Pith. sign in

Paper Citation Record · LEDGER

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters

As of 13 August 2026, this Paper Citation Record lists 93 of 93 outbound references and 0 inbound Pith citation observations for arXiv:2607.26347.

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

pith.paper-citation-record.v1
2607.26347 v1

Coverage vector

measured 93 of 93 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-01T00:09:12.353801Z

measured 93 of 93 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-13T06:32:02.005865+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

93 of 93 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved93
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

No source-named external measurement is stored.

Outbound references

Observation 6bb29ee2-bade-443b-96ba-57b9a146da6e · outbound

This paper cites 2021, A&A, 656, A149.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters 2021, A&A, 656, A149

Reference 1

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:06.477231Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:06.477231Z digest=sha256:22112b0559f4d8e07149bc02f09f6d0f540e6d6fc683d992153482a87f21f86c

Observation 16789dc7-bfe0-41b9-bb22-0e695a10401b · outbound

This paper cites & Plez, B.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters & Plez, B

Reference 2

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:06.575954Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:06.575954Z digest=sha256:ea4b9d80313a1e4bad4266084298709923dcfa42badb6e2ad7ae86a3151866e2

Observation 449f139e-f397-4aa2-883b-bc2b4de6a38b · outbound

This paper cites 2024, 687, A101.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters 2024, 687, A101

Reference 3

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:06.691680Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:06.691680Z digest=sha256:4189b43707e5a58944bab108bcb89134d7d12329f83ff4f3ea3ef9d175ac2efd

Observation 48563fc4-54b2-4f52-9420-3104f603edd9 · outbound

This paper cites & Grevesse, N.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters & Grevesse, N

Reference 4

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:06.867098Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:06.867098Z digest=sha256:9f59c8a59f48027febf51d5f043794a45ea0aa426a32942397a961be8b2aa1aa

Observation 9c10d448-50fa-4610-b30d-6529546a9087 · outbound

This paper cites R., Hayes, C.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters R., Hayes, C

Reference 5

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:07.038605Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:07.038605Z digest=sha256:d86517aed5ce064cc6edcafc98c2a0c786d790a4ef13b1010e9213e5c120f4de

Observation 27067b85-3755-4365-9735-7fa4f4505329 · outbound

This paper cites 2017, ApJ, 837, 8.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters 2017, ApJ, 837, 8

Reference 6

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:07.202274Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:07.202274Z digest=sha256:7e938420b85af00f945daa41c9f27af27462d9a3a04f065b5bd2afd21c33340e

Observation 350c8761-6e84-464d-850a-34599de4387e · outbound

This paper cites & Montes, F.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters & Montes, F

Reference 7

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:07.429959Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:07.429959Z digest=sha256:46199207047c21d5d1a77fbf2eb5b91d38bf855ef0de2331885e7cb3071404bd

Observation 2fbcbe93-d3fb-49ee-90e6-fce24f8907b0 · outbound

This paper cites & Thielemann, F.-K.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters & Thielemann, F.-K

Reference 8

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:07.631158Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:07.631158Z digest=sha256:db0b2e0a601a91cb2c0e9c07815978099107c8e299b6979478d21ff558a5f700

Observation 285dfa84-f874-411e-b398-dc688930c2db · outbound

This paper cites & Goriely, S.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters & Goriely, S

Reference 9

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:07.847317Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:07.847317Z digest=sha256:79361a7a26302525a75f102afa0e3ed35940fd9a6498793b5ee0387d7367b271

Observation 0addd30b-ec72-4d2c-b6ec-3c7de4b80e43 · outbound

This paper cites J., & Scott, P.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters J., & Scott, P

Reference 10

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:08.061806Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:08.061806Z digest=sha256:feb44556efb970de2a26b97ca183177f1c237bdd87aa5e4d0535b1a6b1b69b8b

Observation 29d5c809-2c3f-4716-844e-3b5f99d1b1d0 · outbound

This paper cites 2021, A&A, 653, A67.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters 2021, A&A, 653, A67

Reference 11

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:08.239363Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:08.239363Z digest=sha256:20bdb3c2a8ee06604c1536f5d7e0ae265124b1f9cd26d530e115131ae8205c7b

