Bose-Einstein Condensate Dark Matter Halos Confronted with Galactic Rotation Curves

Table 3

The best fit BEC and NFW parameters of the LSB I and II type galaxies (the first and last three galaxies, respectively). is taken from [38]. The rest of the parameters are rotation curve fits. For LSB I galaxies the BEC DM model gives significantly better fitting velocity curves (within 1 confidence level) than the NFW model. However the velocity curves are outside the 1 confidence level for LSB II galaxies.

Galaxy			(BEC)			(BEC)	(NFW)			(NFW)	1
	Mpc	kpc		kg/m^3	kpc			kg/m^3	kpc
DDO 189	12.6	1.9	2.71	0.38	8.3	0.519	2.16	16	70	1.09	7.03
NGC 4455	6.8	2.3	0.231	1.44	5.5	9.29	0.11	25.04	66	5.39	18.11
UGC 10310	15.6	5.2	0.443	0.98	7.8	2.66	0.9	14.9	88	5.76	13.74
NGC 2366	3.4	1.5	2.43	0.22	5.3	110.73	2.5	0.2	1000	116.93	26.72
NGC 5023	4.8	0.8	0.894	2.45	5.6	53.2	0.0449	457	13	143.08	32.05
NGC 3274	6.7	0.5	1.1	1.69	6.4	269.8	0.252	2373	4	148.44	20.27