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Paper Citation Record · LEDGER

Isochrone Fitting of Galactic Globular Clusters -- VIII. Homogeneous estimates of parameters for 27 clusters

As of 9 August 2026, this Paper Citation Record lists 69 of 69 outbound references and 1 inbound Pith citation observation for arXiv:2605.28505.

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

pith.paper-citation-record.v1
2605.28505 v1

Coverage vector

measured 69 of 69 reference resolution

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Source: paper_references, paper_reference_links, observed 2026-06-29T11:14:12.391735Z

measured 70 of 70 standing notices

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Source: scholarly_work_events, retraction_status_cache, observed 2026-08-09T06:31:02.800959+00:00

measured 1 of 1 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T16:21:40.996957Z

measured 0 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: cited_works

Reference resolution

69 of 69 outbound references displayed

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External citation measurements

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Outbound references

Observation 55f01019-f98c-49df-a78e-6f60920e8d57 · outbound

This paper cites 2025, , 704, A255.

Isochrone Fitting of Galactic Globular Clusters -- VIII. Homogeneous estimates of parameters for 27 clusters 2025, , 704, A255

Reference 1

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source=arxiv_source observed=2026-06-29T11:14:12.391735Z digest=sha256:d1070cc7badd49a801cc89307c700231356a7f35fd42598ff800e6ab0c855c3a

Observation 7073a60a-c439-46b6-be26-c3967a01b1c7 · outbound

This paper cites 2012, , 143, 70.

Isochrone Fitting of Galactic Globular Clusters -- VIII. Homogeneous estimates of parameters for 27 clusters 2012, , 143, 70

Reference 2

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source=arxiv_source observed=2026-06-29T11:14:12.391735Z digest=sha256:98f8de338fab4718aceaa29e9e79387026919edcbfeb4c0f92afeb0b0cbd3ace

Observation 26052e49-92f3-49e3-adb4-3025aac61c27 · outbound

This paper cites 2014, , 113, 191302.

Isochrone Fitting of Galactic Globular Clusters -- VIII. Homogeneous estimates of parameters for 27 clusters 2014, , 113, 191302

Reference 3

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Observation fb85c52e-7c25-4b63-bc99-0837c6f1f36b · outbound

This paper cites T., & Bobylev , V.

Isochrone Fitting of Galactic Globular Clusters -- VIII. Homogeneous estimates of parameters for 27 clusters T., & Bobylev , V

Reference 4

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source=arxiv_source observed=2026-06-29T11:14:12.391735Z digest=sha256:614615a3f39684489865cd36e0b4a048766822782331ea4d137e7a089676231a

Observation 7756b6f8-0751-43b6-a48e-fb4f4a54e521 · outbound

This paper cites 2021, , 505, 5957.

Isochrone Fitting of Galactic Globular Clusters -- VIII. Homogeneous estimates of parameters for 27 clusters 2021, , 505, 5957

Reference 5

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Observation 340b93d4-700c-470f-b8b2-701fb99c7458 · outbound

This paper cites 2025, , 704, A81.

Isochrone Fitting of Galactic Globular Clusters -- VIII. Homogeneous estimates of parameters for 27 clusters 2025, , 704, A81

Reference 6

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Observation 2ffc5548-c028-4516-a29e-a064c3641836 · outbound

This paper cites an unresolved cited work.

Isochrone Fitting of Galactic Globular Clusters -- VIII. Homogeneous estimates of parameters for 27 clusters Unresolved cited work

Reference 7

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Observation 21e42fe2-4f57-437f-9778-f9844abc6012 · outbound

This paper cites G., Pepper , J., et al.

Isochrone Fitting of Galactic Globular Clusters -- VIII. Homogeneous estimates of parameters for 27 clusters G., Pepper , J., et al

Reference 8

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Observation cf0a2784-a782-408c-acfb-6c505b3d017c · outbound

This paper cites M., Cautun , M., Deason , A.

Isochrone Fitting of Galactic Globular Clusters -- VIII. Homogeneous estimates of parameters for 27 clusters M., Cautun , M., Deason , A

Reference 9

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Observation a85bec09-50be-401c-af64-e3959f11eced · outbound

This paper cites A., Clayton , G.

