1 [3.6]-[4.5]=0.04, [5.8]-[8]=0.5, so small excess at longer bands (Section 4.2); among 14 reddest BRC 27 sources in JHK_s_ diagram, high A_V_ likely (Section 5.2); literature optical points discontinuous with respect to rest of SEDs, not clear exactly why (Section 5.3.1).
 2 [3.6]-[4.5]=0.07, [5.8]-[8]~-0.3, but very faint at [8], so large error (Section 4.2); no significant IR excess.
 3 Among 14 reddest BRC 27 sources in JHK_s_ diagram, high A_V_ likely (Section 5.2).
 4 Possible very small [8] excess; no convincing indication of IR excess, despite likely YSO in literature; bright in r (Section 5.1); blue in JHK_s_ (Section 5.2).
 5 No special notes.
 6 Small IRAC colors (Section 4.2) and small but apparently significant 24{mu}m excess (Section 4.3); contamination possible, so "IRx:"; bright in r, though with large errors (Section 5.1); r seems too high in SED (Section 5.3.1).
 7 Literature optical points discontinuous with respect to rest of SED, not clear exactly why (Section 5.3.1).
 8 Possible very small [5.8], [8] excess (Section 4.4); very weak evidence for IR excess.
 9 No special notes.
10 Bright in r (Section 5.1); blue in JHK_s_ (Section 5.2).
11 Among 4 reddest BRC 27 objects in JHK_s_ diagram, high A_V_ likely (Section 5.2, Section 5.3.1); SED slope within 0.1 of borderline between SED class Flat and II (Section 5.3.2).
12 Among 14 reddest BRC 27 sources in JHK_s_ diagram, high A_V_ likely (Section 5.2).
13 Among 4 reddest BRC 27 objects in JHK_s_ diagram, high A_V_ likely (Section 5.2); reasonably deeply embedded SED (Section 5.3.1); when SED slope calculated between 2 and 8{mu}m, class changes from a Flat to Class II (Section 5.3.2).
14 Among 14 reddest BRC 27 sources in JHK_s_ diagram, high A_V_ likely (Section 5.2, Section 5.3.1).
15 Bright in r (Section 5.1).
16 r, i optical detections place below ZAMS (Section 5.1); among 4 reddest BRC 27 objects in JHK_s_ diagram, high A_V_ likely (Section 5.2); somewhat unusually shaped SED (Section 5.3.1); on bright rim, bright source with nearby nebulosity and point sources in [3.6], [4.5] (Section 5.3.1).
17 Among 14 reddest BRC 27 sources in JHK_s_ diagram, high A_V_ likely (Section 5.2).
18 Among 14 reddest BRC 27 sources in JHK_s_ diagram, high A_V_ likely (Section 5.2).
19 Bright in r (Section 5.1); somewhat unusually shaped SED (see Section 5.3.1); 8{mu}m bright from PAH emission? (Section 5.3.1); very bright, may be nebulous companion to bright 070402.7-112325, row 20 (Section 5.3.1); when SED slope calculated between 2 and 8{mu}m, class changes from a Flat to Class I (Section 5.3.2).
20 Bright in r (Section 5.1); blue in JHK_s_ (Section 5.2); "flat" class (Section 5.3.2 from fitting K_s_ to [8] but very bright star, small fractional IR excess, K_s_ not at peak of SED.
21 Reasonably deeply embedded SED (Section 5.3.1).
22 Two previously identified sources are unresolved (Section 2); reasonably deeply embedded SED (Section 5.3.1); when SED slope calculated between 2 and 8{mu}m, class changes from a Flat to Class II (Section 5.3.2).
23 Among 14 reddest BRC 27 sources in JHK_s_ diagram, high A_V_ likely (Section 5.2); reasonably deeply embedded SED (Section 5.3.1).
24 Among 14 reddest BRC 27 sources in JHK_s_ diagram, high A_V_ likely (Section 5.2); literature optical points discontinuous with respect to rest of SEDs, not clear exactly why (Section 5.3.1).
25 No detectable IRAC excess (Section 4.2) and undetected at [24]; no significant IR excess; bright in r (Section 5.1); blue in JHK_s_ (Section 5.2).
26 Among 4 reddest BRC 27 objects in JHK_s_ diagram, high A_V_ likely (Section 5.2); SED suggests substantial disk (Section 5.3.1); SED slope within 0.1 of borderline between SED Class I and Flat (Section 5.3.2).
