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Paper Citation Record · LEDGER

Something new under the Sun: A magnetically driven CH/CN anti-correlation

As of 7 August 2026, this Paper Citation Record lists 100 of 298 outbound references and 0 inbound Pith citation observations for arXiv:2608.02721.

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

pith.paper-citation-record.v1
2608.02721 v1

Coverage vector

measured 100 of 298 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-07T00:15:39.572422Z

measured 100 of 100 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-07T06:34:17.273281+00:00

measured 0 of 0 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links

measured 0 of 1 external citation measurements

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

Source: cited_works

Reference resolution

100 of 298 outbound references displayed

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  • verified fuzzy0
  • unresolved85
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External citation measurements

No source-named external measurement is stored.

Outbound references

Observation 08bd6a0d-7bee-4652-99db-944c11438cf8 · outbound

This paper cites an unresolved cited work.

Something new under the Sun: A magnetically driven CH/CN anti-correlation Unresolved cited work

Reference 1

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Unavailable: canonical work link unavailable.

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Observation 4a33b2e5-e94e-4c88-a986-129b3150a6fc · outbound

This paper cites Expanding the time domain of multiple populations: evidences of nitrogen variations in the ~1.5 Gyr old star cluster NGC 1783.

Something new under the Sun: A magnetically driven CH/CN anti-correlation Expanding the time domain of multiple populations: evidences of nitrogen variations in the ~1.5 Gyr old star cluster NGC 1783

Reference 2

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Observation dbbba9e1-7a9b-4be9-9b15-78c36bcb7302 · outbound

This paper cites Relative Frequencies of Blue Stragglers in Galactic Globular Clusters: Constraints for the Formation Mechanisms.

Something new under the Sun: A magnetically driven CH/CN anti-correlation Relative Frequencies of Blue Stragglers in Galactic Globular Clusters: Constraints for the Formation Mechanisms

Reference 3

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Observation 3c77b09b-6bfa-432b-b265-0ea7cf628944 · outbound

This paper cites The Gaia-ESO Survey: No sign of multiple stellar populations in open clusters from their sodium and oxygen abundances.

Something new under the Sun: A magnetically driven CH/CN anti-correlation The Gaia-ESO Survey: No sign of multiple stellar populations in open clusters from their sodium and oxygen abundances

Reference 4

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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 9647343b-25fa-4023-9e0d-91d317b48d2d · outbound

This paper cites Globular cluster chemistry in fast rotating dwarf stars belonging to intermediate age open clusters.

Something new under the Sun: A magnetically driven CH/CN anti-correlation Globular cluster chemistry in fast rotating dwarf stars belonging to intermediate age open clusters

Reference 5

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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T00:15:36.475800Z digest=sha256:8c52461c5f6e3a6dafe4dff99a045ac76a31890bb8c92b21df7099f25745c201

Observation 7e327bf6-a072-4dc1-b03e-d4d36c91f4a9 · outbound

This paper cites Leveraging HST with MUSE: I. Sodium abundance variations within the 2 Gyr-old cluster NGC 1978.

Something new under the Sun: A magnetically driven CH/CN anti-correlation Leveraging HST with MUSE: I. Sodium abundance variations within the 2 Gyr-old cluster NGC 1978

Reference 6

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Observation b6c000f4-dc9a-4f00-b892-4029cbf9c8dc · outbound

This paper cites On the Nitrogen variation in ~2 Gyr old massive star clusters in the Large Magellanic Cloud.

Something new under the Sun: A magnetically driven CH/CN anti-correlation On the Nitrogen variation in ~2 Gyr old massive star clusters in the Large Magellanic Cloud

Reference 7

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no resolver link, observed 2026-08-07T00:15:36.767817Z

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Unavailable: canonical work link unavailable.

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Observation 4c68a92d-eed0-4c76-95df-eed4b5780c6b · outbound

This paper cites Age as a Major Factor in the Onset of Multiple Populations in Stellar Clusters.

Something new under the Sun: A magnetically driven CH/CN anti-correlation Age as a Major Factor in the Onset of Multiple Populations in Stellar Clusters

Reference 8

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no resolver link, observed 2026-08-07T00:15:36.927888Z

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Observation bc64a4c5-937f-40bf-a438-33079d9432e0 · outbound

This paper cites Annual Review of Astronomy and Astrophysics , year =.

Something new under the Sun: A magnetically driven CH/CN anti-correlation Annual Review of Astronomy and Astrophysics , year =

Reference 9

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Observation e1a267fd-c4cc-44be-9fa9-b79af868fa31 · outbound

This paper cites , keywords =.

Something new under the Sun: A magnetically driven CH/CN anti-correlation , keywords =

Reference 10

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Observation 4fb77122-aef5-402d-9f03-32ddaa9547fa · outbound

This paper cites Dynamical Formation of Close Binary Systems in Globular Clusters.

Something new under the Sun: A magnetically driven CH/CN anti-correlation Dynamical Formation of Close Binary Systems in Globular Clusters

Reference 11

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Observation 6dbe4e59-dd1b-4594-9ed8-3679365063cf · outbound

This paper cites A Deep Chandra Survey of the Globular Cluster 47 Tucanae: Catalog of Point Sources.

Something new under the Sun: A magnetically driven CH/CN anti-correlation A Deep Chandra Survey of the Globular Cluster 47 Tucanae: Catalog of Point Sources

Reference 12

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no resolver link, observed 2026-08-07T00:15:37.490630Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 59ab3720-2e21-4e03-84ba-f9de592313f6 · outbound

This paper cites X-ray Sources in Galactic Globular Clusters.

Something new under the Sun: A magnetically driven CH/CN anti-correlation X-ray Sources in Galactic Globular Clusters

Reference 13

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Unavailable: canonical work link unavailable.

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Observation f472afbe-b25d-49fe-9be8-cd90ca140a41 · outbound

This paper cites 2012 , publisher=.

Something new under the Sun: A magnetically driven CH/CN anti-correlation 2012 , publisher=

Reference 14

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Observation 7dac9209-3ca1-49cf-8ccf-ac0fc5b8c1fe · outbound

This paper cites Living Reviews in Solar Physics , volume=.

