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ChemZz I: Comparing Oxygen and Iron Abundance Patterns in the Milky Way, the Local Group and Cosmic Noon

As of 14 August 2026, this Paper Citation Record lists 100 of 176 outbound references and 0 inbound Pith citation observations for arXiv:2507.14094.

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pith.paper-citation-record.v1
2507.14094 v2

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ChemZz I: Comparing Oxygen and Iron Abundance Patterns in the Milky Way, the Local Group and Cosmic Noon Unresolved cited work

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This paper cites 2020, ApJS, 249, 3, doi:10.3847/1538-4365/ab929e Alencastro Puls, A., Casagrande, L., Monty, S., et al.

ChemZz I: Comparing Oxygen and Iron Abundance Patterns in the Milky Way, the Local Group and Cosmic Noon 2020, ApJS, 249, 3, doi:10.3847/1538-4365/ab929e Alencastro Puls, A., Casagrande, L., Monty, S., et al

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This paper cites M., Nissen, P.

ChemZz I: Comparing Oxygen and Iron Abundance Patterns in the Milky Way, the Local Group and Cosmic Noon M., Nissen, P

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This paper cites M., Lind, K., Osorio, Y., et al.

ChemZz I: Comparing Oxygen and Iron Abundance Patterns in the Milky Way, the Local Group and Cosmic Noon M., Lind, K., Osorio, Y., et al

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This paper cites 2023, ApJS, 267, 8, doi:10.3847/ 1538-4365/acd53e Andrews,B.H.,Weinberg,D.H.,Schönrich,R.,&Johnson,J.A.2017,ApJ, 835, 224, doi:10.3847/1538-4357/835/2/224.

ChemZz I: Comparing Oxygen and Iron Abundance Patterns in the Milky Way, the Local Group and Cosmic Noon 2023, ApJS, 267, 8, doi:10.3847/ 1538-4365/acd53e Andrews,B.H.,Weinberg,D.H.,Schönrich,R.,&Johnson,J.A.2017,ApJ, 835, 224, doi:10.3847/1538-4357/835/2/224

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ChemZz I: Comparing Oxygen and Iron Abundance Patterns in the Milky Way, the Local Group and Cosmic Noon Unresolved cited work

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This paper cites 2022, A&A, 666, A109, doi:10.1051/0004-6361/202244258 Asplund,M.,Amarsi,A.M.,&Grevesse,N.2021,A&A,653,A141,doi:10.

ChemZz I: Comparing Oxygen and Iron Abundance Patterns in the Milky Way, the Local Group and Cosmic Noon 2022, A&A, 666, A109, doi:10.1051/0004-6361/202244258 Asplund,M.,Amarsi,A.M.,&Grevesse,N.2021,A&A,653,A141,doi:10

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This paper cites A., Phillips, M.

ChemZz I: Comparing Oxygen and Iron Abundance Patterns in the Milky Way, the Local Group and Cosmic Noon A., Phillips, M

Reference 8

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This paper cites J., Cullen, F., et al.

ChemZz I: Comparing Oxygen and Iron Abundance Patterns in the Milky Way, the Local Group and Cosmic Noon J., Cullen, F., et al

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This paper cites 2022, MNRAS, 514, 689, doi:10.1093/ mnras/stac1267 —.

ChemZz I: Comparing Oxygen and Iron Abundance Patterns in the Milky Way, the Local Group and Cosmic Noon 2022, MNRAS, 514, 689, doi:10.1093/ mnras/stac1267 —

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This paper cites L., Fattahi, A., et al.

ChemZz I: Comparing Oxygen and Iron Abundance Patterns in the Milky Way, the Local Group and Cosmic Noon L., Fattahi, A., et al

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This paper cites 2003, A&A, 410, 527, doi:10.

ChemZz I: Comparing Oxygen and Iron Abundance Patterns in the Milky Way, the Local Group and Cosmic Noon 2003, A&A, 410, 527, doi:10

Reference 12

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This paper cites 2017, A&A, 605, A89, doi:10.

ChemZz I: Comparing Oxygen and Iron Abundance Patterns in the Milky Way, the Local Group and Cosmic Noon 2017, A&A, 605, A89, doi:10

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This paper cites The Orbits and Total Mass of the Magellanic Clouds.

ChemZz I: Comparing Oxygen and Iron Abundance Patterns in the Milky Way, the Local Group and Cosmic Noon The Orbits and Total Mass of the Magellanic Clouds

Reference 14

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This paper cites 2021, A&A, 647, A130, doi:10.1051/0004-6361/202038366.

