Constraining the intrinsic population of long gamma-ray bursts: Implications for spectral correlations, cosmic evolution, and their use as tracers of star formation

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Table 2.

Summary of the various mock samples created for our population model.

Sample name	E_min, obs – E_max, obs	Threshold
CGRO/BATSE	50–300 keV	0.067 ph s⁻¹ cm⁻²
Fermi/GBM^bright	50–300 keV	0.9 ph s⁻¹ cm⁻²
Swift/eBAT6	15–150 keV	2.6 ph s⁻¹ cm⁻²

HETE2	2–10 keV	1 ph s⁻¹ cm⁻²
	30–400 keV	1 ph s⁻¹ cm⁻²
SHOALS	15–150 keV	1 × 10⁻⁶ erg cm⁻²

Notes. The top part of the table corresponds to the samples used for fitting the observation constraints presented in Sect. 3. The bottom part of the table lists additional samples used for predictions or additional crosschecks.

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