Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum | Paper Citation Record

Observation d2988fa6-c861-47db-9e60-55a188814d01 · outbound

This paper cites Stellar Surface Magneto-Convection as a Source of Astrophysical Noise. I. Multi-component Parameterisation of Absorption Line Profiles.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum Stellar Surface Magneto-Convection as a Source of Astrophysical Noise. I. Multi-component Parameterisation of Absorption Line Profiles

Reference 1

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Observation df3ac795-efa9-4dc3-b26a-19ca8dcd9f5f · outbound

This paper cites Amplitudes of solar-like oscillations: a new scaling relation.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum Amplitudes of solar-like oscillations: a new scaling relation

Reference 2

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Observation 5a183c8a-cb92-4d5e-9cb3-9f0aa4775fb3 · outbound

This paper cites Future Missions in Solar, Heliospheric & Space Plasma Physics , year = 1985, editor =.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum Future Missions in Solar, Heliospheric & Space Plasma Physics , year = 1985, editor =

Reference 3

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Observation 4ecf6436-52f6-489f-a63b-cc561f72fbfe · outbound

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Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum , keywords =

Reference 4

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Observation 17bf42cd-ccb2-4b71-88cd-7d8e42be0c9e · outbound

This paper cites IV - The Fe I curve of growth.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum IV - The Fe I curve of growth

Reference 5

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Observation 8da3cce8-c853-4fd0-a03c-c204a8b9d255 · outbound

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

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum MPS-ATLAS: A fast all-in-one code for synthesising stellar spectra

Reference 6

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Observation b0dac90d-548f-48cb-ac47-be38819c114d · outbound

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

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum Small-scale dynamo in cool main sequence stars. II. The effect of metallicity

Reference 7

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Observation 33f6b9b8-35d5-47d9-9da1-0214a6c1acc0 · outbound

This paper cites Three-dimensional simulations of near-surface convection in main-sequence stars. IV. Effect of small-scale magnetic flux concentrations on centre-to-limb variation and spectral lines.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum Three-dimensional simulations of near-surface convection in main-sequence stars. IV. Effect of small-scale magnetic flux concentrations on centre-to-limb variation and spectral lines

Reference 8

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Observation 134806a0-9fd2-4190-8a4e-2226bba032aa · outbound

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

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum Equations, methods, and results of the MURaM code

Reference 9

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Observation ffed061d-0d2a-4705-a255-e05f368aa3e9 · outbound

This paper cites Towards understanding stellar variability at the sub m/s level: Isolating granulation signals in synthetic spectral lines.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum Towards understanding stellar variability at the sub m/s level: Isolating granulation signals in synthetic spectral lines

Reference 10

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Observation d6b80812-9637-4890-8221-7820e3821a3a · outbound

This paper cites Characterizing Solar Center-to-Limb Radial-Velocity Variability with SDO.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum Characterizing Solar Center-to-Limb Radial-Velocity Variability with SDO

Reference 11

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Observation 3fb4d492-11e0-46dc-b2b0-1074381691b4 · outbound

This paper cites Stellar Surface Magneto-Convection as a Source of Astrophysical Noise II. Center-to-Limb Parameterisation of Absorption Line Profiles and Comparison to Observations.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum Stellar Surface Magneto-Convection as a Source of Astrophysical Noise II. Center-to-Limb Parameterisation of Absorption Line Profiles and Comparison to Observations

Reference 12

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Observation 43e78d3b-62b5-41be-bca7-74480065db73 · outbound

This paper cites Stellar Surface Magneto-Convection as a Source of Astrophysical Noise III. Sun-as-a-star Simulations and Optimal Noise Diagnostics.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum Stellar Surface Magneto-Convection as a Source of Astrophysical Noise III. Sun-as-a-star Simulations and Optimal Noise Diagnostics

Reference 13

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Observation 81dfccfb-5d14-4260-bb83-4dcaf68c1bcf · outbound

This paper cites High-accuracy observations of spectral lines in the visible , author=.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum High-accuracy observations of spectral lines in the visible , author=

Reference 14

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Observation a968bc30-3b98-4179-a9ed-fed394d86e85 · outbound

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

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum Testing MURaM and MPS-ATLAS against the quiet solar spectrum

Reference 15

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Observation 9a49fe69-649e-45a4-9124-724fc246b84b · outbound

This paper cites Numerical simulations of quiet Sun magnetism: On the contribution from a small-scale dynamo.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum Numerical simulations of quiet Sun magnetism: On the contribution from a small-scale dynamo

Reference 16

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Observation 02f80845-e9e3-4931-851f-a1627b2fe57b · outbound

