Table 2: Galactic longitude and latitude (in degrees), velocity (km s^-1), widths (km s^-1), and intensities (K) of the CS lines. In addition, the SiO to CS intensity ratio is also shown. The numbers in parentheses are the uncertainties on the last digit. The positions observed with the IRAM 30 m telescope are indicated with a superscript. All the other positions have been observed with the 12 m telescope.
l b v $\Delta v$ I(CS) $\frac{I({\rm SiO})}{I({\rm CS})}$

l=1.3-complex region

+1.403^a -0.150 29(1) 22(1) 0.58(3) 0.19(2)

+1.310^a -0.130 33(1) 23(1) 1.58(9) 0.33(3)

+1.403^a -0.150 123(2) 16(1) 0.36(3) 0.17(3)

+1.403^a -0.150 72(1) 33(1) 0.49(3) 0.33(3)

+1.310^a -0.130 85(1) 32(1) 1.53(9) 0.33(3)

+1.310^a -0.130 135(1) 11(4) 0.16(9) $\leq$ 0.42

+1.218 +0.100 119(4) 56(7) 0.39(3) 0.63(8)

+1.218 +0.100 119(2) 17(1) 0.91(3) 0.24(3)

+1.218 +0.100 163(3) 28(4) 0.26(3) 0.34(11)

+1.460^a +0.270 78(1) 32(5) 1.43(7) 0.28(2)

+1.460^a +0.270 116(2) 16(1) 0.64(7) 0.25(6)

+1.698^a -0.150 3(3) 15(3) 0.09(3) 0.7(3)

+1.522^a -0.150 11(2) 24(1) 0.41(4) 0.27(4)

+1.560 -0.300 -26(1) 29(1) 0.54(4) 0.46(6)

+1.522^a -0.150 -23(2) 23(1) 0.22(4) 0.18(6)

+1.403^a -0.150 -41(1) 8(1) 0.15(3) $\leq$ 0.11

+1.403^a -0.150 -22(2) 15(1) 0.30(3) 0.20(4)

+1.310^a -0.130 -13(2) 23(1) 0.73(9) 0.25(7)

+1.620 -0.050 152(5) 30(8) 0.10(6) 0.6(6)

+1.708 -0.150 40(2) 25(2) 0.20(2) 0.57(9)

+1.698^a -0.150 42(3) 19(3) 0.39(3) 0.31(4)

+1.522^a -0.150 56(2) 26(1) 0.27(4) 0.22(5)

+1.620 -0.050 55(5) 16(1) 0.54(5) 0.57(7)

Clump 2

+3.329 +0.425 30(1) 33(1) 1.22(6) 0.34(3)

+3.329 +0.425 150(1) 32(4) 0.24(6) 0.3(2)

+3.235 +0.425 68(3) 22(3) 0.59(6) 0.47(7)

+3.235 +0.425 26(3) 31(3) 0.63(6) 0.32(5)

+3.219 +0.250 84(1) 34(3) 0.38(6) 0.30(10)

+3.219 +0.250 152(1) 58(4) 0.33(6) 0.47(13)

+3.210 +0.263 77(1) 27(2) 0.45(6) 0.32(8)

+3.210 +0.263 146(1) 55(3) 0.33(6) 0.29(11)

+3.193 +0.100 101(1) 27(2) 0.78(6) 0.35(7)

+3.193 +0.100 142(1) 27(3) 0.46(6) 0.22(11)

+3.172 +0.175 119(1) 45(1) 0.72(5) 0.44(7)

+3.172 +0.175 183(2) 31(6) 0.16(5) 0.9(4)

+3.171 +0.300 29(1) 29(2) 0.33(5) 0.41(12)

+3.171 +0.300 84(2) 33(1) 0.92(5) 0.32(4)

+3.171 +0.300 143(1) 37(4) 0.19(5) 0.3(2)