Isochrone Fitting of Galactic Globular Clusters -- VIII. Homogeneous estimates of parameters for 27 clusters A., Clayton , G

Reference 10

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Observation 69d8f3cf-8d7f-4547-bde7-d74c5bb2e570 · outbound

This paper cites 2025, Physical Research, 1117, 1.

Isochrone Fitting of Galactic Globular Clusters -- VIII. Homogeneous estimates of parameters for 27 clusters 2025, Physical Research, 1117, 1

Reference 11

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Observation bb4f95d2-881f-4f98-8027-fe7a5521cf68 · outbound

This paper cites 2009, , 508, 695.

Isochrone Fitting of Galactic Globular Clusters -- VIII. Homogeneous estimates of parameters for 27 clusters 2009, , 508, 695

Reference 12

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Observation ddc942c6-990b-4507-8306-3dcf30bdaa74 · outbound

This paper cites G., et al.

Isochrone Fitting of Galactic Globular Clusters -- VIII. Homogeneous estimates of parameters for 27 clusters G., et al

Reference 13

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Isochrone Fitting of Galactic Globular Clusters -- VIII. Homogeneous estimates of parameters for 27 clusters Unresolved cited work

Reference 14

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Isochrone Fitting of Galactic Globular Clusters -- VIII. Homogeneous estimates of parameters for 27 clusters Unresolved cited work

Reference 15

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Isochrone Fitting of Galactic Globular Clusters -- VIII. Homogeneous estimates of parameters for 27 clusters Unresolved cited work

Reference 16

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Observation f79d6b1f-270d-4eb9-abe5-6c58ad7c73ef · outbound

This paper cites an unresolved cited work.

Isochrone Fitting of Galactic Globular Clusters -- VIII. Homogeneous estimates of parameters for 27 clusters Unresolved cited work

Reference 17

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Observation 76255b4b-0871-4276-bd0b-6c363d5ef843 · outbound

This paper cites 2018, in IAU Symposium, Vol.

Isochrone Fitting of Galactic Globular Clusters -- VIII. Homogeneous estimates of parameters for 27 clusters 2018, in IAU Symposium, Vol

Reference 18

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Observation 02d6a405-b411-42f8-989f-7108a740cc6f · outbound

This paper cites 2025, , 704, A256.

Isochrone Fitting of Galactic Globular Clusters -- VIII. Homogeneous estimates of parameters for 27 clusters 2025, , 704, A256

Reference 19

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Observation 77e9cd7f-8bde-42d0-a405-0b19c9f7c51e · outbound

This paper cites 2017, in European Physical Journal Web of Conferences, Vol.

Isochrone Fitting of Galactic Globular Clusters -- VIII. Homogeneous estimates of parameters for 27 clusters 2017, in European Physical Journal Web of Conferences, Vol

Reference 20

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Observation a4589ca5-761a-4c31-9ee1-5d796160999c · outbound

This paper cites J., Hiskens , F.

Isochrone Fitting of Galactic Globular Clusters -- VIII. Homogeneous estimates of parameters for 27 clusters J., Hiskens , F

Reference 21

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Observation 0329a047-4d54-4727-b76c-562453bd9388 · outbound

This paper cites P., Lagioia , E.

Isochrone Fitting of Galactic Globular Clusters -- VIII. Homogeneous estimates of parameters for 27 clusters P., Lagioia , E

Reference 22

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Observation 493f2a97-d312-42b9-bff1-201044970dec · outbound

This paper cites 2007, , 134, 376.

Isochrone Fitting of Galactic Globular Clusters -- VIII. Homogeneous estimates of parameters for 27 clusters 2007, , 134, 376

Reference 23

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Observation e8c939fe-0734-4143-a3cd-2fb6db2a2cbd · outbound

This paper cites 2008, , 178, 89.

Isochrone Fitting of Galactic Globular Clusters -- VIII. Homogeneous estimates of parameters for 27 clusters 2008, , 178, 89

Reference 24

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Observation 294125e4-9b07-4cee-9969-ecb8e7a1e2f9 · outbound

This paper cites 2010, , 708, 698.