Observation 2e6ace42-cbad-4747-9e1b-b5dd4b324ea2 · outbound

This paper cites an unresolved cited work.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters Unresolved cited work

Reference 12

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:08.335333Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:08.335333Z digest=sha256:56f796f676a4829b0ffa6fafd3e5e819f17004f6ae7afecb03e95d7de444b437

Observation 4513dc55-9dbd-40a8-be3d-a28c88619ab7 · outbound

This paper cites 2014, ApJ, 787, 10.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters 2014, ApJ, 787, 10

Reference 13

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:08.558381Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:08.558381Z digest=sha256:45a513036199ddb0be6c22ad8abc2e75d1cf366b5f06e88517cc44aa3d98b016

Observation 321a2be9-87ad-4c8b-a05a-2d2b97fe09dd · outbound

This paper cites an unresolved cited work.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters Unresolved cited work

Reference 14

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:08.728985Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:08.728985Z digest=sha256:fdad5986fb6e9842d3324288829dd348fc50eca4c3bd5f0298c2dfab8318c39e

Observation 81ebc59d-5ed1-4816-b197-47313fd62936 · outbound

This paper cites 2019, Astronomy and Astro- physics, 623.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters 2019, Astronomy and Astro- physics, 623

Reference 15

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:08.940057Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:08.940057Z digest=sha256:88170c4770ea5b316a8d2008d30fe71087278edf5a5650b734a844672e954283

Observation 1aefba59-ec4e-4dbb-916e-e8663a8f31e3 · outbound

This paper cites M., Burbidge, G.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters M., Burbidge, G

Reference 16

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:09.119304Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:09.119304Z digest=sha256:f65462a8adbe2f5e81d72bbed38a6810a85f7c3abd60cf6a5206df0d44204743

Observation a704e36e-689a-4895-b8b2-efde3d351e21 · outbound

This paper cites an unresolved cited work.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters Unresolved cited work

Reference 17

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:09.122028Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:09.122028Z digest=sha256:cb3bcd0d13718ad8fb79547ef0aebfef611fc2bc04b29e043d593b5022c1c62a

Observation 29d62e5d-e4fc-40f9-89e1-3c5a14805167 · outbound

This paper cites 2020, A&A, 640, A1.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters 2020, A&A, 640, A1

Reference 18

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:09.192005Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:09.192005Z digest=sha256:05e6992d6059a395ace8e2b23635919213503e1fe84860c2e8c61004b8a0ca06

Observation 3895e78d-de42-4697-b4d2-a93c4e4991bd · outbound

This paper cites 2018, Astronomy and Astro- physics, 618.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters 2018, Astronomy and Astro- physics, 618

Reference 19

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:09.304852Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:09.304852Z digest=sha256:71f2c032b00775f869450c6fea163e2841c974ac27dd8602fe9e1e7101fe6f6c

Observation 8217eb4d-6e98-474e-98b4-8083fbdb0fa3 · outbound

This paper cites 2024, 687, A239.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters 2024, 687, A239

Reference 20

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:09.404556Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:09.404556Z digest=sha256:b28ddb851be68a05901d2beaf7316e0da6b5115e0af1f000f953da4e194783f3

Observation a1895b3a-46e6-485d-a0cc-cc9860bfc365 · outbound

This paper cites 2022, Astronomy & Astro- physics, 663.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters 2022, Astronomy & Astro- physics, 663

Reference 21

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:09.514072Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:09.514072Z digest=sha256:3f1dda8f0d1838f985854f26216c8e9f9c25b93968dbe477b78b74aa0fab4b7f

Observation 68c503e4-4c89-467c-b380-649c1e834ada · outbound

This paper cites 2019, Astronomy and Astro- physics, 627.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters 2019, Astronomy and Astro- physics, 627

Reference 22

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:09.653736Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:09.653736Z digest=sha256:ee21791f29402a4cbc9b5004bf59133f8ee8562797affc9ce4e6a23059bd4c63

Observation 1c0c4b14-1a3a-42cc-94d9-b40879c3024a · outbound

This paper cites 2020, A&A, 643, A12.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters 2020, A&A, 643, A12

Reference 23

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:09.817173Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:09.817173Z digest=sha256:7b3921fa07c286eb49e5380b015d665f788f33272a561a332cca3f904ebd7a1e