ChemZz I: Comparing Oxygen and Iron Abundance Patterns in the Milky Way, the Local Group and Cosmic Noon 2021, A&A, 647, A130, doi:10.1051/0004-6361/202038366

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This paper cites 2023, MNRAS, 522, 6010, doi:10.1093/mnras/stad1378.

ChemZz I: Comparing Oxygen and Iron Abundance Patterns in the Milky Way, the Local Group and Cosmic Noon 2023, MNRAS, 522, 6010, doi:10.1093/mnras/stad1378

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This paper cites Mass-dependent chemical enrichment sequences of SDSS star-forming galaxies out to z~0.3 revealed by direct O & Ar abundances.

ChemZz I: Comparing Oxygen and Iron Abundance Patterns in the Milky Way, the Local Group and Cosmic Noon Mass-dependent chemical enrichment sequences of SDSS star-forming galaxies out to z~0.3 revealed by direct O & Ar abundances

Reference 17

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This paper cites 2016, ARA&A, 54, 529, doi:10.1146/ annurev-astro-081915-023441.

ChemZz I: Comparing Oxygen and Iron Abundance Patterns in the Milky Way, the Local Group and Cosmic Noon 2016, ARA&A, 54, 529, doi:10.1146/ annurev-astro-081915-023441

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This paper cites 2020, MNRAS, 491, 3672, doi:10.1093/mnras/stz3126.

ChemZz I: Comparing Oxygen and Iron Abundance Patterns in the Milky Way, the Local Group and Cosmic Noon 2020, MNRAS, 491, 3672, doi:10.1093/mnras/stz3126

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ChemZz I: Comparing Oxygen and Iron Abundance Patterns in the Milky Way, the Local Group and Cosmic Noon A., et al

Reference 20

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This paper cites 2015, ApJS, 216, 29, doi:10.1088/0067-0049/216/2/29.

ChemZz I: Comparing Oxygen and Iron Abundance Patterns in the Milky Way, the Local Group and Cosmic Noon 2015, ApJS, 216, 29, doi:10.1088/0067-0049/216/2/29

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ChemZz I: Comparing Oxygen and Iron Abundance Patterns in the Milky Way, the Local Group and Cosmic Noon J., Owers, M

Reference 22

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ChemZz I: Comparing Oxygen and Iron Abundance Patterns in the Milky Way, the Local Group and Cosmic Noon The GALAH Survey: Data Release 4

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ChemZz I: Comparing Oxygen and Iron Abundance Patterns in the Milky Way, the Local Group and Cosmic Noon A., Law, D

Reference 24

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ChemZz I: Comparing Oxygen and Iron Abundance Patterns in the Milky Way, the Local Group and Cosmic Noon J., Saxena, A., Cameron, A

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ChemZz I: Comparing Oxygen and Iron Abundance Patterns in the Milky Way, the Local Group and Cosmic Noon M., Burbidge, G

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ChemZz I: Comparing Oxygen and Iron Abundance Patterns in the Milky Way, the Local Group and Cosmic Noon W., Latham, D

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This paper cites The eventful life of a luminous galaxy at z = 14: metal enrichment, feedback, and low gas fraction?.

ChemZz I: Comparing Oxygen and Iron Abundance Patterns in the Milky Way, the Local Group and Cosmic Noon The eventful life of a luminous galaxy at z = 14: metal enrichment, feedback, and low gas fraction?

Reference 28

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ChemZz I: Comparing Oxygen and Iron Abundance Patterns in the Milky Way, the Local Group and Cosmic Noon C., Lee, Y

Reference 29

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ChemZz I: Comparing Oxygen and Iron Abundance Patterns in the Milky Way, the Local Group and Cosmic Noon 2009, A&A, 505, 139, doi:10.1051/0004-6361/200912097

Reference 30

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ChemZz I: Comparing Oxygen and Iron Abundance Patterns in the Milky Way, the Local Group and Cosmic Noon G., et al

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

ChemZz I: Comparing Oxygen and Iron Abundance Patterns in the Milky Way, the Local Group and Cosmic Noon 2024, ApJ, 972, 143, doi:10.3847/1538-4357/ad5f88

Reference 32

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This paper cites A comparative high-resolution spectroscopic analysis of in situ and accreted globular clusters.

