Radial distribution of the multiple stellar populations in Centauri

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Table 1:

Data sets used in this work.
Data set	Filter	$\char93$ images ${\times }$ Exp. time (s)
$3\times3$ ACS/WFC	F435W	$27\times 340$ , $9\times12$
inner mosaic
	F625W	$27\times 340$ , $9\times8$
ACS/WFC	F606W	$2\times1285$ , $2\times1300$ ,
$\sim$ 17 $^{\prime }$		$2\times1331$ , $2\times1375$
	F814W	$4\times1331$ , $2\times1340$ , $2\times1375$
WFPC2@HST	F606W	$2\times 300$ , $1\times600$
$\sim$ 7 $^{\prime }$	F814W	$2\times400$ , $1\times 1000$
FORS1@VLT	B	$20\times 1100$
	R	$20\times 395$
WFI@2.2m	B	$1\times10$ , $1\times15$ , $11\times30$ , $1\times40$ ,
		$1\times60$ , $1\times120$ , $2\times240$ , $2\times 300$
	$R_{\rm C}$	$1\times5$ , $1\times10$ , $1\times15$ , $1\times30$ , $5\times60$
	V	$6\times5$ , $9\times10$ , $1\times15$ , $3\times20$ ,
		$2\times30$ , $10\times40$ , $4\times45$ , $3\times60$ ,
		$10\times90$ , $7\times120$ , $1\times150$ , $3\times240$

Source LaTeX | All tables | In the text

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