Simultaneous and panchromatic observations of the fast radio burst FRB 20180916B

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Table 1.

Details of the radio instruments involved in the R3 MWL campaign.

Telescope	Receiver	ν_c	BW	dt	dν	SEFD
		[MHz]	[MHz]	[μs]	[kHz]	[Jy]	[Jy ms]
SRT	L/PL-band	1547	512	125	1000	37	0.4
	L/PP-band	336	80	128	250	215	4.6
uGMRT	Band-3	400	200	81.92	97.65	(502/N_A)	0.6

Notes. For each instrument we report the central frequency ν_c, observational bandwidth BW, sampling time dt, spectral resolution dν, system equivalent flux density (SEFD) and the fluence density^(a) threshold (S/N = 6) . N_A is the number of antennas deployed with the uGMRT array.

^(a)

Throughout this work, we refer to the source irradiated energy per surface unit as the ‘fluence’, and to the fluence per frequency unit as the ‘fluence density’.

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