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Paper Citation Record · LEDGER

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

As of 20 August 2026, this Paper Citation Record lists 100 of 219 outbound references and 1 inbound Pith citation observation for arXiv:2607.05651.

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

pith.paper-citation-record.v1
2607.05651 v1

Coverage vector

measured 100 of 219 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-07-11T04:19:29.170180Z

measured 101 of 101 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-20T06:33:59.587034+00:00

measured 1 of 1 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T00:15:39.150193Z

measured 0 of 1 external citation measurements

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

Source: cited_works

Reference resolution

100 of 219 outbound references displayed

  • verified exact56
  • verified fuzzy0
  • unresolved42
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch2

External citation measurements

No source-named external measurement is stored.

Outbound references

Observation 70f35042-b569-4294-a42b-768ea1c90b99 · outbound

This paper cites A New Look at an Old Cluster: The Membership, Rotation, and Magnetic Activity of Low-Mass Stars in the 1.3-Gyr-Old Open Cluster NGC 752.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet A New Look at an Old Cluster: The Membership, Rotation, and Magnetic Activity of Low-Mass Stars in the 1.3-Gyr-Old Open Cluster NGC 752

Reference 1

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verified exact
local_arxiv, observed 2026-07-11T04:27:48.763220Z

Source-reported events for the cited work

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Observation 52213aa9-79e2-4313-9786-1324bff86980 · outbound

This paper cites Magnetic and tidal migration of close-in planets. Influence of secular evolution on their population.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet Magnetic and tidal migration of close-in planets. Influence of secular evolution on their population

Reference 2

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verified exact
local_arxiv, observed 2026-07-11T04:27:48.695286Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

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Observation 89bff080-c6ea-463b-8ea9-021bed99722a · outbound

This paper cites , keywords =.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet , keywords =

Reference 3

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unresolved
no resolver link, observed 2026-07-11T04:19:29.170180Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 35a20489-97c2-4d4f-b06d-306dc47c65a3 · outbound

This paper cites Impact of Space Weather on Climate and Habitability of Terrestrial Type Exoplanets.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet Impact of Space Weather on Climate and Habitability of Terrestrial Type Exoplanets

Reference 4

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local_arxiv, observed 2026-07-11T04:27:48.209720Z

Source-reported events for the cited work

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Observation 71da7ed7-1470-4b3d-9ee6-d7bfc49d15fa · outbound

This paper cites , keywords =.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet , keywords =

Reference 5

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verified exact
doi, observed 2026-07-11T04:27:48.335192Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

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Observation 4f7005c3-6f1d-4eeb-8d4a-5567197b9bfe · outbound

This paper cites an unresolved cited work.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet Unresolved cited work

Reference 6

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unresolved
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Source-reported events for the cited work

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Observation 4d357b6b-d438-4ef6-b7ba-a44db81fbdf9 · outbound

This paper cites Calibrating Gyrochronology using Kepler Asteroseismic targets.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet Calibrating Gyrochronology using Kepler Asteroseismic targets

Reference 7

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local_arxiv, observed 2026-07-11T04:27:49.379196Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

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Observation b7385630-7312-484b-9ae6-765c58d0ee33 · outbound

This paper cites Towards precise stellar ages: combining isochrone fitting with empirical gyrochronology.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet Towards precise stellar ages: combining isochrone fitting with empirical gyrochronology

Reference 8

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local_arxiv, observed 2026-07-11T04:27:48.597173Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

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Observation d58dc5ff-a66c-4ffd-ab1e-eb88211e4935 · outbound

This paper cites Exploring the evolution of stellar rotation using Galactic kinematics.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet Exploring the evolution of stellar rotation using Galactic kinematics

Reference 9

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verified exact
local_arxiv, observed 2026-07-11T04:27:48.651057Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

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Observation 6f187e7e-8179-43ce-aef2-fd976ef26744 · outbound

This paper cites Solar Models: current epoch and time dependences, neutrinos, and helioseismological properties.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet Solar Models: current epoch and time dependences, neutrinos, and helioseismological properties

Reference 10

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local_arxiv, observed 2026-07-11T04:27:48.559134Z

Source-reported events for the cited work

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Observation cc2ba02f-4107-48aa-9685-07ae3f70e10b · outbound

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Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet Unresolved cited work

Reference 11

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Source-reported events for the cited work

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Observation 4117e7be-b094-429c-a8a2-2206f7227ad7 · outbound

This paper cites On the rotational evolution of solar- and late-type stars, its magnetic origins, and the possibility of stellar gyrochronology.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet On the rotational evolution of solar- and late-type stars, its magnetic origins, and the possibility of stellar gyrochronology

Reference 12

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unresolved
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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 852f3fd8-8cd5-427c-9f65-930eba1efefe · outbound

This paper cites Ages for illustrative field stars using gyrochronology: viability, limitations and errors.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet Ages for illustrative field stars using gyrochronology: viability, limitations and errors

Reference 13

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unresolved
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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 76a824e6-4bb6-484b-8ef0-7c4d89440ec9 · outbound

This paper cites Testing tidal theory for evolved stars by using red-giant binaries observed by Kepler.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet Testing tidal theory for evolved stars by using red-giant binaries observed by Kepler

Reference 14

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unresolved
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Source-reported events for the cited work

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Observation 705ebb5a-e106-4af3-bae6-374114fb6c06 · outbound

This paper cites Constraining stellar and orbital co-evolution through ensemble seismology of solar-like oscillators in binary systems -- A census of oscillating red-giants and main-sequence stars in Gaia DR3 binaries.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet Constraining stellar and orbital co-evolution through ensemble seismology of solar-like oscillators in binary systems -- A census of oscillating red-giants and main-sequence stars in Gaia DR3 binaries

Reference 15

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Source-reported events for the cited work

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Observation 6a188fb1-5df2-4032-94da-c922cd0beb33 · outbound

This paper cites , keywords =.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet , keywords =

Reference 16

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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 2026-08-20T06:33:59.587034+00:00.