Something new under the Sun: A magnetically driven CH/CN anti-correlation Living Reviews in Solar Physics , volume=

Reference 15

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Unavailable: canonical work link unavailable.

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Observation eebc3fd2-37d5-457e-a676-7c63d36a28e3 · outbound

This paper cites Living Reviews in Solar Physics , volume=.

Something new under the Sun: A magnetically driven CH/CN anti-correlation Living Reviews in Solar Physics , volume=

Reference 16

Resolution
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Observation 0c3c2d51-7135-42ec-b6ae-325e50601367 · outbound

This paper cites Ap stars with resolved magnetically split lines: Magnetic field determinations from Stokes $I$ and $V$ spectra.

Something new under the Sun: A magnetically driven CH/CN anti-correlation Ap stars with resolved magnetically split lines: Magnetic field determinations from Stokes $I$ and $V$ spectra

Reference 17

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Observation 935eb2ac-3b98-408c-898f-bae715d455bb · outbound

This paper cites The incidence of magnetism in blue and yellow straggler stars.

Something new under the Sun: A magnetically driven CH/CN anti-correlation The incidence of magnetism in blue and yellow straggler stars

Reference 18

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no resolver link, observed 2026-08-07T00:15:38.276865Z

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Observation 46c2e865-bb98-4fc8-b0f5-ec48d3691b8b · outbound

This paper cites Two distinct sequences of blue straggler stars in the globular cluster M30.

Something new under the Sun: A magnetically driven CH/CN anti-correlation Two distinct sequences of blue straggler stars in the globular cluster M30

Reference 19

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Observation a7a7e73f-5539-49b2-b815-8a51ec34f4f1 · outbound

This paper cites A Survey of Stellar Families: Multiplicity of Solar-Type Stars.

Something new under the Sun: A magnetically driven CH/CN anti-correlation A Survey of Stellar Families: Multiplicity of Solar-Type Stars

Reference 20

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no resolver link, observed 2026-08-07T00:15:38.567662Z

Source-reported events for the cited work

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Observation 97f19bde-8afe-4a16-ae1c-41d4eb6e8cc4 · outbound

This paper cites How mergers magnetise massive stars.

Something new under the Sun: A magnetically driven CH/CN anti-correlation How mergers magnetise massive stars

Reference 21

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Observation 529618fa-861d-41a5-bba7-bee1f8ac01af · outbound

This paper cites A catalogue of masses, structural parameters and velocity dispersion profiles of 112 Milky Way globular clusters.

Something new under the Sun: A magnetically driven CH/CN anti-correlation A catalogue of masses, structural parameters and velocity dispersion profiles of 112 Milky Way globular clusters

Reference 22

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Observation ee91a9f5-c709-4cea-b58c-caed360754d9 · outbound

This paper cites Binary properties of the globular cluster 47 Tuc (NGC 104). A dearth of short-period binaries.

Something new under the Sun: A magnetically driven CH/CN anti-correlation Binary properties of the globular cluster 47 Tuc (NGC 104). A dearth of short-period binaries

Reference 23

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Observation f475b469-05b9-4c96-a7e5-f1b3790f3b5d · outbound

This paper cites , keywords =.

Something new under the Sun: A magnetically driven CH/CN anti-correlation , keywords =

Reference 24

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Observation 60777d34-321a-4258-b455-7e323cc4e7b3 · outbound

This paper cites , title = ".

Something new under the Sun: A magnetically driven CH/CN anti-correlation , title = "

Reference 25

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Source-reported events for the cited work

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Observation 37cbcb46-25a3-46fc-8ff2-b5bdb06c7e21 · outbound

This paper cites $^{22}$Ne and $^{23}$Na ejecta from intermediate-mass stars: The impact of the new LUNA rate for $^{22}$Ne(p,$\gamma$)$^{23}$Na.

Something new under the Sun: A magnetically driven CH/CN anti-correlation $^{22}$Ne and $^{23}$Na ejecta from intermediate-mass stars: The impact of the new LUNA rate for $^{22}$Ne(p,$\gamma$)$^{23}$Na

Reference 26

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Observation bf5604d6-1aa7-4467-8ccf-0a2c3af1cf42 · outbound

This paper cites At least one in a dozen stars exhibits evidence of planetary ingestion.

Something new under the Sun: A magnetically driven CH/CN anti-correlation At least one in a dozen stars exhibits evidence of planetary ingestion

Reference 27

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Observation 16d49efc-b2e7-4017-91f4-a2bfa4afdded · outbound

This paper cites The peculiar composition of the Sun is not related to giant planets.

Something new under the Sun: A magnetically driven CH/CN anti-correlation The peculiar composition of the Sun is not related to giant planets

Reference 28

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Unavailable: canonical work link unavailable.

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Observation ea898dd3-d5ca-477e-8b52-159b68d08670 · outbound

This paper cites , keywords =.

Something new under the Sun: A magnetically driven CH/CN anti-correlation , keywords =

Reference 29

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verified exact
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

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Observation b7a8b815-5683-4727-9931-dec3d4d200e2 · outbound

This paper cites Improving Our Knowledge of the Solar Near-Surface Shear Layer: The Special Case of the Leptocline.

Something new under the Sun: A magnetically driven CH/CN anti-correlation Improving Our Knowledge of the Solar Near-Surface Shear Layer: The Special Case of the Leptocline

Reference 30

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metadata mismatch
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

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Observation 97e906db-1ad3-4aa2-807d-d6fcfa710b89 · outbound

This paper cites Changes in the subsurface stratification of the Sun with the 11-year activity cycle.

Something new under the Sun: A magnetically driven CH/CN anti-correlation Changes in the subsurface stratification of the Sun with the 11-year activity cycle

Reference 31

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Observation 2a552aef-9dac-4c98-9749-7b4c84e3a0a0 · outbound

This paper cites , keywords =.

Something new under the Sun: A magnetically driven CH/CN anti-correlation , keywords =

Reference 32

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verified exact
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

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Observation 3f9975f6-2aa5-46c6-ace3-6fe6b5244daf · outbound

This paper cites First Calculations of Starspot Spectra based on 3D Radiative Magnetohydrodynamics Simulations.