Observation 800ee4c6-be19-480a-91e4-706d738b455f · outbound

This paper cites 2016, Monthly Notices of the Royal Astronomical Society, 458.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters 2016, Monthly Notices of the Royal Astronomical Society, 458

Reference 24

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:09.979733Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:09.979733Z digest=sha256:7239d878b71ee39e47e1e752451a62f1c73151e3642cf583dae21d2eaa1866d0

Observation 4970ebbb-63bc-491e-9d94-f3b4cbddc2e8 · outbound

This paper cites 2021, A&A, 652, A25.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters 2021, A&A, 652, A25

Reference 25

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:10.160785Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:10.160785Z digest=sha256:2274bd23209e3bcf40f105dc3051d27879cf6aece689329130d03f5ccf81bab7

Observation 896dd4a4-a4c0-414a-8bdc-ef11048e5361 · outbound

This paper cites 2021, A&A, 648, A119.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters 2021, A&A, 648, A119

Reference 26

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:10.420459Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:10.420459Z digest=sha256:eaee2ab88877370878324d2a491bc3a08cacd421547baf4d6474e6e674133471

Observation ecdb1d40-5803-4e84-9097-85e384926445 · outbound

This paper cites 2014, in Ground-based and Airborne Instrumentation for Astronomy V , V ol.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters 2014, in Ground-based and Airborne Instrumentation for Astronomy V , V ol

Reference 27

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:10.592749Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:10.592749Z digest=sha256:caf10745484d29387986b724aa600c6309427866e0da92f5fbb01499f198f35c

Observation 3638001f-223a-48bf-aa21-65a479a3f2ca · outbound

This paper cites 2012, in Society of Photo-Optical Instru- mentation Engineers (SPIE) Conference Series, V ol.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters 2012, in Society of Photo-Optical Instru- mentation Engineers (SPIE) Conference Series, V ol

Reference 28

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:10.834542Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:10.834542Z digest=sha256:2e213105bbb1ca22eb07f666298527051a0100f4a3f75b345ba4d115e67c779d

Observation 5c6ee90b-189a-4a24-9758-bf07b7df51b0 · outbound

This paper cites an unresolved cited work.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters Unresolved cited work

Reference 29

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:11.007119Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:11.007119Z digest=sha256:b3c4a857f8d65816b7b4b4d4824bfbd7d97a0806142fbd9f3fd35c0f02895dc4

Observation d89edda0-abc5-42a7-8b9a-d88fbb307742 · outbound

This paper cites J., Sneden, C., Lawler, J.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters J., Sneden, C., Lawler, J

Reference 30

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:11.060152Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:11.060152Z digest=sha256:78d1f241bccb14e6632f12e92d602c80dfeb0d9d978fcd401b47a83f6fe1928e

Observation c58e5d52-675b-426f-9a0a-c70852a16a70 · outbound

This paper cites 2010, ApJ, 712, 1359.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters 2010, ApJ, 712, 1359

Reference 31

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:11.116008Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:11.116008Z digest=sha256:9cc2bb238d9d282e9722de22f6361458ab9f424450b8a01ea39d576755b96721

Observation b69104bd-e250-4fce-86b5-f92c3fbaa620 · outbound

This paper cites W., Lang, D., & Goodman, J.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters W., Lang, D., & Goodman, J

Reference 32

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:11.224942Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:11.224942Z digest=sha256:b9e8597031686ef971e38f46ce5f241f9b84769c66f9eeb9604d86a170efa5cd

Observation 1a85f165-2f50-4f56-9c22-cd71159cde86 · outbound

This paper cites W., & Morton, T.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters W., & Morton, T

Reference 33

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:11.385458Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:11.385458Z digest=sha256:22e4493169d2966aa362bffe95605aa3867fb105600842da573b1bddb5b22f0b

Observation 00eb8e31-7db4-4db6-83da-beb51f91a2a2 · outbound

This paper cites 2019, A&A, 631, A113.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters 2019, A&A, 631, A113

Reference 34

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:11.478015Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:11.478015Z digest=sha256:8b62c26520cc5fcd85ec99b8c548c0dc1ea8e5530b3319268fe8e7fd7b44302b

