The optical counterparts of accreting millisecond X-ray pulsars during quiescence

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Table 2:

Results of photometry of XTE J1814-338.
Filter	${\lambda}_{\rm c}$	Mean magnitude	Semiamplitude	$A_{\lambda}$
	(Å)		(mag)	(mag)
V	5270	$23.29 \pm 0.04$	$0.52 \pm 0.08$	$0.87 \pm 0.03$
R	6440	$22.52 \pm 0.03$	$0.32 \pm 0.08$	$0.68 \pm 0.03$

All the values are uncorrected for reddening. In column five are reported the reddening parameters used to correct our optical photometry, computed assuming $E(B-V)=0.29 \pm 0.03$ mag (see Sect. 3.3 for details).

Source LaTeX | All tables | In the text

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