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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:f10e91351bcc7d943d884959fce10baa92f0c8e2b2b658be66eb525d7b765dbe

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:b278416ead77b05a5e7994fddc39973b69a7d875c06b1edeb53a7e732504e023

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=sha256:11eb716eabd4856cfde754ea93a8ac6f0e029c329dfe8d16cbed467ad1fff794

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=sha256:32fb333765b1dc468209923d92b0b615bb0861756fa76ec3e7f9c770bfdc3e1d

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

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

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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.577896Z digest=sha256:60a59afeb9048ab764899433974ab049564f1a612bfcbbb9e61af5602bf41cf1

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=sha256:5aa7c9b1983161c35a0978c01f7f25d79026aaccb6642a13f331ff47e337a3ff

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=sha256:738f02d0bebe4df6607e3a8a99af5ffe8a9ffd49c315dc07c3b31518538b876b

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=sha256:8f1ac7ba79185b9d896ae0603e41a6191c6eacbe8eb46d08c7623266b815b2be

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=sha256:7f0fb738ff2698c8b34444ea4b514d63edc7f477fbd9e79c743707d981fe7c29

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=sha256:144550b6bf7d3720a481f23d2cebdbd2bcca38778a0e5e9d00f7fb015cc5f3be

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=sha256:0f2d0731d162b64474e21bb101158329f232d2be4b5733a93afb8377a3eb4434

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

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

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

Reference 12

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

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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.610137Z digest=sha256:4a32a9596d89bda1f06beee4a52fe0f6832ff6b7f65ff045ce04f62c28c936b9

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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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=sha256:53f777cce79d16ec34de953bed9894720cdd48f893a8a00f32b01c0ce2d36d13

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=sha256:74895600686284c998620814fe1d2d3b4b830b395eddba8523c65f8c6e333b51

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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unresolved
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=sha256:63fbe99b338f141fcea44560580631ed80096d85453fad364fe05a6554896346

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:adb7b379ccc9198d94ea8d98a1216fb538ca5473450910dd020a200432968ed2

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

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

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

Reference 17

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

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source=arxiv_source observed=2026-08-16T00:12:17.634526Z digest=sha256:8206eb75adb05fbc065a3b168c081d356a31dd8a1b54ee57cd1b5f7ae4bd3c2f

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

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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:17.639093Z digest=sha256:3f2cdb0c072dc6a811cbaeeb54a17e9495315a8a03b6ef92a414845e319aa73f

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:d1e92f971ac362a72043a59a478d1352f4897b27cbe000fb718037deb6fa5d21

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=sha256:6475e4526d24426be5902f1e474d29c6ca8a8118b34a23e4466a82fc905b27c4

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=sha256:9bfbb9a9acdb71f1b1b505bafb7c19b9a17f57f4bf41560ab52a533d16838802

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=sha256:0838c9531d89e6074ab75dbeb729c2ad2a93801fbaba19ae0ce8e73616d153ca

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

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

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

Reference 23

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

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source=arxiv_source observed=2026-08-16T00:12:17.662921Z digest=sha256:a151d4080d4ae38766d8843c44749a427f2d0545119561f21cf5bfae7b4c3161

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:eb7acd3d14a65a1d46d5bb1d10b8531e5cd70863dfc34bd436ab952cfa120eb7

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=sha256:7cc36d5b3f2626d81d73fef0d404b37a3f05fbb7ea160d1fda4be6f39cbb79dd

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=sha256:752c9f3c8fb4127ec1052207bfaf4f7b3c13091c1686995eeb3e7fe98b4f5d5b

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=sha256:920684c8bfaca27f3e00eadc51e4a75f3ae8f56d9738ba6e47668ec91614f8ff

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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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=sha256:273454469e60d374c6aba33ba854834572d534caf34b5717775bc9e846556095

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:f7c369fe5020d8a3e535e80e5d260c727aa0a76f5dfae8e263d7b61333c127bc

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:f536dce010c3e74c2fb6d2a2012b2acdf38427288722d409dbf76ef3f4296ab7

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=sha256:6db35d3b579c034469725d5ae58a2f52c6f6ae3e69f342eef840f1dbc3315054

