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

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Table 4:

Results of PSF-photometry of XTE J0929-314.
Filter	${\lambda}_{\rm c}$	Mean magnitude	$A_{\lambda}$	Absolute mag
	(Å)		(mag)
V	5270	$28.2 \pm 0.4$	$0.46 \pm 0.02$	$13.2 \pm 0.4$
R	6440	$27.1 \pm 0.3$	$0.36 \pm 0.02$	$12.3 \pm 0.3$
I	7980	$26.9 \pm 0.4$	$0.28 \pm 0.02$	$12.1 \pm 0.4$

Values in column three are uncorrected for reddening. In column four we list the reddening parameters used to correct our optical photometry computed assuming $E(B-V)=0.15 \pm 0.02$ mag. The absolute magnitudes are computed assuming a distance of 8 kpc (Wijnands et al. 2005; see Sect. 4.1.1 for details).

Source LaTeX | All tables | In the text

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