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Table 2:

Integrated photometric properties.

Object 		RA Dec $m_{\rm FUV}$(AB) $F_{\rm FUV}$ $L_{\rm FUV}$ $m_{\rm NUV}$(AB) $F_{\rm NUV}$ $L_{\rm NUV}$ FUV-NUV SFR $_{\rm FUV}$
  (2000) (2000)                
Galaxy 184.8776 14.87777 17.66 $\pm$ 0.12 2.466 6.41 16.26 $\pm$ 0.01 8.241 21.43 1.31 8.9
Clump 1 184.8732 14.89737 22.68 $\pm$ 0.39 0.0308 0.0800 22.06 $\pm$ 0.31 0.0544 0.142 0.62 0.112
Clump 2 184.8762 14.88732 21.18 $\pm$ 0.24 0.123 0.318 20.92 $\pm$ 0.19 0.156 0.405 0.26 0.446
Clump 3 184.8603 14.87558 20.69 $\pm$ 0.19 0.192 0.500 20.59 $\pm$ 0.18 0.212 0.548 0.10 0.700
Clump 4 184.8589 14.86833 21.61 $\pm$ 0.31 0.082 0.214 21.23 $\pm$ 0.24 0.117 0.304 0.38 0.300
Clump 5 184.8554 14.86131 21.32 $\pm$ 0.22 0.108 0.280 21.15 $\pm$ 0.23 0.123 0.327 0.17 0.392
Clump 6 184.8801 14.86162 22.13 $\pm$ 0.31 0.0510 0.133 21.70 $\pm$ 0.30 0.0759 0.197 0.43 0.186

Notes. (1) Coordinates are given in degrees; (2) fluxes are in units of 10-27 erg s-1 cm-2 Hz-1; (3) luminosities are in units of 1026 erg s-1 Hz-1; (4) SFRs are in units of $10^{-2}~M_{\odot}$ yr-1.


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