A scaled-up planetary system around a supernova progenitor

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Table 6

Details of the observations of μ² Sco.

UT Date	Instr.	Filter	DIT (s)	N_exp	Rot(°)	Seeing(")	Strehl H band	Airmass	True north corr. (°)	Platescale (mas pixel⁻¹)
2018-04-24	IFS	YJH	16	174	53.0	0.35	0.91	1.03	−1.761 ± 0.06	7.46 ± 0.02
2018-04-24	IRDIS	K12	16	104	43.8	0.35	0.91	1.03	−1.761 ± 0.06	12.256 ± 0.016
2021-06-04	IFS	YJH	16	186	53.2	0.33	0.90	1.03	−1.780 ± 0.07	7.46 ± 0.02
2021-06-04	IRDIS	K12	16	161	51.3	0.33	0.90	1.03	−1.780 ± 0.07	12.261 ± 0.005

Notes. DIT is the integration time, N_exp the number of frames after selection (out of 192 frames), Rot is the total FoV rotation. The seeing and the Strehl ratio are averages over the duration of the exposures.

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