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=sha256:149863035dddad509aa722e6bf1eba7a6c5db21c42d8d190b68857ed8f8a736b

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:b6db30e124505642449959da53381d94967378ad624cda430a22e1266d6c63ee

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:f997ee9a1cac742db918920ebdb5441e357e0cb0549f87ecc94d028a4a8e8a24

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=sha256:1a81d9b96e421aa575210bca9ebd029f37f7b2e92df19efb6e3a54a45613db65

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:af1e4e6f8dd345aa151d84ae49ea97bb5523366e05edaa6e61d30414e0b635a3

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:d4e7cf4db7779841dea993d699f80e4dcb8475db430d30f3cd9174a0de5c1c5c

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=sha256:9fedefd41d5f974ec51354fd3d051561f4f138edd8733dfda4800a09127c4635

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=sha256:605602311e17eada70478fef8fab5d4a4ff9c9a26ff1e877fdc839958095febe

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:a28414d44704806acaabae2e34f9bdefe37a06066684d7f07bc90777fcec30af

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=sha256:115aa2c3c7475a0f065445d083dafba4a4489eeeb6e982e16174991b4c7389f5

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=sha256:4ca622202ee5e6a69209cc767d14647d65e15baae154df6dc88def79f2d5f85a

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=sha256:752d3a74bf177a68f1ae716022ae2e7739bb545da3cadb7f1558d177b6ba9f7c

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:c834335ebd5751d02f443034c747d54dacc31b7d05c574329b53b740b2880b27

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=sha256:8715969a7e44e2d48790ec277fee201a54c7896d0e035899838ae0e84356c8a7

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=sha256:8410c5f5c00433736e3c6c6fbf55d1d52306efa265e36b3fff1051b05d5025db

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:eca7d1a8970458149cfbe9556df9a2a844a6c7e798c5fed513bcbcba7b59b61f

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=sha256:8ab7fd843a53bbd237d1b90b19ea86c64e3f1ac451c168d552d520abe264e52d

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=sha256:4947ab7ee19b9fa4ac665290096d0e4d9b72738aee22a49c8fdff9750d9f2869

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=sha256:992c06cc152adb4b79d76367beed65be1751706d198f334abd29d8950c469b44

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=sha256:4973d2523315ada1d288e81554816fa8432f466a96e7bca4f2b73269225d4eaf

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:a8a1324a9b566361bf0360de9a5585fa7869d227e43742cff95dcf2a49af16c7

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=sha256:4ec38b96b775c19ce4d28816ba0d4bff203bdb16cbc729f33341be725a38f404

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=sha256:4e56a73d0ccc013e77b468b576157a0148c083801bd42656f21da1e772f5f9c1

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=sha256:05184255190ec5d40050fe82b6503119cb4ba2407863f2b823062240ed566daf

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:ce190f51f9c137e43063afb9fa9f9b8c4d34010d08070524352da1891a15cc59

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=sha256:2800d0a168cc6cb80e3a456a0b0022b4cee596d8031ba0c13aab45a8bafe280c

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:ff0e605418418515f31ba0998b8cfb5f5240885a045d466fa85ebab9d5aa3626

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:a3b78d68bcc59f4a75a4932aeeee9ba04f00ecfdc91889b486463a5ee25c6ea0

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=sha256:72fdb170f46bee750860b404e640f1437ebadf11c0ac58a49097ed7719aed115

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=sha256:1e22e218bcafa090988116ecfc0233e81156d4a1df86a3a4416e2d647d82bf32

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=sha256:3262fcc295a7eab37eca6de1e02b04e6f008c9c0a197c6764dbe5862e1b8920f

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=sha256:5a8c90be2d6350c170dafffb5d0f80e72540daf646233d100389402ddc10ad17

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:ec0b277be77e3ea152c7c4528c32ba6e2f376a56ed80dd7db595017f5a01a44b

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:f615bacec3b52c775ad55a260b66956d72e63a9920efb60fc1ccc71b470520f8

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=sha256:28638d6e4cf6464a023b2a3dc5cc4283ce84b5ed0bf937c8f7ff652f6f632307

