Table 3: Potential candidates for the host galaxy of GRB 000214. The table displays the coordinates, magnitudes, and inferred photometric redshifts for the four best host galaxy candidates. See Sect. 4 for a more extended description. The SEDs of these four objects can be seen in Fig. 3.
N RA(J2000) Dec (J2000) U B V R I photo-z

1 18:54:23.34 -66:28:19.8 >22.8 23.34 $\pm$ 0.11 22.11 $\pm$ 0.03 21.09 $\pm$ 0.04 20.32 $\pm$ 0.04 $\rm0.49^{+0.05}_{-0.07}$

2 18:54:29.34 -66:27:36.7 >22.8 23.85 $\pm$ 0.09 21.77 $\pm$ 0.02 21.03 $\pm$ 0.04 20.49 $\pm$ 0.04 $\rm0.32^{+0.05}_{-0.02}$

3 18:54:24.38 -66:26:41.4 >22.8 23.06 $\pm$ 0.11 22.45 $\pm$ 0.04 21.58 $\pm$ 0.11 21.32 $\pm$ 0.11 $\rm0.53^{+0.03}_{-0.03}$

4 18:54:27.87 -66:26:51.8 >22.8 23.91 $\pm$ 0.18 23.11 $\pm$ 0.06 21.84 $\pm$ 0.12 >22.2 $\rm0.57^{+0.06}_{-0.04}$

**Table 3:** Potential candidates for the host galaxy of GRB 000214. The table displays the coordinates, magnitudes, and inferred photometric redshifts for the four best host galaxy candidates. See Sect. 4 for a more extended description. The SEDs of these four objects can be seen in Fig. 3.
N	RA(J2000)	Dec (J2000)	U	B	V	R	I	photo-z
1	18:54:23.34	-66:28:19.8	>22.8	23.34 $\pm$ 0.11	22.11 $\pm$ 0.03	21.09 $\pm$ 0.04	20.32 $\pm$ 0.04	$\rm0.49^{+0.05}_{-0.07}$
2	18:54:29.34	-66:27:36.7	>22.8	23.85 $\pm$ 0.09	21.77 $\pm$ 0.02	21.03 $\pm$ 0.04	20.49 $\pm$ 0.04	$\rm0.32^{+0.05}_{-0.02}$
3	18:54:24.38	-66:26:41.4	>22.8	23.06 $\pm$ 0.11	22.45 $\pm$ 0.04	21.58 $\pm$ 0.11	21.32 $\pm$ 0.11	$\rm0.53^{+0.03}_{-0.03}$
4	18:54:27.87	-66:26:51.8	>22.8	23.91 $\pm$ 0.18	23.11 $\pm$ 0.06	21.84 $\pm$ 0.12	>22.2	$\rm0.57^{+0.06}_{-0.04}$

Source LaTeX | All tables | In the text

	1 Introduction
	2 Observations
	3 Results and discussion
	4 Conclusions
	References