A deep optical/near-infrared catalogue of Serpens | Astronomy & Astrophysics (A&A)

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Table 2:

Mean photometric calibration coefficients for our WFC-INT observing run.
Filter	K $^{\dagger}$	ZP	c
R	0.0734	$25.30\pm0.03$	$-0.033\pm0.024$
Z	0.0103	$23.52\pm0.03$	$0.021\pm0.022$

Notes. $^{(\dagger)}$ K = mean atmospheric extinction coefficients for La Palma.
$^{(\ddagger)}$ ZP = photometric zero point (see Eq. (2)). ^(*) c = photometric colour term (see Eq. (2)).

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