This directory contains the .jpg images that will be available as online
figure sets through AJ.

The naming convention reflects the organization of the AJ online figure sets.
This file provides a translation table between the figure numbers and source
names (as given in the tables).

Figure Set 1 (Sources in Table 1, 97 sources)

Global figure set title: IRAC and MIPS images of "Likely" MYSO Outflow Candidates
(Table 1)

Caption:
(a) Five-panel image showing IRAC 3.6 um (upper left), 4.5 um (upper middle),
5.8 um (upper right), 8.0 um (lower left), and MIPS 24 um (lower middle)
images.  The polygonal source aperture used for IRAC photometry is overlaid in
all panels.  The circular or elliptical aperture used for MIPS photometry is
overlaid on the 24 um image.  For fields in which other IRAC sources are
present near the EGO, the MIPS aperture is also overlaid on an IRAC image for
reference.  Apertures with a red slash were excluded from the photometry.  (b)
Three-color GLIMPSE IRAC image showing 8.0 um (red), 4.5 um (green), and 3.6
um (blue).  The polygonal source aperture used for IRAC photometry is
overlaid.  Note that the field of view and scale of Figures (a) and (b) may be
different.

(b) Three-color GLIMPSE IRAC image showing 8.0 um (red), 4.5 um (green), and
3.6 um (blue).  The polygonal source aperture used for IRAC photometry is
overlaid.

f1_1	   g11.92-0.61
f1_2	   g12.02-0.21
f1_3	   g12.91-0.03
f1_4	   g14.33-0.64
f1_5	   g14.63-0.58
f1_6	   g16.61-0.24
f1_7	   g18.67+0.03
f1_8	   g18.89-0.47
f1_9	   g19.01-0.03
f1_10      g19.88-0.53
f1_11	   g22.04+0.22
f1_12	   g23.01-0.41
f1_13      g23.96-0.11
f1_14	   g24.00-0.10
f1_15	   g24.17-0.02
f1_16	   g24.94+0.07
f1_17  	   g25.27-0.43
f1_18  	   g27.97-0.47
f1_19	   g28.83-0.25
f1_20	   g34.41+0.24
f1_21	   g35.03+0.35
f1_22	   g35.04-0.47
f1_23	   g35.13-0.74
f1_24	   g35.15+0.80
f1_25	   g35.20-0.74
f1_26	   g35.68-0.18
f1_27	   g35.79-0.17
f1_28	   g36.01-0.20
f1_29	   g37.48-0.10
f1_30	   g39.10+0.49
f1_31	   g40.28-0.27
f1_32	   g44.01-0.03
f1_33	   g45.47+0.05
f1_34	   g49.27-0.34
f1_35	   g54.45+1.02
f1_36	   g56.13+0.22
f1_37	   g58.09-0.34
f1_38	   g59.79+0.63
f1_39	   g298.26+0.74
f1_40	   g298.89+0.37
f1_41	   g298.90+0.36
f1_42	   g305.48-0.10
f1_43	   g305.52+0.76
f1_44	   g305.57-0.34
f1_45	   g305.62-0.34
f1_46	   g305.82-0.11
f1_47	   g305.89+0.02
f1_48      g309.15-0.35
f1_49	   g309.38-0.13a
f1_50	   g309.99+0.51a
f1_51	   g310.08-0.23
f1_52	   g312.11+0.26
f1_53	   g317.42-0.67
f1_54	   g317.46-0.40b
f1_55	   g317.87-0.15
f1_56	   g317.88-0.25
f1_57	   g321.94-0.01
f1_58	   g324.19+0.41
f1_59	   g324.72+0.34
f1_60	   g326.27-0.49
f1_61	   g326.31+0.90
f1_62	   g326.78-0.24
f1_63	   g326.79+0.38
f1_64	   g326.86-0.67
f1_65	   g326.97-0.03
f1_66	   g327.12+0.51
f1_67	   g327.39+0.20
f1_68	   g327.40+0.44
f1_69	   g328.14-0.43
f1_70	   g329.18-0.31
f1_71	   g329.47+0.52
f1_72	   g329.61+0.11
f1_73	   g332.35-0.12
f1_74	   g332.56-0.15
f1_75	   g332.81-0.70
f1_76	   g332.94-0.69
f1_77	   g332.96-0.68
f1_78	   g333.18-0.09
f1_79	   g335.59-0.29
f1_80	   g337.30-0.87
f1_81	   g338.39-0.40
f1_82	   g339.95-0.54
f1_83	   g340.97-1.02
f1_84	   g341.24-0.27
f1_85	   g341.73-0.97
f1_86	   g341.99-0.10
f1_87	   g343.12-0.06
f1_88	   g343.50-0.47
f1_89	   g343.72-0.18a
f1_90	   g343.72-0.18b
f1_91	   g344.58-0.02
f1_92	   g345.72+0.82
f1_93	   g345.99-0.02
f1_94	   g347.08-0.40
f1_95	   g348.55-0.98
f1_96	   g348.58-0.92
f1_97	   g349.15-0.98

