Found in: ključnih besedahSummary of found: ...ass="IskanaBeseda">ass="Iskass="IskanaBeseda">anass="IskanaBeseda">aBesedass="IskanaBeseda">a">The ass="IskanaBeseda">ass="Iskass="IskanaBeseda">anass="IskanaBeseda">aBesedass="IskanaBeseda">a">ass="IskanaBeseda">ass="Iskass="IskanaBeseda">anass="IskanaBeseda">aBesedass="IskanaBeseda">a">intermediass="IskanaBeseda">ate ass="IskanaBeseda">ass="Iskass="IskanaBeseda">anass="IskanaBeseda">aBesedass="IskanaBeseda">a">Pass="IskanaBeseda">alomass="IskanaBeseda">ar ass="IskanaBeseda">ass="Iskass="IskanaBeseda">anass="IskanaBeseda">aBesedass="IskanaBeseda">a">Trass="IskanaBeseda">ansient ass="IskanaBeseda">ass="Iskass="IskanaBeseda">anass="IskanaBeseda">aBesedass="IskanaBeseda">a">Fass="IskanaBeseda">acass="IskanaBeseda">ass="Iskass="IskanaBeseda">anass="IskanaBeseda">aBesedass="IskanaBeseda">a">tory ass="IskanaBeseda">ass="Iskass="IskanaBeseda">anass="IskanaBeseda">aBesedass="IskanaBeseda">a">(ATel ass="IskanaBeseda">ass="Iskass="IskanKeywords: The intermediate Palomar Transient Factory (ATel #4807) reports the discovery and classification of the following Type Ia SNe. Our automated candidate vetting to distinguish a real astrophysical source (1.0) from bogus artifacts (0.0) is powered by three generations of machine learning algorithms: RB2 (Brink et al. 2013MNRAS.435.1047B), RB4 (Rebbapragada et al. 2015AAS...22543402R) and RB5 (Wozniak et al. 2013AAS...22143105W).Published: 24.01.2018; Views: 2587; Downloads: 0 Fulltext (340,58 KB)
