Center-to-limb variation of spectral lines and continua observed with SST/CRISP and SST/CHROMIS

Observations of center-to-limb variations (CLV) spectral lines and continua provide a good test for the accuracy models solar stellar atmospheric structure spectral-line formation. They are also widely used to constrain elemental abundances becoming increasingly important in studies exoplanets. However, only few such data sets exist chromospheric lines. We aim create set standard profiles by means mosaics made with CRISP CHROMIS instruments Swedish 1-m Solar Telescope (SST), as well explore robustness said obtained using this method. For each line we use mosaic that ranges from center limb. Each these averaged down 50 individual profiles, spaced 0.02 $\mu$ scale. These corrected p-mode oscillations, their parameters (equivalent width, shift, full-width at half-maximum, depth) then compared against literature values where possible. present average equidistantly along cosine heliocentric angle ($\mu$) steps five continuum points between 4001 7772 \AA, ten most commonly observed SST (Ca II H & K, H$\beta$, Mg I 5173 C 5380 Fe 6173 6301 H$\alpha$, O Ca 8542 \AA). Center-to-limb variation shared CDS machine-readable tables; providing quantitative constraint on theoretical model atmospheres.