Table B.1
Observation log for the GRB 050219A field.
| Filter | Wavelength | Telesc./Instr. | Magnitudes | AB Magnitudes | Flux density | Upper | Lower |
| (μm) | (Observed) | (Ext. cor.) | (μJy) | (μJy) | (μJy) | ||
|
|
|||||||
| FUV | 0.152 | GALEX | > 21.6 | > 20.5 | < 23.89 | – | – |
| NUV | 0.193 | GALEX | > 21.7 | > 20.6 | < 20.99 | – | – |
| uvw2 | 0.225 | Swift/UVOT | > 21.3 | > 21.8 | < 7.19 | – | – |
| uvm2 | 0.227 | Swift/UVOT | > 20.5 | > 20.7 | < 18.86 | – | – |
| uvw1 | 0.260 | Swift/UVOT | > 21.3 | > 21.7 | < 7.42 | – | – |
| u | 0.347 | Swift/UVOT | > 21.4 | > 21.6 | < 8.56 | – | – |
| b | 0.430 | Swift/UVOT | > 21.7 | > 20.8 | < 16.90 | – | – |
| v | 0.543 | Swift/UVOT | 20.82 ± 0.12 | 20.31 | 27.86 | 31.12 | 24.95 |
| g ′ | 0.459 | 2.2 m/GROND | 21.49 ± 0.04 | 20.85 | 16.96 | 17.64 | 16.38 |
| r ′ | 0.622 | 2.2 m/GROND | 20.17 ± 0.04 | 19.76 | 46.20 | 47.72 | 44.74 |
| i ′ | 0.764 | 2.2 m/GROND | 19.70 ± 0.04 | 19.38 | 65.55 | 67.89 | 63.30 |
| z ′ | 0.899 | 2.2 m/GROND | 19.41 ± 0.04 | 19.18 | 78.77 | 81.58 | 76.06 |
| J | 1.240 | 2.2 m/GROND | 17.74 ± 0.04 | 18.52 | 145.06 | 149.82 | 140.46 |
| H | 1.647 | 2.2 m/GROND | 17.01 ± 0.10 | 18.30 | 178.52 | 195.74 | 162.81 |
| K s | 2.170 | 2.2 m/GROND | 16.66 ± 0.12 | 18.44 | 156.30 | 174.56 | 139.94 |
| R | 0.660 | VLT/FORS2 | 20.2 ± 0.1 | 20.0 | 37.19 | 33.91 | 40.78 |
| 3.6 μm | 3.543 | Spitzer/IRAC | 19.10 ± 0.02 | 19.10 | 85.00 | 87.00 | 83.00 |
| 5.8 μm | 5.711 | Spitzer/IRAC | 19.5 ± 0.2 | 19.5 | 58.00 | 66.00 | 50.00 |
| 24 μm | 23.68 | Spitzer/MIPS | 20.7 ± 0.3 | 20.7 | 19.00 | 24.00 | 14.00 |
| 100 | 100 | Herschel/PACS | > 14.6 | > 14.6 | < 5400 | – | – |
| 160 | 160 | Herschel/PACS | > 14.4 | > 14.4 | < 15600 | – | – |
| 250 | 250 | Herschel/SPIRE | > 13.4 | > 13.4 | < 16500 | – | – |
| 350 | 350 | Herschel/SPIRE | > 13.1 | > 13.1 | < 21000 | – | – |
| 500 | 500 | Herschel/SPIRE | > 12.9 | > 12.9 | < 24600 | – | – |
Notes. Column 4 gives observed magnitudes and their errors in the native system of the filters. Column 5 has AB magnitudes corrected for Galactic extinction (E(B − V) = 0.16 mag). The last 3 columns are the corresponding flux densities and their upper and lower value in μJy after correction for Galactic extinction. The upper limits are 3σ above the background. To convert UVOT magnitudes into the AB system we used the following conversion: uvw2 = + 1.73, uvm2 = + 1.69, uvw1 = + 1.51, u = + 1.02, b = + 0.13, v = ± 0.01. For the FORS2/R-band we used R = + 0.23.
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