Something new under the Sun: A magnetically driven CH/CN anti-correlation First Calculations of Starspot Spectra based on 3D Radiative Magnetohydrodynamics Simulations

Reference 33

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Observation 5ba89697-67a0-44e8-a23b-d60f789bb4a6 · outbound

This paper cites Are solar brightness variations faculae- or spot-dominated?.

Something new under the Sun: A magnetically driven CH/CN anti-correlation Are solar brightness variations faculae- or spot-dominated?

Reference 34

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Observation 41345e8c-253d-4740-b80b-d39e574703ae · outbound

This paper cites an unresolved cited work.

Something new under the Sun: A magnetically driven CH/CN anti-correlation Unresolved cited work

Reference 35

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Observation cfe7df29-2e0e-4670-acb7-55fb06a2e4d5 · outbound

This paper cites Living Reviews in Solar Physics , keywords =.

Something new under the Sun: A magnetically driven CH/CN anti-correlation Living Reviews in Solar Physics , keywords =

Reference 36

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Observation d5cde75e-a52c-4409-8a45-ba1218090546 · outbound

This paper cites , keywords =.

Something new under the Sun: A magnetically driven CH/CN anti-correlation , keywords =

Reference 37

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unresolved
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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T00:15:39.012050Z digest=sha256:ee24ae2bb9e25ebc035166ce22ac99b1d86782c729aed88b0eb372284e4fd33d

Observation 5e0637ba-03ea-4410-bdd9-8b5039cbd0dc · outbound

This paper cites , year = 2016, volume =.

Something new under the Sun: A magnetically driven CH/CN anti-correlation , year = 2016, volume =

Reference 38

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no resolver link, observed 2026-08-07T00:15:39.021270Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T00:15:39.021270Z digest=sha256:2691a85b3635a3643b47e7e0f7e9aaaabff67a6626489ffdb8e06bf0d02f1b8b

Observation ffd27eb4-0f24-4948-b480-987099a551a5 · outbound

This paper cites , year = 2014, volume =.

Something new under the Sun: A magnetically driven CH/CN anti-correlation , year = 2014, volume =

Reference 39

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unresolved
no resolver link, observed 2026-08-07T00:15:39.032043Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T00:15:39.032043Z digest=sha256:607447eee7ce012fb23fae776691a863c4828d7f62b47f350687034ad0163c5b

Observation c2b07af8-de63-4789-957a-440fb2d09ea4 · outbound

This paper cites , year = 2022, volume =.

Something new under the Sun: A magnetically driven CH/CN anti-correlation , year = 2022, volume =

Reference 40

Resolution
unresolved
no resolver link, observed 2026-08-07T00:15:39.047949Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T00:15:39.047949Z digest=sha256:3160c537430eafdc5538b3cd427ff7dbd771b409cc6d4206076738679573e824

Observation b24fdf86-27b9-4de8-bbe4-adf1f8c85cfb · outbound

This paper cites Effect of spots and plages on radial velocity measurements.

Something new under the Sun: A magnetically driven CH/CN anti-correlation Effect of spots and plages on radial velocity measurements

Reference 41

Resolution
unresolved
no resolver link, observed 2026-08-07T00:15:39.056215Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T00:15:39.056215Z digest=sha256:c76224cf70bef9963b3e58d95934aeac08a582bfcb1ce2c3e1cb553fe7cb46e3

Observation 5b77b713-e9c3-40d5-94b4-cd1fec55c6ea · outbound

This paper cites , year = 2019, volume =.

Something new under the Sun: A magnetically driven CH/CN anti-correlation , year = 2019, volume =

Reference 42

Resolution
unresolved
no resolver link, observed 2026-08-07T00:15:39.062761Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T00:15:39.062761Z digest=sha256:71edddee17daeec9fe35d7d94aa23b8cead93daf7d9e4a452c78d17d4a0de095

Observation 686955c0-a2fa-4855-9df1-0aa2c43d9e4b · outbound

This paper cites , year = 2019, volume =.

Something new under the Sun: A magnetically driven CH/CN anti-correlation , year = 2019, volume =

Reference 43

Resolution
unresolved
no resolver link, observed 2026-08-07T00:15:39.091510Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T00:15:39.091510Z digest=sha256:f5c171361ed79b6ed26317ab0b541138ffa51dda941411bb14acdea8b3bef030

Observation f475e640-a691-44a1-a9c9-e14fa0fc554e · outbound

This paper cites , year = 2020, volume =.

Something new under the Sun: A magnetically driven CH/CN anti-correlation , year = 2020, volume =

Reference 44

Resolution
unresolved
no resolver link, observed 2026-08-07T00:15:39.108245Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T00:15:39.108245Z digest=sha256:4285ead0cdc158277e7866e1556e7addd704add204e83dd43454f745ab9c0fa4

Observation 4ba16563-3c56-4107-9040-1b6825853c38 · outbound

This paper cites an unresolved cited work.

Something new under the Sun: A magnetically driven CH/CN anti-correlation Unresolved cited work

Reference 45

Resolution
unresolved
no resolver link, observed 2026-08-07T00:15:39.113346Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T00:15:39.113346Z digest=sha256:4ed5ff5e17c067a667c157284fb369d9b85d456afc90470327aac37a683399b7

Observation 4112da49-b67e-4824-b319-c716f7ed466d · outbound

This paper cites , year = 2022, volume =.

Something new under the Sun: A magnetically driven CH/CN anti-correlation , year = 2022, volume =

Reference 46

Resolution
unresolved
no resolver link, observed 2026-08-07T00:15:39.125928Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T00:15:39.125928Z digest=sha256:a1c80a7681606a1eda671b95ec95ce99670436259fdd4e1345029bb4560a7a4a

Observation 9b3af2d3-9058-4533-887a-ba6b654053c0 · outbound

This paper cites The Hubble Space Telescope UV Legacy Survey of Galactic Globular Clusters. III. A quintuple stellar population in NGC2808.

Something new under the Sun: A magnetically driven CH/CN anti-correlation The Hubble Space Telescope UV Legacy Survey of Galactic Globular Clusters. III. A quintuple stellar population in NGC2808

Reference 47

Resolution
unresolved
no resolver link, observed 2026-08-07T00:15:39.132899Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T00:15:39.132899Z digest=sha256:7289ea47762c6858400b4dfe41a4e0183c564cefeb76577a761b171b196bd2eb

Observation 2fcbb8c6-7694-482a-9f59-3576938d0068 · outbound

This paper cites Lessons learned from the Milky Way globular clusters.

