activity
20192026
most citedThree Years of HARPS-N High-Resolution Spectroscopy and Precise Radial Velocity Data for the Sun

122 citations · 1.3k across the 55 of their papers we have counts for

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12 papers · 1 filter

astro-ph.SR2026

gr8stars II : judgement day for spectroscopic parameter model systematics

Alix Violet Freckelton, Annelies Mortier, Megan Bedell +18

Many areas of astrophysics, including exoplanetary studies, rely on precise and accurate stellar parameters. This demands that uncertainties on these parameters truly reflect all b…

astro-ph.SR2025★ 3 cited

A Decade of Solar High-Fidelity Spectroscopy and Precise Radial Velocities from HARPS-N

X. Dumusque, K. Al Moulla, M. Cretignier +53

We recently released 10 years of HARPS-N solar telescope and the goal of this manuscript is to present the different optimisations made to the data reduction, to describe data cura…

astro-ph.SR2025★ 2 cited

Solar Flux Atlases: The new HARPS-N Quiet Sun Benchmark and Ca II H & K Lines Continuum Normalisation

F. Hanassi-Savari, A. G. M. Pietrow, M. K. Druett +2

Context. Solar flux atlases observe the spatially integrated light from the Sun, treating it as a star. They are fundamental tools for gaining insight into the composition of the S…

astro-ph.SR2025

Measuring the Suns radial velocity variability due to supergranulation over a magnetic cycle

Niamh K. O'Sullivan, Suzanne Aigrain, Michael Cretignier +9

In recent years supergranulation has emerged as one of the biggest challenges for the detection of Earth-twins in radial velocity planet searches. We used eight years of Sun-as-a-s…

astro-ph.SR2024★ 5 cited

Precise and efficient modeling of stellar-activity-affected solar spectra using SOAP-GPU

Yinan Zhao, Xavier Dumusque, Michael Cretignier +4

One of the main obstacles in exoplanet detection when using the radial velocity (RV) technique is the presence of stellar activity signal induced by magnetic regions. In this conte…

astro-ph.SR2024

Stellar surface information from the Ca II H&K lines -- II. Defining better activity proxies

M. Cretignier, N. C. Hara, A. G. M. Pietrow +6

In our former paper I, we showed on the Sun that different active regions possess unique intensity profiles on the Ca II H & K lines. We now extend the analysis by showing how thos…