Pulsar Classification For Class Prediction
Features of Pulsar Obs. For Prediction Models
@kaggle.brsdincer_pulsar_classification_for_class_prediction
Features of Pulsar Obs. For Prediction Models
@kaggle.brsdincer_pulsar_classification_for_class_prediction
17898 entries
Data can be useful for prediction models of classification.
COLUMNS:
Based on Integrated Profile of Observation
Mean_Integrated: Mean of Observations
SD: Standard deviation of Observations
EK: Excess kurtosis of Observations
Skewness: In probability theory and statistics, skewness is a measure of the asymmetry of the probability distribution of a real-valued random variable about its mean. Skewness of Observations.
Mean _ DMSNR _ Curve: Mean of DM SNR CURVE of Observations
SD _ DMSNR _ Curve: Standard deviation of DM SNR CURVE of Observations
EK _ DMSNR _ Curve: Excess kurtosis of DM SNR CURVE of Observations
Skewness _ DMSNR _ Curve: Skewness of DM SNR CURVE of Observations
Class: Class 0 - 1
WHAT IS DM SNR CURVE:
Radio waves emitted from pulsars reach earth after traveling long distances in space which is filled with free electrons. The important point is that pulsars emit a wide range of frequencies, and the amount by which the electrons slow down the wave depends on the frequency. Waves with higher frequency are sowed down less as compared to waves with higher frequency. It means dispersion.
TARGET:
Class
0 -- It is not
1 -- It is
CREATE TABLE pulsar (
"mean_integrated" DOUBLE,
"sd" DOUBLE,
"ek" DOUBLE,
"skewness" DOUBLE,
"mean_dmsnr_curve" DOUBLE,
"sd_dmsnr_curve" DOUBLE,
"ek_dmsnr_curve" DOUBLE,
"skewness_dmsnr_curve" DOUBLE,
"class" BIGINT
);
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