Something new under the Sun: A magnetically driven CH/CN anti-correlation Lessons learned from the Milky Way globular clusters

Reference 48

Resolution
unresolved
no resolver link, observed 2026-08-07T00:15:39.143342Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T00:15:39.143342Z digest=sha256:8630cbb56a2206f37b6e0508b80e75dad5a56eb5a04f0224c9c974ed921ccb60

Observation eef4a921-1d5b-4022-8fb6-234116d91ae2 · outbound

This paper cites Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet.

Something new under the Sun: A magnetically driven CH/CN anti-correlation Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet

Reference 49

Resolution
unresolved
no resolver link, observed 2026-08-07T00:15:39.150193Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T00:15:39.150193Z digest=sha256:7b38de044a1dad0808cecd51ed6e3c67c75b9b93d498e5e58e559f04388e0509

Observation 1d009b60-543f-4fc3-bad3-ac5e9121cbfe · outbound

This paper cites The Atlas of multiple stellar populations.

Something new under the Sun: A magnetically driven CH/CN anti-correlation The Atlas of multiple stellar populations

Reference 50

Resolution
unresolved
no resolver link, observed 2026-08-07T00:15:39.155429Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T00:15:39.155429Z digest=sha256:ab1abbb417742bcdd82eae08987dda9e70738d70753fdf8398520c91a6f77970

Observation b9122711-25af-426c-9c3d-8d7eb13940d6 · outbound

This paper cites , year = 2018, volume =.

Something new under the Sun: A magnetically driven CH/CN anti-correlation , year = 2018, volume =

Reference 51

Resolution
unresolved
no resolver link, observed 2026-08-07T00:15:39.167664Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T00:15:39.167664Z digest=sha256:a6106f48cf143a003f630c79005421bd9f92c6261a094b6fcfe9797f97cfb747

Observation 82b57a46-4418-4374-89d9-d64bb391352e · outbound

This paper cites , year = 2020, volume =.

Something new under the Sun: A magnetically driven CH/CN anti-correlation , year = 2020, volume =

Reference 52

Resolution
unresolved
no resolver link, observed 2026-08-07T00:15:39.172600Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T00:15:39.172600Z digest=sha256:9cf95f3837472629b204bdae430e64f68062078c025dadd9011096af650ceb3f

Observation 0d6c8dbd-7cb4-4e11-9336-d99f9ed8e5de · outbound

This paper cites Modern Technologies in Space- and Ground-based Telescopes and Instrumentation II , year = 2012, editor =.

Something new under the Sun: A magnetically driven CH/CN anti-correlation Modern Technologies in Space- and Ground-based Telescopes and Instrumentation II , year = 2012, editor =

Reference 53

Resolution
unresolved
no resolver link, observed 2026-08-07T00:15:39.177749Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T00:15:39.177749Z digest=sha256:8a18b726881da6e8f23b68b54c2ff7f9328f68ce42cfb3de4c3f79775a7a8abf

Observation 8a50a9ac-7df0-4b12-a231-481336ab6d0f · outbound

This paper cites C and N abundances in globular clusters. I. The case of 47 Tuc and the effect of the first dredge-up.

Something new under the Sun: A magnetically driven CH/CN anti-correlation C and N abundances in globular clusters. I. The case of 47 Tuc and the effect of the first dredge-up

Reference 54

Resolution
unresolved
no resolver link, observed 2026-08-07T00:15:39.182754Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T00:15:39.182754Z digest=sha256:e3517388b121f232d1db11a5d911b7fd88a109f5373d4eca7625a90cc554aac2

Observation 2b234ed8-5574-42b4-ad46-35f56f2f5f59 · outbound

This paper cites The globular cluster M10: Reassessment of stellar membership, distance and age using its variable and HB stars.

Something new under the Sun: A magnetically driven CH/CN anti-correlation The globular cluster M10: Reassessment of stellar membership, distance and age using its variable and HB stars

Reference 55

Resolution
unresolved
no resolver link, observed 2026-08-07T00:15:39.191150Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T00:15:39.191150Z digest=sha256:a08e7070cfaf039b716973b7edde35507ec82c71a4779f1a3003ef0696c684c9

Observation cf7f997e-9326-489d-b0ed-3602c2128cf5 · outbound

This paper cites To Grow Old and Peculiar: A Survey of Anomalous Variable Stars in M80 and Age Determination using K2 and Gaia.

Something new under the Sun: A magnetically driven CH/CN anti-correlation To Grow Old and Peculiar: A Survey of Anomalous Variable Stars in M80 and Age Determination using K2 and Gaia

Reference 56

Resolution
unresolved
no resolver link, observed 2026-08-07T00:15:39.196242Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T00:15:39.196242Z digest=sha256:7fe925fe7802473833a1c7646eb4d565b355e5ad6870e37795ff6add3ff400d3

Observation 0522c0cf-0b05-4dac-b009-e9ff8f5d8652 · outbound

This paper cites Discovery of three magnetic helium-rich hot subdwarfs with SALT.

Something new under the Sun: A magnetically driven CH/CN anti-correlation Discovery of three magnetic helium-rich hot subdwarfs with SALT

Reference 57

Resolution
metadata mismatch
local_arxiv, observed 2026-08-07T00:15:47.526922Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=arxiv_source observed=2026-08-07T00:15:39.201210Z digest=sha256:8c2487224f48bfde1cc5586ed0aede26ec50a90bba98c07cf8ad7214c5a999f9

Observation c7894a88-6ddc-4394-8731-7c55e548c24e · outbound

This paper cites 2024 , eprint=.

Something new under the Sun: A magnetically driven CH/CN anti-correlation 2024 , eprint=

Reference 58

Resolution
unresolved
no resolver link, observed 2026-08-07T00:15:39.206546Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T00:15:39.206546Z digest=sha256:3103ebc42afd5dcc4629e96127d69bc05b5f5fa982f8d996e636a8fa81009952

Observation fc3a74ec-b5cf-4c3f-a515-41e1a6303fc6 · outbound

This paper cites MPS-ATLAS library of stellar model atmospheres and spectra.