+3.138 +0.425 7(1) 23(2) 0.54(4) 0.32(5)

+3.138 +0.425 88(2) 28(1) 1.03(4) 0.34(3)

+3.138 +0.425 130(1) 30(2) 0.46(4) 0.27(6)

+3.136 +0.250 131(4) 32(7) 0.11(5) 0.4(4)

+3.136 +0.250 88(1) 30(3) 0.35(5) 0.29(12)

+3.136 +0.250 31(2) 29(1) 0.53(5) 0.47(9)

+3.074 +0.375 18(2) 37(1) 0.52(6) 0.38(8)

+3.047 -0.013 59(1) 34(2) 0.35(5) 0.4(2)

+3.020 +0.150 156(1) 46(1) 0.67(6) 0.45(7)

+3.020 +0.050 136(1) 17(1) 0.62(4) 0.36(6)

+2.895 +0.050 116(1) 56(3) 0.74(2) 0.39(2)

Galactic center ring

Sgr E

-1.178 +0.050 -182(2) 21(8) 0.15(2) $\leq$ 0.87

-1.178 +0.050 -203(2) 14(3) 0.16(2) $\leq$ 0.87

Sgr B

+0.830^a -0.180 31(2) 32(3) 1.12(7) 0.29(5)

+0.830^a -0.180 56(1) 27(1) 1.71(7) 0.32(3)

Sgr A

+0.227 -0.050 74(2) 21(1) 0.97(5) 0.21(2)

+0.150^a -0.050 25(2) 13(1) 0.52(6) $\leq$ 0.19

+0.150^a -0.050 61(2) 23(2) 1.30(6) 0.08(1)

+0.145^a -0.080 52(1) 36(2) 2.21(9) 0.20(2)

+0.145^a -0.150 28(1) 22(1) 0.59(3) 0.12(4)

+0.145^a -0.120 32(2) 8(1) 0.44(7) 0.30(7)

+0.145^a -0.120 50(1) 29(1) 0.97(7) 0.25(3)

+0.100^a -0.120 30(3) 25(3) 2.53(7) 0.15(1)

+0.100^a -0.120 68(3) 15(3) 0.85(7) $\leq$ 0.16

Other sources

+0.830^a -0.180 99(1) 17(1) 0.67(7) $\leq$ 0.20

+0.945 -0.150 73(2) 17(1) 1.18(6) 0.21(2)

+0.945^a -0.050 86(2) 23(2) 1.31(8) 0.28(2)

+0.410^a +0.030 17(3) 20(3) 1.84(4) 0.41(2)

+0.410^a +0.030 37(3) 13(3) 1.38(4) $\leq$ 0.10

+0.410^a +0.030 -51(3) 19(3) 0.52(4) 0.35(7)

+0.410^a +0.030 -21(3) 21(3) 0.26(4) 0.3(2)

+0.401 -0.150 12(1) 35(3) 0.24(4) $\leq$ 0.22

+0.390^a -0.150 -3(1) 9(2) 0.42(2) $\leq$ 0.11

+0.390^a -0.150 13(1) 28(4) 0.30(2) $\leq$ 0.15

+0.227 -0.050 29(1) 18(2) 1.51(5) 0.10(1)

+0.227 -0.050 -30(2) 28(4) 0.14(5) $\leq$ 0.51

+0.150^a
-0.050 -92(2) 13(2) 0.27(6) $\leq$ 0.33

+0.150^a -0.050 -65(1) 14(3) 0.14(6) $\leq$ 0.54

+0.145^a -0.080 -14(1) 10(1) 1.68(9) $\leq$ 0.08

+0.100^a
-0.120 -2(3) 14(3) 0.35(7) $\leq$ 0.35

-0.198 -0.050 27(2) 27(1) 0.63(5) 0.11(3)

-0.198 -0.050 85(3) 33(8) 0.10(5) 0.5(3)