Figure Set 3 (Sources in Table 2, 36 sources).  

Global title: IRAC and MIPS images of "Likely" MYSO Outflow Candidates
(Table 2)

Caption:
(a) Five-panel image showing IRAC 3.6 um (upper left), 4.5 um
(upper middle), 5.8 um (upper right), 8.0 um (lower left), and MIPS 24 um
(lower middle) images.  The polygonal source aperture used for IRAC photometry
is overlaid in all panels.  Apertures with a red slash were excluded from the
photometry.  (b) Three-color GLIMPSE IRAC image showing 8.0 um (red), 4.5 um
(green), and 3.6 um (blue).  The polygonal source aperture used for IRAC
photometry is overlaid. Note that the field of view and scale of Figures (a)
and (b) may be different.

(b) Three-color GLIMPSE IRAC image showing 8.0 um (red), 4.5 um
(green), and 3.6 um (blue).  The polygonal source aperture used for
IRAC photometry is overlaid.  

f3_1	  g10.29-0.13
f3_2	  g10.34-0.14
f3_3	  g16.59-0.05
f3_4	  g19.36-0.03
f3_5	  g19.61-0.12
f3_6	  g25.38-0.15
f3_7	  g28.28-0.36
f3_8	  g34.39+0.22
f3_9	  g48.66-0.30
f3_10	  g49.42+0.33
f3_11	  g309.90+0.23
f3_12	  g317.46-0.40a
f3_13	  g318.04+0.09
f3_14	  g318.05+0.09
f3_15	  g320.23-0.28
f3_16	  g324.17+0.44
f3_17	  g326.32-0.39
f3_18	  g326.47+0.70
f3_19	  g326.48+0.70
f3_20	  g326.61+0.80b
f3_21	  g328.25-0.53
f3_22	  g329.03-0.20
f3_23	  g329.41-0.46
f3_24	  g329.47+0.50
f3_25	  g330.88-0.37
f3_26	  g331.13-0.24
f3_27	  g332.12+0.94
f3_28	  g332.60-0.17
f3_29	  g332.73-0.62
f3_30	  g333.47-0.16
f3_31	  g335.06-0.43
f3_32	  g335.79+0.18
f3_33	  g337.91-0.48
f3_34	  g341.22-0.26a
f3_35	  g342.48+0.18
f3_36	  g344.23-0.57

Figure Set 5 (Sources in Table 3, 75 sources)

Global title: IRAC and MIPS images of "Possible" MYSO Outflow Candidates
(Table 3)

Caption:
(a) Five-panel image showing IRAC 3.6 um (upper left), 4.5 um
(upper middle), 5.8 um (upper right), 8.0 um (lower left), and MIPS 24 um
(lower middle) images.  The polygonal source aperture used for IRAC photometry
is overlaid in all panels.  The circular or elliptical aperture used for MIPS
photometry is overlaid on the 24 um image.  For fields in which other IRAC
sources are present near the EGO, the MIPS aperture is also overlaid on an
IRAC image for reference.  Apertures with a red slash were excluded from the
photometry.  (b) Three-color GLIMPSE IRAC image showing 8.0 um (red), 4.5 um
(green), and 3.6 um (blue).  The polygonal source aperture used for IRAC
photometry is overlaid.  Note that the field of view and scale of Figures (a)
and (b) may be different.

