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Table A.2:

The rest of PNe (non-Galactic Bulge) observed within Spitzer/IRS program $\char93 $3633.
IRAS name PN name RA Dec Spectral typea Optical diameterf Distance from GC Dust type
    J2000.0 J2000.0   (arcsec) ( $\hbox{$^\circ$ }$)  

17597-1442
GLMP 698 18 02 38.3 -14 42 03 [WC8]b - 14.77 O
18307-1109 M 1-51 18 33 29.2 -11 07 26 [WC4-6]c 9.5 21.03 mixed
17534-1628 M 1-32 17 56 20.3 -16 29 08 [WC4]d 7.6 12.70 mixed
18408-1347 M 1-60 18 43 38.4 -13 44 56 [WC4]d <10.0 20.30 mixed
17260-1913 M 1-20 17 28 57.6 -19 15 53 welse <7.0 10.40 C
18295-2510 NGC 6644 18 32 34.7 -25 07 44 welsd 2.6 11.14 mixed
18425-3323 IC 4776 18 45 50.7 -33 20 34 welsd 7.5 13.60 mixed
17561-1532 M1-33 17 58 59.2 -15 32 20 unknown 0.0 13.76 mixed
17119-5926 Hen 3-1357 17 16 21.1 -59 29 23 unknown - 31.16 O
17225-4408 Cn 1-3 17 26 12.3 -44 11 26 unknown <5.0 15.75 O
17360-1815 Hen 2-260 17 38 57.4 -18 17 36 noned <10 10.77 O
17358-2854 19W32 17 39 02.9 -28 56 35 unknown 24.0 1.44 O
18308-2241 IC 4732 18 33 54.6 -22 38 40 unknown 4.0 12.57 O
17418-4604 Tc 1 17 45 35.3 -46 05 23 unknown 9.6 17.20 C
a None - neither [WC] nor wels; b Parker & Morgan (2003); c Tylenda et al. (1993), Górny et al. (2001); d Górny et al. (2004); e Górny et al. (2008); f Strasbourg-ESO Catalogue of Galactic Planetary Nebulae (Acker et al. 1992), 0.0 - PN is a point-like source, - PN is not listed in the catalogue.

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