-0.198 -0.050 -18(1) 21(2) 0.35(5) $\leq$ 0.17

-0.460 -0.300 45(4) 34(9) 0.18(4) $\leq$ 0.25

-0.460 -0.300 72(2) 18(4) 0.18(4) $\leq$ 0.25

-0.503^a -0.050 -53(1) 21(2) 0.16(4) 0.9(5)

-0.503^a -0.050 -147(1) 8(3) 0.17(4) 0.6 (5)

-0.503^a -0.050 -103(1) 11(2) 1.42(4) 0.18(5)

-0.590^a -0.050 -148(2) 25(6) 0.12(2) $\leq$ 1.24

-0.590^a -0.050 -116(2) 14(1) 1.02(2) 0.28(1)

-0.688^a -0.050 -129(1) 17(2) 0.31(4) $\leq$ 0.61

-0.754 -0.050 -132(2) 61(4) 0.17(4) $\leq$ 0.25

F

-0.655 +0.100 -165(2) 20(4) 0.14(3) $\leq$ 0.24

-0.655 +0.100 -117(2) 15(4) 0.10(3) $\leq$ 0.33

-0.503^a +0.150 -145(6) 21(2) 0.59(5) $\leq$ 0.17

-0.503^a +0.150 -112(1) 20(3) 0.28(5) $\leq$ 0.33

-0.285 +0.100 -87(4) 20(9) 0.07(3) $\leq$ 0.77

-0.285 +0.100 -51(4) 22(7) 0.09(2) $\leq$ 0.72

L

-0.503^a -0.050 144(3) 17(4) 0.07(4) $\leq$ 1.26

-0.590^a -0.050 132(1) 8(1) 0.12(2) $\leq$ 1.24

-0.590^a -0.050 152(1) 7(2) 0.10(2) $\leq$ 1.44

-0.688^a -0.050 142(1) 10(1) 0.30(4) $\leq$ 0.63

-0.754 -0.050 118(2) 41(5) 0.16(4) $\leq$ 0.26

-0.503^a +0.150 171(4) 52(9) 0.12(4) $\leq$ 0.63

-0.655 +0.100 161(6) 20(2) 0.29(3) 0.21(5)

-0.862 +0.100 152(1) 18(1) 0.54(4) 0.24(2)

-0.950 +0.150 129(1) 23(2) 0.42(5) 0.40(10)

-0.982 +0.100 130(2) 18(2) 0.30(3) 0.27(5)

O

+2.895 +0.050 8(2) 24(4) 0.30(2) $\leq$ 0.38

+2.880 +0.113 9(1) 22(2) 0.32(4) 0.28(1)

+2.720 -0.150 9(4) 19(6) 0.07(4) $\leq$ 0.55

+2.610 +0.000 -9(2) 28(5) 0.14(3) $\leq$ 0.47

+2.610 +0.000 -39(3) 16(6) 0.07(3) $\leq$ 0.78

+2.568 +0.150 4(2) 23(4) 0.12(3) $\leq$ 0.60

+2.121 -0.150 -47(1) 13(3) 0.14(3) $\leq$ 0.37

+2.121 -0.150 25(4) 49(8) 0.06(3) $\leq$ 0.68

+2.056 -0.300 1(2) 23(2) 0.17(3) $\leq$ 0.31

+2.056 -0.300 36(1) 18(3) 0.11(3) $\leq$ 0.44

P

-0.590^a -0.050 -41(1) 14(2) 0.28(2) $\leq$ 0.59

-0.688^a -0.050 -41(1) 26(3) 0.42(4) $\leq$ 0.47

-0.688^a -0.050 -17(1) 16(2) 0.57(4) 0.51(7)

-0.688^a -0.050 2(1) 25(2) 0.59(4) 0.47(7)

-0.754 -0.050 -10(2) 37(3) 0.32(4) 0.15(4)

