Preparation for an unsupervised massive analysis of SPHERE high-contrast data with PACO - Optimization and benchmarking on 24 solar-type stars

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Volume 675 (July 2023)

A&A, 675 (2023) A205

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Table A.3

Star sample observation logs (continuation of Table A.2).

STAR	DATE OBS	FILTER	DIT(s)×Nframe	ΔPA (°)^a	Seeing (")^b	Airmass^b	τ₀ (ms)^a,b	Program ID
HD49855	2015-12-28	DB_H23	64x64	21.4	0.84	1.48	2.9	096.C-0241(C)
HD49855	2015-12-28	OBS_YJ	64x64	21.5	0.83	1.48	2.9	096.C-0241(C)

HD61005	2015-02-03	DB_NDH23	64x64	93.0	0.66	1.01	23.1	095.C-0298(H)
HD61005	2015-02-03	OBS_YJ	64x66	96.9	0.67	1.01	23.1	095.C-0298(H)

HD8558	2015-09-24	DB_H23	64x64	28.8	2.05	1.19	0.9	095.C-0298(D)
HD8558	2015-09-24	OBS_YJ	64x64	28.9	2.05	1.19	0.9	095.C-0298(D)
HD8558	2015-10-28	DB_H23	64x64	28.2	1.02	1.2	2	096.C-0241(A)
HD8558	2015-10-28	OBS_YJ	64x64	28.4	1.02	1.2	2	096.C-0241(A)
HD8558	2016-10-14	DB_H23	64x64	28.2	0.56	1.2	2.8	198.C-0209(A)
HD8558	2016-10-14	OBS_YJ	64x64	28.3	0.56	1.2	2.8	198.C-0209(A)

HD90712	2016-01-03	DB_H23	64x64	74.8	0.67	1.02	6.1	096.C-0241(C)
HD90712	2016-01-03	OBS_YJ	64x64	74.9	0.65	1.02	6.1	096.C-0241(C)

HD987	2016-10-15	DB_H23	64x90	29.7	0.71	1.56	2.2	198.C-0209(A)
HD987	2016-10-15	OBS_YJ	64x90	29.7	0.71	1.56	2.2	198.C-0209(A)

Notes: ^a: DIT corresponds to the detector integration time per frame, ΔPA is the amplitude of the parallactic rotation, τ₀ corresponds to the coherence time. ^b: Values extracted from the updated DIMM info and averaged over the sequence.

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