170x Filetype PPTX File size 0.43 MB Source: www.naoj.org
Background: Current and near Future 1. Significant reduction of operation budget from government 2. Reconfiguration of instruments with wide-field survey type instruments • HSC, PFS, ULTIMATE-Subaru will be the main instruments (Queue mode) Reduce the operation cost Efficient survey type • Reduce Users travel costs(3 千千千 ) operation • Reduce traffics to summit • • Queue mode operation Reduce HP expenses (2千千千) • • Increase observer’s role Limited number of open-use nights Future Operation Modes • No summit attendant Full Remote • Observers at Mitaka/Hilo/Other Observation sites • SA/Operator at Hilo • Survey (SSP: HSC, PFS, ULTIMATE) Queue • IRD <-> SCExAO/CHARIS or IRCS mode • SA(1)+OSA(1) operation Transition…. 1 ) Operator e at Hilo t emo R ll Fu ( l a ssic a l C 1-3 Observer 1 Operator 1 SA Operation at Mitaka/Hilo Qu eu e mo de 1 Operation at summit Operator 1 SA Operation at Hilo Benefits Con. Reduce workloads of SAs Difficulty of troubleshooting Full Remote Reduce summit traffic Accommodation/food service in Hilo Reduce travel/HP expenses Difficulty of communication with observers Data quality control Needs easy UI for observers (soft wares) Queue Efficient survey observation Needs more work for staffs (Queue Coordinator, FQA staff, IQA by SA) Allow Time Series observation (Cadency, Variable,...) Queue Mode Operation: HSC, PFS, NsIR • Currently only HSC since S16A. • Open Use (several nights) + HSC SSP (several nights) • Based on observational constraints: Seeing, Transparency, Moon phase and separation angle. • Observational block shorter than 100 minutes. • 千 SA (1) + OSA (1) operation • PFS operation is planning to do queue mode operation. • NsIR platform: SCExAO <->CHARIS<->IRD (between PI instruments) • IRD requests hour base observational planning. • SCExAO/CHARIS necessary very good seeing condition. • The switching between instrument is take just a few minutes. • Support staff must know how to handle all SCExAO/CHARIS/IRD instruments.
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