cf954e289cf187bf71a40ef146c8aab61ddae48d21c9be7c20f8c47ee5024

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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source=arxiv_source observed=2026-08-16T00:12:17.690539Z digest=sha256:4146cd4fe22a938d98bf7248f2f06afc0f1f172edce4320259995808f55a02d9

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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source=arxiv_source observed=2026-08-16T00:12:17.694985Z digest=sha256:395f0e81f5f379eb49b3ab32dc8f8d6e6899f64dbac9807e29138a1233c0bff2

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:edf0da9404b9095e57a63e5d4ba88e1407566b494a7adfcd7ab6751f162ef63c

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=sha256:025954e7110332739ee1518d891d5fd4941c0d272e76196c23a8320958f49a19

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:eb8432f4d4f4731fb2cac1095d82a1025e259ff8bbbf5f2ce1e7ba7075540805

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:ee5616e167af367ba5824daec1e9c1691afb3fe8019ad561f93322168a00b522

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:c8fea145bbbf7b2e46a5ee8da664dfa5c4592b07d278f6cf6b31e8041d997d84

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=sha256:43e85c301ef0a758074d90476858f2bf127077c409a9e6c51c8145b3765f755c

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=sha256:3ad2c25c925bd42bc48bb04ca89f2bf7c8b75673be1d949185909dc8d63917d5

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=sha256:1d06514a64fc68afc0aa6a4a8b6c7fef4ddb9d34920b2c6b20454bfbef8fe711

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=sha256:785d5927ab0b2fd72d60942aa8cbbea20121825d5fbdc5af2f06b0ee76289e3a

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:d95a2a676943f37f9af5b4da57fd934462644ba480ce148853604ee7b05b22ee

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=sha256:11b005580325122fded7c92c2f56f8452249fdb34cee8174f969efe16b00eebc

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=sha256:9d6b69916c607e4767db1c9d0334da3a0e1ce23ef1b458b96b75f207cb09a071

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=sha256:10fa65127831af2e5761af11110d8c1448d9c8e029dccdef46d774d74f3fe81f

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=sha256:75cce19a702372ed3e92fb30d43894ab749685068aee7597b861e24bd7c64d7c

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=sha256:9d19e96ca018afda505a2d0cbabf771f64a775c2d3f51573db538ded7f53c4c0

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=sha256:21de37b37dd8d3599a95c40b4c1065fc4444062ab0e253945733303201b4595f

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=sha256:394f49a0f99fed1e2170d5c79d693e842f929a5a180ca9319d16f6ab3419df64

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=sha256:68b013fe42aa7f1166583bfbfb663dbfbdec29b58b628f6250f414bdf81014dc

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:a65deacec35b099e3bfaa62f1d2eb810add7b38c9732764404dec5662e7b0c05

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=sha256:444df4826f3b6c9bf07d3dbe364081a7ae946c7d5adbc6989974a7e9993e2a00

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:cbde0a41314a313bab52299ec0eac08e02d87b58a71537e70dbf792c51a428d4

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=sha256:7da7a33e15cc97ba9ac59713b6b74717e869b0fc774c8c3e3a62874839f81288

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:d0028dd520f9b2845dc12a750fd2fe72427bf7eed7094d2ccc59a9fdf7058e02

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=sha256:3c874a3423a72d33a2f8af6e96668306d3898ac2a6984cea35020a0896323cde

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:edb8da8a7e5708ab90131b1e29196b3e159a915763a0172b8b33f9c5a0b62d7c

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=sha256:5b3f4e486fd99ba3fd73606f94d739aec0d66983a30d5c8a877b24a12c40f21f

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=sha256:4c3abbf80288af8cd9eb79f1c5f7e9e599e3aa72ab99477c5ec1bccd76ce7fd9

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=sha256:4ac9c16c4f542d73b6be259489f284fbeadd59322031308ea8120c20fc46a569

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=sha256:8d7acadd1b8fcb0162b885d8797bc9e2ee07518ad5f6f9e8aa99a7f17c2ae921

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:dc2e0ad2b7ce542c920e4739252a77d0da0000c73b5c4abab865382346bfefc0

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:ae5a9d02a2aa2674e6399f30182d4d171a8d9a5a8b9f4d963a8aa8b727b05481

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=sha256:710fba44ea2595fb2df78ee727d0c169d1e3fc031e9116ae8cddffbe090a6630

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:d7cb84ad93d9e448b56c1c3bc0221e64ec7870731aecc291fe322197138f436f

