Difference between revisions of "GAL05"
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=== Observational settings/limits === | === Observational settings/limits === | ||
| − | + | Min zenith = 0 deg | |
| + | Max zenith = 30 deg (priority under 20 deg) | ||
| + | NSB: Dark (never moon conditions) | ||
| + | Wobbles: Standard | ||
| + | Total time requested: 50 hrs | ||
| − | |||
| − | + | The weather conditions should be good since we want to reduce the energy threshold down to 15-20 GeV. Therefore: | |
| − | + | - Transmission > 0.8 | |
| + | |||
| + | - If LIDAR is not working or there are doubts about the correct working on the LIDAR (e.g LIDAR profile or overall values do not seem reasonable based on the images from the AllSKyCamera), you can check that the rates are correct and that there are not too many clouds in the direction of the source to make a decision on the conditions to observe. | ||
Latest revision as of 10:38, 15 June 2023
Proposal[edit]
Proposal: GAL05: Search for Very High Energy pulsed emission from PSR J2021+3651
PI: Alvaro Mas-Aguilar (alvmas@ucm.es)
Source: PSR J2021+3651
RA (J2000) 305.2725000 deg
DEC (J2000) 36.8512500 deg
Observational settings/limits[edit]
Min zenith = 0 deg Max zenith = 30 deg (priority under 20 deg) NSB: Dark (never moon conditions) Wobbles: Standard Total time requested: 50 hrs
The weather conditions should be good since we want to reduce the energy threshold down to 15-20 GeV. Therefore:
- Transmission > 0.8
- If LIDAR is not working or there are doubts about the correct working on the LIDAR (e.g LIDAR profile or overall values do not seem reasonable based on the images from the AllSKyCamera), you can check that the rates are correct and that there are not too many clouds in the direction of the source to make a decision on the conditions to observe.