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=sha256:6f38c7d13ddd8a27c99d52987b3305bf12c4e12d3f2b1c5ed527a5278a092bf0

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=sha256:0f2ad6df327e66497c7bcfd3f68a9f5f16a4378cdd3e699ecef82cafa32d376b

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:f1c31d5e5cdd7ebf85bae929f5dc73df101ee9167a837a89c7dcefbbfc1091c0

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=sha256:51e78a56353ccb425e5af7b212bcb6e99f5a477e3f8b0fdb18defa0df6f1579b

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=sha256:959ba86c8c0ba07aff6b9743d904d30bdea4a6eca93187672c7a2c8f1826127d

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=sha256:8248bfb93540718d98892265b9f249d669a934d018d7ec2ff9674443289971d1

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=sha256:8325eef84fc2a750b7808b38e4907fd0082d406665001fc952d7d5689662ead8

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=sha256:451036a91e8bf73cad641e4888ee62ef2728f9423513dfbe2455b7ecb5479759

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=sha256:98dcaff3b3e06a155885da35c9ac1f104bb22aec5714f69ef6cabcebf9f02aa3

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:d3bdb9ce3fd29f5ed44eef938b921df5fd79e9c4c02a64c9087166c76e39458f

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=sha256:3546c26f5734b3601351d8421d6c1baffffa08f7e471a8739420dc9373fc4e8b

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:acd9fee94be16be8ab58b0c5e56ac87c657e48b37e89bc1f857b883ea165c449

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=sha256:8d0b5a977910290b59a3ee633420cf8241fa25f9611624b8c402d12f735b28e0

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:d3583a9b9a9a8ae4118e82a6ed9784fab224c6c9ef91bb7d081e606df541ef90

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=sha256:1af019c82bcf31545bbf5a4610bce2b9e73835e966427504b70f99389607a1e1

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=sha256:8b57dd6e829a2dc520f52ca928e45d26ebb028fc0533bb625286ef4bc5ea933f

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=sha256:3d5690dc918af2e582144eaf140e0154cba5abffab400e2d0c3927d41647911b

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:e40425fa388f791fcea4abffe73c00e21c05fc7e6ae91a7f8f9c085c784bd1c0

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=sha256:5d3fed6989948c97746bed2ceb77c2ff6c983a4e9f95b91a8def57e3ef99d59f

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=sha256:6549ea69d851ef37e8e4562dec288255cdacf49602efdf08713d238d747aa2b5

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:df33fe39afb5429af6a62bed8316667d51acbcb94e5ce437a6159cc0020cb0a4

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:d294b9e097fbb158eaea41ee8f73df84d77c024d9f0d0c94726e990d04a65271

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=sha256:90695d26e57e3691bd4c5b80b5fd7419161fa08286f85f723b04b5e6277cf0dd

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:a08a819007cc9d790a64043d20656311fbbf2bc59538234b68c18e73d0ebbf82

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=sha256:4b425ae2deb683fe2afe37b9763956643764ab4c4ef64b246fa35125baa60c60

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=sha256:7788e9179d621ee5ba84cc9477e86bd2e974302af0804b0f8a876f0c1dc50d66

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=sha256:64471b67268b580cb723d5d395100de428995cc4f2234aafd341d94bd3ffa38d

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:e26b4f4c0b5f6575cb02d26204614240c160e731d2d85889427d459e9b722876

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=sha256:1c8bd71208816141134b447d6ffc4658d7a1ab5fffa2ed33c7f6fb57d5cbed0a

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=sha256:3c55f7b487f92902a507f155a0d1e8835c45c1c1b81903eff9c62499ce920414

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:f6ceb8754e58501e38e8af57a952fac1c455947f1e401c80a1f9ecd0d7d5d46a

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=sha256:61b4897803b89beb268555ab1bfec23a5388e2321579b0566d8f283b6f3b7353

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:a0741b9490719c79ea13b653ae3cd8f7a203ae9b9ea3e3a317bad320017e3b5f

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:c68418a1985b0a586c61c8eff5de85787aa390948eb0ec7d74b416e4ddc0cdf9

Pith citing papers

No inbound Pith citation observations are available.