-0.829 -0.300 -18(1) 40(2) 0.22(3) $\leq$ 0.35

-0.906 -0.150 -2(2) 39(2) 0.40(5) 0.24(4)

-0.655 +0.100 2(2) 24(7) 0.09(3) $\leq$ 0.35

-0.862 +0.100 -1(1) 23(3) 0.25(4) 0.24(5)

J

+2.720 -0.150 96(1) 23(3) 0.29(4) 0.45(8)

+2.056 -0.300 141(2) 23(2) 0.16(3) $\leq$ 0.33

+1.958^a -0.100 122(3) 27(1) 0.56(6) 0.25(3)

K

+1.958^a -0.100 247(1) 9(3) 0.22(6) $\leq$ 0.32

+1.708 -0.150 221(4) 31(6) 0.08(2) $\leq$ 0.85

+1.698^a -0.150 220(3) 20(3) 0.16(3) $\leq$ 0.20

+1.522^a -0.150 219(3) 16(1) 0.42(4) $\leq$ 0.09

+1.403^a -0.150 214(6) 21(5) 0.14(3) 0.14(4)

+1.310^a -0.130 204(2) 19(4) 0.11(9) $\leq$ 0.53

+0.401 -0.150 192(3) 28(8) 0.08(4) $\leq$ 0.49

+0.390^a -0.150 195(2) 8(1) 0.39(2) $\leq$ 0.12

+0.145^a -0.150 175(2) 7(1) 0.20(3) $\leq$ 0.38

+1.698^a -0.150 185(3) 12(3) 0.11(3) 0.5(2)

+1.698^a -0.150 163(3) 13(3) 0.12(3) $\leq$ 0.25

+1.708 -0.150 157(6) 48(9) 0.53(2) $\leq$ 0.01

+0.227 -0.050 176(1) 10(1) 0.20(5) $\leq$ 0.39

+0.150^a -0.050 154(1) 4(1) 0.20(6) $\leq$ 0.42

+0.145^a -0.080 177(2) 12(4) 0.21(9) $\leq$ 0.47

M

+0.401 -0.150 -102(4) 53(8) 0.10(4) $\leq$ 0.42

+0.390^a -0.150 -92(2) 12(4) 0.06(2) 0.7(3)

+0.390^a -0.150 -71(3) 18(8) 0.05(2) 1.0(5)

+0.145^a -0.150 -131(1) 8(3) 0.09(3) $\leq$ 0.71

+0.145^a -0.150 -107(5) 64(9) 0.10(3) $\leq$ 0.66

+0.063 -0.300 -140(2) 38(4) 0.12(3) $\leq$ 0.40

-0.460 -0.300 -118(1) 22(1) 0.60(4) 0.09(2)

-0.829 -0.300 -123(3) 39(9) 0.10(3) $\leq$ 0.66

-0.906 -0.150 -133(1) 22(3) 0.19(5) $\leq$ 0.27

-0.906 -0.150 -169(2) 27(8) 0.11(5) $\leq$ 0.40

+0.945^a -0.050 -81(2) 14(3) 0.23(8) 0.3(2)

+0.945^a -0.050 -65(2) 14(3) 0.22(8) 0.18(9)

N

-1.102 -0.250 -44(2) 39(4) 0.21(5) 0.26(11)

-1.189 -0.300 -4(1) 13(4) 0.19(4) $\leq$ 0.58

-1.189 -0.300 -42(1) 41(3) 0.43(4) 0.21(5)

-1.189 -0.300 -103(3) 15(6) 0.08(4) $\leq$ 1.08

-1.211 -0.150 -118(2) 25(2) 0.50(4) 0.26(6)

-1.211 -0.150 -42(1) 34(2) 0.46(4) 0.28(6)

