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Table A.1.

Spitzer IRS and MIPS fluxes and 9.7 μm silicate strength.

IRAS name S9.7 μm(a) IRS 34 μm (b) MIPS 70 μm MIPS 160 μm
00091−0738 −3.20 ± 0.12 1.07
00188−0856 −2.72 ± 0.08 0.80 2.65 1.91
00509+1225 0.30 ± 0.01 1.34
01572+0009 0.19 ± 0.02 1.17
F05189−2524 −0.32 ± 0.01 7.30
07251−0248 −2.77 ± 0.06 2.62
09022−3615 −1.04 ± 0.01 3.53
F10190+1322 −1.09 ± 0.02 0.85 3.55
11095−0238 −3.43 ± 0.07 1.54 2.95 1.28
F12072−0444 −1.42 ± 0.02 1.20
F12112+0305 −1.35 ± 0.03 2.06
13120−5453 −1.18 ± 0.01 10.1
F13451+1232 −0.32 ± 0.02 1.03 2.04 1.41
F14348−1447 −1.89 ± 0.03 1.98
F14378−3651 −1.44 ± 0.05 1.85
F15327+2340 −2.74 ± 0.01 34.4
16090−0139 −2.65 ± 0.06 1.07
16155+0146 −2.41 ± 0.07 0.75
17208−0014 −1.56 ± 0.01 8.67
F19297−0406 −1.49 ± 0.04 2.12
19542+1110 −0.97 ± 0.02 2.19
20087−0308 −1.82 ± 0.04 0.99
20100−4156 −2.79 ± 0.06 1.81 4.56 2.33
20414−1651 −1.62 ± 0.08 1.25
F22491−1808 −1.19 ± 0.03 2.20

Notes. Fluxes are in Jy. The flux uncertainties are dominated by the ∼10% calibration uncertainty.

(a)

9.7 μm silicate strength from the IDEOS database (Hernán-Caballero et al. 2020; Spoon et al., in prep.) based on the IRS spectroscopy of these ULIRGs.

(b)

34 μm observed wavelength flux measured in the Spitzer/IRS spectrum.

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