Table 1: VRIJHKs photometry of #1916. Near-IR magnitudes are measured within 1.5 arcsec apertures on seeing matched images. Limiting magnitudes in the visible bands correspond to a detection limit of $1~\sigma$ within the near-IR reference seeing aperture, which is equivalent to a 3 $~\sigma$ detection on 4 ISAAC pixels. Table entries denote the filter name (Col. 1), effective wavelength (2), total exposure time (3), the image quality/seeing (4), and the observed magnitudes in the Vega (5) and AB (6) systems.
Filter $\lambda_{\rm eff}$ $t_{\rm exp}$ Seeing mag mag

[ $\mu$ m] [ks] [''] [Vega] [AB]

V 0.54 3.75 0.76 >28.5 >28.6

R 0.66 5.4 0.69 >28.5 >28.7

I 0.81 4.5 0.78 >27.6 >28.1

J 1.26 6.48 0.65 25.83 $\pm$ 1.00 26.77 $\pm$ 1.00

H 1.65 13.86 0.5 23.59 $\pm$ 0.25 25.00 $\pm$ 0.25

Ks 2.16 18.99 0.38 23.64 $\pm$ 0.36 25.51 $\pm$ 0.36

**Table 1:** *VRIJHK*s photometry of #1916. Near-IR magnitudes are measured within 1.5 arcsec apertures on seeing matched images. Limiting magnitudes in the visible bands correspond to a detection limit of $1~\sigma$ within the near-IR reference seeing aperture, which is equivalent to a 3 $~\sigma$ detection on 4 ISAAC pixels. Table entries denote the filter name (Col. 1), effective wavelength (2), total exposure time (3), the image quality/seeing (4), and the observed magnitudes in the Vega (5) and AB (6) systems.
Filter	$\lambda_{\rm eff}$	$t_{\rm exp}$	Seeing	mag	mag
	[ $\mu$ m]	[ks]	['']	[Vega]	[AB]
V	0.54	3.75	0.76	>28.5	>28.6
R	0.66	5.4	0.69	>28.5	>28.7
I	0.81	4.5	0.78	>27.6	>28.1
J	1.26	6.48	0.65	25.83 $\pm$ 1.00	26.77 $\pm$ 1.00
H	1.65	13.86	0.5	23.59 $\pm$ 0.25	25.00 $\pm$ 0.25
Ks	2.16	18.99	0.38	23.64 $\pm$ 0.36	25.51 $\pm$ 0.36

Source LaTeX | All tables | In the text