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Observation 2317f869-88e6-4e8b-8fe6-9d83d9c1159e · outbound

This paper cites , keywords =.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet , keywords =

Reference 17

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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 2026-08-20T06:33:59.587034+00:00.

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Observation 1d420daa-efe1-4f6e-86c0-a8321ac42918 · outbound

This paper cites The Zwicky Transient Facility: System Overview, Performance, and First Results.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet The Zwicky Transient Facility: System Overview, Performance, and First Results

Reference 18

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unresolved
no resolver link, observed 2026-07-11T04:19:29.170180Z

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Observation 88be63ad-9c25-4d6e-be36-3814310f8fd2 · outbound

This paper cites Spectroscopic and seismic analysis of red giants in eclipsing binaries discovered by Kepler.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet Spectroscopic and seismic analysis of red giants in eclipsing binaries discovered by Kepler

Reference 19

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verified exact
local_arxiv, observed 2026-07-11T04:27:48.316564Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

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Observation e0f5eb9c-4678-4e8b-83c8-809a4e0fcff1 · outbound

This paper cites The Gaia-Kepler Stellar Properties Catalog. I. Homogeneous Fundamental Properties for 186,301 Kepler Stars.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet The Gaia-Kepler Stellar Properties Catalog. I. Homogeneous Fundamental Properties for 186,301 Kepler Stars

Reference 20

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unresolved
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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 0736b4eb-dad9-4d19-8a2f-703d563a9c0c · outbound

This paper cites The Kraft Break Sharply Divides Low Mass and Intermediate Mass Stars.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet The Kraft Break Sharply Divides Low Mass and Intermediate Mass Stars

Reference 21

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Observation e56f86a3-2e11-499e-b2ef-e32cb4dfd4c3 · outbound

This paper cites Three-dimensional modeling of the Ca II H&K lines in the solar atmosphere.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet Three-dimensional modeling of the Ca II H&K lines in the solar atmosphere

Reference 22

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Source-reported events for the cited work

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Observation 0d20736e-adb9-4384-b265-fffa58786b42 · outbound

This paper cites , keywords =.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet , keywords =

Reference 23

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no resolver link, observed 2026-07-11T04:19:29.170180Z

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Observation 3dbd0541-b718-4a99-a906-abf07264743f · outbound

This paper cites , keywords =.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet , keywords =

Reference 24

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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation a31efd73-b0ca-4def-ac0b-3ddab765d529 · outbound

This paper cites Chromospheric activity catalogue of 4454 cool stars. Questioning the active branch of stellar activity cycles.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet Chromospheric activity catalogue of 4454 cool stars. Questioning the active branch of stellar activity cycles

Reference 25

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no resolver link, observed 2026-07-11T04:19:29.170180Z

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Unavailable: canonical work link unavailable.

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Observation 22d89516-0f9a-452b-bebd-506e8fcf4d68 · outbound

This paper cites Science , keywords =.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet Science , keywords =

Reference 26

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no resolver link, observed 2026-07-11T04:19:29.170180Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 4a7fd161-e4c5-4575-8273-3465e6040b4b · outbound

This paper cites The Empirical Limits of Gyrochronology.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet The Empirical Limits of Gyrochronology

Reference 27

Resolution
verified exact
local_arxiv, observed 2026-07-11T04:27:48.660509Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

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Observation 853ac55e-3bef-4375-9e9e-79945bf11a8b · outbound

This paper cites Enhanced stellar activity for slow antisolar differential rotation?.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet Enhanced stellar activity for slow antisolar differential rotation?

Reference 28

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verified exact
local_arxiv, observed 2026-07-11T04:27:48.749825Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

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Observation 1cc7c9b1-3977-4e7a-85b4-de1af63e0448 · outbound

This paper cites , keywords =.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet , keywords =

Reference 29

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doi, observed 2026-07-11T04:27:49.102851Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

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Observation 134f840a-d412-4d73-bca0-ff9c76bd388c · outbound

This paper cites Kepler Input Catalog: Photometric Calibration and Stellar Classification.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet Kepler Input Catalog: Photometric Calibration and Stellar Classification

Reference 30

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unresolved
no resolver link, observed 2026-07-11T04:19:29.170180Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation bc243af9-315a-4d11-a530-4356c3c3639f · outbound

This paper cites Linking chromospheric activity and magnetic field properties for late-type dwarf stars.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet Linking chromospheric activity and magnetic field properties for late-type dwarf stars