Isochrone Fitting of Galactic Globular Clusters -- VIII. Homogeneous estimates of parameters for 27 clusters 2010, , 708, 698

Reference 25

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Isochrone Fitting of Galactic Globular Clusters -- VIII. Homogeneous estimates of parameters for 27 clusters Unresolved cited work

Reference 26

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Isochrone Fitting of Galactic Globular Clusters -- VIII. Homogeneous estimates of parameters for 27 clusters Unresolved cited work

Reference 27

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Observation 65e2830c-62a7-4cb1-a3fc-097cbdbf1a99 · outbound

This paper cites B., Anderson , J., et al.

Isochrone Fitting of Galactic Globular Clusters -- VIII. Homogeneous estimates of parameters for 27 clusters B., Anderson , J., et al

Reference 28

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This paper cites A., Khovritchev , M.

Isochrone Fitting of Galactic Globular Clusters -- VIII. Homogeneous estimates of parameters for 27 clusters A., Khovritchev , M

Reference 29

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Observation 0c35b945-1192-44f6-9380-710a739584fe · outbound

This paper cites A., Marchuk , A.

Isochrone Fitting of Galactic Globular Clusters -- VIII. Homogeneous estimates of parameters for 27 clusters A., Marchuk , A

Reference 30

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This paper cites A., Mosenkov , A.

Isochrone Fitting of Galactic Globular Clusters -- VIII. Homogeneous estimates of parameters for 27 clusters A., Mosenkov , A

Reference 31

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Observation d28a8573-3d0a-4e5e-87f4-8bf4c0ff7465 · outbound

This paper cites A., Khovritchev , M.

Isochrone Fitting of Galactic Globular Clusters -- VIII. Homogeneous estimates of parameters for 27 clusters A., Khovritchev , M

Reference 32

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This paper cites A., Khovritchev , M.

Isochrone Fitting of Galactic Globular Clusters -- VIII. Homogeneous estimates of parameters for 27 clusters A., Khovritchev , M

Reference 33

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Observation 5c2ff4c2-9b78-46c6-b6f1-e2429ac02cc6 · outbound

This paper cites A., Bonatto , C.

Isochrone Fitting of Galactic Globular Clusters -- VIII. Homogeneous estimates of parameters for 27 clusters A., Bonatto , C

Reference 34

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This paper cites A., Savchenko , S.

Isochrone Fitting of Galactic Globular Clusters -- VIII. Homogeneous estimates of parameters for 27 clusters A., Savchenko , S

Reference 35

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This paper cites A., Savchenko , S.

Isochrone Fitting of Galactic Globular Clusters -- VIII. Homogeneous estimates of parameters for 27 clusters A., Savchenko , S

Reference 36

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Isochrone Fitting of Galactic Globular Clusters -- VIII. Homogeneous estimates of parameters for 27 clusters Unresolved cited work

Reference 37

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Observation e362be33-ca5e-471e-baf7-245294e8df02 · outbound

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Isochrone Fitting of Galactic Globular Clusters -- VIII. Homogeneous estimates of parameters for 27 clusters L., Pietrinferni , A., Cassisi , S., et al

Reference 38

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Observation 28716245-861f-489c-869a-46be3e3a3af1 · outbound

This paper cites P., Legnardi , M.

Isochrone Fitting of Galactic Globular Clusters -- VIII. Homogeneous estimates of parameters for 27 clusters P., Legnardi , M

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source=arxiv_source observed=2026-06-29T11:14:12.391735Z digest=sha256:4e12303ca6b02d6560431ab11604fa6ca13f257a78206221e8c7f9dbb83b6a1a

Observation 312d8a14-1b5b-4fa5-829f-ec246d49938b · outbound

This paper cites P., Marino , A.

Isochrone Fitting of Galactic Globular Clusters -- VIII. Homogeneous estimates of parameters for 27 clusters P., Marino , A

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source=arxiv_source observed=2026-06-29T11:14:12.391735Z digest=sha256:732be60990ec7efbae8efde1b187137cf704ea9b577092a4235fb03c69723bde

Observation faeebf59-ef89-43d6-b1ec-388c4abd0546 · outbound

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source=arxiv_source observed=2026-06-29T11:14:12.391735Z digest=sha256:9ec2fa15b8abfd1f9bebe78eb30634de9e51422f588b0299bc1a6fc44ce664f3