**Table 2:** Galactic longitude and latitude (in degrees), velocity (km s^-1), widths (km s^-1), and intensities (K) of the CS lines. In addition, the SiO to CS intensity ratio is also shown. The numbers in parentheses are the uncertainties on the last digit. The positions observed with the IRAM 30 m telescope are indicated with a superscript. All the other positions have been observed with the 12 m telescope.
l	b	v	$\Delta v$	I(CS)	$\frac{I({\rm SiO})}{I({\rm CS})}$
l=1.3-complex region
+1.403^a	-0.150	29(1)	22(1)	0.58(3)	0.19(2)
+1.310^a	-0.130	33(1)	23(1)	1.58(9)	0.33(3)
+1.403^a	-0.150	123(2)	16(1)	0.36(3)	0.17(3)
+1.403^a	-0.150	72(1)	33(1)	0.49(3)	0.33(3)
+1.310^a	-0.130	85(1)	32(1)	1.53(9)	0.33(3)
+1.310^a	-0.130	135(1)	11(4)	0.16(9)	$\leq$ 0.42
+1.218	+0.100	119(4)	56(7)	0.39(3)	0.63(8)
+1.218	+0.100	119(2)	17(1)	0.91(3)	0.24(3)
+1.218	+0.100	163(3)	28(4)	0.26(3)	0.34(11)
+1.460^a	+0.270	78(1)	32(5)	1.43(7)	0.28(2)
+1.460^a	+0.270	116(2)	16(1)	0.64(7)	0.25(6)
+1.698^a	-0.150	3(3)	15(3)	0.09(3)	0.7(3)
+1.522^a	-0.150	11(2)	24(1)	0.41(4)	0.27(4)
+1.560	-0.300	-26(1)	29(1)	0.54(4)	0.46(6)
+1.522^a	-0.150	-23(2)	23(1)	0.22(4)	0.18(6)
+1.403^a	-0.150	-41(1)	8(1)	0.15(3)	$\leq$ 0.11
+1.403^a	-0.150	-22(2)	15(1)	0.30(3)	0.20(4)
+1.310^a	-0.130	-13(2)	23(1)	0.73(9)	0.25(7)
+1.620	-0.050	152(5)	30(8)	0.10(6)	0.6(6)
+1.708	-0.150	40(2)	25(2)	0.20(2)	0.57(9)
+1.698^a	-0.150	42(3)	19(3)	0.39(3)	0.31(4)
+1.522^a	-0.150	56(2)	26(1)	0.27(4)	0.22(5)
+1.620	-0.050	55(5)	16(1)	0.54(5)	0.57(7)
Clump 2
+3.329	+0.425	30(1)	33(1)	1.22(6)	0.34(3)
+3.329	+0.425	150(1)	32(4)	0.24(6)	0.3(2)
+3.235	+0.425	68(3)	22(3)	0.59(6)	0.47(7)
+3.235	+0.425	26(3)	31(3)	0.63(6)	0.32(5)
+3.219	+0.250	84(1)	34(3)	0.38(6)	0.30(10)
+3.219	+0.250	152(1)	58(4)	0.33(6)	0.47(13)
+3.210	+0.263	77(1)	27(2)	0.45(6)	0.32(8)
+3.210	+0.263	146(1)	55(3)	0.33(6)	0.29(11)
+3.193	+0.100	101(1)	27(2)	0.78(6)	0.35(7)
+3.193	+0.100	142(1)	27(3)	0.46(6)	0.22(11)
+3.172	+0.175	119(1)	45(1)	0.72(5)	0.44(7)
