UVOT Mode: 0x0377
The following table summarizes this mode, ordered by the filter sequence:
| Filter | Event FOV | Image FOV | Bin Size | Max. Exp. Time | Weighting | Comments |
|---|---|---|---|---|---|---|
| u | 17 | 2 | 3000 | 3000 | Unscaled Tiling Observation that fails over to bluer filters if we have bright stars | |
| uvw1 | 17 | 2 | 3000 | 3000 | Unscaled Tiling Observation that fails over to bluer filters if we have bright stars | |
| uvw2 | 17 | 2 | 3000 | 3000 | Unscaled Tiling Observation that fails over to bluer filters if we have bright stars | |
| uvm2 | 17 | 3000 | Unscaled Tiling Observation that fails over to bluer filters if we have bright stars | |||
| Blocked | 17 | 1 | 3000 | 1000 | Unscaled Tiling Observation that fails over to bluer filters if we have bright stars |
Filter: The particular filter in the sequence.
Event FOV: The size of the FOV (in arc-minutes) for UVOT event data.
Image FOV: The size of the FOV (in arc-minutes) for UVOT image data.
Max. Exp. Time: The maximum amount of time the snapshot will spend on the particular filter in the sequence.
Weighting: Ratio of time spent on the particular filter in the sequence.
Comments: Additional notes that may be useful to know.
Swift Mission Operations Center
The Pennsylvania State University301 Science Park Road,
Building 2 Suite 332,
State College, PA 16801
USA
☎ +1 (814) 865-6834
📧 swiftods@swift.psu.edu
Swift MOC Team Leads
Mission Director: John NousekScience Operations: Jamie Kennea
Flight Operations: Mark Hilliard
UVOT: Michael Siegel
XRT: Jamie Kennea
Swift Partners
UK: UCL MSSL Univ. of LeicesterUSA: NASA/GSFC LANL Omitron SwRI
Italy: SSDC/ASI INAF OA-Brera