Table 2
Filter list of the LARS data.
LARS | U | B | I | K |
---|---|---|---|---|
01 | 114 | 135 | 108 | Ks |
02 | 114 | 135 | 108 | Ks |
03 | 135 | Ks | ||
04 | 114 | 135 | 108 | Ks |
05 | F336W | F438W | F775W | Ks |
06 | 114 | 135 | F775W | Ks |
07 | 114 | 135 | 108 | Ks |
08 | F336W | F438W | F775W | Ks |
09 | 109 | 135 | 108 | Ks |
10 | 109 | 135 | F775W | Ks |
11 | F336W | F438W | F775W | Ks |
12 | F336W | F438W | F775W | Ks |
13 | F390W | F475W | F850LP | Ks |
14 | F390W | F475W | F850LP | Ks |
Notes. All data were obtained with NOT MOSCA, except Ks (CFHT/WIRCAM), LARS06 U-band (NOT/ALFOSC), and the HST/WFC3 data. The ground-based data uses U #114 (according to the NOT numbering scheme) for LARS01–07 and #109 for LARS 09-10. #114 has λeff = 347 nm and FWHM = 38 nm, while #109 has λeff = 353 nm and FWHM = 55 nm. The B filter is a custom-made private filter, assigned a NOT id of #135, with λeff = 458 nm and FWHM = 66 nm for LARS 01-10. The custom-made B-band filter was designed to avoid the strongest emission lines. The NOT I #108 filter has λeff = 817 nm and FWHM = 163 nm. All “F”-filter names are HST/WFC3 filters (see Östlin et al. (2014) for details).
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