Something new under the Sun: A magnetically driven CH/CN anti-correlation MPS-ATLAS library of stellar model atmospheres and spectra

Reference 59

Resolution
unresolved
no resolver link, observed 2026-08-07T00:15:39.211030Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T00:15:39.211030Z digest=sha256:05bceec76d04c3633663ce1e24d4f0304473ad5158778e3ca08b2ada9d6217dc

Observation 300e6d69-8298-4130-a6f0-3c4ec6430270 · outbound

This paper cites Stellar limb darkening. A new MPS-ATLAS library for Kepler, TESS, CHEOPS, and PLATO passbands.

Something new under the Sun: A magnetically driven CH/CN anti-correlation Stellar limb darkening. A new MPS-ATLAS library for Kepler, TESS, CHEOPS, and PLATO passbands

Reference 60

Resolution
unresolved
no resolver link, observed 2026-08-07T00:15:39.216073Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T00:15:39.216073Z digest=sha256:4bdc8bcbeaa0643c344fa85b5a13ccb0c5f323ea60fb71f6cb4b035ef18baf52

Observation 309f1383-8b60-4b1e-80e8-7ff714677a6a · outbound

This paper cites Testing MURaM and MPS-ATLAS against the quiet solar spectrum.

Something new under the Sun: A magnetically driven CH/CN anti-correlation Testing MURaM and MPS-ATLAS against the quiet solar spectrum

Reference 61

Resolution
unresolved
no resolver link, observed 2026-08-07T00:15:39.221281Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T00:15:39.221281Z digest=sha256:9aac63c4f10aee206f73593098ef7b8f6e77ec0d4e0e0beb6a8e525549461b38

Observation d821c807-7cc9-4c53-8487-b3c64716d468 · outbound

This paper cites MPS-ATLAS: A fast all-in-one code for synthesising stellar spectra.

Something new under the Sun: A magnetically driven CH/CN anti-correlation MPS-ATLAS: A fast all-in-one code for synthesising stellar spectra

Reference 62

Resolution
unresolved
no resolver link, observed 2026-08-07T00:15:39.226136Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T00:15:39.226136Z digest=sha256:0f402af346d24980312e098419fed3e19bd340245933695fc7eb67908cf37804

Observation df4086fc-3892-4971-8836-f7526b582d0a · outbound

This paper cites Small-scale dynamo in cool main sequence stars. II. The effect of metallicity.

Something new under the Sun: A magnetically driven CH/CN anti-correlation Small-scale dynamo in cool main sequence stars. II. The effect of metallicity

Reference 63

Resolution
unresolved
no resolver link, observed 2026-08-07T00:15:39.230960Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T00:15:39.230960Z digest=sha256:7edccaf2532a5147bde21350f385f3f9fb188949026441da5bd7b030d3c36f1d

Observation eb2a8a3c-24e3-4c93-b21c-1cc955f04db8 · outbound

This paper cites Equations, methods, and results of the MURaM code.

Something new under the Sun: A magnetically driven CH/CN anti-correlation Equations, methods, and results of the MURaM code

Reference 64

Resolution
unresolved
no resolver link, observed 2026-08-07T00:15:39.235895Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T00:15:39.235895Z digest=sha256:36bcdbf85a92d23e15c567aed80c2707f68238d8b84943798c7fc9d9ac968a6e

Observation df5e23fd-68d3-4e53-8b30-88ba25e3ce83 · outbound

This paper cites Reconstruction of total and spectral solar irradiance from 1974 to 2013 based on KPVT, SoHO/MDI and SDO/HMI observations.

Something new under the Sun: A magnetically driven CH/CN anti-correlation Reconstruction of total and spectral solar irradiance from 1974 to 2013 based on KPVT, SoHO/MDI and SDO/HMI observations

Reference 65

Resolution
unresolved
no resolver link, observed 2026-08-07T00:15:39.241932Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T00:15:39.241932Z digest=sha256:96d5bbaad77752cbb9daf2605d36c52e3362c7249f336783b5cd62d6100e4ec3

Observation 5c50521f-43d1-494f-8964-e5a1453a8346 · outbound

This paper cites A roadmap for the atmospheric characterization of terrestrial exoplanets with JWST.

Something new under the Sun: A magnetically driven CH/CN anti-correlation A roadmap for the atmospheric characterization of terrestrial exoplanets with JWST

Reference 66

Resolution
unresolved
no resolver link, observed 2026-08-07T00:15:39.246745Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T00:15:39.246745Z digest=sha256:6b69b12cacef29710dff7aafaf50f54c90463425ab03640a8476698f3dfa021b

Observation 651f120d-c62c-4337-b38a-70792ac5f7dc · outbound

This paper cites The Blue Straggler Population in Dwarf Galaxies.

Something new under the Sun: A magnetically driven CH/CN anti-correlation The Blue Straggler Population in Dwarf Galaxies

Reference 67

Resolution
unresolved
no resolver link, observed 2026-08-07T00:15:39.251687Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T00:15:39.251687Z digest=sha256:656382ca71b5f115057579fc33924cd1817ccf0690e6f209f8e3b5085a547eb6

Observation 4fc3e72a-0fd9-47df-a426-e93e28b3b191 · outbound

This paper cites Solar internetwork magnetic fields: Statistical comparison between observations and MHD simulations.

Something new under the Sun: A magnetically driven CH/CN anti-correlation Solar internetwork magnetic fields: Statistical comparison between observations and MHD simulations

Reference 68

Resolution
metadata mismatch
local_arxiv, observed 2026-08-07T00:15:47.481069Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=arxiv_source observed=2026-08-07T00:15:39.257182Z digest=sha256:7ae1b1ff559e681b16630a34bbc27e07007e76ba2091605fbc7f257dc7e3b640

Observation 9bdad221-8a54-42d1-b528-33e0eb53d392 · outbound

This paper cites Magnetic Field Amplification during Stellar Collisions between Low-Mass Stars.

