Table C.1
CO line fluxes in 10-20 W cm-2.
Trans. | λlab (μm) | Central position flux (10-20 W cm-2) | |||||||||||
G327-0.6a | W51N-e1 | DR21(OH) | W33Aa | G34.26+0.15 | NGC 6334-I | NGC 7538-I1 | AFGL2591 | W3IRS5 | G5.89-0.39 | ||||
|
|||||||||||||
CO 14–13 | 185.9990 | 8.52(0.48) | 40.93(1.26) | 29.93(0.67) | 7.96(0.23) | 23.05(1.14) | 40.07(1.60) | 17.79(0.52) | 10.86(0.45) | 76.67(1.38) | 80.36(0.74) | ||
CO 15–14 | 173.6310 | 9.34(0.36) | 50.65(1.83) | 22.65(1.07) | 4.91(0.32) | 26.30(1.07) | 52.70(2.39) | 14.54(0.33) | 7.72(0.57) | 86.13(1.76) | 103.91(1.41) | ||
CO 16–15 | 162.8120 | 8.82(0.51) | 43.10(1.43) | 24.71(0.92) | 4.12(0.18) | 22.71(1.06) | 43.88(1.59) | 11.78(0.39) | 8.00(0.27) | 99.73(1.08) | 105.49(1.76) | ||
CO 17–16 | 153.2670 | 3.00(0.76) | 36.94(1.54) | 16.19(1.21) | 2.74(0.24) | 18.52(1.63) | 31.37(2.46) | 8.60(0.56) | 5.67(0.38) | 86.40(1.31) | 96.31(1.67) | ||
CO 18–17 | 144.7840 | 2.13(0.48) | 27.78(1.89) | 17.40(1.13) | 4.35(0.39) | 18.27(1.53) | 20.93(2.02) | 5.82(0.47) | 5.02(0.53) | 83.05(1.69) | 82.73(1.67) | ||
CO 19–18 | 137.1960 | 6.76(0.64) | 24.18(1.81) | 13.82(1.07) | 3.41(0.37) | 20.16(1.68) | 36.07(2.02) | 4.96(0.42) | 3.02(0.58) | 79.39(1.54) | 60.19(2.14) | ||
CO 20–19 | 130.3690 | 6.68(0.81) | 25.73(1.42) | 15.02(0.93) | 3.54(0.52) | 21.93(1.93) | 37.25(2.19) | 5.31(0.54) | 4.34(0.64) | 77.08(2.27) | 59.14(1.27) | ||
CO 21–20 | 124.1930 | 3.96(1.24) | 22.77(3.15) | 11.38(0.87) | <0.75 | 18.69(2.02) | 34.56(5.43) | 4.62(0.72) | 2.97(0.61) | 60.64(2.13) | 51.31(2.90) | ||
CO 22–21 | 118.5810 | 4.61(1.16) | 20.31(3.29) | 9.79(1.23) | <0.77 | 21.66(3.21) | 35.05(5.02) | 3.97(0.89) | <0.90 | 63.44(2.81) | 44.98(3.84) | ||
CO 24–23 | 108.7630 | <1.78 | < 7.05 | 5.18(1.40) | <0.54 | 18.86(5.45) | 12.89(3.28) | <1.68 | <0.86 | 49.51(3.75) | 21.89(3.45) | ||
CO 27–26 | 96.7730 | <0.86 | 4.71(0.79) | 3.68(0.56) | <1.50 | 4.34(1.22) | 9.46(1.76) | <2.49 | <1.01 | 23.29(2.65) | 6.16(0.81) | ||
CO 28–27 | 93.3490 | <1.75 | 6.28(1.21) | <0.94 | <0.91 | 5.06(1.35) | 11.75(1.99) | <4.97 | <1.04 | 24.72(1.75) | 9.71(1.63) | ||
CO 29–28 | 90.1630 | <1.24 | 5.23(1.54) | <1.23 | <1.25 | 3.67(1.30) | 10.80(5.36) | <6.35 | <1.70 | 20.23(1.94) | 5.38(3.49) | ||
CO 30–29 | 87.1900 | <1.10 | 3.59(0.72) | <1.00 | <1.72 | 4.48(1.10) | <7.00 | <2.10 | <1.57 | 14.38(2.03) | 6.32(2.59) | ||
