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swift [2019/02/21 13:23] Déborah Paradis |
swift [2023/04/11 15:32] Déborah Paradis |
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| 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.\\ |
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| + | Healpix maps made by D. Paradis. | ||
| === References === | === References === | ||
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| </html> | </html> | ||
| - | 24-35 keV : [[http://cade.irap.omp.eu/documents/Ancillary/SWIFT/BAT_20_35_1_512.fits|BAT_20_35_1_512.fits]] | + | 24-35 keV : [[http://cade.irap.omp.eu/documents/Ancillary/SWIFT/BAT_24_35_1_512.fits|BAT_24_35_1_512.fits]] |
| <html> | <html> | ||
| <button class="aladin-btn" type="button" onclick="connector.runWithConnection(bat_20_35)">Aladin</button> | <button class="aladin-btn" type="button" onclick="connector.runWithConnection(bat_20_35)">Aladin</button> | ||
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| </script> | </script> | ||
| </html> | </html> | ||
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| + | ===HiPS === | ||
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| + | Swift/BAT HiPS are available in Aladin Collections/Image | ||
| === Original WCS Data === | === Original WCS Data === | ||