(b) Three-color GLIMPSE IRAC image showing 8.0 um (red), 4.5 um
(green), and 3.6 um (blue).  The polygonal source aperture used for
IRAC photometry is overlaid.  

f5_1	   g11.11-0.11
f5_2	   g16.58-0.08
f5_3	   g24.63+0.15
f5_4	   g29.84-0.47
f5_5	   g29.96-0.79
f5_6	   g34.28+0.18
f5_7	   g40.28-0.22
f5_8	   g45.80-0.36
f5_9	   g49.07-0.33
f5_10	   g49.27-0.32
f5_11	   g50.36-0.42
f5_12	   g53.92-0.07
f5_13	   g54.11-0.08
f5_14	   g54.45+1.01
f5_15	   g58.79+0.63
f5_16	   g62.70-0.51
f5_17	   g304.89+0.64
f5_18	   g309.91+0.32
f5_19	   g309.97+0.59
f5_20	   g309.99+0.51b
f5_21	   g311.51-0.45
f5_22	   g324.11+0.44
f5_23	   g326.36+0.88
f5_24	   g326.41+0.93
f5_25	   g326.57+0.20
f5_26	   g326.61+0.80a
f5_27	   g326.61+0.80c
f5_28	   g326.65+0.75
f5_29	   g326.80+0.51
f5_30	   g326.92-0.31
f5_31	   g327.30-0.58
f5_32	   g327.72-0.38
f5_33	   g327.86+0.19
f5_34	   g327.89+0.15
f5_35	   g328.55+0.27
f5_36	   g329.07-0.31a
f5_37	   g329.07-0.31b
f5_38	   g329.16-0.29
f5_39	   g329.18-0.30
f5_40	   g331.08-0.47
f5_41	   g331.37-0.40
f5_42	   g331.62+0.53
f5_43	   g331.71+0.58
f5_44	   g331.71+0.60
f5_45	   g332.28-0.07
f5_46	   g332.33-0.12
f5_47	   g332.36+0.60
f5_48	   g332.47-0.52
f5_49	   g332.58+0.15
f5_50	   g332.59+0.04a
f5_51	   g332.59+0.04b
f5_52	   g332.91-0.55
f5_53	   g333.08-0.56
f5_54	   g334.04+0.35
f5_55	   g334.25+0.07
f5_56	   g335.43-0.24
f5_57	   g336.87+0.29
f5_58	   g336.96-0.98
f5_59	   g337.16-0.39
f5_60	   g338.32-0.41
f5_61	   g340.75-1.00
f5_62	   g340.77-0.12
f5_63	   g340.78-0.10
f5_64	   g341.20-0.26
f5_65	   g341.23-0.27
f5_66	   g342.15+0.51
f5_67	   g342.90-0.12
f5_68	   g343.19-0.08a
f5_69	   g343.40-0.40
f5_70	   g343.42-0.33
f5_71	   g343.50+0.03
f5_72	   g343.53-0.51a
f5_73	   g343.78-0.24
f5_74	   g344.21-0.62
f5_75	   g348.17+0.46

Figure Set 6 (Sources in Table 4, 90 sources)

Global title: IRAC and MIPS images of "Possible" MYSO Outflow Candidates
(Table 4)

Caption:
(a) Five-panel image showing IRAC 3.6 um (upper left), 4.5 um
(upper middle), 5.8 um (upper right), 8.0 um (lower left), and MIPS 24 um
(lower middle) images.  The polygonal source aperture used for IRAC photometry
is overlaid in all panels.  Apertures with a red slash were excluded from the
photometry.  (b) Three-color GLIMPSE IRAC image showing 8.0 um (red), 4.5 um
(green), and 3.6 um (blue).  The polygonal source aperture used for IRAC
photometry is overlaid. Note that the field of view and scale of Figures (a)
and (b) may be different.

