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

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Table 6:

Upper limits ( $3\sigma$ ) on the optical counterpart of XTE J1751-305.
Filter	${\lambda}_{\rm c}$	Limiting magnitude	$A_{\lambda}$	Absolute mag
	(Å)		(mag)
R	6500	>23.1	$4.03 \pm 0.02$	>4.6
I	8000	>21.6	$2.91 \pm 0.02$	>4.2
Z	9625	>20.6	$2.12 \pm 0.02$	>4.0
J	12500	>19.6	$1.35 \pm 0.02$	>3.7

Values in column three are uncorrected for reddening (from Jonker et al. 2003). In column four are reported the dereddening parameters we used to correct for interstellar absorption computed assuming $E(B-V)=1.69 \pm 0.02$ mag The absolute magnitudes are computed assuming a distance of 8 kpc (Wijnands et al. 2005; see Sect. 4.3.1 for details).

Source LaTeX | All tables | In the text

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