Table 3
Percent line contribution MIRI filters.
| NGC 7023 | |||||
|---|---|---|---|---|---|
| ATM | DF1 | DF2 | MOL | DF3 | |
| F560W | 0.05(0.05,0.0) | 0.9(0.9,0.0) | 0.8(0.8,0.0) | 0.7(0.7,0.0) | 0.9(0.9,0.0) |
| F770W | 0.04(0.04,0.0) | 0.6(0.6,0.0) | 0.6(0.6,0.0) | 0.5(0.5,0.0) | 0.7(0.7,0.0) |
| F1000W | 0.4(0.4,0.0) | 3.5(3.5,0.0) | 3.3(3.3,0.0) | 2.8(2.8,0.0) | 4.8(4.8,0.0) |
| F1130W | 0.0 | 0.0 | 0.0 | 0.0 | 0.0 |
| F1280W | 0.3(0.3,0.0) | 0.7(0.7,0.0) | 0.8(0.8,0.0) | 0.8(0.8,0.0) | 2.3(2.3,0.0) |
| F1500W | 0.11(0.03,0.08) | 0.05(0.04,0.01) | 0.05(0.04,0.01) | 0.12(0.09,0.03) | 0.11(0.1,0.01) |
| F1800W | 1.0(1.0,0.0) | 1.7(1.7,0.0) | 1.7(1.7,0.0) | 1.8(1.8,0.0) | 5.0(5.0,0.0) |
| F2100W | 0.0 | 0.0 | 0.0 | 0.0 | 0.0 |
| F2550W | 0.0 | 0.05(0.04,0.01) | 0.05(0.04,0.01) | 0.0 | 0.0 |
| Horsehead | |||||
| HIIa | DF1 | DF2 | MO1 | DF3 | |
| F560W | 0.0 | 6.0(6.0,0.0) | 2.3(2.3,0.0) | 2.6(2.6,0.0) | 0.0 |
| F770W | 100.0(7.4,92.6) | 7.9(4.2,3.7) | 4.8(1.9,2.9) | 3.1(2.3,0.8) | 4.1(1.7,2.4) |
| F1000W | 8.8(8.8,0.0) | 19.8(19.8,0.0) | 12.3(12.3,0.0) | 13.5(13.5,0.0) | 12.1(12.1,0.0) |
| F1130W | 0.0 | 0.0 | 0.0 | 0.0 | 0.0(0.0,0.0) |
| F1280W | 85.4(1.9,83.5) | 27.0(7.2,19.8) | 26.0(8.3,17.7) | 13.4(8.7,4.7) | 31.2(12.7,18.5) |
| F1500W | 2.2(0.1,2.1) | 0.7(0.3,0.4) | 0.6(0.3,0.3) | 0.5(0.4,0.1) | 2.6(2.6,0.0) |
| F1800W | 41.9(1.9,40.0) | 15.8(8.0,7.9) | 14.7(8.1,6.6) | 12.9(10.9,2.0) | 69.6(38.3,31.3) |
| F2100W | 19.3(0.0,19.3) | 4.7(0.0,4.7) | 3.7(0.0,3.7) | 1.3(0.0,1.3) | 19.9(0.0,19.9) |
| F2550W | 0.0 | 0.0 | 0.0 | 0.0 | 0.0 |
Notes. Line contribution percentages are presented as ftotal(fH2, fother) where fH2 is the percentage of signal contributed by H2 in the band pass, fother is all other lines in the band pass and ftotal = fH2 + fother. aContinuum is poorly defined short-wards of 15 μm resulting in uncertain calculation.
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