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Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum Unresolved cited work

Reference 17

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Observation 3d95dc9f-374e-4b57-9b9c-9a67d92b0aeb · outbound

This paper cites Using the Sun to estimate Earth-like planets detection capabilities II. Impact of plages.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum Using the Sun to estimate Earth-like planets detection capabilities II. Impact of plages

Reference 18

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Observation 874a6b93-822e-411d-ac23-f34ecf98f20a · outbound

This paper cites Ground-based and airborne instrumentation for astronomy vi , volume=.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum Ground-based and airborne instrumentation for astronomy vi , volume=

Reference 19

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Observation 798207bb-f95a-4642-ac5e-52f9166e09a9 · outbound

This paper cites The Messenger , year = 2013, month = sep, volume =.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum The Messenger , year = 2013, month = sep, volume =

Reference 20

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Observation 927180ec-304e-4500-bf99-a70aa744d2e5 · outbound

This paper cites Identifying Exoplanets with Deep Learning. IV. Removing Stellar Activity Signals from Radial Velocity Measurements Using Neural Networks.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum Identifying Exoplanets with Deep Learning. IV. Removing Stellar Activity Signals from Radial Velocity Measurements Using Neural Networks

Reference 21

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Observation 3c908eae-a7a2-48b2-8b87-58af22bd031a · outbound

This paper cites The EXPRES Stellar Signals Project II. State of the Field in Disentangling Photospheric Velocities.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum The EXPRES Stellar Signals Project II. State of the Field in Disentangling Photospheric Velocities

Reference 22

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Observation 04933e6e-99b9-4faf-ad96-839fe8ab51e0 · outbound

This paper cites The Impact of Stellar Surface Magnetoconvection and Oscillations on the Detection of Temperate, Earth-Mass Planets Around Sun-Like Stars.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum The Impact of Stellar Surface Magnetoconvection and Oscillations on the Detection of Temperate, Earth-Mass Planets Around Sun-Like Stars

Reference 23

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Observation c7c19dfd-fcf8-46ab-893e-165ac5cfb3a1 · outbound

This paper cites , volume=.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum , volume=

Reference 24

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Observation 4431d4f1-4f99-492a-95e9-b117284835bc · outbound

This paper cites 15856 , author=.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum 15856 , author=

Reference 25

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Observation db164aea-6f3d-4779-9982-f2bc0a28a758 · outbound

This paper cites A Gaussian process framework for modelling stellar activity signals in radial velocity data.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum A Gaussian process framework for modelling stellar activity signals in radial velocity data

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Observation 5c615920-4f7d-4493-99a3-a23103365434 · outbound

This paper cites Improving Exoplanet Detection Power: Multivariate Gaussian Process Models for Stellar Activity.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum Improving Exoplanet Detection Power: Multivariate Gaussian Process Models for Stellar Activity

Reference 27

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Observation f8cef320-2305-4d87-a080-297fd5393c47 · outbound

This paper cites Planetary detection limits taking into account stellar noise. I. Observational strategies to reduce stellar oscillation and granulation effects.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum Planetary detection limits taking into account stellar noise. I. Observational strategies to reduce stellar oscillation and granulation effects

Reference 28

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Observation a0deb917-7b5c-434b-9d53-bc292f790108 · outbound

This paper cites , keywords =.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum , keywords =

Reference 29

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Observation 0b835fed-7ccc-4f38-bd60-ffacd1906685 · outbound

This paper cites Granulation in K-type Dwarf Stars. I. Spectroscopic observations.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum Granulation in K-type Dwarf Stars. I. Spectroscopic observations

Reference 30

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Observation 05fcfe06-1e38-44c0-8fef-5fd0a7570da0 · outbound

This paper cites Fe I line shifts in the optical spectrum of the Sun.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum Fe I line shifts in the optical spectrum of the Sun

Reference 31

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Observation 1af0d7d3-3c8d-434a-a070-bdfe7dfe8c44 · outbound

This paper cites Three Years of HARPS-N High-Resolution Spectroscopy and Precise Radial Velocity Data for the Sun.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum Three Years of HARPS-N High-Resolution Spectroscopy and Precise Radial Velocity Data for the Sun

Reference 32

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Observation 1acf1a84-d3f2-4d99-a51d-7c369e5cb49c · outbound

This paper cites Journal of Machine Learning Research , volume =.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum Journal of Machine Learning Research , volume =

Reference 33

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Observation 3fe13781-751a-4e72-906c-4e4e2889c2a6 · outbound