Reference 31

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unresolved
no resolver link, observed 2026-07-11T04:19:29.170180Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation b17f32e9-80ba-4526-b3b8-804d07f6ae19 · outbound

This paper cites EAS2024, European Astronomical Society Annual Meeting , year = 2024, month = jul, eid =.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet EAS2024, European Astronomical Society Annual Meeting , year = 2024, month = jul, eid =

Reference 32

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unresolved
no resolver link, observed 2026-07-11T04:19:29.170180Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation ceb70d45-004c-4a8d-8e05-a69eb02de62a · outbound

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

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet Living Reviews in Solar Physics , keywords =

Reference 33

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no resolver link, observed 2026-07-11T04:19:29.170180Z

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source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:6e529f003aed50ec52057eb4307e430dee98cf93a4a552bffeab65ae71117564

Observation 9c025bbe-b00c-45a6-9848-d1e8f7104439 · outbound

This paper cites , keywords =.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet , keywords =

Reference 34

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unresolved
no resolver link, observed 2026-07-11T04:19:29.170180Z

Source-reported events for the cited work

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source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:2e12739b33746499ae6bc415ded9c227c44924f831451644267ad3bd8fcc217b

Observation bc0bd71b-72cb-4c1e-b276-726b9d6bc1b3 · outbound

This paper cites an unresolved cited work.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet Unresolved cited work

Reference 35

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no resolver link, observed 2026-07-11T04:19:29.170180Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:78c7f43a95764a45d6e4644ef8aa2d3d403d21f5cf60f3495d53c6ff903317a3

Observation 20a4988e-ebae-4f21-a865-a6dc81be0f52 · outbound

This paper cites Starspots and Magnetism: Testing the Activity Paradigm in the Pleiades and M67.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet Starspots and Magnetism: Testing the Activity Paradigm in the Pleiades and M67

Reference 36

Resolution
verified exact
local_arxiv, observed 2026-07-11T04:27:48.014070Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:0860cacd01e8e7ad478290548f546c4f3641cc5b70c28538b9737aedabc4e01a

Observation 248d49ff-152d-4b99-9ffc-90f36a4a6ad4 · outbound

This paper cites Core-envelope decoupling drives radial shear dynamos in cool stars.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet Core-envelope decoupling drives radial shear dynamos in cool stars

Reference 37

Resolution
verified exact
local_arxiv, observed 2026-07-11T04:27:47.756430Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:16e653a0cc2a2e3eb37eb9a29216bcea73797bc0ee5f82a3ee79d3dd82a68a12

Observation c61f7f7d-0b70-44f6-951d-186a16e599bb · outbound

This paper cites A New Age-Activity Relation For Solar Analogs that Accounts for Metallicity.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet A New Age-Activity Relation For Solar Analogs that Accounts for Metallicity

Reference 38

Resolution
verified exact
local_arxiv, observed 2026-07-11T04:27:47.706401Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:09b94e213fd905ef130bed4f2cc91df209d6774b0645999c94e3fc7783106d12

Observation 2d34fc59-9e77-4493-9e4e-23590d4dc6d3 · outbound

This paper cites Surface rotation of Kepler red giant stars.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet Surface rotation of Kepler red giant stars

Reference 39

Resolution
unresolved
no resolver link, observed 2026-07-11T04:19:29.170180Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:d971c00a844fd82b97f2e54e804feb5720357c46e006bc68ac5196dfba80b582

Observation 1b8aea3f-6021-4525-be35-6724a79df8f5 · outbound

This paper cites Unravelling the Period Gap using LAMOST Chromospheric Activity Indices.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet Unravelling the Period Gap using LAMOST Chromospheric Activity Indices

Reference 40

Resolution
verified exact
local_arxiv, observed 2026-07-11T04:27:47.679974Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:842e578497239f732b1bc279aed7c6ee6ddd4492b9c108764f3a7809f5528ba2

Observation 93c46124-6341-42db-9393-34d3c6d4f9b5 · outbound

This paper cites , year = 2014, month = aug, volume =.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet , year = 2014, month = aug, volume =

Reference 41

Resolution
unresolved
no resolver link, observed 2026-07-11T04:19:29.170180Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:d533bef38db049cbad55cd9a686c30d56939c86589bd91adf3bdaefc99b4eeff

Observation 3ebb5d81-ee13-4675-bb31-52356a63ed8e · outbound

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

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet Living Reviews in Solar Physics , keywords =

Reference 42

Resolution
unresolved
no resolver link, observed 2026-07-11T04:19:29.170180Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:d1083f61b0caf28b4d44fc2b0ebdd77176814b669b216a3e6a3aedd2a62ebf32

Observation 9c89236c-3527-4323-a890-c192db9f41aa · outbound

This paper cites Chemical Evolution in the Milky Way: Rotation-based ages for APOGEE-Kepler cool dwarf stars.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet Chemical Evolution in the Milky Way: Rotation-based ages for APOGEE-Kepler cool dwarf stars

Reference 43

Resolution
verified exact
local_arxiv, observed 2026-07-11T04:27:48.930631Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:a98d273aee2da79c6ece23b6e49dd3d4d9df128472259270d16b34448043713a

Observation 38eb7a7a-dfd3-43b3-869a-fada79a437df · outbound

This paper cites New Rotation Periods from the Kepler Bonus Background Light Curves.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet New Rotation Periods from the Kepler Bonus Background Light Curves