Something new under the Sun: A magnetically driven CH/CN anti-correlation Magnetic Field Amplification during Stellar Collisions between Low-Mass Stars

Reference 69

Resolution
unresolved
no resolver link, observed 2026-08-07T00:15:39.262025Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T00:15:39.262025Z digest=sha256:74cd2af01ae874b7e99b09e4fbeb46d614f0a2cca1dde9a109b8c8026a03810f

Observation b7402eb0-8655-498f-9eaa-1d746d5ee051 · outbound

This paper cites Blue Stragglers After the Main Sequence.

Something new under the Sun: A magnetically driven CH/CN anti-correlation Blue Stragglers After the Main Sequence

Reference 70

Resolution
unresolved
no resolver link, observed 2026-08-07T00:15:39.266851Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T00:15:39.266851Z digest=sha256:adaaa39276e7954c279e6ab7476d683aac2cda17399e7fe608c25ef82018d71c

Observation 7a387641-4272-4d89-87b1-93859e3149eb · outbound

This paper cites , year = 1976, month = feb, volume =.

Something new under the Sun: A magnetically driven CH/CN anti-correlation , year = 1976, month = feb, volume =

Reference 71

Resolution
unresolved
no resolver link, observed 2026-08-07T00:15:39.272169Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T00:15:39.272169Z digest=sha256:78f58fb4116c3f9372621e9f89595dd95237b0c68775ca331e7d33dccd8d2b39

Observation 90af07a8-b011-4a70-bed5-5b858a8e591a · outbound

This paper cites 2026 , eprint=.

Something new under the Sun: A magnetically driven CH/CN anti-correlation 2026 , eprint=

Reference 72

Resolution
unresolved
no resolver link, observed 2026-08-07T00:15:39.285751Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T00:15:39.285751Z digest=sha256:012cc942bbeef4e290d2b7966264cc94cea23966076e4095e44d1d62e78dcb5f

Observation ad69b683-501c-431b-9ec9-6ee7d4d9f764 · outbound

This paper cites The Curious Case of Dark Faculae on M Dwarf Stars.

Something new under the Sun: A magnetically driven CH/CN anti-correlation The Curious Case of Dark Faculae on M Dwarf Stars

Reference 73

Resolution
unresolved
no resolver link, observed 2026-08-07T00:15:39.294740Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T00:15:39.294740Z digest=sha256:68d8cd7460c5d16e4cc53bb45c5f1ba2e9b03e4706b3ba25abfa3de8beb78eb0

Observation 0ce9090e-c151-4d1f-8784-4a09a34d028d · outbound

This paper cites Grand minima and maxima of solar activity: New observational constraints.

Something new under the Sun: A magnetically driven CH/CN anti-correlation Grand minima and maxima of solar activity: New observational constraints

Reference 74

Resolution
unresolved
no resolver link, observed 2026-08-07T00:15:39.312837Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T00:15:39.312837Z digest=sha256:1ec4d3bbeab38950bd008967766e78c56d2a50d164c999ad303646f5caba28b7

Observation 885edaa5-eaec-4081-b024-809cb1ed38ae · outbound

This paper cites Six decades of TIGRE and Mount Wilson chromospheric monitoring in the H and K lines: The quest for an understanding of solar-type activity.

Something new under the Sun: A magnetically driven CH/CN anti-correlation Six decades of TIGRE and Mount Wilson chromospheric monitoring in the H and K lines: The quest for an understanding of solar-type activity

Reference 75

Resolution
unresolved
no resolver link, observed 2026-08-07T00:15:39.318895Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T00:15:39.318895Z digest=sha256:3fc55ac99f467b822585045a267932966245c3d4b32aff5b9a34c73d9a652b83

Observation f0106a72-0244-4ea2-aa3b-72bae619837c · outbound

This paper cites Globular Clusters in the Time of the JWST. I. Survey Design and First Results on Multiple Populations and Beyond.

Something new under the Sun: A magnetically driven CH/CN anti-correlation Globular Clusters in the Time of the JWST. I. Survey Design and First Results on Multiple Populations and Beyond

Reference 76

Resolution
unresolved
no resolver link, observed 2026-08-07T00:15:39.324979Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T00:15:39.324979Z digest=sha256:00e47d7089bd359526745aec10016f4d83932aa3edd29bd019c5869aeb2c8683

Observation 750530d3-49a4-4f74-a10d-4aea5f79b8a8 · outbound

This paper cites Effect of surface magnetic fields on limb darkening in main-sequence stars.

Something new under the Sun: A magnetically driven CH/CN anti-correlation Effect of surface magnetic fields on limb darkening in main-sequence stars

Reference 77

Resolution
unresolved
no resolver link, observed 2026-08-07T00:15:39.329913Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T00:15:39.329913Z digest=sha256:daa8a99da36867fee3d6dab42e81fa2c165fa8ab69f0649ce678e18b0631df14

Observation 8b6514a5-b22d-461a-ae0f-ca69ca373d98 · outbound

This paper cites The Magnetic Fields at the Surface of Active Single G-K Giants.

Something new under the Sun: A magnetically driven CH/CN anti-correlation The Magnetic Fields at the Surface of Active Single G-K Giants

Reference 78

Resolution
unresolved
no resolver link, observed 2026-08-07T00:15:39.335346Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T00:15:39.335346Z digest=sha256:495e7862453c83d399bacd05a830747e707a9177fd85d79d9731194dde2dcda2

Observation b611277c-5228-4533-8e05-5b0587f1e8e7 · outbound

This paper cites , keywords =.

Something new under the Sun: A magnetically driven CH/CN anti-correlation , keywords =

Reference 79

Resolution
verified exact
doi, observed 2026-08-07T00:15:47.453540Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=arxiv_source observed=2026-08-07T00:15:39.341138Z digest=sha256:377c237e0afa404eaaa06e27b7763f80be3eaba09e53e56346f2083071a95d27

Observation bafac1c9-e853-4278-bc52-1f9843e513e6 · outbound

This paper cites Total Solar Irradiance during the Last Five Centuries.

Something new under the Sun: A magnetically driven CH/CN anti-correlation Total Solar Irradiance during the Last Five Centuries

Reference 80

Resolution
unresolved
no resolver link, observed 2026-08-07T00:15:39.345908Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T00:15:39.345908Z digest=sha256:01580d2580a3c54d301324941e9a479033bdce37e4d0bc73c6cc621f46f40537

Observation 3b53e297-314c-47cb-aa65-b9a069988830 · outbound

This paper cites Reconstruction of the Total Solar Irradiance during the last Millenium.

