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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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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.558653Z digest=sha256:fdef18fa5bf02b6d9ef3482ffc98c9f1c79cf4609ace96f1935ea6cc8775e396

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=sha256:3c017ae66e8b39284d786ac25325c7d8e6177e8f2ec62fc1898e27062a040627

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=sha256:23c8b7db078960a995e0374fcab2d713e793aca1bccc5b583d87cfde5a12c5c1

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=sha256:990336d5d6abe850afce9634690d5d294c8b6621d7971535e54f1da4b4807246

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=sha256:98e69e10d671b5c1ab6d70ab7a59077740d5e2e93548155301047494d98e7cd6

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=sha256:52cbf83038eaef4438384a62b65fbfeb8498ffebb6a6786ebca11a2fc7dde248

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=sha256:098d1030e218c769154a18335298a4bcdbecef33369f9c52c6b140ecd6fc53f3

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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source=arxiv_source observed=2026-08-16T00:12:17.592489Z digest=sha256:c197497235d72880e7c60e1fc2ed8b36fa66096fae62b1c5da82a1b231536c15

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:a14bd41caec8360f0b6209148c665072f08c0da25e94c20fd9bd9523c193b9a5

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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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:ebb20eb2ff9738683d4b71690df91acc6f24cf704980498370e85ffe61c71901

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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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.605933Z digest=sha256:7dabacd16444048fe0e16a48a4d6e078eeb5dc8858ba3e2c15328f11519a6a01

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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unresolved
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=sha256:5f84f8bb0af408440c6b30c1687f190f53aead6cdfc831ba6e642b770b353f42

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=sha256:89d9a3a20d4b117789f92c94b63e315755c9b6fe17ae429f2938ed637c160e0e

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=sha256:51711ac2f7f78e724fc9e11d74b769847e66c72f38e522c67adf7d85565ba40c

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:df87a019df2b73be4b692c86aae7c09bbc2f3cb74256723e7dbcefa141448b99

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:bf270940b9c9180094c78e480edd5cffd2e4275436f84460b186864f6f8e7f1f

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=sha256:3f46cd547e6c770a634efb9f743af5acba999b0663e22eb325e24b3192120e6f

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=sha256:1c39e25904cc84780c9129e2b7dec7105d58abd1660966397cbfe19c79e6f032

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=sha256:812fdfad86c22fa9aa6f49bcdd4f36a45e9b88d8c117ff4f213780e4d4f83fab

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:bac82949594af7cbb564af99192a7acdcd5894a622ed7e9bd5302ac7851d342d

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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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.652787Z digest=sha256:c3ddaadd632ab70bc6a500b2a57096400cf538a8ba6a756e79d6eb7aa1e6a896

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=sha256:9387db399a8a243b0406a66098fd9e66ee8c1cceef1038d813edc6f261e7f4b1

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:b3a5aec6aa818940c1b82b6a97c1b51c842443bc827d3027d42fa4bb68d80135

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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unresolved
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:a83a8ab405df8e95198a6ed581d4a4f440b62e9cad8de4dffb98fb7996e44917

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:dbbaaf6c3e04674c68e8dd1992f0eb98eda2f8ab8d4ae5089b7de6a98bbcb6b6

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=sha256:6343c071616f055297d9aba172edfd4e8db4adb974b6a0bf5a47c9d2b20f77e9

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=sha256:7cda7d1d14a4b4cab3467ddffd70d5ecb559dd480f9ea4b7326372691bddcb05

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:e395a5f979316923bc4f6a56092663e29be156b69e60e5e702047d86826d8ac3

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:da5fd27c1536dd57fd3bd0386a0d112cd5c96869702b024635e252c270879f9a

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:b642fcda86b29150b45ff3db79b83b4329665a5ec536665c08876d8b7c2e7356

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:a90f54e857c99740f0cecd8c9956eb1e6ebf9354d6a54973956e12d14994a7d9

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:ea326d21b8d333155e30966fabbbe5e8da6add954fda846903cc336d78a6f85d

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:cfd2e3e9dfcd612d6394ed5473b25cc773eabe193624b8aa0212b89ba8e22900