ChemZz I: Comparing Oxygen and Iron Abundance Patterns in the Milky Way, the Local Group and Cosmic Noon A comparative high-resolution spectroscopic analysis of in situ and accreted globular clusters

Reference 33

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ChemZz I: Comparing Oxygen and Iron Abundance Patterns in the Milky Way, the Local Group and Cosmic Noon 2003, PASP, 115, 763, doi:10.1086/376392

Reference 34

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Observation 933f592a-9d35-4793-b9fd-db1d0b138a24 · outbound

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ChemZz I: Comparing Oxygen and Iron Abundance Patterns in the Milky Way, the Local Group and Cosmic Noon 2023, A&A, 673, L7, doi:10.1051/0004-6361/202346410

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Observation 3ec6fb60-b74f-4a67-b70d-7886d2fe1b3f · outbound

This paper cites B., Rudie, G.

ChemZz I: Comparing Oxygen and Iron Abundance Patterns in the Milky Way, the Local Group and Cosmic Noon B., Rudie, G

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Observation 68afe1df-41d0-4b9b-80eb-ad6317a04f0f · outbound

This paper cites The Extreme Low-mass End of the Mass-Metallicity Relation at $z\sim7$.

ChemZz I: Comparing Oxygen and Iron Abundance Patterns in the Milky Way, the Local Group and Cosmic Noon The Extreme Low-mass End of the Mass-Metallicity Relation at $z\sim7$

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Observation e4f76e66-039c-4682-899d-17962c5e7cdb · outbound

This paper cites 2024, Publ.

ChemZz I: Comparing Oxygen and Iron Abundance Patterns in the Milky Way, the Local Group and Cosmic Noon 2024, Publ

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Observation ccc237f8-88eb-4410-80e0-839dd12ade92 · outbound

This paper cites 2023, Nature Astronomy, 7, 771, doi:10.1038/s41550-023-01953-7.

ChemZz I: Comparing Oxygen and Iron Abundance Patterns in the Milky Way, the Local Group and Cosmic Noon 2023, Nature Astronomy, 7, 771, doi:10.1038/s41550-023-01953-7

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Observation 396214c0-67ff-4371-8a22-d26485eb7b7e · outbound

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ChemZz I: Comparing Oxygen and Iron Abundance Patterns in the Milky Way, the Local Group and Cosmic Noon R., Bayliss, M., et al

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Observation 94438347-ca63-4bb6-b870-588ea7219c8d · outbound

This paper cites 2012, Research in Astronomy and Astrophysics, 12, 1197, doi:10.1088/1674-4527/12/9/003.

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Observation beb5a6c9-f353-4db5-ab23-af1e0bfec49c · outbound

This paper cites J., Dunlop, J.

ChemZz I: Comparing Oxygen and Iron Abundance Patterns in the Milky Way, the Local Group and Cosmic Noon J., Dunlop, J

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Observation 8a81f13a-d2a2-4d0a-b4c6-92f2810888a1 · outbound

This paper cites E., McLure, R.

ChemZz I: Comparing Oxygen and Iron Abundance Patterns in the Milky Way, the Local Group and Cosmic Noon E., McLure, R

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Observation e9e088b4-3791-4896-b02f-95e451101001 · outbound

This paper cites C., Abrams, D.

ChemZz I: Comparing Oxygen and Iron Abundance Patterns in the Milky Way, the Local Group and Cosmic Noon C., Abrams, D

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source=pdf_text observed=2026-08-06T16:16:46.062773Z digest=sha256:29aa41f715eac547927c1a98817d9c06a82ccaa52136cc758f9a7ecc41d214fe

Observation 059943f0-d6ca-47ab-a948-ebb14bb27f6e · outbound

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ChemZz I: Comparing Oxygen and Iron Abundance Patterns in the Milky Way, the Local Group and Cosmic Noon Blind source separation of the stellar halo

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source=pdf_text observed=2026-08-06T16:16:46.065752Z digest=sha256:ac49cd6a4df6af7f00a7845fe99ff93a5d236428d0f7dfafcf3f15bc83ae3f8f

Observation 5dba52cf-71cd-4127-8bd6-0fcfdc8524db · outbound

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ChemZz I: Comparing Oxygen and Iron Abundance Patterns in the Milky Way, the Local Group and Cosmic Noon 2010, A&A, 510, A26, doi:10.1051/0004-6361/200913337 Dey,A.,Najita,J.R.,Koposov,S.E.,etal.2023,ApJ,944,1,doi:10.3847/ 1538-4357/aca5f8

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source=pdf_text observed=2026-08-06T16:16:46.069149Z digest=sha256:ab20accd84bb638cc06ea8fa5a51aa50d6384f1aa8c736a2ea99607b92ad0c8a

Observation 913a54b0-117e-40e8-91f9-93dcd963bf8e · outbound

This paper cites E., Guhathakurta, P., Seth, A.