+3.172	+0.175	183(2)	31(6)	0.16(5)	0.9(4)
+3.171	+0.300	29(1)	29(2)	0.33(5)	0.41(12)
+3.171	+0.300	84(2)	33(1)	0.92(5)	0.32(4)
+3.171	+0.300	143(1)	37(4)	0.19(5)	0.3(2)
+3.138	+0.425	7(1)	23(2)	0.54(4)	0.32(5)
+3.138	+0.425	88(2)	28(1)	1.03(4)	0.34(3)
+3.138	+0.425	130(1)	30(2)	0.46(4)	0.27(6)
+3.136	+0.250	131(4)	32(7)	0.11(5)	0.4(4)
+3.136	+0.250	88(1)	30(3)	0.35(5)	0.29(12)
+3.136	+0.250	31(2)	29(1)	0.53(5)	0.47(9)
+3.074	+0.375	18(2)	37(1)	0.52(6)	0.38(8)
+3.047	-0.013	59(1)	34(2)	0.35(5)	0.4(2)
+3.020	+0.150	156(1)	46(1)	0.67(6)	0.45(7)
+3.020	+0.050	136(1)	17(1)	0.62(4)	0.36(6)
+2.895	+0.050	116(1)	56(3)	0.74(2)	0.39(2)
Galactic center ring
Sgr E
-1.178	+0.050	-182(2)	21(8)	0.15(2)	$\leq$ 0.87
-1.178	+0.050	-203(2)	14(3)	0.16(2)	$\leq$ 0.87
Sgr B
+0.830^a	-0.180	31(2)	32(3)	1.12(7)	0.29(5)
+0.830^a	-0.180	56(1)	27(1)	1.71(7)	0.32(3)
Sgr A
+0.227	-0.050	74(2)	21(1)	0.97(5)	0.21(2)
+0.150^a	-0.050	25(2)	13(1)	0.52(6)	$\leq$ 0.19
+0.150^a	-0.050	61(2)	23(2)	1.30(6)	0.08(1)
+0.145^a	-0.080	52(1)	36(2)	2.21(9)	0.20(2)
+0.145^a	-0.150	28(1)	22(1)	0.59(3)	0.12(4)
+0.145^a	-0.120	32(2)	8(1)	0.44(7)	0.30(7)
+0.145^a	-0.120	50(1)	29(1)	0.97(7)	0.25(3)
+0.100^a	-0.120	30(3)	25(3)	2.53(7)	0.15(1)
+0.100^a	-0.120	68(3)	15(3)	0.85(7)	$\leq$ 0.16
Other sources
+0.830^a	-0.180	99(1)	17(1)	0.67(7)	$\leq$ 0.20
+0.945	-0.150	73(2)	17(1)	1.18(6)	0.21(2)
+0.945^a	-0.050	86(2)	23(2)	1.31(8)	0.28(2)
+0.410^a	+0.030	17(3)	20(3)	1.84(4)	0.41(2)
+0.410^a	+0.030	37(3)	13(3)	1.38(4)	$\leq$ 0.10
+0.410^a	+0.030	-51(3)	19(3)	0.52(4)	0.35(7)
+0.410^a	+0.030	-21(3)	21(3)	0.26(4)	0.3(2)
+0.401	-0.150	12(1)	35(3)	0.24(4)	$\leq$ 0.22
+0.390^a	-0.150	-3(1)	9(2)	0.42(2)	$\leq$ 0.11
+0.390^a	-0.150	13(1)	28(4)	0.30(2)	$\leq$ 0.15
+0.227	-0.050	29(1)	18(2)	1.51(5)	0.10(1)
+0.227	-0.050	-30(2)	28(4)	0.14(5)	$\leq$ 0.51
+0.150^a	-0.050	-92(2)	13(2)	0.27(6)	$\leq$ 0.33
+0.150^a	-0.050	-65(1)	14(3)	0.14(6)	$\leq$ 0.54
+0.145^a	-0.080	-14(1)	10(1)	1.68(9)	$\leq$ 0.08
