P2.4 Align SHARK-NIR to the telescope

• Phase : 2
• Status : Draft
• Category : Daytime testing (functionality and operability) (C2)
• Recurrence : after instrument installation at telescope platform
• Duration : 3 days

Description

• SHARK-NIR is aligned to the telescope and daytime collimation model is acquired.

Prerequisites

• All electronics and services up and running.
• SHARK-NIR shutter open, and deployable arm (dichroic + IN-TT) deployed to get the light directed into SHARK-NIR.

Procedure

• Since SHARK-NIR has the same focal station of LBTI, the telescope is set to LBTI collimation model to start the alignment of SHARK-NIR to the telescope.
• RR is mounted on the SX side. Using RR / ARGOS on-axis calibration light source, M2 and M3 of the LBT are moved to have the on-axis spot on the reference position on SCICAM (also TECCAM), identified during the internal alignment of the instrument. (Do you want to use the IN-TT mirror for the alignment?) Coma, if present, is minimized looking at the out of focus image, shifting and tilting M2 and keeping the spot fixed on SCICAM. Astigmatism, if present, can be reduced by applying the astigmatism terms to M2 shape. Focus is adjusted shifting M2 along the optical axis. The daytime collimation model is recorded.
• Do we need to check if LBTI is getting the light in their detectors? Do we ever run both SHARK-NIR and LBTI parallelly? Maybe it is required for running the LBTI AO system?

Success criteria

• On-axis spot from the RR/ARGOS light source at the reference pixel of the SCICAM.
• The daytime SHARK-NIR collimation model recorded.
• Something with LBTI?

Notes

• SCICAM has large persistence. Avoid super-bright stars. Use TECHCAM first, and then SCICAM (with ND filter) later for the alignment.

LBTO support

• Mount the RR on SX
• Support from LBTI?

Associated SHARK-NIR personnel

Date performed and by whom