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Paper Citation Record · LEDGER

The AURORA Survey: Multiple Balmer and Paschen Emission Lines for Individual Star-forming Galaxies at z=1.5-4.4. II. Implications for Nebular Dust Corrections, Nebular SFRs, and Differential Reddening

As of 6 August 2026, this Paper Citation Record lists 96 of 96 outbound references and 0 inbound Pith citation observations for arXiv:2605.30427.

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

pith.paper-citation-record.v1
2605.30427 v1

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measured 96 of 96 reference resolution

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Outbound references

Reference 1

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Reference 2

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Reference 7

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Reference 9

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Observation ff3a19f3-eb64-4420-bf1f-f3e713ec6d57 · outbound

This paper cites L., & Storchi-Bergmann, T.

The AURORA Survey: Multiple Balmer and Paschen Emission Lines for Individual Star-forming Galaxies at z=1.5-4.4. II. Implications for Nebular Dust Corrections, Nebular SFRs, and Differential Reddening L., & Storchi-Bergmann, T

Reference 11

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Reference 12

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Reference 13

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Reference 14

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Reference 17

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Observation 220f6283-10d5-47e4-a2e7-8d47bddc124c · outbound

This paper cites J., Chatzikos, M., Guzm´an, F., et al.

The AURORA Survey: Multiple Balmer and Paschen Emission Lines for Individual Star-forming Galaxies at z=1.5-4.4. II. Implications for Nebular Dust Corrections, Nebular SFRs, and Differential Reddening J., Chatzikos, M., Guzm´an, F., et al

Reference 23

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Reference 24

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Reference 25

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Reference 26

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Reference 27

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Observation 8f9ab1ba-c332-426b-a470-24aeb1909251 · outbound

This paper cites 1999, MNRAS, 306, 843 20.

The AURORA Survey: Multiple Balmer and Paschen Emission Lines for Individual Star-forming Galaxies at z=1.5-4.4. II. Implications for Nebular Dust Corrections, Nebular SFRs, and Differential Reddening 1999, MNRAS, 306, 843 20

Reference 28

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Reference 29

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Reference 30

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Reference 31

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Reference 32

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Observation 6f8c4725-da27-4d7f-98d3-300a1540df43 · outbound

This paper cites F., Kereˇs, D., O˜norbe, J., et al.

The AURORA Survey: Multiple Balmer and Paschen Emission Lines for Individual Star-forming Galaxies at z=1.5-4.4. II. Implications for Nebular Dust Corrections, Nebular SFRs, and Differential Reddening F., Kereˇs, D., O˜norbe, J., et al

Reference 33

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Reference 34

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Reference 35

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Observation 0346a6d4-a4b3-4bbf-a3ac-2c162efc13b6 · outbound

This paper cites D., Rodighiero, G., et al.

The AURORA Survey: Multiple Balmer and Paschen Emission Lines for Individual Star-forming Galaxies at z=1.5-4.4. II. Implications for Nebular Dust Corrections, Nebular SFRs, and Differential Reddening D., Rodighiero, G., et al

Reference 36

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Reference 37

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Observation 0fe785cc-8021-42a6-8f5b-c722d52b122e · outbound

This paper cites C., Tamblyn, P., & Congdon, C.

The AURORA Survey: Multiple Balmer and Paschen Emission Lines for Individual Star-forming Galaxies at z=1.5-4.4. II. Implications for Nebular Dust Corrections, Nebular SFRs, and Differential Reddening C., Tamblyn, P., & Congdon, C

Reference 38

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Reference 39

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Reference 40

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Reference 41

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Reference 46

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Reference 48

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Reference 49

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Reference 50

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Reference 51

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Reference 53

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Reference 54

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Observation bec36fa3-9730-4763-a605-676d39fbcdce · outbound

This paper cites J., Shapley, A., Steidel, C.

The AURORA Survey: Multiple Balmer and Paschen Emission Lines for Individual Star-forming Galaxies at z=1.5-4.4. II. Implications for Nebular Dust Corrections, Nebular SFRs, and Differential Reddening J., Shapley, A., Steidel, C

Reference 55

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Observation 7a6c85cb-a6e6-46c0-b124-d6ffdb2fbd9f · outbound

This paper cites J., Shapley, A., Reddy, N.

The AURORA Survey: Multiple Balmer and Paschen Emission Lines for Individual Star-forming Galaxies at z=1.5-4.4. II. Implications for Nebular Dust Corrections, Nebular SFRs, and Differential Reddening J., Shapley, A., Reddy, N

Reference 56

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Reference 57

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Observation 62701ec8-03c1-4066-ad95-918ec7a46878 · outbound

This paper cites H., Kriek, M., Brammer, G.