+0.100^a	-0.120	-2(3)	14(3)	0.35(7)	$\leq$ 0.35
-0.198	-0.050	27(2)	27(1)	0.63(5)	0.11(3)
-0.198	-0.050	85(3)	33(8)	0.10(5)	0.5(3)
-0.198	-0.050	-18(1)	21(2)	0.35(5)	$\leq$ 0.17
-0.460	-0.300	45(4)	34(9)	0.18(4)	$\leq$ 0.25
-0.460	-0.300	72(2)	18(4)	0.18(4)	$\leq$ 0.25
-0.503^a	-0.050	-53(1)	21(2)	0.16(4)	0.9(5)
-0.503^a	-0.050	-147(1)	8(3)	0.17(4)	0.6 (5)
-0.503^a	-0.050	-103(1)	11(2)	1.42(4)	0.18(5)
-0.590^a	-0.050	-148(2)	25(6)	0.12(2)	$\leq$ 1.24
-0.590^a	-0.050	-116(2)	14(1)	1.02(2)	0.28(1)
-0.688^a	-0.050	-129(1)	17(2)	0.31(4)	$\leq$ 0.61
-0.754	-0.050	-132(2)	61(4)	0.17(4)	$\leq$ 0.25
F
-0.655	+0.100	-165(2)	20(4)	0.14(3)	$\leq$ 0.24
-0.655	+0.100	-117(2)	15(4)	0.10(3)	$\leq$ 0.33
-0.503^a	+0.150	-145(6)	21(2)	0.59(5)	$\leq$ 0.17
-0.503^a	+0.150	-112(1)	20(3)	0.28(5)	$\leq$ 0.33
-0.285	+0.100	-87(4)	20(9)	0.07(3)	$\leq$ 0.77
-0.285	+0.100	-51(4)	22(7)	0.09(2)	$\leq$ 0.72
L
-0.503^a	-0.050	144(3)	17(4)	0.07(4)	$\leq$ 1.26
-0.590^a	-0.050	132(1)	8(1)	0.12(2)	$\leq$ 1.24
-0.590^a	-0.050	152(1)	7(2)	0.10(2)	$\leq$ 1.44
-0.688^a	-0.050	142(1)	10(1)	0.30(4)	$\leq$ 0.63
-0.754	-0.050	118(2)	41(5)	0.16(4)	$\leq$ 0.26
-0.503^a	+0.150	171(4)	52(9)	0.12(4)	$\leq$ 0.63
-0.655	+0.100	161(6)	20(2)	0.29(3)	0.21(5)
-0.862	+0.100	152(1)	18(1)	0.54(4)	0.24(2)
-0.950	+0.150	129(1)	23(2)	0.42(5)	0.40(10)
-0.982	+0.100	130(2)	18(2)	0.30(3)	0.27(5)
O
+2.895	+0.050	8(2)	24(4)	0.30(2)	$\leq$ 0.38
+2.880	+0.113	9(1)	22(2)	0.32(4)	0.28(1)
+2.720	-0.150	9(4)	19(6)	0.07(4)	$\leq$ 0.55
+2.610	+0.000	-9(2)	28(5)	0.14(3)	$\leq$ 0.47
+2.610	+0.000	-39(3)	16(6)	0.07(3)	$\leq$ 0.78
+2.568	+0.150	4(2)	23(4)	0.12(3)	$\leq$ 0.60
+2.121	-0.150	-47(1)	13(3)	0.14(3)	$\leq$ 0.37
+2.121	-0.150	25(4)	49(8)	0.06(3)	$\leq$ 0.68
+2.056	-0.300	1(2)	23(2)	0.17(3)	$\leq$ 0.31
+2.056	-0.300	36(1)	18(3)	0.11(3)	$\leq$ 0.44
P
-0.590^a	-0.050	-41(1)	14(2)	0.28(2)	$\leq$ 0.59
-0.688^a	-0.050	-41(1)	26(3)	0.42(4)	$\leq$ 0.47
-0.688^a	-0.050	-17(1)	16(2)	0.57(4)	0.51(7)
-0.688^a	-0.050	2(1)	25(2)	0.59(4)	0.47(7)
