Difference between revisions of "NOvA Experiment"

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[[Image:NOvA_Picture_of_May1_2019.png | 300 px]]
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[[Image:NOvA_Picture_of_August_2019.png | 300 px]]
 
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'''May-2019''' ROC-Dubna excursion by [[Alexander Antoshkin at NOvA|Alexander Antoshkin]]
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[[Image:NOvA_Picture_of_May2_2019.png | 300 px]]
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'''May-2019''' Results presented at AYSS-2019 conference by [[Anastasia Kalitkina at NOvA|Anastasia Kalitkina]]
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[[Image:NOvA_Picture_of_June_2019.png | 300 px]]
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'''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_July_2019.png | 300 px]]
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'''July-2019''' SN Betelgeuse neutrino signal simulation based on SND data . The picture by [[Maria Petropavlova at NOvA|Maria Petropavlova]]
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'''August-2019''' First proceedings at AYSS-2019 conference by [[Anastasia Kalitkina at NOvA|Anastasia Kalitkina]]
 
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[[User:OlegSamoylov|OlegSamoylov]] ([[User talk:OlegSamoylov|talk]]) 01:04, 1 October 2018 (MSK)
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[[User:OlegSamoylov|OlegSamoylov]] ([[User talk:OlegSamoylov|talk]]) 12:07, 18 September 2019 (MSK)

Revision as of 12:07, 18 September 2019

NOvA In short
NOvA Graphic 14-0241-01.jpeg
Picture of the month Archive

NOvA Picture of August 2019.png

August-2019 First proceedings at AYSS-2019 conference by Anastasia Kalitkina

OlegSamoylov (talk) 12:07, 18 September 2019 (MSK)