Table A.3
Magnitudes of the target OGLE-2011-BLG-0417.
| Spectral band | Magnitude | Error |
|
|
||
| J | 13.98 | 0.05 |
| H | 13.16 | 0.03 |
| Ks | 12.94 | 0.03 |
|
|
||
| 3400–3500 | 22.372 | 0.129 |
| 3500–3600 | 22.163 | 0.091 |
| 3600–3700 | 21.637 | 0.053 |
| 3700–3800 | 21.501 | 0.043 |
| 3800–3900 | 21.744 | 0.045 |
| 3900–4000 | 21.035 | 0.030 |
| 4000–4100 | 20.296 | 0.024 |
| 4100–4200 | 20.235 | 0.023 |
| 4200–4300 | 20.027 | 0.023 |
| 4300–4400 | 19.801 | 0.023 |
| 4400–4500 | 19.522 | 0.023 |
| 4900–5000 | 18.717 | 0.021 |
| 5000–5100 | 18.605 | 0.020 |
| 5100–5200 | 18.513 | 0.020 |
| 5200–5300 | 18.306 | 0.020 |
| 5300–5400 | 18.087 | 0.020 |
| 5400–5500 | 17.991 | 0.020 |
| 5500–5600 | 17.845 | 0.020 |
| 5600–5700 | 17.723 | 0.020 |
| 5900–6000 | 17.500 | 0.020 |
| 6000–6100 | 17.414 | 0.020 |
| 6100–6200 | 17.383 | 0.020 |
| 6200–6300 | 17.343 | 0.020 |
| 6300–6400 | 17.267 | 0.020 |
| 6400–6500 | 17.174 | 0.020 |
| 6500–6600 | 17.089 | 0.020 |
| 6600–6700 | 16.985 | 0.020 |
| 6700–6800 | 16.929 | 0.020 |
|
|
||
| 10000–10500 | 15.511 | 0.021 |
| 10500–11000 | 15.402 | 0.021 |
| 11000–11500 | 15.340 | 0.021 |
| 11500–12000 | 15.257 | 0.020 |
| 12000–12500 | 15.182 | 0.020 |
| 12500–13000 | 15.112 | 0.021 |
| 15000–15500 | 14.899 | 0.020 |
| 15500–16000 | 14.880 | 0.020 |
| 16000–16500 | 14.822 | 0.020 |
| 16500–17000 | 14.794 | 0.020 |
| 17000–17500 | 14.822 | 0.020 |
| 17500–18000 | 14.872 | 0.021 |
| 20000–20500 | 14.979 | 0.021 |
| 20500–21000 | 15.009 | 0.021 |
| 21000–21500 | 15.041 | 0.021 |
| 21500–22000 | 15.064 | 0.021 |
| 22000–22500 | 15.085 | 0.021 |
| 22500–23000 | 15.134 | 0.021 |
| 23000–23500 | 15.220 | 0.022 |
| 23500–24000 | 15.271 | 0.023 |
| 24000–24500 | 15.320 | 0.032 |
Notes. The spectral bands J, H, and Ks are referenced in the Vega system, while the other ones are referenced in the AB system, i.e. the zero-magnitude corresponds to a flux of 3631 Jy. The spectral domains of the custom bands are expressed in Angstrom. The lines indicate the limits between the three sets of SED.
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