GAL03

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Revision as of 16:32, 12 June 2023 by Shoaro (talk | contribs) (Observational settings/limits)
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Proposal

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

  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: 
    - 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. 
    - 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.