This paper cites The chemical make-up of the Sun: A 2020 vision.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum The chemical make-up of the Sun: A 2020 vision

Reference 34

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Observation ee1457cd-d2f5-4239-9324-e83d310739ad · outbound

This paper cites Stellar signal components seen in HARPS and HARPS-N solar radial velocities.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum Stellar signal components seen in HARPS and HARPS-N solar radial velocities

Reference 35

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Observation 3dc45382-f694-4b5e-9fc6-69a567edc546 · outbound

This paper cites Modelling stochastic and quasi-periodic behaviour in stellar time-series: Gaussian process regression versus power-spectrum fitting.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum Modelling stochastic and quasi-periodic behaviour in stellar time-series: Gaussian process regression versus power-spectrum fitting

Reference 36

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Observation 65cd3d93-fdc4-4787-a964-b34d8a645a2c · outbound

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Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum , keywords =

Reference 37

Resolution: verified exact; doi, observed 2026-08-04T10:58:21.223513Z

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Observation a1ba7be2-9a10-445e-991a-e223b7e44a8c · outbound

This paper cites Spectral Line Depth Variability in Radial Velocity Spectra.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum Spectral Line Depth Variability in Radial Velocity Spectra

Reference 38

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Observation 8542c1c7-4fd4-4831-adbe-bca1f94cdade · outbound

This paper cites $\texttt{GRASS}$: Distinguishing Planet-induced Doppler Signatures from Granulation with a Synthetic Spectra Generator.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum $\texttt{GRASS}$: Distinguishing Planet-induced Doppler Signatures from Granulation with a Synthetic Spectra Generator

Reference 39

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Observation de926881-9ab6-4da9-8ceb-05e5bc5507fb · outbound

This paper cites GRASS II: Simulations of Potential Granulation Noise Mitigation Methods.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum GRASS II: Simulations of Potential Granulation Noise Mitigation Methods

Reference 40

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Observation 1c706a1d-6c0d-4caf-8c7a-b031e5039a44 · outbound

This paper cites The CARMENES search for exoplanets around M dwarfs. Line-by-line sensitivity to activity in M dwarfs.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum The CARMENES search for exoplanets around M dwarfs. Line-by-line sensitivity to activity in M dwarfs

Reference 41

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Observation 4554a7c1-d0e9-4d25-8a12-c46f5d1a1a55 · outbound

This paper cites Measuring precise radial velocities on individual spectral lines. III. Dependence of stellar activity signal on line formation temperature.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum Measuring precise radial velocities on individual spectral lines. III. Dependence of stellar activity signal on line formation temperature

Reference 42

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Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum Unresolved cited work

Reference 43

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Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum Unresolved cited work

Reference 44

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This paper cites An Open Source, Massively Parallel Code for Non-LTE Synthesis and Inversion of Spectral Lines and Zeeman-induced Stokes Profiles.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum An Open Source, Massively Parallel Code for Non-LTE Synthesis and Inversion of Spectral Lines and Zeeman-induced Stokes Profiles

Reference 45

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Observation 1f643c0e-6200-4c5a-8929-3a9c361953ae · outbound

This paper cites Does the radial-tangential macroturbulence model adequately describe the spectral line broadening of solar-type stars?.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum Does the radial-tangential macroturbulence model adequately describe the spectral line broadening of solar-type stars?

Reference 46

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Observation 728b18f1-a43b-424c-b13b-206b2dbb50db · outbound

This paper cites Why one-dimensional models fail in the diagnosis of average spectra from inhomogeneous stellar atmospheres.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum Why one-dimensional models fail in the diagnosis of average spectra from inhomogeneous stellar atmospheres

Reference 47

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Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum Unresolved cited work

Reference 48

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Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum , keywords =

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Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum Unresolved cited work

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This paper cites Cambridge Astrophysics Series.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum Cambridge Astrophysics Series

Reference 51

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Observation 7e3dd4ee-f2ce-4035-9de8-a19f2fa542fa · outbound

This paper cites Convective blueshifts in the solar atmosphere, I. Absolute measurements with LARS of the spectral lines at 6302 {\AA}.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum Convective blueshifts in the solar atmosphere, I. Absolute measurements with LARS of the spectral lines at 6302 {\AA}

Reference 52

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Observation 167b4ea8-c160-46fd-a170-eb753e29622e · outbound

This paper cites Sensitivity of spectral lines to granulation: The Sun.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum Sensitivity of spectral lines to granulation: The Sun

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Observation 3c1ae0be-ec07-4fed-a5bb-681674a3500e · outbound

This paper cites The PLATO 2.0 Mission.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum The PLATO 2.0 Mission

