Source code for feets.extractors.ext_eta_color

#!/usr/bin/env python
# -*- coding: utf-8 -*-

# The MIT License (MIT)

# Copyright (c) 2017 Juan Cabral

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# =============================================================================
# FUTURE
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from __future__ import unicode_literals


# =============================================================================
# DOC
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__doc__ = """"""


# =============================================================================
# IMPORTS
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import numpy as np

from .core import Extractor


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# EXTRACTOR CLASS
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[docs]class EtaColor(Extractor): """ **Eta_color** (:math:`\eta_{color}`) Variability index Eta_e (:math:`\eta^e`) calculated from the color light-curve. .. code-block:: pycon >>> fs = feets.FeatureSpace(only=['Eta_color']) >>> features, values = fs.extract(**lc_normal) >>> dict(zip(features, values)) {'Eta_color': 1.991749074648397} References ---------- .. [kim2014epoch] Kim, D. W., Protopapas, P., Bailer-Jones, C. A., Byun, Y. I., Chang, S. W., Marquette, J. B., & Shin, M. S. (2014). The EPOCH Project: I. Periodic Variable Stars in the EROS-2 LMC Database. arXiv preprint Doi:10.1051/0004-6361/201323252. """ data = ['aligned_magnitude', 'aligned_time', 'aligned_magnitude2'] features = ["Eta_color"]
[docs] def fit(self, aligned_magnitude, aligned_time, aligned_magnitude2): N = len(aligned_magnitude) B_Rdata = aligned_magnitude - aligned_magnitude2 w = 1.0 / np.power(aligned_time[1:] - aligned_time[:-1], 2) w_mean = np.mean(w) N = len(aligned_time) sigma2 = np.var(B_Rdata) S1 = sum(w * (B_Rdata[1:] - B_Rdata[:-1]) ** 2) S2 = sum(w) eta_B_R = (w_mean * np.power(aligned_time[N - 1] - aligned_time[0], 2) * S1 / (sigma2 * S2 * N ** 2)) return {"Eta_color": eta_B_R}