Ho I Target 1: RA: 9:40:44.2 Dec: +71:10:54 Peak surface brightness (24 micron): 0.57 MJy/sr Description: This is the brightest 24 micron source in Ho I and may be representative of similar sources in irregular galaxies. It has an optical counterpart and counterparts in all MIPS wavebands, and a visual comparison of the three MIPS bands suggests that the dust is strongly heated. SAME AS CANNON SUGGESTION; TOO FAINT Ho II Target 1: RA: 8:19:28.9 Dec: +70:43:01 Peak surface brightness (24 micron): 22.3 MJy/sr Description: This is one of the two brightest 24 micron sources in Ho II. It has an optical counterpart and counterparts in all MIPS wavebands. SAME AS CANNON #5 Target 2: RA: 8:19:12.9 Dec: +70:43:07.6 Peak surface brightness (24 micron): 16.7 MJy/sr Description: This is the center of HoII; if it is already being observed, then this entry can be disregarded. This target is one of the two brightest 24 micron sources in Ho II. It has an optical counterpart and counterparts in all MIPS wavebands. ALREADY DID THIS ONE. IC 2574 Target 1: RA: 10:28:48.3 Dec: +68:28:03 Peak surface brightness (24 micron): 21.1 MJy/sr Description: This is a bright knot in a large supergiant shell at the northeast end of the optical disk for IC 2574. (Fabian Walter has more information on this object.) SAME AS CANNON #1 Target 2: RA: 10:28:43.5 Dec: +68:28:25 Peak surface brightness (24 micron): 5.1 MJy/sr Description: This is a bright knot in a large supergiant shell at the northeast end of the optical disk for IC 2574. (Fabian Walter has more information on this object.) SAME AS CANNON #2 IC 4710 Target 1: RA: 18:28:39.7 Dec: -66:58:22 Peak surface brightness (24 micron): 10.8 MJy/sr Description: This is the brightest 24 micron source in IC 4710 and may be representative of similar sources in irregular galaxies. It has an optical counterpart and counterparts in all MIPS wavebands, and color maps made with the three MIPS bands suggests that the dust is strongly heated. NGC 584 Target 1: RA: 1:31:19.6 Dec: -06:51:30 Peak surface brightness (24 micron): 0.91 MJy/sr Description: This is a bright 24 micron source northwest of the nucleus of NGC 584. It has not optical counterpart or 8 micron counterpart and only a possible weak counterpart in the 70 micron band. It is not clear as to what this is; this target should be treated with caution and possibly should not be scheduled for follow-up observations. TOO FAINT NGC 628 Target 1: RA: 1:36:45.3 Dec: +15:47:48 Peak surface brightness (24 micron): 88 MJy/sr Description: This is the brightest 24 micron source in NGC 628. ALREADY DID THIS ONE. NGC 1291 Target 1: RA: 3:17:00.0 Dec: -41:04:24 Peak surface brightness (24 micron): 1.21 MJy/sr Description: This is the brightest infrared source in the outer ring of NGC 1291. It has an optical counterpart and counterparts in all MIPS wavebands, but it has no H alpha counterpart. The data suggest that it is a small star formation region where all photoionizing stars have evolved off the main sequence but the remaining stellar population is still luminous enough to enhance the dust emission. TOO FAINT NGC 1404 Target 1: RA: 3:38:54.9 Dec: -35:35:01 Peak surface brightness (24 micron): 2.59 MJy/sr Description: This is the brightest 24 micron source outside of the center of NGC 1404. It is the only object in this galaxy with a counterpart at 70 and 160 microns, and it has an optical counterpart. The nature of this region is unclear from these data alone. TOO FAINT NGC 2403 Target 1: RA: 7:37:06.9 Dec: +65:36:39 Peak surface brightness (24 micron): 292 MJy/sr Description: This is the brightest 24 micron source in NGC 2403. SAME AS DALE SUGGESTION NGC 2976 Target 1: RA: 9:47:07.7 Dec: +67:55:54 Peak surface brightness (24 micron): 138 MJy/sr Description: This is the brightest infrared source in NGC 2976. SAME AS DALE SUGGESTION Target 2: RA: 9:47:15.2 Dec: +67:55:00 Peak surface brightness (24 micron): 31.4 MJy/sr Description: This is the second brightest infrared source in NGC 2976. SAME AS DALE SUGGESTION; FORTUNATELY