Difference between revisions of "GAL03"

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(Created page with "== Proposal == Proposal: GAL03: Studying the large scale, diffuse emission around the Gal Center with the LST1 <br> PI: Shotaro Abe (shotaro@icrr.u-t...")
 
 
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== Proposal ==
 
== Proposal ==
Proposal: [[Media:GAL03_Abe.pdf|GAL03: Studying the large scale, diffuse emission around the Gal Center with the LST1 ]] <br>
+
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:<br>
+
   Source Name: GalCenter field1
     RA (J2000)   <br>
+
     RA [deg] = 266.41, DEC [deg] = -29.01
     DEC (J2000) <br>
+
    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.