Observation d6cda26f-300a-4dd3-a47b-3141914faf70 · outbound

This paper cites M., & Johansen, A.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters M., & Johansen, A

Reference 35

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:11.574242Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:11.574242Z digest=sha256:f62e68c94a7e1a568b51401783c26b56fe5ef804b7184e4e360ad195795f230d

Observation 6d2284d0-765d-4221-9b0e-e4465b1f8379 · outbound

This paper cites 2019, A&A, 632, A16.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters 2019, A&A, 632, A16

Reference 36

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:11.652173Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:11.652173Z digest=sha256:e52201d95f8ab4bff725cc375d2a40211dbb851898ddd9fb65e5a1672c8de159

Observation ea6c426a-b648-4fb5-a5f3-617838b9379b · outbound

This paper cites an unresolved cited work.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters Unresolved cited work

Reference 37

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:11.740193Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:11.740193Z digest=sha256:3b22df39db9849350d2c67ed35a8724efbb75ef0af7ebfb9a7c760a461d7904e

Observation 3b851345-3957-485b-b648-c5a66975ff3b · outbound

This paper cites 1998, ApJ, 497, 388.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters 1998, ApJ, 497, 388

Reference 38

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:11.791197Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:11.791197Z digest=sha256:2dfdb24cc5f820b3462abf2ba0630368ae943d931d339c2641d6bb6cd1608717

Observation 06382d6e-6c22-4089-9f53-825ab4958202 · outbound

This paper cites M., Magg, E., Plez, B., et al.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters M., Magg, E., Plez, B., et al

Reference 39

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:11.853666Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:11.853666Z digest=sha256:895cd40f1326bed89097ad40d7bfb2a7d81bbc1aa7bfab0edae42557ac30a796

Observation 240bbe4f-ed63-4ac7-8dfb-4faab1383afa · outbound

This paper cites 2012, The Messenger, 147.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters 2012, The Messenger, 147

Reference 40

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:11.914172Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:11.914172Z digest=sha256:1c8f3cd8d589accfb6614c686b6496e0268ac95983c4b50c49976f96338ed570

Observation 88efbcf7-68ef-43d5-9bfc-6a0014d6242e · outbound

This paper cites E., Magrini, L., Schiappacasse-Ulloa, J., Randich, S., & Merle, T.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters E., Magrini, L., Schiappacasse-Ulloa, J., Randich, S., & Merle, T

Reference 41

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:11.946013Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:11.946013Z digest=sha256:8bc4d7c42f9c2de8d69ff74d294bdf576c17ce9ecba7596b34fc1dc7b79fff31

Observation b0dfbd91-0ca7-420a-8a73-e7d9fc143994 · outbound

This paper cites E., Vescovi, D., Magrini, L., et al.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters E., Vescovi, D., Magrini, L., et al

Reference 42

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:12.017025Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:12.017025Z digest=sha256:5bce3966cc9ebc8ccfa5bb0a8f4632106d470f56688a3b799b2e25853549414a

Observation fe96d6d6-093a-4ec5-a1ab-de5bed3ccfa9 · outbound

This paper cites an unresolved cited work.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters Unresolved cited work

Reference 43

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:12.109803Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:12.109803Z digest=sha256:8562d29dd8815da8b16a9da59b61feb80e56ed09dcaa38d3b4c92544540b5357

Observation 9a6c8ea1-6b1c-496c-b115-8d238ce2948d · outbound

This paper cites J., Andersen, A.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters J., Andersen, A

Reference 44

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:12.172761Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:12.172761Z digest=sha256:306ab22a796db1ba959955676d1b30dffbc216e45089185bc10df6ae237d1852

Observation f93c970d-1265-4665-a15e-29da6f6977fd · outbound

This paper cites J., Primas, F., Hartman, H., et al.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters J., Primas, F., Hartman, H., et al

Reference 45

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:12.219072Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:12.219072Z digest=sha256:3aa322b548aca6e1575c8b5ec444063ba83183f866749cd299798a0c17119421

Observation 87c6d707-4ae4-4a21-8e81-7100b0312c35 · outbound

This paper cites 2021, A&A, 645, A106.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters 2021, A&A, 645, A106

Reference 46

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:12.221919Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:12.221919Z digest=sha256:7541424225f7d45c612c9d60ec7326dd9d42ffa1942664f225a9cc3fd4aac4da

