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Home All issues Volume 507 / No 2 (November IV 2009) A&A, 507 2 (2009) 713-721 Full HTML
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Table 2:

Parameters from the Spitzer IRS spectra.
2MASS LW2 / F15 F24 F35 [Ne III] [S III]
  6-10 $\mu $m mJy mJy mJy 15.55 18.71
00285431-7726146 0.57 7.03 9.3 27.2 6.1 16.0
00445167-2653191     4.8 11.7 - -
01051501-2612466 0.49 2.88 4.6 11.6 5.8 12.0
02542961+1509122 0.52 2.15 3.0 8.1 1.6 4.2
03574895-1340458 0.61 14.48 25.2 85.0 3.6 19.1
06033357-4509412     89.3 468.5 - -
12482307-0344102     4.7 12.0 - 2.4
13165999-3336459     5.3 14.2 - 2.6
13371721+0904430     6.2 22.8 - 2.1
15160785-1608098     3.3 9.5 - 3.0
15554606+1532218$^{\rm ~*}$ 0.40 2.88 5.3 13.7 2.5 5.9
16132299+4203418     13.6 51.4 - 6.1
19184395-3815471     7.7 24.8 - 0.8
21573517+0114331 0.42 3.06 3.9 9.6 <0.7 3.2
22023161-5657577 0.58 4.34 7.6 18.7 <2.0 8.1
22565483-3649515 0.58 1.60 2.2 6.0 <1.0 5.2
23055422-3539591     3.0 7.7 - -
23075850+0537063     3.2 9.5 - -
23080919+0538305 0.41 3.22 4.6 11.6 <0.7 4.1

The second column gives the fraction of the 6-10 $\mu $m flux seen in the LW2 passband (5-8.5 $\mu $m). F15 refers to the flux integrated over the ISOCAM LW3 passband (12-18 $\mu $m). The uncertainty of the continua F15, F24, and F35 are about 10%. Emission line fluxes are given in 10 $^{\rm -15}$ erg/s/cm2 with $\sim$10-20% uncertainties; *) absolute photometry uncertain, see footnote in Sect. 3.2.


Source LaTeX | All tables | In the text

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