Difference between revisions of "NOvA pictures of the month"

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Image:NOvA_Picture_of_January_2019.png | '''Jan-2019''' West (blue) and East (orange) fluxes of cosmic 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]]
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Image:NOvA_Picture_of_August_2019.png | '''August-2019''' First proceedings at AYSS-2019 conference by [[Anastasia Kalitkina at NOvA|Anastasia Kalitkina]]
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Image: NOvA_Picture_of_July_2019.png | '''July-2019''' SN Betelgeuse neutrino signal simulation based on SND data . The picture by [[Maria Petropavlova at NOvA|Maria Petropavlova]]
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Image: NOvA_Picture_of_June_2019.png | '''June-2019''' Efficiency vs. SN distance for various methods of detectors combination. Percents show the fraction of SN candidates in our galaxy, covered by the combined trigger.
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Last combination method - "Comb" is the best way to do it, where we set a weight to each detector, proportional to their sensitivity to SN signal. The picture by [[Andrey Sheshukov at NOvA|Andrey Sheshukov]]
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Image: NOvA_Picture_of_May2_2019.png | '''May-2019''' Results presented at AYSS-2019 conference by [[Anastasia Kalitkina at NOvA|Anastasia Kalitkina]]
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Image: NOvA_Picture_of_May1_2019.png | '''May-2019''' ROC-Dubna excursion by [[Alexander Antoshkin at NOvA|Alexander Antoshkin]]
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Image: NOvA_Picture_of_April_2019.png | '''Apr-2019''' GENIE comparison workshop at Liverpool, 8-12 April 2019. The picture by [[Igor Kakorin at NOvA|Igor Kakorin]]
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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]]
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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]]
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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_December_2018.png | '''Dec-2018''' Christmas tree in light and dark. Would you see a CP-violation here?. The picture by [[Oleg Samoylov at NOvA|Oleg Samoylov]]
 
Image:NOvA_Picture_of_December_2018.png | '''Dec-2018''' Christmas tree in light and dark. Would you see a CP-violation here?. The picture by [[Oleg Samoylov at NOvA|Oleg Samoylov]]
 
Image:NOvA_Picture_of_November_2018.png | '''Nov-2018''' Пример работы триггера регистрации нейтринного сигнала от взрыва Сверхновых звезд. Как различные формы ожидаемых сигналов будут определять время пришедшего сигнала. The picture by [[Andrey Sheshukov at NOvA|Andrey Sheshukov]]
 
Image:NOvA_Picture_of_November_2018.png | '''Nov-2018''' Пример работы триггера регистрации нейтринного сигнала от взрыва Сверхновых звезд. Как различные формы ожидаемых сигналов будут определять время пришедшего сигнала. The picture by [[Andrey Sheshukov at NOvA|Andrey Sheshukov]]

Latest revision as of 12:10, 18 September 2019

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