Table 3: Mid-IR MSX fluxes.
IRAS field IR $\Delta\alpha$ $\Delta\delta$ F8.3 F12.1 F14.7 F21.4
    ( $^{\prime \prime}$) ( $^{\prime \prime}$) (Jy)
05137+3919 A +12 +8 3.1 4.9 6.3 15
  B -4 -25 1.0 1.7 1.1 5.3
05345+3157 A +18 -7 8 11.1 4 8.2
  B +62 +36 - - - 2.7
05373+2349 A +1 -4 2.2 3.5 6.6 14.4
08211-4158 A +2 +6 7.6 10.8 8.2 17
  B -88 -125 1.0 1.4 2.1 6.9
08470-4243 A +1 +12 13.6 18.8 12.6 56.7
  B -33 -9 2.0 3.0 1.4 1.2
  E -86 29 - - 1.0 4.5
08477-4359 A +3 +3 12.0 12.3 6.3 14
08563-4225 A +3 +1 12.8 15.3 14.1 29.2
08589-4714 A +12 -9 0.6 0.3 0.7 5.2
  B +52 -72 0.3 1.0 - 1
09131-4723 A -23 +21 10.9 11.9 6.9 16.1
  B -51 +98 4.5 6.3 5.8 7.1
10019-5712 A +12 -2 4.2 6.2 4.6 31.1
  B -11 +11 3.6 4.1 2.5 11.5
10095-5843 A +2 +6 6.7 8.8 5.5 12.5
  B +162 -89 1.1 2.1 0.94 0.26
10184-5748 A +14 -19 3.6 10.1 44 240
  B +9 +26 1.3 6.5 15 36
  C +10 -98 4.5 4.0 5.9 17
  G -67 -155 1.8 3.1 1.6 8.9
10501-5556 A +3 -6 2.6 2.1 5.6 34
10555-6242 A -2 +13 3.1 3.7 3.9 17.8
11380-6311 A -5 +4 3.3 2.4 2.8 7.8
12063-6259 A +3 -1 36 74 91 331
12127-6244 A +2 -4 39 94 162 590
14000-6104 A -19 -33 14 13 14 35
  B +212 -126 7.7 8,.4 4.6 11
  C +91 -30 3.1 4.8 8 10.6
  D -229 +146 8.4 13.7 18.8 22.7
  E +313 -92 0.2 0.3 0.9 1
  F -87 +101 1.6 3.6 3.3 10.7
  G -51 +68 - 0.7 1.7 4.1
  H -28 +123 0.1 - 0.5 2.7
  I -31 +172 0.5 0.75 1 2.6
14057-6032 A +12 -2 0.6 1.1 2.3 11.2
15068-5733 A +6 0 2.8 3.9 5.5 52
  B -91 +59 1.4 2.2 1.7 0.7
  C +168 -7 1.1 1 1.1 4.2
  E +83 -125 - - 1.3 3.4
15454-5335 A +28 -13 2 1.8 4.3 22.2
  B -93 +47 0.6 0.9 3.8 20.2
15519-5430 A 0 +10 3.5 5.1 2.1 4
  B -253 +144 10 13 10.4 12.3
  G -87 -154 - 1 1.5 5
15557-5337 A -1 +11 64.5 187 208 713
  B -19 -23 36.9 108 129 440
  C +41 -51 - 32 33 145
  D +23 +39 8.1 13 10.6 79
16148-5011 A +20 -2 32 46 26 72
  B +382 -330 48 87 71 57.3
  C +215 -301 7 9 7.5 36.7
  D +126 -254 2.6 2.2 2.6 2.4
  E +33 +322 3 3.8 6 5.5
16232-4917 A -7 -5 10.6 14 12.1 26.7
16501-4314 A +3 -4 5.8 7.6 6 13
16535-4300 A +12 -1 1.2 2.3 1.7 2.2
  C +72 -256 4.1 6 11.7 12.7
17082-4114 A -8 -6 12.4 14.5 8.7 17
  B -53 -60 7.7 8.7 4.9 10.8
17425-3017 A -3 -4 2.9 2.4 1.6 3.1
  F -228 -52 0.9 0.9 1 1.8
18024-2119 G +3 +9 - - - 1.2

IRAS field IR $\Delta\alpha$ $\Delta\delta$ F8.3 F12.1 F14.7 F21.4
    (s) ( $^{\prime \prime}$) (Jy)
18144-1723 A +6 -3 1.4 3.4 5.4 18.2
  B -178 -12 8.2 4 2.1 1.7
  C +155 +87 1.2 1.9 6 1 0.9  
  D -63 -159 0.8 0.5 0.4 0.4
  E -32 -86 - - 0.7 1.2
18278-1009 A +15 +3 5 9.7 15.6 15.5
  B -68 -38 1.3 2.7 1.8 1.9
  C -12 -169 2.5 3.6 3.6 2.8
  D +140 -45 4.5 4.8 3.9 2.2
18511+0146 Aa +2 +5 18.3 26.5 36.1 47.1
19092+0841 Aa +15 +16 3 3.1 1.7 4.1
  C -172 +64 2.7 4 2.8 2.5
  D +224 -108 1.7 1.5 1.1 4.4
20062+3550 A +17 +3 1 1.3 2.7 17.2
20106+3545 A +9 +4 2.6 2.5 2.5 10.4
  B +34 +65 8 3.5 3.1 3.1
21307+5049 Aa +3 +2 1 1.1 2.7 6.5
21519+5613 A +10 -5 0.75 1.4 2.2 10.8
22172+5549 A +2 +18 2 5.8 3.2 7
22305+5803 A +3 +5 1.2 1.1 2.4 12.1
22506+5944 A +2 +5 4.7 6.7 5.7 18.4
23385+6053 Aa +25 +27 2.5 6.4 0.5 0.7
  Ba -16 +23 0.7 1.5 0.2 0.1
  C -87 +12 0.9 0.9 - 0.8

a Source also observed with ISOCAM in LW2 and LW3 filters (see Table 4).

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