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Program

Instrument(s)

Estimated time

SA and other staff involved

Science verification of DEIMOS polo migration to Linux and rotator controller upgrade. Test GUIs and operation scripts on sky with a DEIMOS observer.

DEIMOS

Two 0.5 nights separated by two weeks.

C. Alvarez.

S. Kwok, K. Lanclos and W. Deich (UCSC) on call.

Solid on-sky time with TRICK NGS and LGS, smooth out all TRICK’s edges. Observe a wide range of targets, e.g. point sources, faint extended sources, nonsidereal targets, etc.

OSIRIS

2

J. Lyke, JC Guerra, S. Yeh, S. Cetre

PyWFS and SH switch back and forth on sky (procedure needs to be practiced during daytime BEFORE nighttime engineering)

NIRC2

P. Gomez, JC Guerra, C. Bond, S. Cetre

NGS-AO performances and stability using 1.0 plate scale for KI and KII

OSIRIS NIRC2

JC Guerra

NIRES engineering:
daytime:

  1. slit-viewing camera guiding work 24 hours (need cold NIRES, no tel access)

  2. spectral flexure 8 hours (full tel access)

night time:

  1. optical guider flexure 2 hours

  2. throughput measurements 0.5 hours

  3. slit-viewing guiding 2 hours

NIRES

5 hours

P. Gomez (all)

M. Baril (daytime 1)

S. Kwok (night time 3)

K. Laclos (daytime 1)

A. Rostopchina (night time 1)

KAPA Laser engineering

OSIRIS

1

J. Lyke, S. Ragland, S. Cetre, E. Wetherell

NIRSPEC SCAM guiding on sky. Test and optimize SCAM acquisition and Magiq/SCAM guiding for M-band objects imaged on SCAM directly. This would make use of the recently optimized detector settings for the high background Mband imaging case.

NIRSPEC

0.5 night

G. Doppmann, S Kwok