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

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

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

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No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

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

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

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No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

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

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

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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

Resolution: metadata mismatch; local_arxiv, observed 2026-07-11T04:27:48.209720Z

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No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

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

Resolution: 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 2026-08-21T06:32:19.484+00:00.

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

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

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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

Resolution: verified exact; local_arxiv, observed 2026-07-11T04:27:49.379196Z

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No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

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

Resolution: verified exact; 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 2026-08-21T06:32:19.484+00:00.

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

Resolution: 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 2026-08-21T06:32:19.484+00:00.

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

Resolution: verified exact; local_arxiv, observed 2026-07-11T04:27:48.559134Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation cc2ba02f-4107-48aa-9685-07ae3f70e10b · 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 11

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

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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

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

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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

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

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Unavailable: canonical work link unavailable.

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

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

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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

Resolution: metadata mismatch; local_arxiv, observed 2026-07-11T04:27:48.841669Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

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

Resolution: verified exact; doi, observed 2026-07-11T04:27:48.639683Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

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

Resolution: verified exact; doi, observed 2026-07-11T04:27:48.811137Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

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

Resolution: 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

Resolution: 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 2026-08-21T06:32:19.484+00:00.

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

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

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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

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

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Unavailable: canonical work link unavailable.

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

Resolution: verified exact; local_arxiv, observed 2026-07-11T04:27:48.154879Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

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

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

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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

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

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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

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

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Unavailable: canonical work link unavailable.

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

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

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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 2026-08-21T06:32:19.484+00:00.

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

Resolution: 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 2026-08-21T06:32:19.484+00:00.

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

Resolution: verified exact; 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 2026-08-21T06:32:19.484+00:00.

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

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

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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

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

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Unavailable: canonical work link unavailable.

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

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

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Unavailable: canonical work link unavailable.

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

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

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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

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

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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

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

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Unavailable: canonical work link unavailable.

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 2026-08-21T06:32:19.484+00:00.

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 2026-08-21T06:32:19.484+00:00.

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 2026-08-21T06:32:19.484+00:00.

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

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Unavailable: canonical work link unavailable.

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 2026-08-21T06:32:19.484+00:00.

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.

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.

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 2026-08-21T06:32:19.484+00:00.

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 2026-08-21T06:32:19.484+00:00.

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 2026-08-21T06:32:19.484+00:00.

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 2026-08-21T06:32:19.484+00:00.

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 2026-08-21T06:32:19.484+00:00.

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 2026-08-21T06:32:19.484+00:00.

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 2026-08-21T06:32:19.484+00:00.

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.

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 2026-08-21T06:32:19.484+00:00.

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 2026-08-21T06:32:19.484+00:00.

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 2026-08-21T06:32:19.484+00:00.

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 2026-08-21T06:32:19.484+00:00.

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 2026-08-21T06:32:19.484+00:00.

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 2026-08-21T06:32:19.484+00:00.

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 2026-08-21T06:32:19.484+00:00.

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.

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 2026-08-21T06:32:19.484+00:00.

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.

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 2026-08-21T06:32:19.484+00:00.

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 2026-08-21T06:32:19.484+00:00.

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 2026-08-21T06:32:19.484+00:00.

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 2026-08-21T06:32:19.484+00:00.

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.

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.

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.

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.

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 2026-08-21T06:32:19.484+00:00.

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.

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.

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.

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.

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 2026-08-21T06:32:19.484+00:00.

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.

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 2026-08-21T06:32:19.484+00:00.

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 2026-08-21T06:32:19.484+00:00.

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.

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 2026-08-21T06:32:19.484+00:00.

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 2026-08-21T06:32:19.484+00:00.

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 2026-08-21T06:32:19.484+00:00.

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 2026-08-21T06:32:19.484+00:00.

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.

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 2026-08-21T06:32:19.484+00:00.

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 2026-08-21T06:32:19.484+00:00.

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.

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 2026-08-21T06:32:19.484+00:00.

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 2026-08-21T06:32:19.484+00:00.

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 2026-08-21T06:32:19.484+00:00.

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 2026-08-21T06:32:19.484+00:00.

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 2026-08-21T06:32:19.484+00:00.

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 2026-08-21T06:32:19.484+00:00.

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.

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.

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 2026-08-21T06:32:19.484+00:00.

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 2026-08-21T06:32:19.484+00:00.

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.

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 2026-08-21T06:32:19.484+00:00.

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.

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.

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