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:ca520b2bb36ac41592ee5dcbfe27fc02d7122ad8d9f58b03930c3934ca89620a

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:acc185e95b29ded70d7a2eb1e405ef8d5d84f6ced30662b3d36467ddd97ee088

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=sha256:95c2d2b68531c7eacc17a2c5e2366190a1deca2da297ed4c2812471d52b3b764

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=sha256:0bdab54a5fda6dd07ec1f1b8ac29d25e8594f45dd0e01142bd0d75b5ba4355d2

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=sha256:5aa3346183ba812f6dfd05a4dd2db71ae4a6ca42a7c641de7d603227fcf93eeb

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:e311b3d5a300b1d118dac79f860aa1b2e7d3e80d1e28f6a2063c775c2cc5f656

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:a6bf37c17aab1ea5b200f9418103fad277422dbf4b1314b922947e623ccf0598

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:db85e333f79759a7497a38f988644526d2984f852c5172f084cc62c93a815bf7

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=sha256:8f8b4021b9f1b36a66e8db8107e224c7118c193f0f5590366503bf212cbd9dad

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:d34541206981c8e7c4f854d0a80657a79ddc5d64a7c21b01694521eccce3f811

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:e06263505e19d7763d4bc16fe2c894d170edc8df2dc307e6f50bb8a033e7f0e7

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=sha256:46ab52e210a73c49556f63159dfaa705a99c9d1e9b54bad4909a9cb3cedb5b6c

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=sha256:2747f70905b17de4a8ec5230fd08cc4a7ff8fee3f14799f54a9795ed6d8a8d0b

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=sha256:409fe4b6d978b5cfb9936f88fac052dcea1f9eb102ef5d8ae7537539b6d48f3f

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:f61e728a31d7384315d717538cd29c96bf3b960cfbcf4e80f4412f05b3ce024c

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=sha256:997452a5adbeeecd8063824d9b9cc349f7236edbaff94a8f34bfb7d7c13c622f

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=sha256:1c3289ac477d236505754f4adb75010e0966295a3466ce020b754b53003bd986

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=sha256:20307fc68851bee7f04397faf94702391d5d5a45171e44c14ab01ba0b8584694

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=sha256:8683ff51fce227abeabfec65edd96a8c0a510be9d5d20b9d73faa05ca28bab5f

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=sha256:25a00d821336508e7754027baa3f15afaf271a8d8d298c20948ab7bd9d8da6f6

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=sha256:0f6e31a65adbb479787ac221e9689cf5814a12655cf23df588b6a66eba0fc1d9

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:a240e6f48699862bd968a6e3ee6e12eb0256f59044bc788db4e01c7ca943f02f

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:f44d0e73b40dbd5de2e2627cf0c1a7747a64f5fbadb46366500ceb86d710d5ac

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:a260e42a086389dea6e567a7264e501f0ec855a69c419db328afba332407bfa6

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=sha256:9a4231c4570c63f27a69af8efc2f4e9e2117999ae00f1f96e91949783763ace5

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=sha256:816ec906ca27c31fdf909bcf886e99c28d5c9963c1f7631352d4df6f21df1c7c

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=sha256:418b11ae30029e3f20a4aeefb8b373a279cd447e84bc1e27fa749285b4d2b6f6

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=sha256:2290ff0ad2c6d1f2f809fcbfdd5f79ef5b5b8f4fc088d5dd3ad5ae3d019e2478

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:c533cdf2318fff98a0231dfaf1a07482f1b0d3f7d3adb1099f3e6946a83fc4d5

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:df82ec157f6ea765c5b93af72a858167277e67dcc7021edc494bf36588db38f2

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=sha256:92ace00af7691cadbedc7167dcc68f093c09ca276d6d369b933b57186fbc41b9

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:a98cee300850d2c7e4839742cf5d666a1d22b8dfad2a8b163dbedcaddc2339c8

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=sha256:7ee5090b8e0b6417411b8c3385240af7d810e62fa2e3789485854018a5f92e3d

