Photometry of the progenitor of SN 2011dh. The Van Dyk et al. (2011) and Maund et al. (2011) magnitudes are the HST F336W, F435W, F555W, F658N, and F814W filters.
| Band . | LBT . | Van Dyk . | Maund . |
|---|---|---|---|
| . | (mag) . | (mag) . | (mag) . |
| U | 23.18 ± 0.07 | 23.434 ± 0.339 | 23.39 ± 0.25 |
| B | 22.30 ± 0.02 | 22.451 ± 0.005 | 22.36 ± 0.02 |
| V | 21.66 ± 0.09 | 21.864 ± 0.006 | 21.83 ± 0.04 |
| R | 21.42 ± 0.04 | 21.392 ± 0.021 | 21.28 ± 0.04 |
| I | 21.216 ± 0.005 | 21.20 ± 0.03 |
| Band . | LBT . | Van Dyk . | Maund . |
|---|---|---|---|
| . | (mag) . | (mag) . | (mag) . |
| U | 23.18 ± 0.07 | 23.434 ± 0.339 | 23.39 ± 0.25 |
| B | 22.30 ± 0.02 | 22.451 ± 0.005 | 22.36 ± 0.02 |
| V | 21.66 ± 0.09 | 21.864 ± 0.006 | 21.83 ± 0.04 |
| R | 21.42 ± 0.04 | 21.392 ± 0.021 | 21.28 ± 0.04 |
| I | 21.216 ± 0.005 | 21.20 ± 0.03 |
Photometry of the progenitor of SN 2011dh. The Van Dyk et al. (2011) and Maund et al. (2011) magnitudes are the HST F336W, F435W, F555W, F658N, and F814W filters.
| Band . | LBT . | Van Dyk . | Maund . |
|---|---|---|---|
| . | (mag) . | (mag) . | (mag) . |
| U | 23.18 ± 0.07 | 23.434 ± 0.339 | 23.39 ± 0.25 |
| B | 22.30 ± 0.02 | 22.451 ± 0.005 | 22.36 ± 0.02 |
| V | 21.66 ± 0.09 | 21.864 ± 0.006 | 21.83 ± 0.04 |
| R | 21.42 ± 0.04 | 21.392 ± 0.021 | 21.28 ± 0.04 |
| I | 21.216 ± 0.005 | 21.20 ± 0.03 |
| Band . | LBT . | Van Dyk . | Maund . |
|---|---|---|---|
| . | (mag) . | (mag) . | (mag) . |
| U | 23.18 ± 0.07 | 23.434 ± 0.339 | 23.39 ± 0.25 |
| B | 22.30 ± 0.02 | 22.451 ± 0.005 | 22.36 ± 0.02 |
| V | 21.66 ± 0.09 | 21.864 ± 0.006 | 21.83 ± 0.04 |
| R | 21.42 ± 0.04 | 21.392 ± 0.021 | 21.28 ± 0.04 |
| I | 21.216 ± 0.005 | 21.20 ± 0.03 |
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