Difference between revisions of "NOvA pictures of the month"

From AstroNuWiki
Jump to: navigation, search
Line 1: Line 1:
 
<gallery widths=500px heights=300px>
 
<gallery widths=500px heights=300px>
 +
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]]
 
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 17:06, 11 April 2019

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