Reference 44

Resolution
verified exact
local_arxiv, observed 2026-07-11T04:27:48.489869Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:16abd6bfe4949bc78ef3f5cd450627c23cce1eacc8b654b34972a0f998b147cb

Observation f7d2057f-945c-4d09-80e1-895a859a0659 · outbound

This paper cites A calibration of the Rossby number from asteroseismology.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet A calibration of the Rossby number from asteroseismology

Reference 45

Resolution
verified exact
local_arxiv, observed 2026-07-11T04:27:48.899123Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:6a0eff73914323cad23d550b2d73bf1cfa3b8aa65983b1298c2ca269bc2aceb8

Observation 56398367-b4cb-4ce7-b922-abf41b726fd7 · outbound

This paper cites A Temporary Epoch of Stalled Spin-Down for Low-Mass Stars: Insights from NGC 6811 with Gaia and Kepler.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet A Temporary Epoch of Stalled Spin-Down for Low-Mass Stars: Insights from NGC 6811 with Gaia and Kepler

Reference 46

Resolution
verified exact
local_arxiv, observed 2026-07-11T04:27:47.718619Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:285046176a65831e3aa75449f9bd1c45e0ccf7af0399659387f92824f8ba5476

Observation 3629b0ff-36a1-43d1-bc8d-d3be4791ac5e · outbound

This paper cites When Do Stalled Stars Resume Spinning Down? Advancing Gyrochronology with Ruprecht 147.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet When Do Stalled Stars Resume Spinning Down? Advancing Gyrochronology with Ruprecht 147

Reference 47

Resolution
verified exact
local_arxiv, observed 2026-07-11T04:27:48.478156Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:6ad66b251711b006dac4aa8d8ec76908cbb8f4c346b6f424296352ffcc3a55d9

Observation 188e7203-4fe3-434b-99f0-7a11782f3710 · outbound

This paper cites Rotating Stars from Kepler Observed with Gaia DR1.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet Rotating Stars from Kepler Observed with Gaia DR1

Reference 48

Resolution
verified exact
local_arxiv, observed 2026-07-11T04:27:47.913462Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:58fc64cdf96bbd084e91d69ec2a8a7bc99c40caaac3ac820fcefb3c89083042b

Observation 0f440da0-57c6-468e-8bb2-83d9b9d6ebb5 · outbound

This paper cites Rotating Stars from Kepler Observed with Gaia DR2.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet Rotating Stars from Kepler Observed with Gaia DR2

Reference 49

Resolution
verified exact
local_arxiv, observed 2026-07-11T04:27:47.743545Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:d4ef4421a61bc016136247a526744f5dd4c70d6c180a3e1077fbfb2adbf1d6c8

Observation 2f780f8f-3f8a-43b0-a1fe-018b7ec3c9b3 · outbound

This paper cites Further Evidence of Modified Spin-down in Sun-like Stars: Pileups in the Temperature-Period Distribution.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet Further Evidence of Modified Spin-down in Sun-like Stars: Pileups in the Temperature-Period Distribution

Reference 50

Resolution
unresolved
no resolver link, observed 2026-07-11T04:19:29.170180Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:683405ef9ebab55af9cf5beb6d6f68c3b2f8a8552412a9ea73d9b3af19b12909

Observation d1b9524a-8c50-48be-b354-599c4d8255ee · outbound

This paper cites Activity of low mass stars in the light of spot signature in the Fourier domain.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet Activity of low mass stars in the light of spot signature in the Fourier domain

Reference 51

Resolution
verified exact
local_arxiv, observed 2026-07-11T04:27:48.837701Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:ff43f183ccceb234f3510dbd002b1531148ca5fb5de01b6c52d592204c74d804

Observation 121b3c8f-8fd0-4eac-b3b6-443e4679f3c6 · outbound

This paper cites YREC: The Yale Rotating Stellar Evolution Code.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet YREC: The Yale Rotating Stellar Evolution Code

Reference 52

Resolution
verified exact
local_arxiv, observed 2026-07-11T04:27:47.767942Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:1bd867d3aeaa6d27d15ec232baa5834f74e20ede2e8153339885a3ab436ebb16

Observation b320c678-7a51-4fcc-930e-ce4208a8248a · outbound

This paper cites , keywords =.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet , keywords =

Reference 53

Resolution
verified exact
doi, observed 2026-07-11T04:27:48.807210Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:1efe23bc11010cf55b3a70ad8260f3ca7f58e870807469bdf14f18c551ced1f1

Observation c72b8a80-e010-4184-80e8-205b0e41b367 · outbound

This paper cites Angular Momentum Transport In Solar-Type Stars: Testing the Timescale For Core-Envelope Coupling.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet Angular Momentum Transport In Solar-Type Stars: Testing the Timescale For Core-Envelope Coupling

Reference 54

Resolution
verified exact
local_arxiv, observed 2026-07-11T04:27:47.794552Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:70713ffd553b66d9448eb42bac68c36af5420ea0357bd8ba0dd501250466b3eb

Observation 16207ec9-d8d2-4d2f-b15a-9c66faac0ea4 · outbound

This paper cites Double-edged sword: the influence of tidal interaction on stellar activity in binaries.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet Double-edged sword: the influence of tidal interaction on stellar activity in binaries