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source=pdf_text observed=2026-08-06T16:16:46.072461Z digest=sha256:448fd2b497f3bdd0550f7361f9d9d1d8486a2b7aa6a004154a23913ed7f2428e

Observation 81e13480-614b-4a1d-bba2-4cf6cee38110 · outbound

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Observation 7122a5f7-4ba1-4507-8bc3-d3a6ac6f87ed · outbound

This paper cites J., & Stanway, E.

ChemZz I: Comparing Oxygen and Iron Abundance Patterns in the Milky Way, the Local Group and Cosmic Noon J., & Stanway, E

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Observation 3555e655-f3e6-48b9-988b-186547c35c55 · outbound

This paper cites The 2013 Release of Cloudy.

ChemZz I: Comparing Oxygen and Iron Abundance Patterns in the Milky Way, the Local Group and Cosmic Noon The 2013 Release of Cloudy

Reference 50

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source=pdf_text observed=2026-08-06T16:16:46.081795Z digest=sha256:023debaf29876af38e17b30a65df01e8f34fc481ccc0275918332ce2cd73e369

Observation 56b38a93-edb0-4579-9422-7836a27a4fd9 · outbound

This paper cites K., Feltzing, S., Sahlholdt, C.

ChemZz I: Comparing Oxygen and Iron Abundance Patterns in the Milky Way, the Local Group and Cosmic Noon K., Feltzing, S., Sahlholdt, C

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Observation 2a868eaa-fc12-41a9-9918-8516db703d52 · outbound

This paper cites T., Lagos, C.

ChemZz I: Comparing Oxygen and Iron Abundance Patterns in the Milky Way, the Local Group and Cosmic Noon T., Lagos, C

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Observation 4302506d-8bc2-468e-afc1-770d8e4abbf8 · outbound

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ChemZz I: Comparing Oxygen and Iron Abundance Patterns in the Milky Way, the Local Group and Cosmic Noon 2019, MN- RAS, 489, 5030, doi:10.1093/mnras/stz2493 Freeman,K.,&Bland-Hawthorn,J.2002,ARA&A,40,487,doi:10.1146/ annurev.astro.40.060401.093840

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Observation 2caec17c-342b-4ced-a5b1-cf27d01c6e9b · outbound

This paper cites 1998, A&A, 338, 161 Gaia Collaboration, Brown, A.

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Observation 9feafda8-800f-43db-b812-26f26099813d · outbound

This paper cites an unresolved cited work.

ChemZz I: Comparing Oxygen and Iron Abundance Patterns in the Milky Way, the Local Group and Cosmic Noon Unresolved cited work

Reference 55

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Observation b6cf8008-b6a7-46bd-807e-9b3c9295f7de · outbound

This paper cites an unresolved cited work.

ChemZz I: Comparing Oxygen and Iron Abundance Patterns in the Milky Way, the Local Group and Cosmic Noon Unresolved cited work

Reference 56

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Observation 071bfc5b-4dbe-4f5c-a933-c80a401e13fd · outbound

This paper cites 2012, The Messenger, 147, 25.

ChemZz I: Comparing Oxygen and Iron Abundance Patterns in the Milky Way, the Local Group and Cosmic Noon 2012, The Messenger, 147, 25

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Observation 6df12f08-194c-421a-ab6f-7afc7395a627 · outbound

This paper cites an unresolved cited work.

ChemZz I: Comparing Oxygen and Iron Abundance Patterns in the Milky Way, the Local Group and Cosmic Noon Unresolved cited work

Reference 58

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source=pdf_text observed=2026-08-06T16:16:46.107895Z digest=sha256:d5e3428421ac54e35673e0a722be97d85109c882cda02e8ea91d2a1d94202393

Observation eb35892a-60fc-4d3a-a24a-bb6ea15560b0 · outbound

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source=pdf_text observed=2026-08-06T16:16:46.110853Z digest=sha256:fa9e41be66fa1c5af2c45c06872c110bd678406ccf4ada6c4d8f0a41fc6a8edb

Observation ad714ef3-11a9-49c2-b9aa-c5f9566b7da3 · outbound

This paper cites G., Carretta, E., Claudi, R., Lucatello, S., & Barbieri, M.

ChemZz I: Comparing Oxygen and Iron Abundance Patterns in the Milky Way, the Local Group and Cosmic Noon G., Carretta, E., Claudi, R., Lucatello, S., & Barbieri, M

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Observation d42ab04a-4c5d-460b-b3e0-021782758e5e · outbound

This paper cites an unresolved cited work.