Something new under the Sun: A magnetically driven CH/CN anti-correlation Reconstruction of the Total Solar Irradiance during the last Millenium

Reference 81

Resolution
unresolved
no resolver link, observed 2026-08-07T00:15:39.350735Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T00:15:39.350735Z digest=sha256:b75dbcd1208892f4e094890d205fe226343eba85312374aaad219bfddf7175cd

Observation 7fbecf47-0995-48d5-9d2f-e2d02fc06415 · outbound

This paper cites Deciphering Solar Magnetic Activity: Some (Unpopular) Thoughts On the Coupling of the Sun's "Weather" and "Climate".

Something new under the Sun: A magnetically driven CH/CN anti-correlation Deciphering Solar Magnetic Activity: Some (Unpopular) Thoughts On the Coupling of the Sun's "Weather" and "Climate"

Reference 82

Resolution
metadata mismatch
local_arxiv, observed 2026-08-07T00:15:47.435773Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=arxiv_source observed=2026-08-07T00:15:39.356434Z digest=sha256:510d5ee41b8338201bc9c590581d4c8c9104f8cfaedf2d4601e74402040d9527

Observation 1d472f4d-a570-42eb-b773-bf31b75bded8 · outbound

This paper cites Journal of the British Astronomical Association , year = 1966, month = jun, volume =.

Something new under the Sun: A magnetically driven CH/CN anti-correlation Journal of the British Astronomical Association , year = 1966, month = jun, volume =

Reference 83

Resolution
unresolved
no resolver link, observed 2026-08-07T00:15:39.375328Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T00:15:39.375328Z digest=sha256:273883cca565d6b09ac04bb913618257599d23c98f7dc6f76cc5856a42e5bc0b

Observation 29efd308-b77f-41f4-b875-77f7b9ab2d48 · outbound

This paper cites Signatures of intrinsic Li depletion and Li-Na anti-correlation in the metal-poor globular cluster NGC6397.

Something new under the Sun: A magnetically driven CH/CN anti-correlation Signatures of intrinsic Li depletion and Li-Na anti-correlation in the metal-poor globular cluster NGC6397

Reference 84

Resolution
unresolved
no resolver link, observed 2026-08-07T00:15:39.388049Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T00:15:39.388049Z digest=sha256:c3cd359a1e4b4b0d5436d6a6219c48d07deecad25ea08b8925e2735004479a43

Observation 742f6c6d-ab4f-4a8a-a37b-1231ae90b40a · outbound

This paper cites , keywords =.

Something new under the Sun: A magnetically driven CH/CN anti-correlation , keywords =

Reference 85

Resolution
verified exact
doi, observed 2026-08-07T00:15:47.403805Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=arxiv_source observed=2026-08-07T00:15:39.399587Z digest=sha256:59ec5de35e2154471fc340d344a40f5f02b52eae571c192e4f931eda23e46b6e

Observation 606f0c9d-83ee-49cf-8d5e-541745baaeab · outbound

This paper cites Mixing processes during the evolution of red giants with moderate metal deficiencies : the role of molecular-weight barriers.

Something new under the Sun: A magnetically driven CH/CN anti-correlation Mixing processes during the evolution of red giants with moderate metal deficiencies : the role of molecular-weight barriers

Reference 86

Resolution
unresolved
no resolver link, observed 2026-08-07T00:15:39.405191Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T00:15:39.405191Z digest=sha256:4ec57fdf417e11c6b78533eb07ab26eba07094e4545ae60fc73cd5c624063e0f

Observation 371bf167-bcf3-4d35-9eaa-a67da34cc117 · outbound

This paper cites A combined study of thermohaline mixing and envelope overshooting with PARSEC: Calibration to NGC 6397 and M4.

Something new under the Sun: A magnetically driven CH/CN anti-correlation A combined study of thermohaline mixing and envelope overshooting with PARSEC: Calibration to NGC 6397 and M4

Reference 87

Resolution
metadata mismatch
local_arxiv, observed 2026-08-07T00:15:47.366477Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=arxiv_source observed=2026-08-07T00:15:39.417716Z digest=sha256:543b3b94ce5e3189c18b89bb1142801991b694dd56d79c25ef1a0663cef42eb3

Observation bfe34984-6fcd-46e1-b066-095c250ecf68 · outbound

This paper cites Asteroseismology of the multiple stellar populations in the Globular Cluster M4.

Something new under the Sun: A magnetically driven CH/CN anti-correlation Asteroseismology of the multiple stellar populations in the Globular Cluster M4

Reference 88

Resolution
unresolved
no resolver link, observed 2026-08-07T00:15:39.422971Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T00:15:39.422971Z digest=sha256:fd0e25324864979fc5746c16e328d28868e481cae3ade2a77b143e4bd4f4c70f

Observation c76e8b4f-cff5-4ce9-a9b7-73ed3b7fdf63 · outbound

This paper cites First Asteroseismic Analysis of the Globular Cluster M80: Multiple Populations and Stellar Mass Loss.

Something new under the Sun: A magnetically driven CH/CN anti-correlation First Asteroseismic Analysis of the Globular Cluster M80: Multiple Populations and Stellar Mass Loss

Reference 89

Resolution
unresolved
no resolver link, observed 2026-08-07T00:15:39.428373Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T00:15:39.428373Z digest=sha256:095eb3472f85b34699b3d9b4b997db62c6b149f8fdcadd13c23f83733e3ea59c

Observation ee2ae4d3-bffe-4662-ad4a-b0d324a732fd · outbound

This paper cites The 10830 Angstrom Helium Line Among Evolved Stars in the Globular Cluster M4.

Something new under the Sun: A magnetically driven CH/CN anti-correlation The 10830 Angstrom Helium Line Among Evolved Stars in the Globular Cluster M4

Reference 90

Resolution
unresolved
no resolver link, observed 2026-08-07T00:15:39.433295Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T00:15:39.433295Z digest=sha256:56a3184e5c29db9899d6a9e0493e6b5e9fe15b06bdd1e9bf5dfd2f6e65c9b097

Observation 385b97e7-4a61-4b56-baf1-4628ec0971da · outbound

This paper cites X-shooter observations of main sequence stars in the globular cluster NGC 2808: first chemical tagging of a He-normal and a He-rich dwarf.

