Difference between revisions of "NOvA pictures of the month"

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Image: NOvA_Picture_of_March_2019.png | '''Mar-2019''' Пример работы сервера, комбинирующего показания с ближнего и дальнего детекторов, а также двух тестовых “экспериментов“. Можно видеть, как число точек на чёрной кривой адаптируется под количество подключенных экспериментов. The picture by [[Andrey Sheshukov at NOvA|Andrey Sheshukov]]
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Image: NOvA_Picture_of_March_2019.png | '''Mar-2019''' A toy example of server, combining supernova observation significances from various "experiments". Currently they are just fake clients, sending the gaussian random values to the server. The black curve is the combined significance. This is the way we expect the experiments to collaborate in the supernova hunt in future! The picture by [[Andrey Sheshukov at NOvA|Andrey Sheshukov]]
 
Image: NOvA_Picture_of_February_2019.png | '''Feb-2019''' Validation of GenieSNova simulation: number of candidates, which passed the reconstruction and selection in SuperNovaDDT (blue line), incomparison with the expected rate (black line: product of analytical signal shape, reconstruction efficiency etc.). Our simulation is correct!. The picture by [[Andrey Sheshukov at NOvA|Andrey Sheshukov]]
 
Image: NOvA_Picture_of_February_2019.png | '''Feb-2019''' Validation of GenieSNova simulation: number of candidates, which passed the reconstruction and selection in SuperNovaDDT (blue line), incomparison with the expected rate (black line: product of analytical signal shape, reconstruction efficiency etc.). Our simulation is correct!. The picture by [[Andrey Sheshukov at NOvA|Andrey Sheshukov]]
 
Image:NOvA_Picture_of_January_2019.png | '''Jan-2019''' West (blue) and East (orange) fluxes of cosmric ray muons stopping in the Far Detector of NOvA (reweighted to corrected reconstruction efficiency effects) in separated energy intervals. The picture by [[Olga Petrova at NOvA|Olga Petrova]]
 
Image:NOvA_Picture_of_January_2019.png | '''Jan-2019''' West (blue) and East (orange) fluxes of cosmric ray muons stopping in the Far Detector of NOvA (reweighted to corrected reconstruction efficiency effects) in separated energy intervals. The picture by [[Olga Petrova at NOvA|Olga Petrova]]

Revision as of 12:17, 12 April 2019

OlegSamoylov (talk) 01:17, 1 October 2018 (MSK)