Difference between revisions of "GAL03"
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== Proposal == | == Proposal == | ||
− | Proposal: [[Media: | + | Proposal: [[Media:GAL03_Abe_updated.pdf|GAL03: Studying the large scale, diffuse emission around the Gal Center with the LST1 ]] <br> |
PI: Shotaro Abe (shotaro@icrr.u-tokyo.ac.jp) <br> | PI: Shotaro Abe (shotaro@icrr.u-tokyo.ac.jp) <br> | ||
− | Source: | + | Source Name: GalCenter field1 |
− | RA ( | + | RA [deg] = 266.41, DEC [deg] = -29.01 |
− | DEC ( | + | Min Zenith [deg] = 57, Max Zenith [deg] = 70 |
+ | Night Sky Background [Moon/Dark/Both] = Dark | ||
+ | Wobbles [Standard/Custom] = On (not wobble) | ||
+ | |||
+ | Source Name: GalCenter field2 | ||
+ | RA [deg] = 262.98, DEC [deg] = -29.01 | ||
+ | Min Zenith [deg] = 57, Max Zenith [deg] = 70 | ||
+ | Night Sky Background [Moon/Dark/Both] = Dark | ||
+ | Wobbles [Standard/Custom] = On (not wobble) | ||
+ | |||
+ | Source Name: GalCenter field3 | ||
+ | RA [deg] = 223.84, DEC [deg] = -29.01 | ||
+ | Min Zenith [deg] = 57, Max Zenith [deg] = 70 | ||
+ | Night Sky Background [Moon/Dark/Both] = Dark | ||
+ | Wobbles [Standard/Custom] = On (not wobble) | ||
=== Observational settings/limits === | === Observational settings/limits === | ||
+ | |||
+ | Min zenith = 57 deg | ||
+ | Max zenith = 70 deg (not strictly) | ||
+ | NSB: Dark | ||
+ | Wobbles: all ON, not wobble | ||
+ | Total time requested: 25 hours for each point | ||
+ | |||
+ | comment for shifters: | ||
+ | - it would be preferable to keep the standard duration of runs: 15 or 20 min, instead of a single long run like 1 hour. | ||
+ | comment for schedulers: | ||
+ | - it is not necessary to forcefully get observations concentrated on the relatively low zenith angles. | ||
+ | instead it would be good to try to take data as much as possible regardless of the zenith angle. | ||
+ | (of course, relatively low zenith angles (<63 deg) would be preferable, though) | ||
+ | - it may be good to carry out the three observations equally in a single night, | ||
+ | so that NSB and air conditions can be as equal as possible among them. | ||
+ | - it may be also good to make equal the zenith distributions among three points. |
Latest revision as of 09:36, 10 July 2023
Proposal[edit]
Proposal: GAL03: Studying the large scale, diffuse emission around the Gal Center with the LST1
PI: Shotaro Abe (shotaro@icrr.u-tokyo.ac.jp)
Source Name: GalCenter field1 RA [deg] = 266.41, DEC [deg] = -29.01 Min Zenith [deg] = 57, Max Zenith [deg] = 70 Night Sky Background [Moon/Dark/Both] = Dark Wobbles [Standard/Custom] = On (not wobble)
Source Name: GalCenter field2 RA [deg] = 262.98, DEC [deg] = -29.01 Min Zenith [deg] = 57, Max Zenith [deg] = 70 Night Sky Background [Moon/Dark/Both] = Dark Wobbles [Standard/Custom] = On (not wobble)
Source Name: GalCenter field3 RA [deg] = 223.84, DEC [deg] = -29.01 Min Zenith [deg] = 57, Max Zenith [deg] = 70 Night Sky Background [Moon/Dark/Both] = Dark Wobbles [Standard/Custom] = On (not wobble)
Observational settings/limits[edit]
Min zenith = 57 deg Max zenith = 70 deg (not strictly) NSB: Dark Wobbles: all ON, not wobble Total time requested: 25 hours for each point comment for shifters: - it would be preferable to keep the standard duration of runs: 15 or 20 min, instead of a single long run like 1 hour. comment for schedulers: - it is not necessary to forcefully get observations concentrated on the relatively low zenith angles. instead it would be good to try to take data as much as possible regardless of the zenith angle. (of course, relatively low zenith angles (<63 deg) would be preferable, though) - it may be good to carry out the three observations equally in a single night, so that NSB and air conditions can be as equal as possible among them. - it may be also good to make equal the zenith distributions among three points.