3 underlying nebula centered to north: 60:e3 11.70 Jy; 100:e10.2 89.42 Jy. 326 60 & 100: strong source -1.3; 100 swamped by nearby source. 4 12:e5.2 5.44 Jy(-0.7); 25:e4.8 5.44 Jy(-0.8). 60:e5.1 45.54 Jy(-1.2); 100:e6.5 191.17 Jy(-1.2). 5 12:e2.6 5.04 Jy(+0.6); 25:e2.5 2.11 Jy(0). 60:e3.2 63.97 Jy(+0.6); 100:e5.5 223.75 Jy(+0.6). DW identifies this as 00108+6519. 333 100: large complex. 334 12: also e2.8 9.48 Jy. 25: also e2.5 4.02 Jy. 60: also e3.2 24.62 Jy. 9 indistinguishable from HBC 8. 340 100: nearby (-3.5) strong source. 341 indistinguishable from HBC 340. 350 indistinguishable from HBC 349. 355 indistinguishable from HBC 354. 357 indistinguishable from HBC 356. 359 indistinguishable from HBC 358. 360 indistinguishable from HBC 360. 30 close to HBC 31. 31 close to HBC 30 but has better positional fit. 373 on wing of stronger source. 374 swamped by HBC 373. 375 nearby (-0.75) strong source. 381 v close to HBC 383 but HBC 383 is a better positional fit. 382 swamped by HBC 380. 383 see HBC 381 note. 386 nearby strong source. 387 indistinguishable from HBC 386. 37 12 & 25: ft e2 source; 60: also e2.6 11.82 Jy; 100: also e5.8 10.81 Jy. 38 PSC assigns IRAS source to HBC 39 (DI Tau) 39 overwhelmed by HBC 38. 40 12: also e4(-0.7) 335.12 Jy; 25: also e4(-0.6) 362.65 Jy; 60: also e4.6(-0.6) 2988.42 Jy. 391 60 & 100 swamped by HBC 40. 42 indistinguishable from HBC 43. 46 strong source at (-0.5): 12: 0.66 Jy; 25:1.15 Jy; 60: 2.82 Jy; 100: 4.90 Jy. This is probably the source identified as 04278+2435 which coincides with anon. red POSS star. 393 slightly extended at 25 and 60. 394 v close to HBC 49 but no observed flux. 50 indistinguishable from HBC 49. 395 indistinguishable from HBC 51. 401 centering is slightly better for HBC 402. 53 indistinguishable from HBC 52. 55 indistinguishable from HBC 404. 404 indistinguishable from and values assigned to HBC 55. 56 swamped by HBC 57. 406 indistinguishable from HBC 60. 414 swamped by HBC 66. 415 swamped by HBC 66. 416 60: also e6.5(-1.2) 2.82 Jy; 100: also e7.3(-0.7) 23.05 Jy. 418 swamped by HBC 67. 419 100: also e7.5(+0.6) 2.35 Jy. 422 centering is slightly better for HBC 423. 423 swamped by HBC 69. 71 100: also e11 0.6 Jy. 424 same coordinates as HBC 73. 82 masked by strong source at -1.2. 81 indistinguishable from HBC 80. 84 60 & 100: strong signal at +1.7. 85 ft extended underlying source. 88 DW assigns to 05272+1211 but HBC 89 is a much better positional fit. 433 indistinguishable from HBC 90. 93 60 & 100: swamped by nearby source. 434 indistinguishable from HBC 435. 94 25: ft underlying extended source. 95 swamped by nearby strong source. 96 100: probably the sum of three sources. 437 signal swamped by nearby source. 102 signal swamped by nearby source. 438 100: complex at -1.4. 105 60 &100 swamped by nearby source. 441 indistinguishable from HBC 111. 111 12: also e2.4 7.63 Jy; 25: e3.8(-0.35) 32.36 Jy. 449 swamped by nearby signals. 125 strong nearby signals. 452 strong nearby signals. 126 strong nearby signals. 128 strong nearby signals. 127 strong nearby signals. 129 strong nearby signals. 453 strong nearby signals. 454 sensor saturated. 131 strong nearby signals. 133 strong nearby signals. 134 strong nearby signals. 132 strong nearby signals. 455 strong nearby signals. 136 strong nearby signals. 456 strong nearby signals. 457 strong nearby signals. 137 strong nearby signals. 458 strong nearby signals. 459 strong nearby signals. 460 strong nearby signals. 461 strong nearby signals. 464 underlying extended source becoming prominent between 60 &100. 468 strong nearby signals. 141 strong nearby signals. 469 strong nearby signals. 146 strong nearby signals. 148 25, 60, and 100 swamped by strong signal at -1.9. 147 strong nearby signals. 150 nearby monster signal. 479 confused with two other sources. 156 strong nearby signals. 158 strong nearby signals. 483 Cohen-Schwartz star. 484 indistinguishable from HBC 167. 486 swamped by nearby source. 487 swamped by nearby source. 488 12: also e4.6 0.66 Jy; 25: also e5.5 0.50 Jy. 172 close to HBC 173 but HBC 172 is a better positional fit. 173 see note for HBC 172. 490 indistinguishable from HBC 491. 491 indistinguishable from HBC 490. 