I RECHECKED HIS COORDINATES, AND HE MISTAKENLY GAVE DATA FOR THE NUCLEUS. MY LIST CORRECTS THIS. NGC 3627 Target 1: RA: 11:20:16.4 Dec: +12:58:43 Peak surface brightness (24 micron): 497 MJy/sr Description: This is near one end of the bar in NGC 3627. It is the brightest source at 24 microns and has counterparts at 70 and 160 microns (it is also the brightest source in the galaxy at 70 microns but not at 160 microns). Target 2: RA: 11:20:13.1 Dec: +13:00:24 Peak surface brightness (24 micron): 124 MJy/sr Description: This is near the other end of the bar in NGC 3627. It is the third brightest source at 24 microns and has counterparts at 70 and 160 microns (it is also the brightest source in the galaxy at 160 microns but not at 70 microns). NGC 3938 Target 1: RA: 11:53:00.3 Dec: +44:07:49 Peak surface brightness (24 micron): 25.8 MJy/sr Description: This is the brightest source in NGC 3938 at 24 microns. It has counterparts at 8, 70, or 160 microns, but these counterparts are not as strongly enhanced as the 24 micron emission. This object also has an H alpha counterpart. It appears to be a strong extranuclear star formation event. It may make a good case study for studying how strong star formation enhances infrared emission. NGC 4236 Target 1: RA: 12:16:17.1 Dec: +69:30:41 Peak surface brightness (24 micron): 64.7 MJy/sr Description: This is the brightest infrared sources in NGC 4236. It has counterparts in the optical and all MIPS bands, and a visual inspection of the data suggests that the dust is strongly heated. NGC 4450 Target 1: RA: 12:28:29.3 Dec: +17:05:39.2 Peak surface brightness (24 micron): 4.8 MJy/sr Description: This is the brightest source outside of the nucleus in NGC 4450. This object is close to the center of the galaxy, so IRS observations should be checked to see if this object was already observed. TOO FAINT NGC 4594 Target 1: RA: 12:39:52.6 Dec: -11:37:34 Peak surface brightness (24 micron): 3.3 MJy/sr Description: This is the brightest source outside of the nucleus in NGC 4594. It has an H alpha counterpart. Oddly, H alpha sources with similar luminosities are not as bright at 24 microns as this source, so further investigation is warranted. TOO FAINT NGC 4631 Target 1: RA: 12:42:10.9 Dec: +32:32:36 Peak surface brightness (24 micron): 198 MJy/sr Description: This is the east end of what looks like an edge-on toroidal structure in NGC 4631. This has bright counterparts in the infrared and submillimeter. Target 1: RA: 12:42:04.3 Dec: +32:32:25 Peak surface brightness (24 micron): 155 MJy/sr Description: This is the west end of what looks like an edge-on toroidal structure in NGC 4631. This has bright counterparts in the infrared and submillimeter. NGC 6822 Target 1: RA: 19:45:04.6 Dec: -14:57:32 Peak surface brightness (24 micron): 10.1 MJy/sr Description: This is a star formation complex in a spur to the south of the galaxy. Although the source is visible in all three MIPS bands, it does not appear to have an optical counterpart (and neither does the surrounding infrared-emitting region, although the region does appear to be an extension of an optical feature). This could therefore be dust emission from a region that just recently underwent gravitational collapse. Target 2: RA: 19:44:48.4 Dec: -14:52:29 Peak surface brightness (24 micron): 87 MJy/sr Description: This is the third brightest source in NGC 6822 in all three MIPS bands, yet the object is in part of a complex with muted H alpha emission. This could therefore be an example of a highly-extincted HII region, in contrast to the optically-selected spectroscopic targets. NGC 7793 Target 1: RA: 23:57:49.0 Dec: -32:34:54 Peak surface brightness (24 micron): 34.0 MJy/sr Description: This is the brightest 24 micron source in NGC 7793. It has counterparts at 70 and 160 microns, but the dust emission is not as enhanced in those bands as it is at 24 microns. This object is close to the center of the galaxy, so IRS observations should be checked to see if this object was already observed.