J1453+0317. One of the three pairs in our sample that are larger than
2.5'. These are two well-separated S-type galaxies, both are detected by
IRAC and MIPS. The eastern galaxy displays a ring formation in both 8 and
24 micron images. The western galaxy was detected in the ISOPHOT 170
micron Serendipity Survey (Stickel et al. 2004), with f_170_ = 1.94 +-
0.58 Jy. This is significantly lower than the MIPS 160 micron flux: f_160_
= 3.03 +- 0.32 Jy.
Paired with UGC 09574 at 2.2, 16