Reference 55

Resolution
verified exact
local_arxiv, observed 2026-07-11T04:27:48.623384Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:eb6210db818e62e48f1eb642982a67a7f58166614f0572cd4a2395fa7fb967c5

Observation 43f3a60f-2707-4e44-a3ba-cfcf17c4fd39 · outbound

This paper cites Rotationally Driven Ultraviolet Emission of Red Giant Stars.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet Rotationally Driven Ultraviolet Emission of Red Giant Stars

Reference 56

Resolution
verified exact
local_arxiv, observed 2026-07-11T04:27:47.827662Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:2c252b5a72681e9cff46278c699a3c5617326f9284b2f26ae281dd3334bbd3cb

Observation 71af088b-67c8-465f-87ed-76f4011bbc11 · outbound

This paper cites Rotationally Driven Ultraviolet Emission of Red Giant Stars II. Metallicity, Activity, Binarity and Sub-subgiants.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet Rotationally Driven Ultraviolet Emission of Red Giant Stars II. Metallicity, Activity, Binarity and Sub-subgiants

Reference 57

Resolution
verified exact
local_arxiv, observed 2026-07-11T04:27:48.097868Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:081cc9d0e87a9572c69c5c61267230d9d717cdbdfd1322307493853fd8feeafe

Observation aff8639f-73ae-4cd5-b06b-42d1b60cbaa4 · outbound

This paper cites Stellar Multiplicity.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet Stellar Multiplicity

Reference 58

Resolution
unresolved
no resolver link, observed 2026-07-11T04:19:29.170180Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:8c128f88c65121c9d4cd16a11c61c00f6858b3e31af94f45ecfa6f5d12b428e0

Observation 2719f9b0-148d-466c-92f2-1c093d768c63 · outbound

This paper cites A 4 Gyr M-dwarf Gyrochrone from CFHT/MegaPrime Monitoring of the Open Cluster M67.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet A 4 Gyr M-dwarf Gyrochrone from CFHT/MegaPrime Monitoring of the Open Cluster M67

Reference 59

Resolution
verified exact
local_arxiv, observed 2026-07-11T04:27:48.731805Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:3bf9725c5e8d57a0a16610cdd365c862129fee27e75cd6810054ae1a5d8e2aab

Observation 80a30be3-fcbb-4859-9edb-8b84ab718c5f · outbound

This paper cites , keywords =.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet , keywords =

Reference 60

Resolution
unresolved
no resolver link, observed 2026-07-11T04:19:29.170180Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:833fb717c89f58531fd9afd69197fecbd549b46b9147d48741c2d7a1c85e5995

Observation df4ccd82-7608-4232-89ea-2e6a037f43bf · outbound

This paper cites How Good a Clock is Rotation? The Stellar Rotation-Mass-Age Relationship for Old Field Stars.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet How Good a Clock is Rotation? The Stellar Rotation-Mass-Age Relationship for Old Field Stars

Reference 61

Resolution
verified exact
local_arxiv, observed 2026-07-11T04:27:48.083390Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:0e7c917e6049901b167a1efde85b19cb9d42d46ecd9695c0d00f9e1a07a09e0e

Observation b0d10f80-dcc5-4926-9099-89fe59858062 · outbound

This paper cites , keywords =.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet , keywords =

Reference 62

Resolution
verified exact
doi, observed 2026-07-11T04:27:49.095727Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:9a947d60e13177c88a2b6db7885bb3f48b46f5adfd64ab47976fe17f9183cb6c

Observation 22039666-7a34-40a2-b1b1-425f40c404d4 · outbound

This paper cites The stellar corona-chromosphere connection. A comprehensive study of X-ray and Ca II IRT fluxes from eROSITA and Gaia.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet The stellar corona-chromosphere connection. A comprehensive study of X-ray and Ca II IRT fluxes from eROSITA and Gaia

Reference 63

Resolution
verified exact
local_arxiv, observed 2026-07-11T04:27:48.425284Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:81275b668412bee031f0d192271102969ed51647c8394c5e37c4538df796c354

Observation 59e12e46-aae0-4d91-9c73-7427369c5f9e · outbound

This paper cites A detailed understanding of the rotation-activity relationship using the 300 Myr old open cluster NGC 3532.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet A detailed understanding of the rotation-activity relationship using the 300 Myr old open cluster NGC 3532

Reference 64

Resolution
verified exact
local_arxiv, observed 2026-07-11T04:27:48.466427Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:4856bc9585e04b3bd4d14942c5f06329132f87f78e40e2bb5a1303c82192d598

Observation 0f57c526-88a5-4ec2-b8f2-f688c22f76f3 · outbound

This paper cites The Kepler Follow-Up Observation Program. II. Stellar Parameters from Medium- and High-Resolution Spectroscopy.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet The Kepler Follow-Up Observation Program. II. Stellar Parameters from Medium- and High-Resolution Spectroscopy

Reference 65

Resolution
unresolved
no resolver link, observed 2026-07-11T04:19:29.170180Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:b597ea742c466d69331fe565728ccd5d66789c165dce738ff2d4e39d08ff9ff5

Observation f509071a-a49f-4ee5-903d-a60219331e08 · outbound

This paper cites The Gaia mission.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet The Gaia mission

