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Table 3

Apparent magnitudes and flux densities of GJ 504b.

Filter λc Δ λ Mag Uncertainty Flux 1σ lower limit 1σ upper-limit Ref.
(μm) (μm) (mag) (mag) (W m-2 μm-1) (W m-2 μm-1) (W m-2 μm-1)
Y2 1.022 0.049 20.98 0.20 2.325e-17 1.934e-17 2.795e-17 This work
Y3 1.076 0.050 20.14 0.09 4.237e-17 3.900e-17 4.603e-17 This work
J2 1.190 0.042 21.28 … … … 1.078e-17 This work
J3 1.273 0.046 19.01 0.17 6.705e-17 5.733e-17 7.841e-17 This work
H2 1.593 0.052 18.95 0.30 3.260e-17 2.473e-17 4.297e-17 This work
H3a 1.667 0.054 21.81 0.35 1.990e-18 1.442e-18 2.747e-18 This work
K1 2.110 0.102 18.77 0.20 1.423e-17 1.184e-17 1.711e-17 This work
K2 2.251 0.109 ≥19.96 … … … 3.690e-18 This work
J 1.252 0.152 19.78 0.10 3.555e-17 3.243e-17 3.898e-17 Janson et al. (2013)
H 1.633 0.288 20.01 0.14 1.131e-17 9.944e-18 1.287e-17 Janson et al. (2013)
Ks 2.139 0.312 19.38 0.11 7.591e-18 6.860e-18 8.401e-18 Janson et al. (2013)
CH4S 1.551 0.139 19.58 0.13 1.974e-17 1.752e-17 2.226e-17 Janson et al. (2013)
CH4L 1.719 0.142 ≥20.63 … … … 5.360e-18 Janson et al. (2013)
L’ 3.770 0.700 16.70 0.17 1.093e-17 9.344e-18 1.278e-17 Kuzuhara et al. (2013)
L_NB6 3.709 0.188 17.59 0.17 5.154e-18 4.407e-18 6.028e-18 Skemer et al. (2016)
L_NB7 3.875 0.234 16.47 0.19 1.229e-17 1.032e-17 1.464e-17 Skemer et al. (2016)
L_NB8 4.000 0.068 15.85 0.17 1.920e-17 1.641e-17 2.245e-17 Skemer et al. (2016)

Notes. The J2 and K2 upper-limit magnitudes correspond to the 3σ detection level. (a)Tentative re-detection at H3. The photometry corresponds to the one extracted from Specal. We considered it as an upper limit for the empirical and atmospheric model analysis.

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