-0.754	-0.050	-10(2)	37(3)	0.32(4)	0.15(4)
-0.829	-0.300	-18(1)	40(2)	0.22(3)	$\leq$ 0.35
-0.906	-0.150	-2(2)	39(2)	0.40(5)	0.24(4)
-0.655	+0.100	2(2)	24(7)	0.09(3)	$\leq$ 0.35
-0.862	+0.100	-1(1)	23(3)	0.25(4)	0.24(5)
J
+2.720	-0.150	96(1)	23(3)	0.29(4)	0.45(8)
+2.056	-0.300	141(2)	23(2)	0.16(3)	$\leq$ 0.33
+1.958^a	-0.100	122(3)	27(1)	0.56(6)	0.25(3)
K
+1.958^a	-0.100	247(1)	9(3)	0.22(6)	$\leq$ 0.32
+1.708	-0.150	221(4)	31(6)	0.08(2)	$\leq$ 0.85
+1.698^a	-0.150	220(3)	20(3)	0.16(3)	$\leq$ 0.20
+1.522^a	-0.150	219(3)	16(1)	0.42(4)	$\leq$ 0.09
+1.403^a	-0.150	214(6)	21(5)	0.14(3)	0.14(4)
+1.310^a	-0.130	204(2)	19(4)	0.11(9)	$\leq$ 0.53
+0.401	-0.150	192(3)	28(8)	0.08(4)	$\leq$ 0.49
+0.390^a	-0.150	195(2)	8(1)	0.39(2)	$\leq$ 0.12
+0.145^a	-0.150	175(2)	7(1)	0.20(3)	$\leq$ 0.38
+1.698^a	-0.150	185(3)	12(3)	0.11(3)	0.5(2)
+1.698^a	-0.150	163(3)	13(3)	0.12(3)	$\leq$ 0.25
+1.708	-0.150	157(6)	48(9)	0.53(2)	$\leq$ 0.01
+0.227	-0.050	176(1)	10(1)	0.20(5)	$\leq$ 0.39
+0.150^a	-0.050	154(1)	4(1)	0.20(6)	$\leq$ 0.42
+0.145^a	-0.080	177(2)	12(4)	0.21(9)	$\leq$ 0.47
M
+0.401	-0.150	-102(4)	53(8)	0.10(4)	$\leq$ 0.42
+0.390^a	-0.150	-92(2)	12(4)	0.06(2)	0.7(3)
+0.390^a	-0.150	-71(3)	18(8)	0.05(2)	1.0(5)
+0.145^a	-0.150	-131(1)	8(3)	0.09(3)	$\leq$ 0.71
+0.145^a	-0.150	-107(5)	64(9)	0.10(3)	$\leq$ 0.66
+0.063	-0.300	-140(2)	38(4)	0.12(3)	$\leq$ 0.40
-0.460	-0.300	-118(1)	22(1)	0.60(4)	0.09(2)
-0.829	-0.300	-123(3)	39(9)	0.10(3)	$\leq$ 0.66
-0.906	-0.150	-133(1)	22(3)	0.19(5)	$\leq$ 0.27
-0.906	-0.150	-169(2)	27(8)	0.11(5)	$\leq$ 0.40
+0.945^a	-0.050	-81(2)	14(3)	0.23(8)	0.3(2)
+0.945^a	-0.050	-65(2)	14(3)	0.22(8)	0.18(9)
N
-1.102	-0.250	-44(2)	39(4)	0.21(5)	0.26(11)
-1.189	-0.300	-4(1)	13(4)	0.19(4)	$\leq$ 0.58
-1.189	-0.300	-42(1)	41(3)	0.43(4)	0.21(5)
-1.189	-0.300	-103(3)	15(6)	0.08(4)	$\leq$ 1.08
-1.211	-0.150	-118(2)	25(2)	0.50(4)	0.26(6)
-1.211	-0.150	-42(1)	34(2)	0.46(4)	0.28(6)

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