Observation 77c3fdba-2f11-4721-a99f-cb9652c99881 · outbound

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source=arxiv_source observed=2026-06-29T11:14:12.391735Z digest=sha256:c5679ab25ee961ae5fcb3a8aaf1fa1c656bca9ba7c7fbb9b7ba9db64ff705155

Observation e1aa12ca-dcd9-43d7-b953-0b1ba7e50234 · outbound

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source=arxiv_source observed=2026-06-29T11:14:12.391735Z digest=sha256:e1a6488d239cafd78465490b41612ac6a51132f21ac94088b89d8ef59cbfee58

Observation 1b5c96e2-9819-4e07-b45a-0ee358923c98 · outbound

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source=arxiv_source observed=2026-06-29T11:14:12.391735Z digest=sha256:50ef3389fc064a203d023d05f005b184bafd6fa9d890c83db304c576b11c6aa3

Observation 136ced4d-cbbe-4819-ab17-2d7929d92af4 · outbound

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source=arxiv_source observed=2026-06-29T11:14:12.391735Z digest=sha256:3a46055a0a41fdcf89be2c0e23b9d5dbf778a53315574a7a578010485dcb0646

Observation 88e34e92-71e1-4ea7-86b9-f05b51f0590f · outbound

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source=arxiv_source observed=2026-06-29T11:14:12.391735Z digest=sha256:d225a2aa29b5c5be1056ad3777e0c491bd0c7ce5b723c1eb5a1bcad380c61ecb

Observation e8b028bd-ed36-485b-bf63-891f737e17de · outbound

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source=arxiv_source observed=2026-06-29T11:14:12.391735Z digest=sha256:55c8ac841e1980846b0e054732db2c2630167fa9aaa40ce9e5128ad4d493088c

Observation 88b0d327-285f-4370-b6b0-3318a7165933 · outbound

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source=arxiv_source observed=2026-06-29T11:14:12.391735Z digest=sha256:09dd27dddf14c6543ee0c1b28c7fc5c4b3f6012cbe23ecf8f4da4a1f771ff183

Observation 1dc37096-9090-4976-bab9-45a7db3de6df · outbound

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source=arxiv_source observed=2026-06-29T11:14:12.391735Z digest=sha256:da82eaf6ecd263432a953813705679052aa915617b942e78e26e41390220276b

Observation 69d2ef3d-919a-4da9-83ee-41ca85ca89b0 · outbound

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source=arxiv_source observed=2026-06-29T11:14:12.391735Z digest=sha256:89135926a16490b412f943a8c7ee2c954435afa5f164460af12c9b0943c237ed

Observation 7be80dca-9137-495f-b05a-42fbb3c5bbdb · outbound

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source=arxiv_source observed=2026-06-29T11:14:12.391735Z digest=sha256:b09ade11523c31ffac7391adaaddef854ae3ba2cd6cd6d73ee7fa74978cb9646

Observation 5ad48fe3-e86d-44b4-a2de-dfabbabc4169 · outbound

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source=arxiv_source observed=2026-06-29T11:14:12.391735Z digest=sha256:d88dd36d0863975611e654c66371308804d3e85384d24584015cd22033756f2d

Observation dbf4c75e-8db4-4e6c-a371-fbb3e0b33bc1 · outbound

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source=arxiv_source observed=2026-06-29T11:14:12.391735Z digest=sha256:c88d3632d9ca2ff6b928fc1359371d676f84253d13a1b22ebc7c336ceeb04b95

Observation 38c38c7b-aaba-40bf-9ffe-889c1d9be3e9 · outbound

This paper cites an unresolved cited work.

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source=arxiv_source observed=2026-06-29T11:14:12.391735Z digest=sha256:6cf14c2f2e4b3aac49bb2a0700fcbf1cec500398527f99d86b52e83bd0a1203a

Observation c4ebfdeb-9348-490a-9fdb-731faf37cdad · outbound

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source=arxiv_source observed=2026-06-29T11:14:12.391735Z digest=sha256:e623d72e0bbd38f23ab2233ac01e9e57123cdf109c69c714d51b90845d84f7e2

Observation 033609d4-ed20-4602-98d2-b0cc3be6f1be · outbound

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source=arxiv_source observed=2026-06-29T11:14:12.391735Z digest=sha256:bb8d02fff8207fe48d28ba5c5c6b3ea15296e3efd8f43d2d7d268c12a2c8837e

Observation 81bb0ed3-2e8b-4bf8-9a07-4b25434ea626 · outbound

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source=arxiv_source observed=2026-06-29T11:14:12.391735Z digest=sha256:866ee85ff7e706226048742f7546fb9ef348b71c424d5a3e4d1d7b0789ebda5b

Observation 8db11db8-0959-4498-8748-3103d809f296 · outbound

This paper cites an unresolved cited work.