492 promising candidate at +0.6: d12: 1.67 Jy; d25: 1.59 Jy; d60e1.8 10.44 Jy; [aaay] 494 swamped by strong source at +1.5 which DW identifies with 05380-0728. THe HBC object has been identified as a reflection nebula illuminated by the nearby IR source. 495 CoKu DL Ori/G4. 497 swamped by nearby signals. 498 CoKu DL Ori/G1. 500 swamped by strong source at +0.8. 508 indistinguishable from HBC 507. 511 swamped by HBC 510. 516 indistinguishable from HBC 190. 191 60: also e3 0.12 Jy peak. 193 12: also e2 1.39 Jy; 25: also e2 9.29 Jy; 60: also e5.3 4.63 Jy; 100: also e6.6 23.16 Jy. 519 60 & 100: swamped by nearby source. 520 indistinguishable from HBC 519. 196 60 & 100: swamped by nearby sources. 202 100: nearby extended source. 521 swamped by HBC 202 and another, redder source at +1.3. 522 indistinguishable from HBC 202. 523 indistinguishable from HBC 202. 203 indistinguishable from HBC 202. 524 indistinguishable from HBC 202. 526 indistinguishable from HBC 527. 527 12: also e3.6 6.54Jy; 25: also e4.5 8.79 Jy; 60: also e4.5 105.27 Jy. 528 indistinguishable from HBC 527. 529 25: also e1.5 3.38 Jy(-0.3). 210 sources at 0.7. 226 strong source at -1.1. 231 underlying nebula. 235 indistinguishable from HBC 236. 236 slightly better positional fit than HBC 235. 238 12: also e4.0 1.48 Jy; 25: also e4.0 1.34 Jy. 60 & 100: extended complex. 547 12: also e2.4(-1.2) 7.79 Jy; 25: also e2(-0.8) 21.78 Jy. 548 PSC measuring source at +2.0. 552 60: also e3.5(-0.4) 7.40 Jy. 558 60: uncertain if extended or confused with nearby sources. 246 60: also e5 ft source; 100: also e10 39.86 Jy. 247 slightly better positional fit than HBC 589. 589 see note for HBC 247. 598 swamped by HBC 248. 618 confused by HBC 619. 619 also extended source at -1: 12: e2.4 6.51 Jy; 25: e3.7 6.71 Jy; 60: e3.7 33.20 Jy; 100: e4.7 78.33 Jy. 620 swamped HBC 619. 623 100: multiple unresolved sources. 632 indistinguishable from HBC 254. 635 above a v messy extended source. 259 extracted from a blended complex. 639 v strong source at -2.0. 262 indistinguishable from HBC 262. 640 60: broad source at 1.3. 641 indistinguishable from HBC 640. 264 12: also e6 2.38 Jy; 25: also e4.7(1.7) 4.48 Jy; 60: also e2.6(1.4) 13.20 Jy; 100: e7(2.8) 75.62: Jy. 644 indistinguishable from HBC 267. 645 indistinguishable from HBC 646. 649 60: also e5.0 2.18 Jy; 100: also e8.0 14.35 Jy. 652 12, 25, 60: (+.5) 657 25: also e4 0.65 Jy; 60: also e4.5 0.79 Jy. 274 60: also e4 1.83 Jy. 275 indistinguishable from HBC 275. 661 indistinguishable from HBC 659. 664 indistinguishable from HBC 663. 666 indistinguishable from HBC 665. 667 indistinguishable from HBC 665. 282 12: also e2.3 1.38 Jy; 25: also e2.8 2.19 Jy; 60: also e3.7 13.06 Jy; 100: also e6.5 26.28 Jy. 668 HBC 670 fits position slightly better. 669 v close to HBC 670. 670 slightly better positional fit than HBC 668; 100:swamped by HBC 669. 671 swamped by HBC 669. 675 swamped HBC 286 but v little if any signal. 287 strong source at -0.7 which DW identifies with TY CrA. 677 25, 60, 100: swamped by nearby source. 289 60: also e4 0.83 Jy. 679 extended complex. 682 indistinguishable from HBC 681. 683 indistinguishable from HBC 681. 685 indistinguishable from HBC 292. 294 100: also e10.5 15.36 Jy. 688 12: also e3 4.96 Jy; 25: also e3 7.47 Jy; 60: also e3.2(0.6) 34.00 Jy; 100: also e3(0.9) 48.47 Jy. 689 swamped by HBC 691. 690 indistinguishable from HBC 691. 699 100: strong source at 3.5. 700 indistinguishable from HBC 699. 708 indistinguishable from HBC 707. 715 swamped by HBC 716. 717 swamped by HBC 716. 298 12: also e4 1.52 Jy. 721 100: strong nearby source. 722 indistinguishable from HBC 724. 723 indistinguishable from HBC 724. 724 best positional fit of HBC 722, 723, or 725. 299 60: strong sources at 0.8. 725 indistinguishable from HBC 724. 726 12: also e2.6 45.78 Jy; 25: also e1.8 113.34 Jy; 60: also e3.3 563.89 Jy; 100: also e5.7 915.00 Jy. 305 swamped by HBC 727. 728 100: strong source at -1.4. 729 e3 complex at all wavelengths. 308 flanked by two close sources. 730 prob. extended and other sources. 731 swamped by nearby source. 309 25: also e3 30.37 Jy; 100: also e9.4 289.66 Jy. 313 12: also e3(-0.2) 1.47 Jy; 25: also e2.4(-0.2) 2.37 Jy; 60: also e6(0.6) 15.62 Jy; 100: also e7.3(1.3) 48.27 Jy. 314 v confused sources. 740 indistinguishable from HBC 317. 318 100: swamped by strong source at 3.4. 323 25: also e5 0.93 Jy; too confused at longer wavelengths.