Reference 66

Resolution
unresolved
no resolver link, observed 2026-07-11T04:19:29.170180Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:3a95b246fb004b5d0a9f4011d6e5f88592639bf4922535614a9ede8f9192b13e

Observation 914b251e-0933-4240-93ec-46e2cfb1332e · outbound

This paper cites Gaia Early Data Release 3: Summary of the contents and survey properties.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet Gaia Early Data Release 3: Summary of the contents and survey properties

Reference 67

Resolution
unresolved
no resolver link, observed 2026-07-11T04:19:29.170180Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:55107a3aed34fee89ba070b6b9e89db68fbbfbd24311a4a6bcaf62568cea90e3

Observation 37f01708-1532-460b-87f1-bbd19139dd65 · outbound

This paper cites Gaia Data Release 3: Summary of the content and survey properties.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet Gaia Data Release 3: Summary of the content and survey properties

Reference 68

Resolution
unresolved
no resolver link, observed 2026-07-11T04:19:29.170180Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:64d68acce6618844869c02b3325db3910932c1d43191018e713b89b641d75cbb

Observation 73e08d5e-4bc8-4782-9435-97b63eaba8f1 · outbound

This paper cites Gaia Data Release 3: Stellar multiplicity, a teaser for the hidden treasure.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet Gaia Data Release 3: Stellar multiplicity, a teaser for the hidden treasure

Reference 69

Resolution
verified exact
local_arxiv, observed 2026-07-11T04:27:48.569368Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:fa66e3961b02716ddd71e77061445ec6a3462a4ee33f0333735cd2e59102f604

Observation a31faa57-5a28-4d07-839b-b46870481efa · outbound

This paper cites Improved angular momentum evolution model for solar-like stars.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet Improved angular momentum evolution model for solar-like stars

Reference 70

Resolution
unresolved
no resolver link, observed 2026-07-11T04:19:29.170180Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:633f0f05ae9a460481a5a52687a4e0bbdccc163c6bb6485493087f59d87a1afa

Observation f4c10cb0-d1c5-4639-82a3-0f2d08d82cc7 · outbound

This paper cites Improved angular momentum evolution model for solar-like stars II. Exploring the mass dependence.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet Improved angular momentum evolution model for solar-like stars II. Exploring the mass dependence

Reference 71

Resolution
unresolved
no resolver link, observed 2026-07-11T04:19:29.170180Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:e1dbc46be30e3c125c84abdab4d323f43d113bb846884749d550fe657e84356e

Observation b9c9192f-f3d1-46d1-a4b7-8be9589d147b · outbound

This paper cites , keywords =.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet , keywords =

Reference 72

Resolution
unresolved
no resolver link, observed 2026-07-11T04:19:29.170180Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:f25bb92b43c5470de95f70f200ccd6f5991815137cf6dae56fb4b6b1f5ea7c65

Observation f018e494-6141-4f53-bc9d-a7f83aa78cd1 · outbound

This paper cites Rotation and magnetism of Kepler pulsating solar-like stars. Towards asteroseismically calibrated age-rotation relations.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet Rotation and magnetism of Kepler pulsating solar-like stars. Towards asteroseismically calibrated age-rotation relations

Reference 73

Resolution
unresolved
no resolver link, observed 2026-07-11T04:19:29.170180Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:28d18c2e46bb317ba8273c9e472f070dd2dda8e357eaf6c8662f6ed717726d52

Observation 370dc7ce-2584-4154-97d7-44ada96bc369 · outbound

This paper cites Impact on asteroseismic analyses of regular gaps in Kepler data.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet Impact on asteroseismic analyses of regular gaps in Kepler data

Reference 74

Resolution
verified exact
local_arxiv, observed 2026-07-11T04:27:48.439405Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:9f382e8fc374d87e16b22251c5d8532a42f6a532eec1a5ababd2f294fb3e854f

Observation e444f2d3-4e45-49a3-9a93-bbb73be8e556 · outbound

This paper cites The Revolution Revolution: magnetic morphology driven spin-down.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet The Revolution Revolution: magnetic morphology driven spin-down

Reference 75

Resolution
unresolved
no resolver link, observed 2026-07-11T04:19:29.170180Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:0f0131a22e5f0103f0e7a202e181ae3bbdad2112e4f1e4f100930322b8ee83b3

Observation 02e6cdc5-99e3-4323-a9f2-36f43920be8a · outbound

This paper cites Surface Activity and Oscillation Amplitudes of Red Giants in Eclipsing Binaries.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet Surface Activity and Oscillation Amplitudes of Red Giants in Eclipsing Binaries

Reference 76

Resolution
verified exact
local_arxiv, observed 2026-07-11T04:27:48.825208Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:998b9e8ac3dbcaf3563143e9a607af87f7734a2ea6cfb42bc444f5bb835cc56d

Observation e8231cdf-fc4f-4661-9dbf-1a424d99ed60 · outbound

This paper cites Active red giants: close binaries versus single rapid rotators.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet Active red giants: close binaries versus single rapid rotators

Reference 77

Resolution
verified exact
local_arxiv, observed 2026-07-11T04:27:48.154310Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:2a3d844d6e1202285851c694cb680ff0637d468a4a835f0de48f0fae1a8f8da1