The AURORA Survey: Multiple Balmer and Paschen Emission Lines for Individual Star-forming Galaxies at z=1.5-4.4. II. Implications for Nebular Dust Corrections, Nebular SFRs, and Differential Reddening H., Kriek, M., Brammer, G

Reference 58

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source=pdf_text observed=2026-06-29T06:25:29.988558Z digest=sha256:70706fb64c1677f6a8f34c297cd98ab0cdb9fb0134a2f0570be671707fca1973

Reference 59

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source=pdf_text observed=2026-06-29T06:25:29.988558Z digest=sha256:ae541e088fa9f0f22f73bb01e0b9e91ccfd41ee4706e16ebb6f8c92bf9581f3e

Observation d8c13d2a-563b-47dd-977f-74b0e28a9ad4 · outbound

This paper cites A., Pettini, M., Steidel, C.

The AURORA Survey: Multiple Balmer and Paschen Emission Lines for Individual Star-forming Galaxies at z=1.5-4.4. II. Implications for Nebular Dust Corrections, Nebular SFRs, and Differential Reddening A., Pettini, M., Steidel, C

Reference 60

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source=pdf_text observed=2026-06-29T06:25:29.988558Z digest=sha256:fb696ea0aa999aeaa0c82695dec6f6a331e9f0182a9ac86b315b2f884736c846

Reference 61

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source=pdf_text observed=2026-06-29T06:25:29.988558Z digest=sha256:8f08ee3a6f0f7d318eb2b8fc002950c0e62c0bca23a4a88b469c2391e24c7e55

Observation d723abe7-0883-48d9-b7d9-09c5c1278e99 · outbound

This paper cites A., Kriek, M., Shapley, A.

The AURORA Survey: Multiple Balmer and Paschen Emission Lines for Individual Star-forming Galaxies at z=1.5-4.4. II. Implications for Nebular Dust Corrections, Nebular SFRs, and Differential Reddening A., Kriek, M., Shapley, A

Reference 62

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source=pdf_text observed=2026-06-29T06:25:29.988558Z digest=sha256:72031e93d2d3b449ca51b6b1c2c2f1c44a498ef8e16df30cb42d8679ff752af4

Reference 63

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source=pdf_text observed=2026-06-29T06:25:29.988558Z digest=sha256:f5b77e9a1d515ecc661cfc293a4887940cb5e38466931f1f8a9e9c131d3ac72b

Reference 64

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source=pdf_text observed=2026-06-29T06:25:29.988558Z digest=sha256:5d8741db6648d9d8d70179e82235d3883f63f93a8b62e91aecfc357e59dd7277

Reference 65

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source=pdf_text observed=2026-06-29T06:25:29.988558Z digest=sha256:286b34702c9a5df6f6d60cb6c65814d9b4f322b80627ae8d36acc41857bc7fe0

Reference 66

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source=pdf_text observed=2026-06-29T06:25:29.988558Z digest=sha256:886a78f38eecb73a96f490cee51efdfb26a5873818efa9e2992ffdff8c70de1a

Reference 67

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source=pdf_text observed=2026-06-29T06:25:29.988558Z digest=sha256:46696a8f49c81b9346474ec58953f89c5e4f8d6f51b40a6da8c9936115a81eb7

Reference 68

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source=pdf_text observed=2026-06-29T06:25:29.988558Z digest=sha256:16bfbaae22d8f9095e54e6133a180d135e4d9d1314a0ebb8a561e67dcbce529d

Reference 69

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Reference 70

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Reference 71

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source=pdf_text observed=2026-06-29T06:25:29.988558Z digest=sha256:54e3f70bad8100b523ef96b18a7623f2a6b6a8675770aa0866662231a4285959

Reference 72

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source=pdf_text observed=2026-06-29T06:25:29.988558Z digest=sha256:13a73d1787cca53470a9496c9b457c70874f9e9b61dbf05fafdffa5da86ac024

Reference 73

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source=pdf_text observed=2026-06-29T06:25:29.988558Z digest=sha256:565d36f2c20714136061e31eed8debf01880b071bd4f364cecabd90fc1714d77

Reference 74

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source=pdf_text observed=2026-06-29T06:25:29.988558Z digest=sha256:6397c430a852f201c40afac42c783cbf71353c7ae3d0447499e978ad0f87a160

Reference 75

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verified exact
arxiv_id, observed 2026-06-29T14:33:31.698311Z

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source=pdf_text observed=2026-06-29T06:25:29.988558Z digest=sha256:4150cabe6cf771c5710f423548d1d545ccc3e9a6cd795b8a6b267422aa7e5950

Reference 76

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Reference 77

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Reference 78

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Reference 79

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source=pdf_text observed=2026-06-29T06:25:29.988558Z digest=sha256:6602bc91207fb2f534dc3e6ca62562b9297a57c9dc18ff3ee26b593e76e672be

Observation 9eb35ba2-d995-41f7-b8d2-4159f26991ee · outbound

This paper cites C., Bogosavljevi´c, M., Shapley, A.

