A blast from the infant Universe: The very high-z GRB 210905A

Open Access

Table 5.

Parameters of the individual prompt emission pulses.

Episode	E_peak, z	Fluence (15 − 1500 keV) ^(a)	E_iso
	(keV)	(10⁻⁵ erg cm⁻²)	(10⁵³ erg)
Pulse 1
Pulse 2
Pulse 3 ^(b)

Total ^(c)

Notes.

^(a)

Fluences were calculated using the fits with the CPL function from Table 2.

^(b)

Only the KW 3-channel spectrum is used.

^(c)

This fluence is integrated over all three emission episodes.

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