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=sha256:85fcdc59f6d9374386784b8f607abb14342c9ad3377d6079528045bf42aea212

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=sha256:770d187651dfc49e256ee5cea6693bbdba306f8b33793d841e5510d29d98c0f0

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=sha256:7355da92d9a779cfeb4e386a115866dfa6e2adf529c1e6e99b7b34e099284a49

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=sha256:3eedbe15861d4ddc5049fadfa377fccd664e7fd4a6f2b2f00ae6281e35303e38

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=sha256:96c6752b8fb13e816e3b0e95decd35c4c2382cc4312e5b7371cd95f8290fceb5

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=sha256:7e3f54086bd397dfbd05ec29bcde6eae48646cea82cd7517a365c8519fda8bf9

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=sha256:1b0084861ab6cdf21ddc7541f88fd70a6ca45d733d999d99dee407b9500cb8fa

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=sha256:3db6dfca3911dc45c23c1f3c969e072600c97d17600f7ced5cbc239ab207ff19

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=sha256:09ac90c61b02cd84908ae8b1ac8e517a33c735df5667e4089ae5faadaf5cde22

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=sha256:603f3888a0a38374487988d979e60a8fce680b6f070d00d75b093a302885a438

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=sha256:532bd998db97632ff04d6b453aeeda47cbe8782e4e9ab30a061d81725351be7c

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=sha256:1f523b90e1b9b83da55610ccaa1dc6b26f7a86675b797a78c724b02d0a83a5ce

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=sha256:97db00ed987a9f82c0c0bceaa15c00ca7444473bee15e4d455d592d527cbb0d9

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=sha256:19e155beaf9a326a079e880a3a77c82883d6aba8dd7a045979ded8a8be95aae5

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=sha256:151b566e06ca1e16eda983dddc6642f7174c63b7d445ba9150303311fe2be92c

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:f25474ab54a308c5d50c3a313471fd22b15cfed1a5c91d533399cf939710944e

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=sha256:32cf7239cead20359cc95778d9c62fa65467dee62b4f8688b90c29fbd47e2071

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=sha256:8eb2a46dafc6625e1a6ea7cf1628bba6898d0a6d4473ec30d2c6a4573012f34b

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=sha256:7bfec1f05538b040d9895993819c1fc80bbcb3d3371a8f8be12ae7ea7245fdea

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:c33975309306652628bf0e166ff0f3b72bbf5da7f3c06b5b9c434d2d67bfb686

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=sha256:8bc0e94f5ea1769c3d2e6c2b97dcfca5c948451d9fd1d188a2577c60719d9836

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=sha256:0a48162c685d95cf320094a7517f866216b3733bfa0e6a27cad742e212085d41

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:c4ec6fd3c31f35446935764dc27f1beafb01cbd82f1269ebfb20383c68a27405

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=sha256:659f6890d9b8bc8ecb18cf4c4938a634f3f5b0a104f742a20476df755e2852cc

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:f1f68cf7052c2f9ca7e02fae3f64a36cc4e906d101bff5142a348b52252c0a93

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:d939e603dd8be8b9e752cb6130f440a1209e8ba85a4811bc9ddb36218481a7d8

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:f8d2c517790298d48f52d425561ae02b278009bccb9bb4880c7dd5c533c944cb

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=sha256:8c6ecdfe2a75e18160d2af9d6b5efc2ecc6e0c03fb79ed733bb5292f112a9fe5

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=sha256:7fab454a6f70168f0b1d4f42a0fa963e7c9d787ec4f191b519b2463bc53b3a17

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=sha256:07c361d4f972b7344afcbff4376a20a93e6fa82cf90c137296b2b61d04c1bffd

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=sha256:2d6c2cdb45a49a9d40624e97a6eceda68e7c156578dd80ad3773a10ea829745e

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=sha256:78bfb1c95649527b04147dff0828d3b984650a2fc43f14e9038c1bce2c6488f3

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=sha256:3fd0fec38507ca60acd2d2f7c9de8d59e0f46b66290ab754696e816376432a89

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=sha256:5800253c9818a4c0a70902b801039447c9cea397d2ee90dbb4f8b121ae11e5b8

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:cc80948450dd4c26b529450da281f8ad25f7bad9b0594132bc29ed4adb97e340

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:dfa201a52e0131b13fdd83252677908a0a31539979d5f8bfaba6c980da686339

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=sha256:495d7e2b04a508d5829001015994d2be19590224bbeac07d35e45d474a440fd4

Pith citing papers

No inbound Pith citation observations are available.