Difference between revisions of "NOvA pictures of the month"

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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]]
 
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]]
 
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]]
 
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.
 
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.

Revision as of 12:10, 18 September 2019

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