Brown dwarfs and very low mass stars in the Praesepe open cluster: a dynamically unevolved mass function?

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Volume 510 (February 2010)

A&A, 510 (2010) A27

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Table 4:

Photometric candidates in our survey that are also photometric candidates in previous surveys.
ID	$\alpha$	$\delta$	Alternative name	Ref.^a
	( $^{\rm h}$ $^{\rm m}$ $^{\rm s}$ )	( $^\circ$ ' '')
005	08 41 08.5	+19 54 02.0	RIZpr18	[3]
010	08 39 06.9	+19 47 08.0	J0839069+194708	[1]
			J08390695+1947080	[2]
011	08 38 55.46	+19 50 33.3	J0838554+195033	[1]
			J08385547+1950334	[2]
012	08 38 54.19	+19 51 44.6	J08385420+1951446	[2]
			J0839030+192415	[1]
			J08390308+1924155	[2]
015	08 39 12.71	+19 30 16.8	J08391272+1930169	[2]
016	08 39 54.39	+19 27 37.1	J0839544+192737	[1]
			J08395441+1927372	[2]
017	08 39 47.82	+19 28 03.1	RIZpr11	[3]
029	08 42 50.50	+20 20 03.8	J0842505+202004	[1]
			J08425052+2020039	[2]
034	08 42 54.58	+20 03 36.3	RIZpr23	[3]
035	08 42 51.96	+20 05 19.4	J0842519+200519	[1]
038	08 43 10.76	+20 01 29.3	J0843107+200129	[1]
040	08 41 11.05	+20 22 38.4	J0841110+202238	[1]
042	08 40 10.59	+20 20 50.4	J0840106+202050	[1]
			J08401060+2020505	[2]
045	08 39 14.51	+20 01 19.1	J0839145+200119	[1]
046	08 39 22.43	+20 04 54.6	J0839224+200454	[1]
			J08392244+2004548	[2]
047	08 38 55.15	+20 13 08.8	J0838551+201308	[1]
			J08385517+2013089	[2]
054	08 40 53.96	+20 05 24.3	J08405397+2005243	[2]
062	08 36 39.46	+20 22 33.8	J08363947+2022339	[2]
064	08 36 44.99	+20 08 45.7	J08364501+2008459	[2]
066	08 37 11.41	+20 13 45.8	J08371143+2013459	[2]
068	08 38 08.0	+20 03 50.1	J08380800+2003505	[2]
070	08 38 12.44	+20 08 02.5	J08381244+2008026	[2]
073	08 38 21.85	+20 05 35.7	J08382186+2005356	[2]
075	08 38 39.27	+19 41 40.1	J08383929+1941401	[2]
081	08 37 24.48	+19 47 11.9	J08372449+1947120	[2]
082	08 37 02.1	+19 52 07.3	RIZpr2	[3]
101	08 41 20.32	+18 57 42.9	J08412034+1857430	[2]
103	08 42 19.21	+19 02 14.8	J08421923+1902148	[2]
108	08 43 09.0	+19 43 11.9	J08430905+1943119	[2]
109	08 43 01.2	+19 49 59.8	RIZpr24	[3]
117	08 42 11.47	+19 52 50.2	RIZpr21	[3]
110	08 43 01.9	+19 54 04.5	J08430186+1954046	[2]
112	08 42 52.26	+19 51 45.9	J08425228+1951460	[2]
116	08 42 15.48	+19 48 57.6	J08421550+1948576	[2]
122	08 43 08.4	+19 28 06.1	J08430839+1928061	[2]
123	08 43 12.63	+19 34 28.9	J08431265+1934290	[2]

^a Objects [1] are from Adams et al. (2002a); [2] are from Kraus & Hillenbrand (2007); and [3] are from Pinfield et al. (1997).

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