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Uute toodete turule toomisel hindame alati nende kestlikkust (nii toote kui ka pakendi osas) ja teeme parimaid valikuid. Vaatame pidevalt üle olemasolevaid pakendilahendusi ja muudame neid paremaks. Teie isikuandmetega tutvuvad ning neid töötlevad isikud, kes tegelevad teie avalduse hindamisega, näiteks personaliosakond ja vastavad juhid. Orkla töötajatel on õigus saada juurdepääs isikuandmetele ainult ulatuses, milles see on vajalik vastava eesmärgi täitmiseks.

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Tegeleme pidevalt biojäätmete tekke vähendamisega. Võrreldes 2016. aastaga oleme biojäätmeid kahandanud 950 tonnilt 650 tonnile ehk umbes 30%. Näiteks sel aastal võtsime kasutusse uue aurukoorija, mis aitab koorimiskadusid vähendada 50%. where normalisation factor F TT (see Eq. (11)) comes from the integration over nuisance parameter a. The χ 2 defines the quantity to be minimised and is defined as where in the second step we applied the Bayes’ theorem. The last expression p( F | z, T) gives the probability that the measured relative fluxes F correspond to the template T at redshift z. We assume that the probability does not depend on the magnitude m 0. The prior p( z, T | m 0) can be further developed using the product ruleLet us denote the set of selected templates as V so that each set V belongs to the overall set containing all possible combinations V⊂ V master while the number of templates in set V is fixed at N T . For every galaxy, we selected the best-matching template and the corresponding value from V by calculating

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However, the galaxies shown in Fig. 14 make up only ~8% of the whole sample. For most of the other galaxies, the effect of the photometric correction is much more subtle and for around 75% of the galaxies in the catalogue, the effect is so negligible that it does not affect their photometric redshift accuracy. Out of the listed factors, we only had considerable control over the templates. We tested different approaches for optimising the set of templates. The optimal base template set depends on the overall configuration of the workflow (with priors, without priors, with priors and added corrections, and so on). In addition, inputs that produce good results with one observational data set may not be the best for others. Most notably, template set tuned for brighter sources is not optimal for fainter, noise-dominated sources. The same may apply for the targeted redshift range; however, the current data did not allow us to investigate such dependencies. Similarly, we can expect that more sophisticated prior, which considers the expected abundance of a given spectral type at a given redshift, can further improve the accuracy of redshifts. The necessary observational information can come from the same data being analysed, but the number of sources has to be considerably larger. For best results, it is necessary to adjust the inputs separately for each specific set of data and also the science goal.From Fig. 3, it can be seen that the 500 brightest galaxies that we used for the template construction have redshifts z≲ 0.7 while the brighter test sample extends farther, z≲ 1. However, since evolutionary effects become important at much higher red-shifts, it is very unlikely that there are galaxy types in our test catalogue that are not represented by the 500 brightest galaxies and therefore no additional templates are needed to compensate for the redshift difference. A test on how under or over-represented templates affect the resulting redshift estimations is discussed in Sect. 6.1.1. where summation is over all observed passbands for a given galaxy. F j and are the observed galaxy flux and its standard deviation through passband j while F T,j is the synthetic flux of a redshifted template T through passband j. Oleme aastaid oma toodetes vähendanud järk-järgult nii suhkru kui ka soola osakaalu. Võrreldes 2015. aastaga sisaldavad meie mahlajoogid 12% vähem lisatud suhkruid kui varem. See teeb 60 tonni vähem suhkrut viie aasta jooksul! Kuid meie suhkruvähendamise protsess ei ole lõppenud. Teeme seda järk-järgult edasi. Aastaks 2025 tahame kahandada meie mahlajookide suhkrusisaldust 15%.