Overview of observations. Median seeing values are derived from observations with a DIMM located at the TNG telescope. The actual seeing at the location of our experiment is expected to be worse due to additional turbulence associated with our telescope enclosure and low-level turbulent layers not sampled by the TNG DIMM. Nevertheless, these values provide a useful indication of relative seeing variations.
| Night . | Runs . | Median seeing (arcsec) . | Time (utc) . |
|---|---|---|---|
| Sep 17 | 36 | 0.51 | 01:00+1–03:30+1 |
| Sep 18 | 60 | 0.41 | 22:00–04:30+1 |
| Sep 19 | 36 | 0.61 | 23:00–01:30+1 |
| Night . | Runs . | Median seeing (arcsec) . | Time (utc) . |
|---|---|---|---|
| Sep 17 | 36 | 0.51 | 01:00+1–03:30+1 |
| Sep 18 | 60 | 0.41 | 22:00–04:30+1 |
| Sep 19 | 36 | 0.61 | 23:00–01:30+1 |
Overview of observations. Median seeing values are derived from observations with a DIMM located at the TNG telescope. The actual seeing at the location of our experiment is expected to be worse due to additional turbulence associated with our telescope enclosure and low-level turbulent layers not sampled by the TNG DIMM. Nevertheless, these values provide a useful indication of relative seeing variations.
| Night . | Runs . | Median seeing (arcsec) . | Time (utc) . |
|---|---|---|---|
| Sep 17 | 36 | 0.51 | 01:00+1–03:30+1 |
| Sep 18 | 60 | 0.41 | 22:00–04:30+1 |
| Sep 19 | 36 | 0.61 | 23:00–01:30+1 |
| Night . | Runs . | Median seeing (arcsec) . | Time (utc) . |
|---|---|---|---|
| Sep 17 | 36 | 0.51 | 01:00+1–03:30+1 |
| Sep 18 | 60 | 0.41 | 22:00–04:30+1 |
| Sep 19 | 36 | 0.61 | 23:00–01:30+1 |
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