Observation 01386197-fc70-41bd-84c9-44d5aa6b09cb · outbound

This paper cites Data analysis recipes: Fitting a model to data.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters Data analysis recipes: Fitting a model to data

Reference 47

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:12.224244Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:12.224244Z digest=sha256:c63c174a330532072317c3c2e4458f0b0bf2f1191dbfd51f4d65e3cad159910b

Observation 5df7c539-32fa-450b-9af3-4f95296e41b1 · outbound

This paper cites 2007, ApJ, 666, 1189.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters 2007, ApJ, 666, 1189

Reference 48

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:12.227203Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:12.227203Z digest=sha256:c4746475a048b70d2364d1347d216021711e63f671e76ee38bd63eb65949ba97

Observation b35df849-859f-4ee1-9ceb-c4643906c98f · outbound

This paper cites an unresolved cited work.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters Unresolved cited work

Reference 49

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:12.230789Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:12.230789Z digest=sha256:a75dd6ca0e04c6000ecfd521724687b122f7bdf76ed12405f9cb6356513d9810

Observation 887ad11d-202d-4327-a629-6378f5224a3d · outbound

This paper cites 2026, MNRAS, 545, staf1797.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters 2026, MNRAS, 545, staf1797

Reference 50

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:12.233079Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:12.233079Z digest=sha256:5f9873b257b8eeb7123f4866481e22abaef18bb3244daa0825e94f37c42a48fc

Observation 07e587a9-fc51-41d6-b1b8-29d10b41b361 · outbound

This paper cites 2024, A&A, 687, A189.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters 2024, A&A, 687, A189

Reference 51

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:12.235641Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:12.235641Z digest=sha256:867a3604d5276c8a552ca00965874d08fede0876d0503042a372b345d14dd8cd

Observation 9c5471fb-402c-4140-a5bc-bc13958a14ee · outbound

This paper cites C., Dalton, G.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters C., Dalton, G

Reference 52

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:12.237838Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:12.237838Z digest=sha256:5d1a4f757b1f98f8387b8b923e13ba270fab08aaf1cae8e71c24425b833f204a

Observation 040128e5-dde8-41dc-9a17-58a843b19397 · outbound

This paper cites an unresolved cited work.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters Unresolved cited work

Reference 53

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:12.240453Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:12.240453Z digest=sha256:dc40a1c8913135492763c81a468caf05edd317d916f008737f5a4e19ff48312b

Observation dd8a4826-4575-4001-b362-fe3008a37129 · outbound

This paper cites & Ezzeddine, R.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters & Ezzeddine, R

Reference 54

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:12.242914Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:12.242914Z digest=sha256:de7a5e1fcad733d23acaf619daa78d3661db45d99202fbbe0268c02ce8c5b26f

Observation f08ac01a-ed26-4b6f-a302-d714d80f4e0e · outbound

This paper cites R., Davis, A.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters R., Davis, A

Reference 55

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:12.245359Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:12.245359Z digest=sha256:b4fc5c737c31d00fefc5c883f2fb08763092efab3cd12e313075e028c9c99f8d

Observation 42daa228-3e26-40ee-b08a-babdecb0b404 · outbound

This paper cites 2022, A&A, 661, A140.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters 2022, A&A, 661, A140

Reference 56

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:12.247886Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:12.247886Z digest=sha256:70f8750510f614e38e056150272f78599b590c12ab1f883ac07968c0f8a928c4

Observation 76b19d24-a0f2-4751-b353-52d5e65fae37 · outbound

This paper cites HRMOS: A High-Resolution Multi-Object Spectrograph for the VLT.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters HRMOS: A High-Resolution Multi-Object Spectrograph for the VLT

Reference 57

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:12.250447Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:12.250447Z digest=sha256:8c63522e3a8351294734ee9a9ecb39d5cc54cc5e45211d9100f447c2b8dc0867

Observation 3258595b-d700-4b05-bab9-d2671f6c94be · outbound

This paper cites 2018, A&A, 617, A106.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters 2018, A&A, 617, A106

Reference 58

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:12.253001Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:12.253001Z digest=sha256:b0c4d4fe4e36905d13cbf49d4ce99d02d0c67f1cc7fc437944ec9c937ddb5f61

