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Table 1:

Near-Infrared photometry of the PHL 5038 binary system and nearby calibration star.
Bandpass $\lambda$ PHL 5038 PHL 5038A PHL 5038B 2MASS J22203205-0040210
  ($\mu$m) (mag) (mag) (mag) (mag)
Y1 1.03 $16.89\pm0.01$ - - -
J1 1.25 $16.73\pm0.02$ - - -
H1 1.63 $16.44\pm0.03$ - - -
K1 2.20 $16.31\pm0.04$ - - -
H2 1.65 - $16.82\pm0.07$ $17.84\pm0.08$ $14.447\pm0.053$
K2 2.19 - $16.72\pm0.07$ $17.18\pm0.08$ $14.161\pm0.051$
1 UKIDSS passbands as described in Hewett et al. (2006). 2 H- and K-band photometry were obtained on a single night. The photometric errors were calculated using a 5% error from the nearby 2MASS star used for flux calibration, a 2-3% photometric measurement error, and an assumed 5% internal error typical of near-infrared arrays. The final column displays the nearby 2MASS calibration star with its 2MASS catalogue photometry and errors. Colour transformations between the filters are of the order of 1% (Carpenter 2001) and so are neglected.

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