Exposure-integrated Gaussian processes allow prediction of both latent stellar signals and instrument-specific binned versions, supporting combination of overlapping EPRV datasets with varying exposure times.
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3D simulations of strongly magnetic solar granulation reveal convective redshifts in absorption lines, originating from hot down-moving elements created by shocks and adiabatic compression in magnetically channeled flows.
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Exposure-averaged Gaussian Processes for Combining Overlapping Datasets
Exposure-integrated Gaussian processes allow prediction of both latent stellar signals and instrument-specific binned versions, supporting combination of overlapping EPRV datasets with varying exposure times.
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Solar photospheric spectrum microvariability III. Radial velocities and line profiles in magnetic active-region granulation
3D simulations of strongly magnetic solar granulation reveal convective redshifts in absorption lines, originating from hot down-moving elements created by shocks and adiabatic compression in magnetically channeled flows.