Table B.1
Spitzer/IRS low-resolution measurements.
| Method | Regular | Optimal | Regular | Optimal | Optimal customa | Regular | Optimal |
|
|
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| SL | 9008640 | 9008640 | 16205568 | 16205568 | 16205568 | 12622848 | 12622848 |
| (Ap.) | (Ap., meth.) | (Pref.) | (Meth.) | (Pref.) | (Ap.) | (Ap., meth.) | |
|
|
|||||||
| H i Huα12.37 μm | < 7 | < 5 | 8.2 ± 2.5 | 4.1 ± 1.5 | 2.6 ± 2.0,5.5 ± 1.8 | 7.0 ± 3.5 | 6.5 ± 3.3 |
| [Ne ii] 12.8 μm | < 9 | < 6 | < 2 | 4.1 ± 1.7 | 3.0 ± 1.6,5.2 ± 2.6 | 8.5 ± 3.5 | 6.0 ± 3.1 |
| [S iv] 10.5 μm | < 10 | < 6 | 40 ± 3 | 19 ± 2 | 14 ± 2,34 ± 2 | 39 ± 4 | 29 ± 3 |
| [Ar ii] 7.0 μm | ... | ... | < 5 | < 3 | ... | < 5 | < 3 |
| [Ar iii] 9.0 μm | < 5 | < 7 | < 8 | < 3 | < 10 | < 15 | < 3 |
|
|
|||||||
| LL | 9008640 | 9008640 | 16205568 | 16205568 | 16205568 | 12622848 | 12622848 |
| (Pref.) | (Pref., meth.) | (Pref.) | (Pref., meth.) | (Pref.) | (Pref.) | (Pref., meth.) | |
|
|
|||||||
| [O iv]+[Fe ii] | 66 ± 19 | 52 ± 12 | 53 ± 22 | 43 ± 11 | 53 ± 11 | 79 ± 20 | 60 ± 15 |
| [Ne iii] 15.5 μm | 71 ± 13 | 66 ± 17 | 83 ± 8 | 65 ± 8 | 76 ± 10 | 104 ± 41 ∗ | 59 ± 13 |
| [Ne iii] 36.0 μm | ... | < 14 | < 11 | < 51 | 46 ± 24 ∗ | 135 ± 70 ∗ | 60 ± 24 ∗ |
| [Ne v] 14.3 μm | < 14 | < 21 | < 7 | < 8 | < 8 | < 21 | < 19 |
| [Ne v] 24.3 μm | < 23 | < 14 | < 10 | < 8 | < 9 | < 18 | < 13 |
| [S iii] 18.7 μm | 39 ± 17 | 46 ± 15 | 43 ± 6 | 40 ± 6 | 47 ± 8 | 42 ± 17 | 56 ± 16 |
| [S iii] 33.5 μm | < 45 | 65 ± 16 | 60 ± 10 | 45 ± 13 | 48 ± 12 | 91 ± 30 | 57 ± 11 |
| [Ar iii] 21.8 μm | < 29 | < 21 | < 13 | < 10 | < 13 | < 23 | < 17 |
| [Fe iii] 23.0 μm | < 28 | < 19 | < 12 | < 10 | < 12 | < 21 | < 15 |
| [Si ii] 34.8 μm | < 75 | 96 ± 30 | 96 ± 14 | 50 ± 11 | 65 ± 12 | 130 ± 63 | 115 ± 24 |
| [Fe ii] 17.9 μm | < 27 | < 24 | < 11 | < 9 | < 11 | < 20 | < 15 |
| H2 S(0) 28.2 μm | < 17 | < 14 | < 10 | < 7 | < 7 | < 14 | < 11 |
| H2 S(1) 17.0 μm | < 17 | < 24 | < 10 | < 9 | < 9 | < 21 | < 17 |
Notes. Fluxes are in units of 10-19 W m-2. Upper limits are 1σ. The line below the AORkey indicates whether the total emission from NW+SE is underestimated due to aperture mispointing (“Ap.”) or underestimated because the optimal extraction method is adapted to point sources (“Meth.”). The preferred determination is indicated with “Pref.”. Line fluxes followed by asterisks are deemed unreliable due to the presence of spurious features. Ellipses indicate that the line flux cannot be determined (because of numerous spurious features).
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