Changes between Version 108 and Version 109 of docs/CommissioningPlan


Ignore:
Timestamp:
01/19/21 18:42:43 (4 years ago)
Author:
kradhakrishnan
Comment:

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  • docs/CommissioningPlan

    v108 v109  
    136136||'''Number'''||'''Activity Name'''||'''Day / Night'''||'''Duration (nights)'''||'''Category'''||'''LBTO Support'''||
    137137||P4.1||[wiki:/docs/CommissioningPlan/P4.1 Direct imaging + field stabilized mode testing (95% cases)]||Night||1.5||C4 + C6||AO support||
    138 ||P4.2||[wiki:/docs/CommissioningPlan/P4.1 Direct imaging + pupil stabilized mode testing (5% cases)]||Night||0.5||C4 + C6||AO support||
    139 ||P4.3||[wiki:/docs/CommissioningPlan/P4.2 Coronagraphic imaging + field stabilization mode testing]||Night||1||C4 + C6||AO support||
    140 ||P4.4||[wiki:/docs/CommissioningPlan/P4.3 Coronagraphic imaging + pupil stabilization mode testing]||Night||3||C4 + C6||AO support||
    141 ||P4.5||[wiki:/docs/CommissioningPlan/P4.4 Long-slit spectrograph mode testing]||Night||2||C4 + C6||AO support||
    142 ||P4.6||[wiki:/docs/CommissioningPlan/P4.6 Exo-planet: Giant planets and brown dwarfs in SFR, stellar associations, & young open clusters]||Night||10||C4 + C6||AO support||
    143 ||P4.7||[wiki:/docs/CommissioningPlan/P4.7 Exo-planet: Astrometry]||Night||4||C4 + C6||AO support||
    144 ||P4.8||[wiki:/docs/CommissioningPlan/P4.8 Exo-planet: Spectroscopic Characterization of known sub-stellar companions]||Night||5||C4 + C6||AO support||
    145 ||P4.9||[wiki:/docs/CommissioningPlan/P4.9 Disk: High-contrast images of circumstellar disks]||Night||1||C4 + C6||AO support||
    146 ||P4.10||[wiki:/docs/CommissioningPlan/P4.10 Disk: Coronagraphic imaging of stellar jets]||Night||1||C4 + C6||AO support||
    147 ||P4.11||[wiki:/docs/CommissioningPlan/P4.11 Disk:  Jets investigated with long-slit spectra]||Night||1||C4 + C6||AO support||
    148 ||P4.12||[wiki:/docs/CommissioningPlan/P4.12 Extragalactic: QSO & AGNs]||Night||4||C4 + C6||AO support||
    149 ||P4.13||[wiki:/docs/CommissioningPlan/P4.13 Solar system: Size and shape of main-belt astroids]||Night||1||C4 + C6||AO support||
    150 ||P4.14||[wiki:/docs/CommissioningPlan/P4.14 Solar system: Surface heterogeneity of trans-neptunian objects]||Night||1||C4 + C6||AO support||
     138||P4.2||[wiki:/docs/CommissioningPlan/P4.2 Direct imaging + pupil stabilized mode testing (5% cases)]||Night||0.5||C4 + C6||AO support||
     139||P4.3||[wiki:/docs/CommissioningPlan/P4.3 Coronagraphic imaging + field stabilization mode testing]||Night||1||C4 + C6||AO support||
     140||P4.4||[wiki:/docs/CommissioningPlan/P4.4 Coronagraphic imaging + pupil stabilization mode testing]||Night||3||C4 + C6||AO support||
     141||P4.5||[wiki:/docs/CommissioningPlan/P4.5 Long-slit spectrograph mode testing]||Night||2||C4 + C6||AO support||
     142||P4.6||[wiki:/docs/CommissioningPlan/P4.6 Exo-planet: Giant planets and brown dwarfs in SFR, stellar associations, & young open clusters]||Night||10||C7||AO support||
     143||P4.7||[wiki:/docs/CommissioningPlan/P4.7 Exo-planet: Astrometry]||Night||4||C7||AO support||
     144||P4.8||[wiki:/docs/CommissioningPlan/P4.8 Exo-planet: Spectroscopic Characterization of known sub-stellar companions]||Night||5||C7||AO support||
     145||P4.9||[wiki:/docs/CommissioningPlan/P4.9 Disk: High-contrast images of circumstellar disks]||Night||1||C7||AO support||
     146||P4.10||[wiki:/docs/CommissioningPlan/P4.10 Disk: Coronagraphic imaging of stellar jets]||Night||1||C7||AO support||
     147||P4.11||[wiki:/docs/CommissioningPlan/P4.11 Disk:  Jets investigated with long-slit spectra]||Night||1||C7||AO support||
     148||P4.12||[wiki:/docs/CommissioningPlan/P4.12 Extragalactic: QSO & AGNs]||Night||4||C7||AO support||
     149||P4.13||[wiki:/docs/CommissioningPlan/P4.13 Solar system: Size and shape of main-belt astroids]||Night||1||C7||AO support||
     150||P4.14||[wiki:/docs/CommissioningPlan/P4.14 Solar system: Surface heterogeneity of trans-neptunian objects]||Night||1||C7||AO support||
    151151
    152152Note: The duration mentioned in Phase 4 will be changed to hours later.