27 No special notes.
28 Large errors on [5.8] and [8], which is the only indication of IR excess (Section 4.4); no significant IR excess; 5.8 and 8{mu}m points discontinuous with rest of SEDs (Section 5.3.1); SED slope within 0.1 of borderline between SED Classes II and III (Section 5.3.2).
29 No special notes.
30 Among 14 reddest BRC 27 sources in JHK_s_ diagram, high A_V_ likely (Section 5.2); SED slope within 0.1 of borderline between SED class Flat and II (Section 5.3.2).
31 5.8 and 8{mu}m points somewhat discontinuous with rest of SED (Section 5.3.1).
32 No special notes.
33 [3.6]-[4.5]=0, [5.8]-[8]=0.23 (Section 4.2); [3.6]-[24]>4mag, though nebular contamination possible (Section 4.3); uncertain IRx; bright in r (Section 5.1); blue in JHK_s_ (Section 5.2); when SED slope calculated between 2 and 8{mu}m, class changes from a Class II to Class III (Section 5.3.2).
34 Among 14 reddest BRC 27 sources in JHK_s_ diagram, high A_V_ likely (Section 5.2); when SED slope calculated between 2 and 8{mu}m, class changes from a Flat to Class II (Section 5.3.2).
35 SED slope within 0.1 of borderline between SED Classes II and III (Section 5.3.2).
36 Possible very small [5.8], [8] excess (Section 4.4), no [24]; very weak evidence for IR excess.
37 r, i optical detections particularly uncertain, and place below ZAMS (Section 5.1); somewhat unusually shaped SED (see Section 5.3.1).
38 No special notes.
39 Selected in Section 4.4 for a ~11{sigma} excess at [8] and no [24]; high A_V_ likely; abrupt change in SED between K_s_ and [3.6] (Section 5.3.1).
40 Bright in r (Section 5.1); large excess at [24]; inner disk hole or contamination (Section 5.3.1)?; when SED slope calculated between 2 and 8{mu}m, class changes from a Class II to Class III (Section 5.3.2).
41 Multi-IRAC band weak excess and no [24] (Section 4.4); SED slope within 0.1 of borderline between SED class II and III (Section 5.3.2).
42 Abrupt change in SED between K_s_ and [3.6] (Section 5.3.1).
43 Identified from [8] excess (Section 4.4) with >10{sigma} significance; inner disk hole?; 5.8 and 8{mu}m points somewhat discontinuous with rest of SED (Section 5.3.1); SED slope within 0.1 of borderline between SED class II and III (Section 5.3.2)
44 Identified from [8] excess (Section 4.4) with >10{sigma} significance; inner disk hole?
45 Identified from [8] excess (Section 4.4) with >10{sigma} significance; inner disk hole?; SED slope within 0.1 of borderline between SED class II and III (Section 5.3.2)
46 Identified from [8] excess (Section 4.4) with >10{sigma} significance; inner disk hole?; located on ZAMS in r, i (Section 5.1); 5.8 and 8{mu}m points somewhat discontinuous with rest of SED (Section 5.3.1)
47 No special notes.
48 This is the only literature YSO or literature YSO candidate in BRC 34.
49 Largest [3.6]-[4.5] (=1.6) of both BRCs (Section 4.2); high A_V_ likely (Section 4.2, 5.3.1); bright at [70]; reasonably deeply embedded SED (Section 5.3.1).
50 Identified from [8] excess (Section 4.4) with >10{sigma} significance; in 4 reddest BRC34 sources in JHK_s_, high A_V_ likely (Section 5.2).
51 Low [5.8]-[8] (=0.21) but high [3.6]-[4.5] (=0.48) (Section 4.2); H-K_s_=1.08, J-H=2.3, high A_V_ likely (Section 5.2, Section 5.3.1).
52 SED slope within 0.1 of borderline between SED class II and III (Section 5.3.2).
53 5.8 and 8{mu}m points rather abruptly rise compared to rest of SED (Section 5.3.1); inner disk hole?; SED slope within 0.1 of borderline between SED class flat and II (Section 5.3.2).
54 5.8 and 8{mu}m points discontinuous with rest of SED (Section 5.3.1); inner disk hole?
55 In 4 reddest BRC34 sources in JHK_s_, high A_V_ likely (Section 5.2, Section 5.3.1).
56 In 4 reddest BRC34 sources in JHK_s_, high A_V_ likely (Section 5.2, Section 5.3.1).