Abundances of carbon-enhanced metal-poor stars as constraints on their formation

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Volume 588 (April 2016)

A&A, 588 (2016) A37

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Table 1

Coordinates, photometry, integration times, and resulting S/Ns for our programme stars.

Name	RA	Dec	B	V	J	K	Int. time [s]	S/N@4000 Å

HE 0058−3449	01:01:21.6	−34:33:11	13.91	13.20	11.78	11.33	380	13
HE 0206−1916	02:09:19.6	−19:01:56	15.12	14.00	12.24	11.66	500	7
HE 0241−3512	02:43 26.7	−35:00:12	15.24	13.91	12.04	11.40	500	8
HE 0400−2030	04:02:14.8	−20:21:53	14.92	14.03	12.49	11.98	400	13
HE 0408−1733	04:11:06.0	−17:25:40	13.51	12.34	10.37	9.67	130	6
HE 0414−0343	04:17:16.4	−03:36:31	12.25	11.05	9.19	8.51	30	8
HE 0430−1609 ^SB	04:32:50.6	−16:03:38	14.41^a	13.21^a	11.39	10.74	230	6
HE 0430−4901	04:31:31.1	−48:54:42	15.16	14.57	13.31	12.81	250	36
HE 0440−3426	04:42:08.1	−34:21:13	12.59	11.42	9.65	8.97	60	10
HE 0448−4806	04:49:33.0	−48:01:08	13.39	12.78	11.59	11.21	400	17
HE 0516−2515	05:18:09.4	−25:12:25	15.44^a	13.66^a	11.25	10.35	600	10
HE 1238−0836	12:41:02.4	−08:53:06	13.56^A	11.79^A	9.19	8.15	400	9
HE 1315−2035	13:17:57.4	−20:50:53	16.81	15.43	13.68	13.05	1100	11
HE 1418+0150	14:21:01.2	01:37:18	14.05^a	12.33^a	9.99	9.13	600	9
HE 1430−0919	14:33:12.9	−09:32:53	15.68	14.31	12.48	11.86	800	10
HE 1431−0245	14:33:54.2	−02:58:33	16.59	15.22	13.57	12.99	800	11
HE 2138−1616	21:41:16.6	−16:02:40	14.81^A	13.68^A	11.90	11.32	350	9
HE 2141−1441	21:44:25.7	−14:27:33	14.53^A	13.37^A	11.40	10.73	280	8
HE 2144−1832	21:46:54.7	−18:18:15	12.65	11.14	8.77	7.96	30	6
HE 2153−2323	21:56:37.6	−23:09:25	16.21	14.67	12.53	11.74	700	8
HE 2155−2043	21:58:42.2	−20:29:15	13.92	13.16	11.57	11.02	300	40
HE 2235−5058	22:38:07.9	−50:42:42	13.83	12.92	11.43	10.89	200	10
HE 2250−4229	22:53:39.6	−42:13:03	12.66^A	11.91^A	10.40	9.87	100	30
HE 2310−4523	23:13:00.0	−45:07:06	12.12^A	11.21^A	9.44	8.81	40	30
HE 2319−5228	23:21:58.1	−52:11:43	14.15^A	13.25^A	11.55	10.96	450	20
HE 2357−2718	23:59:58.1	−27:01:37	14.31^A	13.08^A	11.09	10.42	170	6
HE 2358−4640	00:00:50.9	−46:23:31	14.39^A	13.67^A	12.15	11.64	500	22

Notes.

^(SB)

single-lined spectroscopic binary.

^(A)

APASS (Henden et al. 2015);

^(a)

average of APASS and values in Beers et al. (2007).

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