ChemZz I: Comparing Oxygen and Iron Abundance Patterns in the Milky Way, the Local Group and Cosmic Noon Unresolved cited work

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Observation db313c55-7a3a-4462-92c4-f77757ba6d37 · outbound

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ChemZz I: Comparing Oxygen and Iron Abundance Patterns in the Milky Way, the Local Group and Cosmic Noon 2008, A&A, 486, 951, doi:10.1051/0004-6361:200809724

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Observation 93fe2d7d-385f-4bf7-8209-da39490c8aa6 · outbound

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source=pdf_text observed=2026-08-06T16:16:46.124729Z digest=sha256:7e253540d5770afd3a056a2dee89a2f16aae0502fa627793549733aaf9ff480c

Observation c9c6c2f5-12e7-4daa-ae81-185b46610507 · outbound

This paper cites B., Wang, J.

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source=pdf_text observed=2026-08-06T16:16:46.127884Z digest=sha256:414b792660ac95d562ad03c3cb540f27790a024b17158e9961ba4c715d3f7220

Observation f7bac9a5-b2ee-4cbb-91da-594d60faa57a · outbound

This paper cites R., Millman, K.

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source=pdf_text observed=2026-08-06T16:16:46.131266Z digest=sha256:9c6df9ecbf0287da33796a8fa9184469692f856ab984268b2cb953720db24c08

Observation 4dfa3ee9-cc8b-4f86-b25b-e1783c345d70 · outbound

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source=pdf_text observed=2026-08-06T16:16:46.134563Z digest=sha256:4a43e16f43480ffa23ff2862d5ba046e7b2170ca7856b217ce897d24a3a79f95

Observation d5311691-f5c0-4fd8-87e9-4fb0cf549ef2 · outbound

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source=pdf_text observed=2026-08-06T16:16:46.137998Z digest=sha256:75e91c8727527fb755178f4b2a1b9658dd73192c551ea24f422073a9848c2111

Observation b98ac6de-cc06-47b0-926c-2018611844b7 · outbound

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source=pdf_text observed=2026-08-06T16:16:46.141869Z digest=sha256:995377f0bf1b4e527680aa6ff6eccb0afb0c2e021a92636e1a89e364493c42ea

Observation 3f8c2ecc-3e2e-415e-862c-d0ccbad61c0d · outbound

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source=pdf_text observed=2026-08-06T16:16:46.145508Z digest=sha256:94f6f06b990142e31d5d9a655a58ef8d87b411c9aa5bb5b2f5eced82e88ad80a

Observation 4c4bf79f-3a5e-4fdb-90f4-dab43decb756 · outbound

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Observation 46fe1820-7eda-4c83-adf7-c7db4b0b7518 · outbound

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Observation f21f77cd-9b6e-4c51-93bc-d9140fbe4ec3 · outbound

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Observation 3218203d-a204-4abd-bb86-8a639f1b46f6 · outbound

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Observation 7ddfa107-315b-4648-9a29-a79cece1d711 · outbound

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Observation 89fc41c6-de19-4f54-b3e9-d623024ac1ff · outbound

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Observation 1e485b54-5976-48de-b2b0-46009d1e0267 · outbound

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Observation 8f88d302-22c7-4d04-9969-23055160740e · outbound

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Observation c765ffb5-1e63-45b3-b39e-d5716cd6364d · outbound

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Observation e0407efc-57f5-47a3-83ba-560a34d1c492 · outbound

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Observation aad9ade9-ba85-4fd5-a2d9-44bc3d34b7e8 · outbound

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Observation cffd490c-a8f2-47cf-a1d2-1c43be8bbb19 · outbound

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Observation 9ff30aa1-50d1-4fe4-8d12-55603531a397 · outbound

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Observation a9b9f9ab-ad00-4d74-9cdf-8afdb7dd2a9a · outbound

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Observation f37fa43f-e775-46b3-b655-daa26ecfc9de · outbound

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Observation d27252ec-348e-4e87-88fd-241a173bc170 · outbound

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Observation 9b0bbf25-a097-4e0a-b119-ad59aa3baf9a · outbound

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This paper cites an unresolved cited work.

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Observation 85be5bdb-e0ec-43ec-97e3-bf179a72e827 · outbound

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Observation b39590c7-682a-473f-9ae0-6f46b0ac4a0b · outbound

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Observation cc3267ee-d3d0-4892-b7fc-5b1a6e853f28 · outbound

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Observation f0da7e47-4a4f-4d8c-8993-aaff11dc6a3d · outbound

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Observation abb8f06e-1e90-4bd4-8b42-e824d122901d · outbound

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Observation e535febd-3354-40f8-a276-e8c85c56021f · outbound

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Observation 692d79f9-995e-47fb-bca6-bd807452b591 · outbound

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