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=sha256:71325d3da16fb4836b44bf009c12ced4c14e6bfa22acdfe52c92b28516728931

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=sha256:7fb8687043133ed65fbabe14601c0c9efe2d8e540264182ea55f1a577be65555

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=sha256:25230f2945f34974b572ebec248c2429425262186fa79946c7e63e89ffd2711c

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:d96a9272b7feefd3f0c79147e6cff3927797f7ff48170105eb9744a67bda8b66

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=sha256:348cffdf08a09f9bdf8196c0fc08c2b3e035195bffbb368c2de7b9104b8da1a9

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=sha256:3ce396527f669a3315b6d051ec64df36e903d005d4e2d8602ac44024e904f73c

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=sha256:3e3232ae7dfb85deddb64c7897a007993b8ce7c3b1acd2b47aaf69d8e46929fd

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=sha256:3f94fd17612d0c7aa56f877efcc7826d23739e918d1462fdd64cc0d194d02a6b

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:dc92ddfe98dc96d72b84537a5e52055c118cdaef2d9724b286f52f7aeeb67180

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=sha256:199e71f51d9a4291d4d9e1763b6005821818676b296ee3a5746f7d0fbecd226a

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:dfa6bda8657683e17b53fc0b4eaeb8d8a74128636a8a4a2c230211b5235c9225

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:a8e891714a844299da91c5c18d0f7f3724225df059311c1fae1ecf0ed77c8803

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=sha256:376a494687c37e6f0c65e1eb3b81c8bfa6cf5a919bc7157d5a7cd4e52a1a77c8

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=sha256:9005190f68b8e744c882a56d08489ccff8df4774687bff6fa067d456e65f0eb5

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=sha256:3832117b89a9b5e84b3e467b84019e2d9a2e24913aed9741bd7a57e99e2847cc

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:deeccf49231240165c9f335c19977845fbff416907d77f26acb3ca4c4a2bd8b9

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=sha256:490fd58144cee35f5538127ccaee3ab10cb499c9aa17d882ac6979421d795519

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:d8d4837832d7a511ab8db7e7eb4baf59a393428da9055d1dd725ef3ff00b07f4

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=sha256:3f797080502cee268c4efb74e08c7adb621036d2eaf11908affe9e1043dd9c61

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=sha256:6ffdfe7a250f97e3a524fe8a7988890c9ae3b8bf3a2da8b7088d66b8dc7080db

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=sha256:36bdb5ebbe9a13f8b324854ae8a1118fa8887be7206aab5a9b4b91343014e39e

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=sha256:90c732722cefa6e3cce2050a2230ffb2bf8a5380951864505e6e5c76137e41a2

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=sha256:24f8debb21aee3136852ea8a288d08bd164c0389d085820b57cd06410fb5335b

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=sha256:9aa4ee98d03bc95c3fb206f79f7653766f95c88454b3ab068818c7f9de595713

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=sha256:48901e087ea95fb795a7a63073e4fa897c5f7f6f1983fd94b73d0eeffd92fa47

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=sha256:3e7b054c1b00b737962d2212f79bfdc1e246176961ab5b0faec7cfb3a3b56918

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=sha256:6f8e25788894892d9a360fed3092984a0b0139ca0f98f286c1ee98a11e7eeab5

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=sha256:5f81d6b4a6f2bf951c77ed389f7ccae62518f73af39cdb07f67249eb4c3b63ab

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:a17c59280adb36bfa70e3fc314e4d5edb0855b30efb22c68c2ac153f17661f6e

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:b0c44ceb91512fa8826fa05bc21c035e6f586907e249da3b0a88b100649f432a

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=sha256:746e5e0d741df759668bdc2d7ca8e1fcbf1294774d83d5aaab2b294fd357bd31

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=sha256:2a043cdb812c64c1e3133ae713a64f0e0a1259baefafb0075328fa877b3d001d

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:b3f0bb51a9943975ba34c40937d3960107c29631dde06d4402a3d806253d0db5

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:a1c281322363bde0a0afc7fce0856d8c9da43144effcb055a1296749e64f0708

Pith citing papers

No inbound Pith citation observations are available.