Limits on the luminosity function of Lyα emitters at z = 7.7

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Volume 515 (June 2010)

A&A, 515 (2010) A97

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Table 2:

Table of the $z\sim 7.7$ LAE and T-dwarf candidates.
Name	NB1060	Error	SNR (NB1060)	J	Error	SNR (J)	H	Error	SNR (H)	$K_{\rm s}$	EW^a (Å)
LAE#1	24.0	0.08	14.5	24.5	0.16	6.7	24.7	0.3	4	>24.7	13
LAE#2	24.3	0.17	6.5	>25.0	...	...	>24.7	...	...	>24.7	>16
LAE#3	24.6	0.15	7.2	>25.2	...	...	>24.7	...	...	>24.8	>15
LAE#4	24.8	0.19	5.8	>25.2	...	...	>24.7	...	...	>24.8	>11
LAE#5	24.9	0.2	5.5	>25.2	...	...	>24.7	...	...	>24.8	>9
LAE#6^b	25.1	0.19	5.9	>25.0	...	...	>24.7	...	...	>24.7	>5
LAE#7^b	25.1	0.22	4.9	>25.0	...	...	>24.7	...	...	>24.7	>5
TDW#1^c	24.3	0.12	9.4	24.2	0.15	7.3	>24.7	...	...	>24.7	...

Notes. ^(a) In the restframe. ^(b) These two objects are not unambiguously identified as line emitting objects, but are included in the LAE sample (see text for details). ^(c) This object is not formally part of the sample because it is a likely late type T-dwarf (see text for details).

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