Observation 5d3485b6-1ba6-4c06-8368-b45c9d039602 · outbound

This paper cites Chinese Journal of Space Science , keywords =.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet Chinese Journal of Space Science , keywords =

Reference 78

Resolution
unresolved
no resolver link, observed 2026-07-11T04:19:29.170180Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:b62c380763a9d377f436a160940847ba60882437c5891743a1f7b9c5aba3a8a6

Observation 92ecac9b-078b-4c20-8f0b-32e2033895bd · outbound

This paper cites Surface magnetism of rapidly rotating red giants: single versus close binary stars.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet Surface magnetism of rapidly rotating red giants: single versus close binary stars

Reference 79

Resolution
verified exact
local_arxiv, observed 2026-07-11T04:27:48.087640Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:2dc1b07000162f4e3537b9ce9cc13ad60563255cf8f149b683f7fdc1383121c2

Observation d5c87faa-c113-4edd-9e1f-898caa60d1cf · outbound

This paper cites Magnetic activity of red giants: correlation between the amplitude of solar-like oscillations and chromospheric indicators.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet Magnetic activity of red giants: correlation between the amplitude of solar-like oscillations and chromospheric indicators

Reference 80

Resolution
verified exact
local_arxiv, observed 2026-07-11T04:27:48.490418Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:9f122b2150b5b3a6b7f70496e191283ea7227758bed300412c502c47df34b585

Observation 8c1fd827-187b-4e67-af2c-2a630e51e40d · outbound

This paper cites On the Identification of Wide Binaries in the Kepler Field.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet On the Identification of Wide Binaries in the Kepler Field

Reference 81

Resolution
verified exact
local_arxiv, observed 2026-07-11T04:27:48.104047Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:f8ee26a3b738896c3ec6f97b24c74bdd67fad28e8b6037d99020dd69f2bbcf2b

Observation 4ec8448c-0ff3-4628-8400-631d1204a2ec · outbound

This paper cites Stellar Rotation in the Gaia Era: Revised Open Clusters Sequences.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet Stellar Rotation in the Gaia Era: Revised Open Clusters Sequences

Reference 82

Resolution
verified exact
local_arxiv, observed 2026-07-11T04:27:48.501699Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:3c101eae76b9984177e62034fbfbb170ca8cbd930d642b18fdab18373f132fde

Observation 2bec8d4a-7160-4061-9f5e-de4db74c4b70 · outbound

This paper cites Testing the Limits of Precise Subgiant Characterization with APOGEE and Gaia: Opening a Window to Unprecedented Astrophysical Studies.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet Testing the Limits of Precise Subgiant Characterization with APOGEE and Gaia: Opening a Window to Unprecedented Astrophysical Studies

Reference 83

Resolution
unresolved
no resolver link, observed 2026-07-11T04:19:29.170180Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:8905287dbd5b20eb9bf6fde78f510b90e57692f2931f193a16fb32be38da04a7

Observation e8492bc5-80bb-4fd3-8754-c7a92c9ff690 · outbound

This paper cites Kepler meets Gaia DR3: homogeneous extinction-corrected color-magnitude diagram and binary classification.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet Kepler meets Gaia DR3: homogeneous extinction-corrected color-magnitude diagram and binary classification

Reference 84

Resolution
verified exact
local_arxiv, observed 2026-07-11T04:27:48.512113Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:936f653e7bd9927d2a679ada7965535cb9472743af9327141224b074c8961e0a

Observation 871abeaf-6203-4eda-b5ca-11a443ca0206 · outbound

This paper cites Research Notes of the American Astronomical Society , keywords =.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet Research Notes of the American Astronomical Society , keywords =

Reference 85

Resolution
verified exact
doi, observed 2026-07-11T04:27:48.175847Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:64463febf5c7f4ef1c28964f953c84d6133ae4754723d242941e62e8d759a04e

Observation 86d9ab0d-8db7-4d6a-816d-7b54e8834942 · outbound

This paper cites an unresolved cited work.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet Unresolved cited work

Reference 86

Resolution
unresolved
no resolver link, observed 2026-07-11T04:19:29.170180Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:5c0d4f220f7a0370f3ef61483ee354ba80dfefb423a6bc82c3f5f43da2636f9e

Observation c62f99bf-5b04-4877-b3da-be4aef86b9d3 · outbound

This paper cites , keywords =.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet , keywords =

Reference 87

Resolution
verified exact
doi, observed 2026-07-11T04:27:48.520010Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:236c8b9fe9c9d1d263321a1261f63d55ae4865d4181b820b0149c4b928d7a0d8

Observation dae6b14a-479f-4409-ae68-c491ef084eda · outbound

This paper cites R ^ ' _ HK index signature of a recent burst of star formation.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet R ^ ' _ HK index signature of a recent burst of star formation

Reference 88

Resolution
verified exact
doi, observed 2026-07-11T04:27:48.373739Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:57481223301bd2f943b2f2a5d588b8acc6c346dff773bcd2de87271fcad61041

Observation cea1bb1e-3959-4d16-8bf5-f0f75d409601 · outbound

This paper cites Stellar Rotation in the K2 Sample: Evidence for Modified Spindown.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet Stellar Rotation in the K2 Sample: Evidence for Modified Spindown