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source=arxiv_source observed=2026-06-29T11:14:12.391735Z digest=sha256:e45f6cc1831f90ecd5c03efb150f3b23a5b830b5c0520f4efb0709d3a081e483

Observation c843c944-77e0-4792-900e-9900e209961e · outbound

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source=arxiv_source observed=2026-06-29T11:14:12.391735Z digest=sha256:39fc9100e45b35a9d73d9662daa85a535192c24f0c2ce4b386b56ad5b3e3a855

Observation 109bc563-53c4-4619-a4e5-94cb1ec39f7a · outbound

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source=arxiv_source observed=2026-06-29T11:14:12.391735Z digest=sha256:789f8fcdaec3c9ed8b349248629c75398dfafc7a5e219a0ef779c209e94bd7a2

Observation 86230a50-4b84-4a2b-8fb3-3f8868598c8c · outbound

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source=arxiv_source observed=2026-06-29T11:14:12.391735Z digest=sha256:40c35d3ab018cfd2cfea0d4c999551a9e2cf54f21aa3ac94dcf7b7b13e90649a

Observation 575ac1fe-fd19-4f1e-850b-89553e4e2a51 · outbound

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source=arxiv_source observed=2026-06-29T11:14:12.391735Z digest=sha256:691fa93c666301f10fda5da13ac61f44ca1c0aa0341e4a4ad88536d2cfcf0e0e

Observation 4cf91675-9b1c-42a0-a3e5-90118ae8de0d · outbound

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source=arxiv_source observed=2026-06-29T11:14:12.391735Z digest=sha256:c8124c89f6cfd123e43e54c094e1589506d8594c3e0d3e6db373d0696e3bc700

Observation 615525f5-7100-4755-b2cb-879e7d49791f · outbound

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source=arxiv_source observed=2026-06-29T11:14:12.391735Z digest=sha256:3ccf4b61da018647182daabc15d6d451cf7e44375930f27dc4c7ba0b38912c02

Observation b88011c9-21c4-4c48-8268-7adeebfb35c9 · outbound

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source=arxiv_source observed=2026-06-29T11:14:12.391735Z digest=sha256:576d84280e1bdc8c8aa41985d70f55bc19c98c0e14b86311c02e8e0cd643ff1e

Observation 9c761708-0c3b-4aa6-9e14-7e68c7d96126 · outbound

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source=arxiv_source observed=2026-06-29T11:14:12.391735Z digest=sha256:6ea730ac877dba8ad6575b4bb78ea02c7bc9e9aa0b0d16ba190caa325ed992f5

Observation af242457-2bf7-438a-a580-a337de0891ff · outbound

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source=arxiv_source observed=2026-06-29T11:14:12.391735Z digest=sha256:930d894f71a07ff900cc9633658b1735ea1a94ff5abd556e064d6d135b3f5fdc

Observation 5aac7e06-f5be-4bc8-86ac-e5e3c9449b3a · outbound

This paper cites an unresolved cited work.

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source=arxiv_source observed=2026-06-29T11:14:12.391735Z digest=sha256:22e0ee56e26f589c230e5af539dd6935ae8cd1528261f36764b61379277b91e1

Observation 6f4e3784-dbf8-4b42-b2cd-a45aaa2c6bfc · outbound

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source=arxiv_source observed=2026-06-29T11:14:12.391735Z digest=sha256:1b3276ed15f43a8a127ba9ace948921c3ef4e0951054e2cacea1176cfea3cad6

Pith citing papers

Observation 0555a609-20c5-41d2-bf87-849e7357ad7f · inbound

Isochrone fitting of Galactic globular clusters - IX. Tip of the red-giant branch for 27 clusters and constraints on new particle physics cites this paper.

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