Observation f1f02e0a-56c9-4dce-b970-5def26b7c5d1 · outbound

This paper cites 2022, Universe, 8, 64.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters 2022, Universe, 8, 64

Reference 59

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:12.255579Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:12.255579Z digest=sha256:2731661d05b281ae456194adf0974c7269efa8c555fb2d41cd221db19885b28f

Observation 1e48f373-a325-4698-af9e-fcaa13fd91e2 · outbound

This paper cites 2023, A&A, 669, A119.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters 2023, A&A, 669, A119

Reference 60

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:12.257946Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:12.257946Z digest=sha256:cb86e55f69115aa11af4d6c127564149f26a8a27e7ad8394f447681725b47a8e

Observation 8919853e-36fe-46cb-85a6-03b581ff54f9 · outbound

This paper cites R., Schiavon, R.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters R., Schiavon, R

Reference 61

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:12.260460Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:12.260460Z digest=sha256:d6b0f423713dd6f23c5809811a3bfdb7ab379c0e00b7d751fbe4a90bca05cd2b

Reference 62

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:12.263416Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:12.263416Z digest=sha256:fec6d5aa8aa03b1ed843f91640018428893b37d69fa9bb022eeadbf6365ae659

Observation 078e2813-b0c2-4404-8c18-2188f94afebf · outbound

This paper cites 2026, A&A, 705, A38.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters 2026, A&A, 705, A38

Reference 63

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:12.266208Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:12.266208Z digest=sha256:578ca68418dd74c3d61ce48dcec33ef249d385c1b5b1e5a4014dfcfe047794aa

Observation 0741ae3f-2b0d-40ab-9b36-c1852a7e75b9 · outbound

This paper cites 2015, MNRAS, 446, 3651.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters 2015, MNRAS, 446, 3651

Reference 64

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:12.268430Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:12.268430Z digest=sha256:fbb02af9a69023538ead6611450825ea0f1df4db9a77e7c4255d6aa1a770b4ca

Observation 2fde9b65-0262-479c-b5fe-ad20bf34841b · outbound

This paper cites 2019, Monthly Notices of the Royal Astronomical Society, 489.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters 2019, Monthly Notices of the Royal Astronomical Society, 489

Reference 65

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:12.271024Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:12.271024Z digest=sha256:555768f0177633b9c30f9df4edbc376208a19bff4dcd59103976aa488d4f4201

Observation 620859d4-9216-4e0b-a9d4-20e26663bc18 · outbound

This paper cites C., Cowan, J., et al.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters C., Cowan, J., et al

Reference 66

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:12.273744Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:12.273744Z digest=sha256:50b40d2629fe8f3936d128db18231f14f6fbf4033729811933e81435ad7e2368

Observation c7dc7cf7-5d03-4f81-817e-d5a8d8b8391d · outbound

This paper cites 1955, Journal of the Physical Society of Japan, 10, 919.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters 1955, Journal of the Physical Society of Japan, 10, 919

Reference 67

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:12.276143Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:12.276143Z digest=sha256:f8b3e59948b9e0bfdde1e66e1dd54df43da6efb84d11c40e61dd85bf9810bfdd

Observation 8538d9ba-1668-4a89-9bb6-df6e05b3d341 · outbound

This paper cites 2026, A&A, 708, A17.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters 2026, A&A, 708, A17

Reference 68

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:12.278759Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:12.278759Z digest=sha256:ae4da3f582cb6adfae245e1f661352973c28f1abfa6f797e81c7aa80ff1715af

Observation 80d4b948-f8ec-412b-9512-6baf0dc1c793 · outbound

This paper cites 2019, Astronomy and Astrophysics, 629.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters 2019, Astronomy and Astrophysics, 629

Reference 69

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:12.281770Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:12.281770Z digest=sha256:9f81379e60a5ff04f8376c0972504ce952dc5a7e53e7537df6c04d68a59fcb01

Observation 104c0234-4c0b-49bd-b3f7-f6e3742e212a · outbound

This paper cites C., Friel, E.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters C., Friel, E

Reference 70

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:12.284067Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:12.284067Z digest=sha256:baa76c2f724c7e65fcf140a4bc34e1d70a6004f02af084ff7c84ed23f2a7e682

