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| IRAS name | RA (J2000) | Dec (J2000) | Observation date | rms (Jy) | Classification | Notes |
| Suárez et al. (2006) | ||||||
| 07027-7934 | 06:59:26.4 | -79:38:47 | 2007-FEB-09 | 0.22 | PN | |
| 08046-3844 | 08:06:28.4 | -38:53:24 | 2007-FEB-10 | 0.19 | PN | |
| 08242-3828 | 08:26:03.8 | -38:38:48 | 2007-FEB-08 | 0.19 | No optical counterpart | 1 |
| 08281-4850 | 08:29:40.6 | -49:00:04 | 2007-FEB-12 | 0.21 | Post-AGB | |
| 08351-4634 | 08:36:45.8 | -46:44:46 | 2007-FEB-08 | 0.22 | No optical counterpart | |
| 08355-4027 | 08:37:24.7 | -40:38:04 | 2007-FEB-10 | 0.20 | PN | |
| 08418-4843 | 08:43:29.5 | -48:54:47 | 2007-FEB-10 | 0.17 | PN | |
| 08574-5011 | 08:59:02.3 | -50:23:40 | 2007-FEB-10 | 0.17 | PN | |
| 09362-5413 | 09:37:51.8 | -54:27:09 | 2007-FEB-09 | 0.60 | PN | |
| 09370-4826 | 09:38:53.3 | -48:40:10 | 2007-FEB-08 | 0.25 | No optical counterpart | |
| 09425-6040 | 09:44:01.7 | -60:54:26 | 2007-FEB-12 | 0.23 | Post-AGB | |
| 09500-5236 | 09:51:49.2 | -52:50:53 | 2007-FEB-08 | 0.22 | No optical counterpart | |
| 09517-5438 | 09:53:27.1 | -54:52:40 | 2007-FEB-09 | 0.20 | PN | |
| 10029-5553 | 10:04:40.1 | -56:08:37 | 2007-FEB-09 | 0.21 | PN | |
| 10115-5640 | 10:13:19.7 | -56:55:32 | 2007-FEB-09 | 0.22 | PN | |
| 10178-5958 | 10:19:32.5 | -60:13:29 | 2007-FEB-10 | 0.17 | Transition | |
| 10197-5750 | 10:21:33.9 | -58:05:48 | 2007-FEB-11 | 0.23 | Transition | |
| 10215-5916 | 10:23:19.5 | -59:32:05 | 2007-FEB-11 | 0.25 | Transition | |
| 10256-5628 | 10:27:35.2 | -56:44:20 | 2007-FEB-11 | 0.19 | Post-AGB | |
| 11201-6545 | 11:22:18.9 | -66:01:51 | 2007-FEB-11 | 0.20 | Post-AGB | |
| 11339-6004 | 11:36:20.7 | -60:20:53 | 2007-FEB-08 | 0.18 | No optical counterpart | |
| 11353-6037 | 11:37:42.9 | -60:53:51 | 2007-FEB-11 | 0.22 | Transition | |
| 11381-6401 | 11:40:32.0 | -64:18:35 | 2007-FEB-08 | 0.17 | No optical counterpart | |
| 11387-6113 | 11:41:08.7 | -61:30:17 | 2007-FEB-11 | 0.22 | Post-AGB | |
| 11531-6111 | 11:55:38.0 | -61:28:17 | 2007-FEB-11 | 0.22 | Transition | |
| 12145-5834 | 12:17:16.1 | -58:51:30 | 2007-FEB-12 | 0.24 | Post-AGB | |
| 12262-6417 | 12:29:04.2 | -64:33:37 | 2007-FEB-08 | 0.18 | No optical counterpart | |
| 12302-6317 | 12:33:07.0 | -63:33:43 | 2007-FEB-12 | 0.23 | Post-AGB | |
| 12309-5928 | 12:33:44.6 | -59:45:19 | 2007-FEB-08 | 0.18 | No optical counterpart | |
| 12316-6401 | 12:34:36.0 | -64:18:17 | 2007-FEB-09 | 0.23 | PN | |
| 12405-6219 | 12:43:31.5 | -62:36:14 | 2007-FEB-08 | 0.12 | No optical counterpart | 2 |
| 13203-5917 | 13:23:32.2 | -59:32:50 | 2007-FEB-12 | 0.24 | Post-AGB | |
| 13293-6000 | 13:32:39.2 | -60:15:39 | 2007-FEB-08 | 0.18 | No optical counterpart | |
| 13356-6249 | 13:39:05.8 | -63:04:44 | 2007-FEB-08 | 0.20 | No optical counterpart | |
| 13416-6243 | 13:45:07.3 | -62:58:17 | 2007-FEB-12 | 0.24 | Post-AGB | |
| 13427-6531 | 13:46:25.7 | -65:46:24 | 2007-FEB-08 | 0.20 | No optical counterpart | |
| 13500-6106 | 13:53:34.5 | -61:20:52 | 2007-FEB-08 | 0.15 | No optical counterpart | |
| 2007-FEB-09 | 0.23 | |||||
| 13529-5934 | 13:56:24.6 | -59:48:57 | 2007-FEB-08 | 0.22 | No optical counterpart | |
| 14079-6402 | 14:11:46.3 | -64:16:24 | 2007-FEB-09 | 0.22 | PN | |
| 14122-5947 | 14:15:53.3 | -60:01:38 | 2007-FEB-10 | 0.13 | PN | |
