A search for new hot subdwarf stars by means of Virtual Observatory tools

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Table 3

List of candidates in the Kepler field-of-view.

RA	Dec	FUV	NUV	g′	r′	i′	z′	J	H	K	T _eff	Class.	KIC	Comments
(J2000)	(J2000)										(VOSA)		number

18:42:42	+44:04:06	16.317	16.442	17.056	17.378	17.555	17.630	16.75	16.34	15.78	25 000^*	sdB	8142623	^Q₁ ^,^R^,^a
18:43:07	+42:59:18	14.149	14.737	15.410	15.864	16.208	16.528	16.27	16.13	U:16.24	42 000	sdO+dM	7335517	^Q₃^,^R^,^b
18:47:14	+47:41:47	13.305	13.772	14.489	14.988	15.366	15.725	15.39	15.62	15.47	41 000	He-sdO	10449976	^Q₃^,^N^,^b
18:50:17	+43:58:29	16.501	16.387	16.353	16.649	16.996	17.115	16.71	U:17.15	U:17.00	23 000	B	8077281	^Q₂^,^I^,^a
19:04:35	+48:10:22	15.726	16.057	16.696	17.031	17.236	17.456	16.63	U:16.34	U:17.11	25 000	sdB	10784623	^Q₅^,^R^,^b
19:05:06	+43:18:31	14.208	14.391	15.058	15.516	15.894	16.193	15.81	16.06	U:16.23	30 000	sdB	7668647	^Q₃^,^G^,^b
19:08:25	+45:08:32	15.267	15.518	16.283	16.605	16.755	16.819	16.17	15.78	15.36	26 000^*	sdB	8874184	^Q₄^,^C^,^b
19:08:46	+42:38:31	13.983	14.490	15.146	15.595	15.964	16.295	15.90	16.05	16.02	35 000	sdB	7104168	^Q₃^,^N^,^b
19:09:33	+46:59:04	14.695	15.009	15.483	15.967	16.308	16.607	16.36	U:15.71	U:16.61	35 000	sdB	10001893	^Q₃^,^G^,^b
19:10:00	+46:40:24	14.119	14.496	14.572	14.583	14.613	14.672	13.93	13.80	13.73	18 000^*	sdO+F/G	9822180	^Q₂^,^C^,^a
19:14:28	+45:39:09	15.002	15.339	15.895	16.174	16.297	16.423	16.02	15.57	15.68	26 000	sdB	9211123	^Q₃^,^N^,^b
19:16:12	+47:49:16	15.291	15.413	15.269	15.278	15.339	15.351	14.62	14.42	14.27	15 000^*	sdB+F/G	10593239	^Q_2.5^,^C?^,^a
19:26:51	+49:08:48	14.981	14.813	15.396	15.522	15.565	15.595	14.83	14.52	14.37	21 000^*	sdB+F/G	11350152	^Q₃^,^C^,^b
19:40:32	+48:27:23	13.544	13.969	14.093	14.175	14.269	14.369	13.68	13.56	13.56	20 000^*	sdB+F/G	10982905	^Q₂^,^C^,^a
19:43:44	+50:04:38	13.228	13.888	14.455	14.938	15.320	15.682	15.37	15.36	15.18	50 000^*	DA	11822535	^Q₂^,^N^,^a

Notes. FUV, NUV have been taken from the galex archive; g′,r′,i′,z′ from the Kepler Input Catalogue and J, H, and K from 2mass. “U” means upper limit in the 2mass photometry. T_eff is obtained from the best SED fit performed by VOSA.

^(*)

Indicates that a poor SED fit is obtained. KIC is the number from the Kepler input catalogue.

^Qx

Kepler survey cycle of observation.

Brief description of its light curve:

^(N)

no particular features;

^(R)

reflecting binary;

^(G)

g-mode pulsator;

^(I)

irregular variable;

^(C)

variability from the companion. Spectral classification:

^(a)

from Østensen et al. (2010c);

^(b)

from Østensen et al. (2011).

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