The G292.0+1.8 pulsar wind nebula in the mid-infrared

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Table 1:

Observed magnitudes and fluxes for the presumed infrared/optical pulsar/PWN counterpart of J1124-5916, and de-reddened fluxes for the A_V range of 1.86-2.10.
$\lambda_{\rm eff}$ (band)	Mag.	$\log$ Flux	$\log$ Flux
	observed^a	observed^a	de-reddened^a
( $\mu$ m)	(mag)	( $\mu$ J)	( $\mu$ J)
	Infrared	Spitzer
70	$\ga$ 6.8	$\la$ 3.2	$\la$ 3.2
24	$\ga$ 10.2	$\la$ 2.8	$\la$ 2.85
8.0	14.2(3)	2.13(16)	$\rm 2.18(^{+16}_{-17})$
4.5	15.9(4)	1.90(21)	$\rm 1.95(^{+21}_{-22})$
	Optical	VLT
0.77(I)	23.12(13)	0.13(5)	$\rm0.66(^{+6}_{-10})$
0.66(R)	24.12(13)	-0.17(5)	$\rm0.51(^{+7}_{{-12}})$
0.55(V)	24.29(13)	-0.16(5)	$\rm0.66(^{+7}_{-13})$

^a Numbers in brackets are 1 $\sigma$ uncertainties referring to last significant digits quoted.

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