Something new under the Sun: A magnetically driven CH/CN anti-correlation X-shooter observations of main sequence stars in the globular cluster NGC 2808: first chemical tagging of a He-normal and a He-rich dwarf

Reference 91

Resolution
unresolved
no resolver link, observed 2026-08-07T00:15:39.438689Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T00:15:39.438689Z digest=sha256:d9d04d59e8fcb04abec6d93d1c8a94c3729737b32cfc8658840b1924b8aa6008

Observation c8bf1085-fb01-4c76-bda5-3f1fbaf76622 · outbound

This paper cites Direct Evidence for an Enhancement of Helium in Giant Stars in Omega Centauri.

Something new under the Sun: A magnetically driven CH/CN anti-correlation Direct Evidence for an Enhancement of Helium in Giant Stars in Omega Centauri

Reference 92

Resolution
unresolved
no resolver link, observed 2026-08-07T00:15:39.443913Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T00:15:39.443913Z digest=sha256:e07080fa35684ccd1d3151584c0a63c22908a57fb5b0d3139baa1fea3d03efd9

Observation 7b3ff75e-1d48-40ef-9819-7729ed6f1118 · outbound

This paper cites Exploring Simple-Population and Multiple-Population Globular Clusters in the Outer Galactic Halo using the Hubble Space Telescope.

Something new under the Sun: A magnetically driven CH/CN anti-correlation Exploring Simple-Population and Multiple-Population Globular Clusters in the Outer Galactic Halo using the Hubble Space Telescope

Reference 93

Resolution
unresolved
no resolver link, observed 2026-08-07T00:15:39.450252Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T00:15:39.450252Z digest=sha256:01b739c04a6d206bdea9da5a3c1820fe67c915e78e7755e2dcbfed3bf1304b5c

Observation b2581bfa-7a24-4a96-ab9f-a5a50f525b0d · outbound

This paper cites Simultaneous spectropolarimetric observations in the H$\alpha$ and Ca II 8662 {\AA} lines of an active region.

Something new under the Sun: A magnetically driven CH/CN anti-correlation Simultaneous spectropolarimetric observations in the H$\alpha$ and Ca II 8662 {\AA} lines of an active region

Reference 94

Resolution
metadata mismatch
local_arxiv, observed 2026-08-07T00:15:47.312764Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=arxiv_source observed=2026-08-07T00:15:39.474767Z digest=sha256:328a6ad2e91ff96d1acef721aca32e003ee11f82de34c0bf0015a663c0118b30

Observation f52a0073-41a4-4276-bcd8-b4d2b754624a · outbound

This paper cites New density profile and structural parameters of the complex stellar system Terzan 5.

Something new under the Sun: A magnetically driven CH/CN anti-correlation New density profile and structural parameters of the complex stellar system Terzan 5

Reference 95

Resolution
unresolved
no resolver link, observed 2026-08-07T00:15:39.517714Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T00:15:39.517714Z digest=sha256:97cca27d8c6e69fc89c617b18d2ce730634c1f6a5e97d6b3d49e18041543c2e6

Observation 24f41df8-35b3-4c98-9772-57ae0cc5966a · outbound

This paper cites Magnetograms underestimate even unipolar magnetic flux nearly everywhere on the solar disk.

Something new under the Sun: A magnetically driven CH/CN anti-correlation Magnetograms underestimate even unipolar magnetic flux nearly everywhere on the solar disk

Reference 96

Resolution
metadata mismatch
local_arxiv, observed 2026-08-07T00:15:47.287304Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=arxiv_source observed=2026-08-07T00:15:39.538637Z digest=sha256:7120655bdc3e3f615a63ef6ba08da88aa16110f3c24a1bcd1a437064a34c91af

Observation 0b64395b-200a-4651-b520-f8b1cdd81ccd · outbound

This paper cites an unresolved cited work.

Something new under the Sun: A magnetically driven CH/CN anti-correlation Unresolved cited work

Reference 97

Resolution
verified exact
doi, observed 2026-08-07T00:15:47.259663Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=arxiv_source observed=2026-08-07T00:15:39.546040Z digest=sha256:615f0bc00d2bef2fea54117a38f32003dacb8fb7795dfe5c3c3062a351fb9d18

Observation e6f8983d-87f1-410d-a9b1-2ab767133b95 · outbound

This paper cites Brightness Contrast of Solar Magnetic Elements Observed by Sunrise.

Something new under the Sun: A magnetically driven CH/CN anti-correlation Brightness Contrast of Solar Magnetic Elements Observed by Sunrise

Reference 98

Resolution
metadata mismatch
local_arxiv, observed 2026-08-07T00:15:47.240803Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=arxiv_source observed=2026-08-07T00:15:39.551151Z digest=sha256:4b52627fa62750472e911e7508ef0ebfd6781ddf3212cbc7b09dbe90d3d2ee35

Observation 809a2042-8372-4b03-ad13-59c206318abf · outbound

This paper cites The origin of the reversed granulation in the solar photosphere.

Something new under the Sun: A magnetically driven CH/CN anti-correlation The origin of the reversed granulation in the solar photosphere

Reference 99

Resolution
unresolved
no resolver link, observed 2026-08-07T00:15:39.562226Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T00:15:39.562226Z digest=sha256:252a6c27a32cabb3f1195d80651c0fe2cfc62955a801fb39d740ec595e32653d

Observation 96ea885f-2999-4e1a-ab4b-efeed14d24c8 · outbound

This paper cites an unresolved cited work.

Something new under the Sun: A magnetically driven CH/CN anti-correlation Unresolved cited work

Reference 100

Resolution
verified exact
doi, observed 2026-08-07T00:15:47.212073Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=arxiv_source observed=2026-08-07T00:15:39.572422Z digest=sha256:17f4307749e7c14fcbb237e514b92c551be45c46630dd2784e4f152cd5044a0d

Pith citing papers

No inbound Pith citation observations are available.