(b) Three-color GLIMPSE IRAC image showing 8.0 um (red), 4.5 um
(green), and 3.6 um (blue).  The polygonal source aperture used for
IRAC photometry is overlaid.  

f6_1	   g12.20-0.03
f6_2	   g12.42+0.50
f6_3	   g12.68-0.18
f6_4	   g17.96+0.08
f6_5	   g19.61-0.14
f6_6	   g20.24+0.07
f6_7	   g21.24+0.19
f6_8	   g23.82+0.38
f6_9	   g24.11-0.17
f6_10	   g24.11-0.18
f6_11	   g24.33+0.14
f6_12	   g28.85-0.23
f6_13	   g29.89-0.77
f6_14	   g29.91-0.81
f6_15	   g35.83-0.20
f6_16	   g39.39-0.14
f6_17	   g40.60-0.72
f6_18	   g43.04-0.45a
f6_19	   g43.04-0.45b
f6_20	   g45.47+0.13
f6_21	   g45.50+0.12
f6_22	   g49.91+0.37
f6_23	   g54.11-0.04
f6_24	   g54.11-0.05
f6_25	   g57.61+0.02
f6_26	   g58.78+0.64
f6_27	   g58.78+0.65
f6_28	   g305.77-0.25
f6_29	   g305.80-0.24
f6_30	   g309.38-0.13b
f6_31	   g309.97+0.50
f6_32	   g309.99+0.51c
f6_33	   g310.15+0.76
f6_34	   g310.38-0.30a
f6_35	   g310.38-0.30b
f6_36	   g310.38-0.30c
f6_37	   g310.38-0.30d
f6_38	   g311.04+0.69
f6_39	   g313.71-0.19a
f6_40	   g313.71-0.19b
f6_41	   g313.76-0.86
f6_42	   g317.44-0.37
f6_43	   g320.24-0.29
f6_44	   g323.74-0.26
f6_45	   g325.52+0.42
f6_46	   g326.37+0.94
f6_47	   g326.64+0.76
f6_48	   g326.99-0.03
f6_49	   g327.57-0.85
f6_50	   g327.65+0.13
f6_51	   g328.16+0.59
f6_52	   g328.60+0.27
f6_53	   g328.81+0.63
f6_54	   g330.95-0.18
f6_55	   g331.12-0.46
f6_56	   g331.34-0.35
f6_57	   g331.51-0.34
f6_58	   g332.28-0.55
f6_59	   g332.29-0.09
f6_60	   g332.29-0.55
f6_61	   g332.35-0.44
f6_62	   g333.13-0.56
f6_63	   g333.32+0.10
f6_64	   g335.59-0.30
f6_65	   g336.02-0.83
f6_66	   g336.03-0.82
f6_67	   g337.40-0.40
f6_68	   g338.42-0.41
f6_69	   g338.92+0.55a
f6_70	   g338.92+0.55b
f6_71	   g339.58-0.13
f6_72	   g340.05-0.25
f6_73	   g340.06-0.23
f6_74	   g340.07-0.24
f6_75	   g340.10-0.18
f6_76	   g340.76-0.12
f6_77	   g341.22-0.26b
f6_78	   g342.04+0.43
f6_79	   g343.19-0.08b
f6_80	   g343.42-0.37
f6_81	   g343.53-0.51b
f6_82	   g344.22-0.57
f6_83	   g345.00-0.22a
f6_84	   g345.00-0.22b
f6_85	   g345.13-0.17
f6_86	   g346.04+0.05
f6_87	   g346.28+0.59
f6_88	   g348.18+0.48
f6_89	   g348.72-1.04
f6_90	   g348.73-1.04

Figure Set 10 (Sources in Table 7, ordered as in Table 7, 55 sources)

Global title: IRAC and MIPS images of EGOs with Associated 6.7 GHz
Methanol Masers (Table 7)

