An alternating minimization algorithm with trajectory for direct exoplanet detection - The AMAT algorithm

Open Access

Table A.1

Properties of the datasets.

ID	Telescope/Instr	N_img	N_t	∆_field	Np
		(px × px)		(◦)
sph1	VLT/SPHERE-IRDIS	160×160	252	40.3	1
sph2	VLT/SPHERE-IRDIS	160×160	80	31.5	0
sph3	VLT/SPHERE-IRDIS	160×160	228	80.5	5
nrc1	Keck/NIRC2	32l×32l	29	53.0	4
nrc2	Keck/NIRC2	32l×32l	40	37.3	3
nrc3	Keck/NIRC2	32l×32l	50	166.9	0
lmr1	LBT/LMIRCam	200×200	4838	153.4	2
lmr2	LBT/LMIRCam	200×200	3219	60.6	2
lmr3	LBT/LMIRCam	200×200	4620	91.0	3
51 Eri	VLT/SPHERE-IRDIS	200×200	256	42.0	1

Notes. N_im𝑔 is the size of the images, N_t is the number of frames, ∆_field is the total field rotation of the planets, and N_p is the number of the injected planet for EIDC datasets and the number of the real planet for 51 Eri dataset.

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