The AURORA Survey: Multiple Balmer and Paschen Emission Lines for Individual Star-forming Galaxies at z=1.5-4.4. II. Implications for Nebular Dust Corrections, Nebular SFRs, and Differential Reddening C., Bogosavljevi´c, M., Shapley, A

Reference 80

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source=pdf_text observed=2026-06-29T06:25:29.988558Z digest=sha256:3ffbc0921add84367e8ef4e5494edd1ca5391c24a87892b9ecdd07364e4e329b

Observation 1e599697-4048-4090-ab06-73a9a5e0f48e · outbound

This paper cites C., Pettini, M., & Adelberger, K.

The AURORA Survey: Multiple Balmer and Paschen Emission Lines for Individual Star-forming Galaxies at z=1.5-4.4. II. Implications for Nebular Dust Corrections, Nebular SFRs, and Differential Reddening C., Pettini, M., & Adelberger, K

Reference 81

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source=pdf_text observed=2026-06-29T06:25:29.988558Z digest=sha256:f3cb4d196464d48d6b1651a9e23f1f6f3b90d827edcc1821db943b73074c258e

Reference 82

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source=pdf_text observed=2026-06-29T06:25:29.988558Z digest=sha256:27d6b0eb469f22dfa136b39251631e0b136ca3ca70a78bb74337f98ee157c4c5

Reference 83

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source=pdf_text observed=2026-06-29T06:25:29.988558Z digest=sha256:d31eca3a3e5c7ee15827686c2bc22174aa1a749f94b37d37e1e76ebd353d646f

Reference 84

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source=pdf_text observed=2026-06-29T06:25:29.988558Z digest=sha256:421e89d6b9cf4bdc71e69abacbadaecbb7527ee2238dd301289ec8918115e16e

Reference 85

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Reference 86

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Reference 87

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Reference 88

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Observation 00cd7b59-1278-406c-98bc-9d5c1592d973 · outbound

This paper cites E., Franx, M., Leja, J., et al.

The AURORA Survey: Multiple Balmer and Paschen Emission Lines for Individual Star-forming Galaxies at z=1.5-4.4. II. Implications for Nebular Dust Corrections, Nebular SFRs, and Differential Reddening E., Franx, M., Leja, J., et al

Reference 89

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Reference 90

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source=pdf_text observed=2026-06-29T06:25:29.988558Z digest=sha256:4ea98fd4510a3a1e4161b5aab5cd7c175755265404e1cc92250f7f623808f32b

Reference 91

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verified exact
arxiv_id, observed 2026-06-29T14:33:31.700981Z

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source=pdf_text observed=2026-06-29T06:25:29.988558Z digest=sha256:c4d9ab3d785ab0709725a58a50a5b84a4a4da393734e9a4b217af99d1ac7b60d

Reference 92

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source=pdf_text observed=2026-06-29T06:25:29.988558Z digest=sha256:f45b3e8d675f90045a2e845cc25ed40a39ccbc89ac571dff3bdc2c859b469fd6

Observation 6f35ac5b-9514-48c8-9af7-af11b5cbef07 · outbound

This paper cites G., Adelman, J., Anderson, Jr., J.

The AURORA Survey: Multiple Balmer and Paschen Emission Lines for Individual Star-forming Galaxies at z=1.5-4.4. II. Implications for Nebular Dust Corrections, Nebular SFRs, and Differential Reddening G., Adelman, J., Anderson, Jr., J

Reference 93

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source=pdf_text observed=2026-06-29T06:25:29.988558Z digest=sha256:cc9642fe2840c508d28c8f58a2f59358b4de9bfd7b51986863d44636ceef0609

Reference 94

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source=pdf_text observed=2026-06-29T06:25:29.988558Z digest=sha256:77f49f3492de9082060bb715704f9e23a522fad22ffedd0c7a9d166496cbe58d

Observation 5f9e4367-faef-4966-b1ae-1a21d6433d9a · outbound

This paper cites R., Ciardullo, R., Gronwall, C., et al.

The AURORA Survey: Multiple Balmer and Paschen Emission Lines for Individual Star-forming Galaxies at z=1.5-4.4. II. Implications for Nebular Dust Corrections, Nebular SFRs, and Differential Reddening R., Ciardullo, R., Gronwall, C., et al

Reference 95

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source=pdf_text observed=2026-06-29T06:25:29.988558Z digest=sha256:2cd764c975f232a2739119e01f2727d2b7e5a475c4f496ce5daef5cddf6f40d1

Reference 96

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source=pdf_text observed=2026-06-29T06:25:29.988558Z digest=sha256:256a6d21fa66ebf3b354efefe77c36f7abd3a5e2a35a6cf66f32b4b7cc351559

Pith citing papers

No inbound Pith citation observations are available.