lightcurvelynx.astro_utils.obs_utils
Functions
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Photometric detection efficiency as a simple step function of snr. |
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Spectroscopic follow-up efficiency as a function of peak i band magnitude. |
Module Contents
- phot_eff_function(snr)[source]
Photometric detection efficiency as a simple step function of snr.
- Parameters:
snr (list or numpy.ndarray) – Signal to noise ratio of a list of observations.
- Returns:
eff – The photometric detection efficiency given snr.
- Return type:
list or numpy.ndarray
- spec_eff_function(peak_imag)[source]
Spectroscopic follow-up efficiency as a function of peak i band magnitude.
- Parameters:
peak_imag (list or numpy.ndarray) – Peak magnitude in i band.
- Returns:
eff – The spectroscopic efficiency given peak i band magnitude. Based on Equation (17) in Kessler et al. 2019 s0, s1, s2 are fitted using data from Figure 4 in Kessler et al. 2019
- Return type:
list or numpy.ndarray