Reference 54

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Observation 021914d8-45d9-4b9d-b881-1ce73e235162 · outbound

This paper cites The PLATO Mission.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum The PLATO Mission

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Resolution: unresolved; no resolver link, observed 2026-08-04T10:56:50.600250Z

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Observation 2d68864e-6df5-49e3-a6ab-6f8ba998de4f · outbound

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Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum The PLATO Mission

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Observation 1ad7bf2c-54ff-4d40-81f5-30b57a97c2d2 · outbound

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Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum , keywords =

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Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum , keywords =

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Observation acdf2de4-3c13-44c3-8da3-a29e328753e6 · outbound

This paper cites Line formation in solar granulation: I. Fe line shapes, shifts and asymmetries.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum Line formation in solar granulation: I. Fe line shapes, shifts and asymmetries

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Observation 3f745f88-8ae7-447e-94ff-333d638851c4 · outbound

This paper cites The Messenger , year = 2025, month = mar, volume =.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum The Messenger , year = 2025, month = mar, volume =

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Observation 77af7588-aec2-4a6e-aea8-566fd5d5c65c · outbound

This paper cites 3D magneto-hydrodynamical simulations of stellar convective noise for improved exoplanet detection. I. Case of regularly sampled radial velocity observations.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum 3D magneto-hydrodynamical simulations of stellar convective noise for improved exoplanet detection. I. Case of regularly sampled radial velocity observations

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Observation 81378205-f916-4cd8-8451-952d672dafea · outbound

This paper cites Performance Verification of the EXtreme PREcision Spectrograph.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum Performance Verification of the EXtreme PREcision Spectrograph

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Observation d13865ce-7358-4242-8755-dc8c2485658e · outbound

This paper cites Oxygen lines in solar granulation. I. Testing 3D models against new observations with high spatial and spectral resolution.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum Oxygen lines in solar granulation. I. Testing 3D models against new observations with high spatial and spectral resolution

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Observation 5311c1de-bbb8-4c76-857f-e53beab307de · outbound

This paper cites The IAG spectral atlas of the spatially resolved Sun: Centre-to-limb observations.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum The IAG spectral atlas of the spatially resolved Sun: Centre-to-limb observations

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Resolution: unresolved; no resolver link, observed 2026-08-04T10:56:50.646821Z

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Observation 918c7209-12be-4f2e-8702-e46f21de05ca · outbound

This paper cites Convective blueshift strengths of 810 F to M solar-type stars.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum Convective blueshift strengths of 810 F to M solar-type stars

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Observation 2ad9e515-fdfa-4bf7-a079-10a212f97995 · outbound

This paper cites Convective blueshift strengths for 242 evolved stars.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum Convective blueshift strengths for 242 evolved stars

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Observation 52cd1fcc-5414-4bb1-8359-adb181707040 · outbound

This paper cites The Stagger-grid: A grid of 3D stellar atmosphere models - V. Fe line shapes, shifts and asymmetries.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum The Stagger-grid: A grid of 3D stellar atmosphere models - V. Fe line shapes, shifts and asymmetries

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Observation 3f2e77cf-f79e-4d4a-977c-555f807edd5d · outbound

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Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum Convective characteristics of Fe I lines across the solar disc

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Observation 76e78806-cacd-415c-b611-9874e49e6959 · outbound

This paper cites LARS - An Absolute Reference Spectrograph for solar observations, Upgrade from a prototype to a turn-key system.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum LARS - An Absolute Reference Spectrograph for solar observations, Upgrade from a prototype to a turn-key system

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Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum , keywords =

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Observation 595e5dad-c5e5-4d08-9692-2eaebabbc9bd · outbound

This paper cites 'Ultimate' Information Content in Solar and Stellar Spectra: Photospheric line asymmetries and wavelength shifts.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum 'Ultimate' Information Content in Solar and Stellar Spectra: Photospheric line asymmetries and wavelength shifts

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Observation 0c8131c2-20bc-4021-be04-ef10e6720d40 · outbound

This paper cites Solar Photospheric Spectrum Microvariability I. Theoretical searches for proxies of radial-velocity jittering.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum Solar Photospheric Spectrum Microvariability I. Theoretical searches for proxies of radial-velocity jittering

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Observation 4ae44f0f-4f60-4ed6-bb7a-169f37008c52 · outbound

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Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum Measuring precise radial velocities on individual spectral lines : II. Dependance of stellar activity signal on line depth

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Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum , year = 1994, month = aug, volume =

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Observation 2ec6c2c3-09b2-4b9a-a374-907b0bf17d15 · outbound