Observation 34456aef-896e-4986-ae98-6c0644db5963 · outbound

This paper cites 2016, International Journal of Modern Physics E, 25, 1630003.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters 2016, International Journal of Modern Physics E, 25, 1630003

Reference 71

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:12.286378Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:12.286378Z digest=sha256:d587312df7b8e653acc42e067b4392327142a12b12e1fafb45739d842fce4a6b

Observation 89e30ef2-6cdb-4dcf-9d9b-a6366bff66c5 · outbound

This paper cites 2012, Astrophysics Source Code Library.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters 2012, Astrophysics Source Code Library

Reference 72

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:12.288853Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:12.288853Z digest=sha256:f09857be41398eb6dd2ac2a9cc63dc63d8f55f50eb4e845449c25b52b3dda730

Observation f43e540b-b0a6-4c01-82a9-6e2fcef7184c · outbound

This paper cites 2020, MNRAS, 491, 1832.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters 2020, MNRAS, 491, 1832

Reference 73

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:12.291068Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:12.291068Z digest=sha256:5e497cd71e401052ff64f53a4fd81fa02012b56f510489436b6a5999b4e18763

Observation af401170-aac9-45d9-bf6f-682ebac492f5 · outbound

This paper cites 2024, ApJ, 966, 11.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters 2024, ApJ, 966, 11

Reference 74

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:12.293563Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:12.293563Z digest=sha256:d04f94deba7e795f4766b147632288ba366c9eaa18c2f022a3dd62361c90b12a

Observation ff2d849c-2f26-4a43-a78a-23afcc22c106 · outbound

This paper cites 2022, A&A, 666, A121.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters 2022, A&A, 666, A121

Reference 75

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:12.295957Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:12.295957Z digest=sha256:b22097c46fe2846dab6171d002546a4d9cbcdee948a8896a5bda3fa2d16e536e

Observation b624636b-4fbe-4a4c-a1ac-79571868fe88 · outbound

This paper cites 2013, Reports on Progress in Physics, 76, 066201.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters 2013, Reports on Progress in Physics, 76, 066201

Reference 76

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:12.298329Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:12.298329Z digest=sha256:6040a823378719b904cdb83b04d320c8381ff14f1439ab4b7382055e333ca63f

Observation bcf8be17-fadb-494a-88e7-625e916af1f4 · outbound

This paper cites Á., & Arcones, A.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters Á., & Arcones, A

Reference 77

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:12.300800Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:12.300800Z digest=sha256:77887cd7e9035a8450a29f0f3e8d0989354b3fe003e01577da9e6de25bc38937

Observation 8ceec17f-8df0-4016-9c68-d5e946aa9ab9 · outbound

This paper cites P., Lugaro, M., Pereira, C.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters P., Lugaro, M., Pereira, C

Reference 78

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:12.303200Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:12.303200Z digest=sha256:928f54a71d823c4f18f2a56dcee6101cb639e3e732eab22d37b87fc67cea8f0f

Observation 42adc75b-9b04-41da-9b20-659c7cc36ddf · outbound

This paper cites V ., Daflon, S., Cunha, K., et al.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters V ., Daflon, S., Cunha, K., et al

Reference 79

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:12.305589Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:12.305589Z digest=sha256:1ea9319367a62c12a8d591b66c549002f2eacd3577287217813f2ce362867559

Observation 65140f02-9794-4f1e-ab2b-0aabfc48a41b · outbound

This paper cites J., & Gallino, R.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters J., & Gallino, R

Reference 80

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:12.308157Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:12.308157Z digest=sha256:dcd27ddced038e6dec9c055e48d7c8bb3c6efcf2be221db36d4df830da07e39b

Observation 940fb22d-0e36-4261-a39e-b85d27f73bf5 · outbound

This paper cites J., Lawler, J.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters J., Lawler, J

Reference 81

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:12.312490Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:12.312490Z digest=sha256:1efeea4e797c9d39074f2d188785279b77511db937b268fa61738b6f57c4bddb

Observation 8cc80d08-f89f-4d1f-bc81-66eb751fda44 · outbound

This paper cites 2022, Universe, 8.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters 2022, Universe, 8

