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Table 5

Nature of the other ASAS objects spectroscopically followed up and rejected as RCB or DY Per candidates.

ASAS-3 id Coordinates (J2000) (from ASAS) SIMBAD name Nature of the object

014428+0536.6 01:44:28 +05:36:36 TYC 35-752-1 K4III
020504+1925.4 02:05:04 +19:25:24 SW Ari Mira, M6
020653+1517.7 02:06:53 +15:17:42 TT Ari A star + H, HeI, CaII emission
030615-3942.5 c 03:06:15 −39:42:30 Mira, M6
035412+1810.3 03:54:12 +18:10:18 IRAS 03513+1801 Mira, M8
040907-0914.2 04:09:07 −09:14:12 EV Eri C* (Strong 13C at 4744 angs)
042841+2150.6 04:28:41 +21:50:36 IRAS 04257+2144 Mira, M6
043547+2250.4 04:35:47 +22:50:24 HQ Tau A star reddened + Hα em.
045331+2246.5 04:53:31 +22:46:30 CGCS 808 C* (Strong 13C at 4744 angs)
050430-0347.2 05:04:30 −03:47:12 UX Ori A7V + Hα em.
050500+0856.1 05:05:00 +08:56:06 _ C* (Hα emission)
051314-0844.9 05:13:14 −08:44:54 F8III
052114+0721.3 05:21:14 +07:21:18 V1368 Ori C* (Strong 13C at 4744 angs)
053302+1808.0 05:33:02 +18:08:00 IRAS 05301+1805 C* (Strong 13C at 4744 angs)
053625-6941.5 05:36:25 −69:41:30 TYC 9167-592-1 K2III + H, OI, CaII emission
053659-0609.3 05:36:59 −06:09:18 HD 37258 A3V + Hα em.
053713-0635.0 05:37:13 −06:35:00 BF Ori A7III + Hα em.
053931+2622.5 05:39:30 +26:22:30 RR Tau A star reddened + Hα, CaII em.
054012-0942.2 05:40:12 −09:42:12 V350 Ori A7V + Hα em.
054339-0504.1 05:43:39 −05:04:00 DM Ori G star reddened + Hα em.
054635+2538.1 05:46:35 +25:38:06 CGCS 1049 C* (Strong 13C at 4744 angs)
055343-1023.9 05:53:43 −10:24:00 V1818 Ori A star reddened + Hα, CaII em.
062348-2051.5 06:23:48 −20:51:30 TYC 5946-114-1 G0III + Hα em.
064107+1026.7 06:41:07 +10:26:42 SS Mon K7V + Hα em., PMS?
064854-4249.4 06:48:54 −42:49:24 IRAS 06473-4246 Mira M9
070615-1904.4 07:06:15 −19:04:24 _ A0V + Hα em.
070813-1036.0 a 07:08:13 −10:36:00 ALS 181 A star reddened
071204+2706.3 07:12:04 +27:06:18 TYC 1904-1095-1 Mira, M6
071839-0117.0 07:18:39 −01:17:00 C* (Hα emission)
072221-5049.4 07:22:21 −50:49:24 NY Pup Mira, M6
072419+0912.6 07:24:19 +09:12:30 GSC 00764-00509 Giant, G? reddened
075752-0916.0 07:57:52 −09:16:00 IRAS 07554-0907 C* (Hα, Hβ, Hγ + Hδ em.)
081204-2002.4 08:12:04 −20:02:24 V535 Pup C* (Strong 13C at 4744 angs)
081447-4441.6 08:14:47 −44:41:36 TYC 7672-563-1 G0III + Hα em.
083236-3759.0 08:32:36 −37:59:00 FX Vel A3III + Hα, CaII, OI, OIII em.
095221-4329.7 c 09:52:21 −43:29:42 TYC 7706-560-1 Mira, M6
100731-0918.1 10:07:31 −09:18:06 BD-08 2852 M3III
110204-6209.7 11:02:04 −62:09:42 V802 Car F2III
110815-7733.9 11:08:15 −77:33:54 HP Cha K7V + Hα em., PMS?
111846-5612.6 a 11:18:46 −56:12:36 A7V
120729+0036.9 12:07:29 +00:36:54 K2III + Hα P-cygne em.
122112-4912.7 12:21:12 −49:12:42 SX Cen B5III
133504-6345.9 13:35:04 −63:45:54 TYC 8999-807-1 F0III + Hα em.
141600-6153.9 14:16:00 −61:53:54 V417 Cen F6V reddened + Hα em.
144959-6920.9 14:49:59 −69:20:54 BL Cir Mira, M6
150323-6323.0 15:03:23 −63:23:00 DG Cir A star + nebulae
152008-6148.5 15:20:08 −61:48:24 F6V + Pcygne Hα
152604-7004.0 15:26:04 −70:04:00 IRAS 15211-6953 Mira, M7
153213-2854.3 15:32:13 −28:54:18 BX Lib K7.5III + Hα em.
155517-2924.6 c 15:55:17 −29:24:36 V1317 Sco Mira, M6
164557-4330.1 16:45:57 −43:30:06 _ G0III + Hα P-cygne em.
165449-4032.8 16:54:49 −40:32:48 _ F8V
165452-3037.3 c 16:54:52 −30:37:18 CL Sco Symbiotic star with M giant, M4
165750-3234.7 c 16:57:50 −32:34:42 EW Sco Mira, M6
_ 17:17:22 −20:22:38 V1773 Oph F2III, binary?
172109-4644.1 c 17:21:09 −46:44:06 IRAS 17174-4641 Mira, M7
173540+1535.2 17:35:40 +15:35:12 MW Her Mira, M10
173708-4708.1 17:37:08 −47:08:00 M0III
173729-3743.4 17:37:29 −37:43:24 F8IV reddened
174600-2321.2 c 17:46:00 −23:21:12 F0I reddened
175013-0642.5 c 17:50:13 −06:42:30 Oph 1898 K7III + H, HeI, CaII, OI em. (Nova)
175335-3805.0 17:53:34 −38:05:00 V383 Sco Blend F8I + M6(I to III) + Hα em.
180204-2337.7 18:02:04 −23:37:42 V5097 Sgr Wolf Rayet, WC9 + 2 mag. declines
_ 18:08:36 −15:04:00 GM Ser Mira, M7
181448-1840.3 a,b 18:14:48 −18:40:18 2MASS J18144821-1840219 F0I reddened + Hα em.

Notes. 

(a)

The ASAS light curves of these objects show some variability that are certainly not real but due to some photometric systematics. Nevertheless, we followed-up these objects for completeness in our study.

(b)

The star that was followed-up spectroscopically is 2MASS18144821-1840219. This is the star selected by our IR colour criteria.

(c)

These ASAS objects were selected from the criteria defined to search for DY Per stars (see Sect. 3.4).

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