Table 5.
LSQ gr-band photometry of SNhunt120 in the Swope “natural” system.
| JD | V(a) | Err |
|---|---|---|
| 2456013.80 | 18.951 | 0.054 |
| 2456014.80 | 18.678 | 0.108 |
| 2456017.79 | 18.042 | 0.010 |
| 2456018.79 | 18.001 | 0.060 |
| 2456021.78 | 17.873 | 0.017 |
| 2456022.78 | 17.858 | 0.019 |
| 2456024.70 | 17.850 | 0.100 |
| 2456032.73 | 18.085 | 0.012 |
| 2456034.85 | 18.144 | 0.013 |
| 2456036.71 | 18.237 | 0.036 |
| 2456040.70 | 18.332 | 0.019 |
| 2456048.62 | 18.545 | 0.022 |
| 2456050.66 | 18.511 | 0.057 |
| 2456057.57 | 18.573 | 0.140 |
| 2456071.50 | 19.035 | 0.049 |
| 2456075.53 | 19.377 | 0.082 |
| 2456079.51 | 19.264 | 0.079 |
Notes.
Photometry is computed relative to the V-band magnitude of star with identification (ID) number 3 in Table 1. To facilities good agreement between the LSQ gr-band and CSP-II V-band light curves, a 0.03 mag offset was added to the CSP-II magnitude of star 3 as explained in the text.
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