Reference 89

Resolution
verified exact
local_arxiv, observed 2026-07-11T04:27:48.363803Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:5ae1e723e9672a9f27ee019bc0a6498a31f94559dadfe5eab9ec1d144ec3493d

Observation a8586a36-5047-4eb5-9acc-1cf4577fa07b · outbound

This paper cites Rotation periods for cool stars in the open cluster Ruprecht 147 (NGC 6774): Implications for gyrochronology.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet Rotation periods for cool stars in the open cluster Ruprecht 147 (NGC 6774): Implications for gyrochronology

Reference 90

Resolution
verified exact
local_arxiv, observed 2026-07-11T04:27:48.535485Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:a805caa52b6c0c356615c5e50c8866ee439f94ea296337d21332dfa9c9384c99

Observation 396f0ae4-de40-451a-88b5-878a521a55d0 · outbound

This paper cites Wide binaries demonstrate the consistency of rotational evolution between open cluster and field stars.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet Wide binaries demonstrate the consistency of rotational evolution between open cluster and field stars

Reference 91

Resolution
verified exact
local_arxiv, observed 2026-07-11T04:27:48.294485Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:27f23ee7f88f3128bb075851a536644ec2d27a8469a51609fba1d96366c2f521

Observation dbae7cee-1adb-496b-bfe2-d14606175e6a · outbound

This paper cites New insights into the rotational evolution of near-solar age stars from the open cluster M67.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet New insights into the rotational evolution of near-solar age stars from the open cluster M67

Reference 92

Resolution
verified exact
local_arxiv, observed 2026-07-11T04:27:48.246145Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:05f920d171d24a38cb4dea5b9bdebd0f018553dd066504e7d6ea7acbaf75530d

Observation befbf642-54cb-4b97-831e-d854f4e4003f · outbound

This paper cites The Sun in Time: Activity and Environment.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet The Sun in Time: Activity and Environment

Reference 93

Resolution
unresolved
no resolver link, observed 2026-07-11T04:19:29.170180Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:ae718e5b69a32fb09f484f8ac8ab100936048c41cf09220d879fbbd5f6c07abd

Observation 8640852d-4d94-403f-a953-c18edbf16c95 · outbound

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

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet Living Reviews in Solar Physics , keywords =

Reference 94

Resolution
unresolved
no resolver link, observed 2026-07-11T04:19:29.170180Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:01c0b84359529fb998e23c9f30a6f0873dfc673f728a398e7983e2748c7f1733

Observation aea1803b-ed9d-4873-863f-2e2f1094bb39 · outbound

This paper cites Weakened magnetic braking supported by asteroseismic rotation rates of Kepler dwarfs.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet Weakened magnetic braking supported by asteroseismic rotation rates of Kepler dwarfs

Reference 95

Resolution
verified exact
local_arxiv, observed 2026-07-11T04:27:48.329151Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:f80f52f3990fe3fcde0704a3ece89688a411770087450aeb69e9975b0f698ef0

Observation 2f8a7170-7781-46d7-8d9f-81689dd1ad7d · outbound

This paper cites , keywords =.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet , keywords =

Reference 96

Resolution
verified exact
doi, observed 2026-07-11T04:27:48.558334Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:97b6c6259777b2cd77553c26ebc59d2ae460eba2630d07513e8275daa8fe33e7

Observation 0d9e307a-8e0d-4192-bc56-64243c0d025f · outbound

This paper cites The K2 Mission: Characterization and Early results.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet The K2 Mission: Characterization and Early results

Reference 97

Resolution
unresolved
no resolver link, observed 2026-07-11T04:19:29.170180Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:454cc8afc1e9ca9a8b1eb2dc238782c176ade94c592dd224b282da3802835b18

Observation 7ef6f90e-31ef-4ab3-862d-47e76d4a0fcd · outbound

This paper cites Near-Infrared Ca II Triplet As An Stellar Activity Indicator: Library and Comparative Study.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet Near-Infrared Ca II Triplet As An Stellar Activity Indicator: Library and Comparative Study

Reference 98

Resolution
verified exact
local_arxiv, observed 2026-07-11T04:27:47.860663Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:8375b07de53d9aa2c35c49e9705f7c45688f62bb82c6b2258f3950b0e1a4bcfb

Observation 7a7434ab-c85d-4b1a-9312-15c826717515 · outbound

This paper cites LSST: from Science Drivers to Reference Design and Anticipated Data Products.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet LSST: from Science Drivers to Reference Design and Anticipated Data Products

Reference 99

Resolution
unresolved
no resolver link, observed 2026-07-11T04:19:29.170180Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:42880813c6bbf4930360e485b9352e30e8eb9a1e9a75ef97f9c113617c75769d

Observation 554ba1f0-54a8-4c15-8fd1-5a2fbb039a85 · outbound

This paper cites , keywords =.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet , keywords =

Reference 100

Resolution
unresolved
no resolver link, observed 2026-07-11T04:19:29.170180Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:5d107112f80c6287de7429b20b5e0af3fcdc2b64481f813467437d1788461d8e

Pith citing papers

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

Something new under the Sun: A magnetically driven CH/CN anti-correlation cites this paper.

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:be2835a8b359e9aa2aee6445f16736482d6b3e90c2445287a1811a15c4cae85e