Caption:
(a) Five-panel image showing IRAC 3.6 um (upper left), 4.5 um
(upper middle), 5.8 um (upper right), 8.0 um (lower left), and MIPS 24 um
(lower middle) images.  Apertures used for photometry are overplotted as in
Figure Sets 1,3,5, and 6.  The positions of 6.7 GHz methanol masers are
marked.  (b) Three-color GLIMPSE IRAC image showing 8.0 um (red), 4.5 um
(green), and 3.6 um (blue).  The polygonal source aperture used for IRAC
photometry is overlaid.  Positions of 6.7 GHz methanol masers are marked. Note
that the field of view and scale of Figures (a) and (b) may be different.

(b) Three-color GLIMPSE IRAC image showing 8.0 um (red), 4.5 um
(green), and 3.6 um (blue).  The polygonal source aperture used for
IRAC photometry is overlaid.  Positions of 6.7 GHz methanol masers are marked.


f10_1  g28.83-0.25
f10_2  g298.26+0.74
f10_3  g312.11+0.26
f10_4  g326.86-0.67
f10_5  g327.12+0.51
f10_6  g327.39+0.20
f10_7  g327.40+0.44
f10_8  g329.18-0.31
f10_9  g329.47+0.52
f10_10 g329.61+0.11
f10_11 g332.56-0.15
f10_12 g332.94-0.69
f10_13 g333.18-0.09
f10_14 g335.59-0.29
f10_15 g339.95-0.54
f10_16 g344.58-0.02
f10_17 g10.29-0.13
f10_18 g10.34-0.14
f10_19 g16.59-0.05
f10_20 g19.36-0.03
f10_21 g19.61-0.12
f10_22 g28.28-0.36
f10_23 g320.23-0.28
f10_24 g326.47+0.70
f10_25 g326.48+0.70
f10_26 g328.25-0.53
f10_27 g329.03-0.20
f10_28 g329.41-0.46
f10_29 g329.47+0.50
f10_30 g331.13-0.24
f10_31 g332.60-0.17
f10_32 g332.73-0.62
f10_33 g333.47-0.16
f10_34 g335.06-0.43
f10_35 g335.79+0.18
f10_36 g344.23-0.57
f10_37 g329.07-0.31b
f10_38 g28.85-0.23
f10_39 g313.76-0.86
f10_40 g323.74-0.26
f10_41 g328.81+0.63
f10_42 g330.95-0.18
f10_43 g331.34-0.35
f10_44 g332.29-0.09
f10_45 g332.35-0.44
f10_46 g333.13-0.56
f10_47 g333.32+0.10
f10_48 g336.02-0.83
f10_49 g337.40-0.40
f10_50 g339.58-0.13
f10_51 g340.05-0.25
f10_52 g345.00-0.22a
f10_53 g348.73-1.04
f10_54 g12.91-0.26
f10_55 g345.51+0.35


Figure Set 12 (Sources in Table 5, 6 sources)

Global title: IRAC and MIPS images of "Outflow-only" EGOs
(Table 5)

Caption:
(a) Five-panel image showing IRAC 3.6 um (upper left), 4.5 um
(upper middle), 5.8 um (upper right), 8.0 um (lower left), and MIPS 24 um
(lower middle) images.  The polygonal source aperture used for IRAC photometry
is overlaid in all panels.  Apertures with a red slash were excluded from the
photometry.  (b) Three-color GLIMPSE IRAC image showing 8.0 um (red), 4.5 um
(green), and 3.6 um (blue).  The polygonal source aperture used for IRAC
photometry is overlaid.  Note that the field of view and scale of Figures (a)
and (b) may be different.

(b) Three-color GLIMPSE IRAC image showing 8.0 um (red), 4.5 um
(green), and 3.6 um (blue).  The polygonal source aperture used for
IRAC photometry is overlaid.  

f12_1	   g12.91-0.26
f12_2	   g19.01-0.03_O-N
f12_3	   g19.01-0.03_O-S
f12_4	   g34.26+0.15
f12_5	   g37.55+0.20
f12_6	   g345.51+0.35