| 2007-FEB-11 | 0.22 | |||||
| 14177-5824 | 14:21:19.9 | -58:38:22 | 2007-FEB-10 | 0.19 | PN | |
| 14345-5858 | 14:38:20.0 | -59:11:46 | 2007-FEB-09 | 0.22 | PN | |
| 14482-5725 | 14:51:57.3 | -57:38:19 | 2007-FEB-11 | 0.19 | Post-AGB | |
| 14488-5405 | 14:52:28.7 | -54:17:43 | 2007-FEB-11 | 0.20 | Post-AGB | |
| 15039-4806 | 15:07:27.4 | -48:17:54 | 2007-FEB-11 | 0.20 | Post-AGB | |
| 15066-5532 | 15:10:26.0 | -55:44:13 | 2007-FEB-11 | 0.20 | Transition | |
| 15093-5732 | 15:13:12.4 | -57:43:40 | 2007-FEB-08 | 0.21 | No optical counterpart | |
| 15103-5754 | 15:14:18.5 | -58:05:20 | 2007-FEB-09 | 0.24 | No optical counterpart | 2 |
| 2007-FEB-12 | 0.6 | |||||
| 15144-5812 | 15:18:21.9 | -58:23:12 | 2007-FEB-09 | 0.22 | No optical counterpart | |
| 15154-5258 | 15:19:08.2 | -53:09:47 | 2007-FEB-10 | 0.17 | PN | |
| 15210-6554 | 15:25:31.7 | -66:05:20 | 2007-FEB-11 | 0.19 | Post-AGB | |
| 15534-5422 | 15:57:21.1 | -54:30:46 | 2007-FEB-09 | 0.21 | No optical counterpart | |
| 15559-5546 | 15:59:57.4 | -55:55:34 | 2007-FEB-10 | 0.18 | PN | |
| 15579-5445 | 16:01:50.8 | -54:53:40 | 2007-FEB-10 | 0.17 | PN | |
| 16053-5528 | 16:09:20.2 | -55:36:10 | 2007-FEB-10 | 0.17 | PN | |
| 16114-4504 | 16:15:03.0 | -45:11:54 | 2007-FEB-10 | 0.18 | PN | |
| 16228-5014 | 16:26:31.3 | -50:21:27 | 2007-FEB-09 | 0.22 | No optical counterpart | |
| 16333-4807 | 16:37:06.1 | -48:13:42 | 2007-FEB-09 | 0.20 | No optical counterpart | 2 |
| 16494-3930 | 16:52:55.4 | -39:34:56 | 2007-FEB-10 | 0.20 | Post-AGB | |
| 16518-3425 | 16:55:08.4 | -34:30:10 | 2007-FEB-09 | 0.23 | No optical counterpart | |
| 16529-4341 | 16:56:34.0 | -43:46:15 | 2007-FEB-10 | 0.18 | PN | |
| 16584-3710 | 17:01:52.1 | -37:14:54 | 2007-FEB-09 | 0.21 | No optical counterpart | |
| 16594-4656 | 17:03:11.2 | -47:00:21 | 2007-FEB-10 | 0.19 | Transition | |
| 17009-4154 | 17:04:29.6 | -41:58:39 | 2007-FEB-09 | 0.22 | No optical counterpart | |
| 17010-3810 | 17:04:27.3 | -38:14:42 | 2007-FEB-09 | 0.22 | No optical counterpart | |
| 17088-4227 | 17:12:21.8 | -42:30:50 | 2007-FEB-10 | 0.18 | PN | |
| 17119-5926 | 17:16:21.1 | -59:29:23 | 2007-FEB-10 | 0.17 | PN | |
| 17130-4029 | 17:16:29.0 | -40:32:31 | 2007-FEB-09 | 0.20 | No optical counterpart | |
| 17131-3330 | 17:16:26.2 | -33:33:24 | 2007-FEB-10 | 0.21 | PN | |
| 17153-3814 | 17:18:44.7 | -38:17:21 | 2007-FEB-09 | 0.21 | No optical counterpart | 3 |
| 17234-4008 | 17:26:56.1 | -40:11:04 | 2007-FEB-09 | 0.22 | No optical counterpart | |
| 17311-4924 | 17:35:02.5 | -49:26:26 | 2007-FEB-10 | 0.18 | Transition | |
| 17418-3335 | 17:45:08.7 | -33:36:06 | 2007-FEB-09 | 0.20 | No optical counterpart | 3 |
| 17476-4446 | 17:51:16.4 | -44:47:29 | 2007-FEB-10 | 0.19 | Post-AGB |
| 1 OH maser emission detected by Te Lintel Hekkert et al. (1991). The spectrum does not exhibit the typical double-peaked profile of OH/IR stars, but contains multiple components. This suggests that the source is a post-AGB star; 2 radio continuum emission detected by van de Steene & Pottasch (1993). Thus, we consider this source to be a ``PN candidate''; 3 radio continuum emission detected by Ratag et al. (1990). Thus, we consider this source to be a ``PN candidate''. |
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