Table 5: Radio flux densities integrated over the 12 SWS apertures and the LWS aperture. The official band range in ${\rm ~ \mu m}$ is given for every aperture.
  Integrated flux density (mJy)
Source 1A 1B 1D 1E 2A 2B 2C 3A 3C 3D 3E 4 LWS$^\star$
  (2.38-2.61) (2.60-3.03) (3.02-3.53) (3.52-4.06) (4.05-5.31) (5.30-7.01) (7.00-12.1) (12.0-16.6) (16.5-19.6) (19.5-27.6) (27.5-29.0) (28.9-45.2) (43.0-196.0)
IRAS 01045 205 204 205 206 210 210 207 230 235 232 238 230 $\dagger$
IRAS 10589 766 766 765 770 789 781 769 687 677 678 765 728 1210 (19)
IRAS 11143 284 284 286 288 318 315 314 332 333 345 479 554 1981 (79)
IRAS 12063 1261 1261 1272 1267 1300 1278 1269 1484 1437 1441 1534 1481 1959 (23)
IRAS 12073 3655 3660 3684 3702 3936 3886 3864 4906 4708 4919 4765 5502 14092 (889)
IRAS 12331 231 233 236 238 278 274 277 338 342 371 584 707 3059 (310)
IRAS 15384 1495 1496 1506 1508 1581 1559 1549 1756 1719 1749 1956 2064 4435 (208)
IRAS 15502 1342 1341 1367 1344 1362 1286 1269 1668 1642 1597 1952 1875 2707 (85)
IRAS 16128 390 400 413 415 478 468 489 894 917 1021 1931 2076 7468 (428)
IRAS 17160 563 567 578 575 621 605 611 860 850 890 1223 1300 3940 (267)
IRAS 17221 343 344 347 349 392 386 385 405 419 431 636 731 2451 (181)
IRAS 17279 187 187 187 189 198 196 194 183 185 193 253 282 930 (23)
IRAS 18032 367 367 366 369 380 375 367 288 285 292 349 340 609 (11)
IRAS 18479 2137 2136 2128 2138 2151 2120 2087 1740 1710 1712 2044 1880 2751 (29)
IRAS 19442 73 73 73 73 76 75 75 69 65 65 64 61 93 (2)
IRAS 19598 3348 3348 3351 3353 3401 3410 3396 3352 3326 3264 3348 3030 3662 (29)
DR21 604 603 601 608 640 623 609 381 443 444 694 786 1556 (52)
IRAS 23133 619 619 621 622 626 621 613 670 672 654 702 669 738 (3)
$^\dagger$ No LWS observation available. $^\star$ Given is the average of the integrated flux density obtained from two different methods (see Sect. 5). The number in brackets is the difference
in mJy between these two methods.

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