CO 32–31 | 81.8060 | <1.19 | <5.84 | <1.19 | <1.43 | <2.31 | <4.63 | <1.84 | <2.03 | <9.49 | <3.70 | ||
CO 33–32 | 79.3600 | <3.99 | <11.04 | <1.70 | <2.28 | <3.76 | <18.46 | <2.09 | <1.99 | <3.40 | <13.59 | ||
CO 34–33 | 77.0590 | <1.88 | <4.57 | <1.83 | <1.83 | <3.17 | <2.71 | <1.40 | <2.16 | <5.27 | <6.93 | ||
CO 35–34 | 74.8900 | <2.06 | <2.90 | <0.99 | <1.27 | <2.03 | <3.09 | <2.50 | <1.20 | <1.83 | <18.61 | ||
CO 36–35 | 72.8430 | <0.55 | <0.63 | <0.29 | <0.70 | <1.17 | <1.74 | <0.69 | <0.37 | <7.03 | <3.00 | ||
CO 38–37 | 69.0740 | <1.36 | <1.06 | <1.93 | <0.67 | <1.77 | <1.21 | <3.23 | <2.09 | <2.16 | <2.74 | ||
CO 39–38 | 67.3360 | <1.20 | <0.84 | <0.40 | <1.86 | <0.80 | <2.50 | <2.40 | <0.89 | <1.99 | <3.54 | ||
CO 40–39 | 65.6860 | <0.57 | <2.40 | <0.43 | <1.05 | <2.40 | <1.94 | <2.17 | <0.94 | <2.63 | <2.91 | ||
CO 41–40 | 64.1170 | <1.06 | <1.11 | <0.57 | <1.80 | <1.54 | <2.91 | <1.59 | <1.80 | <5.56 | <4.60 | ||
CO 42–41 | 62.6240 | <1.03 | <2.74 | <0.44 | <1.08 | <2.50 | <2.19 | <1.91 | <2.34 | <4.01 | <5.01 | ||
CO 43–42 | 61.2010 | <0.90 | <1.39 | <0.58 | <1.05 | <1.20 | <4.59 | <2.10 | <2.41 | <4.94 | <6.21 | ||
CO 44–43 | 59.8430 | <0.67 | <1.61 | <0.39 | <0.68 | <1.41 | <3.38 | <2.30 | <1.54 | <2.85 | <3.49 | ||
CO 45–44 | 58.5470 | <0.96 | <1.24 | <0.55 | <1.41 | <1.42 | <1.34 | <1.69 | <1.08 | <6.77 | <4.89 | ||
CO 46–45 | 57.3080 | <2.33 | <10.54 | <1.03 | <1.81 | <4.01 | <6.49 | <3.75 | <2.65 | <6.46 | <8.54 | ||
CO 47–46 | 56.1220 | <0.76 | <1.08 | <0.50 | <2.29 | < 1.85 | <2.51 | <1.39 | <1.71 | <5.78 | <4.79 |
Notes. The uncertainties are 1σ measured in the continuum on both sides of each line; calibration uncertainty of 20% of the flux should be included for comparisons with other modes of observations or instruments. 3σ upper limits calculated using wavelength-dependent values of full-width high maximum for a point source observed with PACS are listed for non-detections. CO 23–22 and CO 31–30 fluxes are not listed due to severe blending with the H2O 414–303 line at 113.537 μm and the OH ,
–
,
line at 84.4 μm, which are often in absorption. CO 25–24, CO 26-25 and CO 37–36 transitions are located in the regions of overlapping orders, where the flux calibration is unreliable.
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