Reference 82

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:12.315300Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:12.315300Z digest=sha256:ecc79fa238aa5fa893ce6616ad58ec0e86cb7394c76d3aaad108088a1034b879

Observation b5f40ecc-340a-4900-8098-8398a76b832e · outbound

This paper cites M., et al.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters M., et al

Reference 83

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:12.318267Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:12.318267Z digest=sha256:1d7b8764694c93302b09743c5e247cbf0a438ccf530e089e0847800d2131b6a2

Observation 0b9b80c8-cdc9-47b1-8949-05545b59c3bd · outbound

This paper cites 2018, A&A, 611, A30.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters 2018, A&A, 611, A30

Reference 84

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:12.320720Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:12.320720Z digest=sha256:0f7171a4d73e1af08539f58ade6f59432af69b1757628b7cedb0ed90c209e9a8

Observation 6ba14bfb-9f6e-4ec6-8b00-6e4a516b35a5 · outbound

This paper cites & Bergemann, M.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters & Bergemann, M

Reference 85

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:12.325484Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:12.325484Z digest=sha256:809ce8fb9da91c909a986789142130e8c5347ae16ad1178e2e4314f586d12ba3

Observation ad953950-fb03-4923-b5b2-e9266b37b58f · outbound

This paper cites 2021, A&A, 647, A19.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters 2021, A&A, 647, A19

Reference 86

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:12.328859Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:12.328859Z digest=sha256:92bee23989813f3e7e4ca449949fc538f052e519e355b984562b022d3aa8fba1

Observation a3f04ba5-267b-4739-b04d-903ebdd403cf · outbound

This paper cites an unresolved cited work.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters Unresolved cited work

Reference 87

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:12.333829Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:12.333829Z digest=sha256:6119690bc474513a7dbb04e8b33e5bb32adf8b5f74942dd0474b110bc3871516

Observation d4c71be3-1de6-40f2-b06b-1537baa869ff · outbound

This paper cites 2004, ApJ, 601, 864 van der Plas, G., van den Ancker, M.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters 2004, ApJ, 601, 864 van der Plas, G., van den Ancker, M

Reference 88

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:12.337256Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:12.337256Z digest=sha256:038cbe6f697e5220c9638ac66991c3517ab5ea90919ae2b3538f7e547213f5eb

Observation 5be0ed0a-f8d7-4755-b591-309f403b236e · outbound

This paper cites B., Mashonkina, L.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters B., Mashonkina, L

Reference 89

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:12.340729Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:12.340729Z digest=sha256:de89819720e489a31bd49ac821365f1683ac9e19ebdca77c4a395512e0345587

Observation b78008b5-4f33-45c6-b5f3-facb71ba4700 · outbound

This paper cites 2011, ApJ, 726, L15.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters 2011, ApJ, 726, L15

Reference 90

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:12.345402Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:12.345402Z digest=sha256:c9ec2e4e32387b1ee1a4af01b2315bc82f956438246ba93da384fbfaf5a5522a

Observation 8f162ff9-10f6-4399-8c27-28fb21091c9e · outbound

This paper cites & Brault, J.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters & Brault, J

Reference 91

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:12.349257Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:12.349257Z digest=sha256:c05947c0cc604135bdbceee6d06014c8c3a90849aec19e48abc7cdd3092d985d

Observation 944b6037-3c8b-48b4-be48-88bca397c0db · outbound

This paper cites E., Salih, S., & Lawler, J.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters E., Salih, S., & Lawler, J

Reference 92

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:12.351566Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:12.351566Z digest=sha256:06941de8f2b5f957bbafc1a4a7fb972902e86817bcfb021ffa64c97f53dec54b

Observation 766d1bd1-8161-4f24-b313-064046fc5e07 · outbound

This paper cites 2022, Astronomy and Astrophysics, 667 Article number, page 13 A&A proofs:manuscript no.

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters 2022, Astronomy and Astrophysics, 667 Article number, page 13 A&A proofs:manuscript no

Reference 93

Resolution
unresolved
no resolver link, observed 2026-08-01T00:09:12.353801Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:09:12.353801Z digest=sha256:21aec6fe7b44d00f489219d9c30dac1434342c3280190fd74053b86beb3c6c55

Pith citing papers

No inbound Pith citation observations are available.