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Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum Predicting convective blueshift and radial-velocity dispersion due to granulation for FGK stars

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Observation 03c446aa-2a3b-411d-aa94-956398d8f3ca · outbound

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Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum The magnetically quiet solar surface dominates HARPS-N solar RVs during low activity

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Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum , keywords =

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Observation b9c04cef-8f53-4f44-971d-606306520246 · outbound

This paper cites Spectral signatures as a function of line-formation temperature.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum Spectral signatures as a function of line-formation temperature

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Observation b4ea5ed0-496e-444f-ba51-9fe14f3a1605 · outbound

This paper cites Three years of Sun-as-a-star radial-velocity observations on the approach to solar minimum.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum Three years of Sun-as-a-star radial-velocity observations on the approach to solar minimum

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Observation 5e87ae81-3e37-4469-9b65-cffe10324aa4 · outbound

This paper cites Separating planetary reflex Doppler shifts from stellar variability in the wavelength domain.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum Separating planetary reflex Doppler shifts from stellar variability in the wavelength domain

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Observation 58651479-06d9-4d87-bcaa-df4c5d2b8d2f · outbound

This paper cites The relationship between photometric and spectroscopic oscillation amplitudes from 3D stellar atmosphere simulations.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum The relationship between photometric and spectroscopic oscillation amplitudes from 3D stellar atmosphere simulations

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Observation a4f2a189-590b-4df5-9703-6211a34ef3e9 · outbound

This paper cites an unresolved cited work.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum Unresolved cited work

Reference 82

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Observation 24343075-698c-407f-b6d9-7c92bd4c267a · outbound

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Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum The IAG solar flux atlas: Accurate wavelengths and absolute convective blueshift in standard solar spectra

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Observation bb205289-4c73-45ce-85fe-bd37431fcfc7 · outbound

This paper cites The Impact of Very High S/N Spectroscopy on Stellar Physics , year = 1988, editor =.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum The Impact of Very High S/N Spectroscopy on Stellar Physics , year = 1988, editor =

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Observation ef6155fb-e7ef-4a32-b997-2d76ccd0610f · outbound

This paper cites First stars V - Abundance patterns from C to Zn and supernova yields in the early Galaxy.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum First stars V - Abundance patterns from C to Zn and supernova yields in the early Galaxy

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Observation a2621d2d-7ea0-42eb-be87-4d300744902d · outbound

This paper cites Extremely Metal-Poor Stars. VIII. High-Resolution, High-Signal-To-Noise Analysis of Five Stars with [Fe/H] < -3.5.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum Extremely Metal-Poor Stars. VIII. High-Resolution, High-Signal-To-Noise Analysis of Five Stars with [Fe/H] < -3.5

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Observation 988da0ff-a27a-494c-9c86-2362cd513bf0 · outbound

This paper cites , year = 2015, month = may, volume =.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum , year = 2015, month = may, volume =

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This paper cites , keywords =.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum , keywords =

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Observation 806fe54f-2394-4f16-92fc-3ee7028fae4e · outbound

This paper cites , keywords =.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum , keywords =

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This paper cites an unresolved cited work.

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Reference 90

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Observation 7fd5519b-6ea4-478a-9541-83ad82c750ad · outbound

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Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum The Stagger-grid: A Grid of 3D Stellar Atmosphere Models - II. Horizontal and Temporal Averaging and Spectral Line Formation

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Observation d2703d58-dca2-4941-a54e-1cb5fe300b02 · outbound

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Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum HARPS3 for a Roboticized Isaac Newton Telescope

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Observation 4bde11f8-9baf-4c77-a3ea-c29f5e4499f6 · outbound

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Observation aa95ec93-45d2-45d9-9069-4ecdd4666257 · outbound

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Observation 53fd3940-4629-4ea1-a3d5-d97b33521df0 · outbound

This paper cites American Astronomical Society Meeting Abstracts \#231 , year = 2018, series =.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum American Astronomical Society Meeting Abstracts \#231 , year = 2018, series =

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Observation f551a5ff-5f21-477b-9148-5b6e95fff804 · outbound

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Observation b7419f36-8735-4776-a4b6-d03f5ad0a9aa · outbound

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Observation ccf3a526-c3e8-4acf-8e48-701c9b6aa4b8 · outbound

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Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum , keywords =

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Resolution: unresolved; no resolver link, observed 2026-08-04T10:56:50.847149Z

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Observation e7647244-754f-4d69-ac8d-13a890d9cb66 · outbound

This paper cites 2023 , eprint=.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum 2023 , eprint=

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