Differences
This shows you the differences between two versions of the page.
| Both sides previous revision Previous revision | Last revision Both sides next revision | ||
|
swift [2021/07/21 14:20] Déborah Paradis |
swift [2023/04/11 15:32] Déborah Paradis |
||
|---|---|---|---|
| Line 4: | Line 4: | ||
| Swift has three co-aligned instruments for studying gamma-ray bursts and their afterglow: the Burst Alert Telescope (BAT), the X-ray Telescope (XRT), and the Ultraviolet/Optical Telescope (UVOT). | Swift has three co-aligned instruments for studying gamma-ray bursts and their afterglow: the Burst Alert Telescope (BAT), the X-ray Telescope (XRT), and the Ultraviolet/Optical Telescope (UVOT). | ||
| - | CADE only serves data obtained with the BAT instrument, in 8 energy bands: 14-20 keV, 20-24 keV, 24-35 keV, 35-50 keV, 50-75 keV, 75-100 keV, 100-150 keV, and 150-195 keV, at an angular resolution of 19.5'. Healpix maps are in units of ''cnts/s/detector''. The detector is an individual piece of CZT in the BAT array with an area of 1.6E-7 m2. | + | CADE only serves data obtained with the BAT instrument, in 8 energy bands: 14-20 keV, 20-24 keV, 24-35 keV, 35-50 keV, 50-75 keV, 75-100 keV, 100-150 keV, and 150-195 keV, at an angular resolution of 19.5'. Healpix maps are in units of ''cnts/s/detector''. The detector is an individual piece of CZT in the BAT array with an area of 1.6E-7 m2.\\ |
| + | |||
| + | Healpix maps made by D. Paradis. | ||
| === References === | === References === | ||