User's Guide to the Shane 3-m Telescope


Table of Contents


Introduction
Hardware
Coude
Diagonal Mirror
TUB Rotation
Arc & Flat-field Lamps
Sofware
pococ
starlists
guidercopy
trouble report
Limits
Pointing
Weather
Target Of Opportunity (TOO)
Remote Operations
Data Archive
Mt. Hamilton Homepage

Shane 3-m Telescope Pointing Limits

Pointing limits are subject to change in response to changing operational constraints. The limits published here are guidelines. Ultimately, responsibility for the telescope, instrument, laser bundle, etc. rests with the Telescope Operator, who has the final say/veto on any attempt to point the telescope, given the prevailing conditions (e.g. safety, operational, meteorological).

East Pointing Limit: -05:40:00.

Expressed as an Hour Angle.

West Pointing Limit: +03:45:00 (as of September 2024).

Expressed as an Hour Angle.

North Pointing Limit: +72.0 degrees (as of May 2018).

As of May 2018, the nominal northern Declination pointing limit for the Shane telescope is: +72.0 degrees. As of May 2018, the absolute northen Declination pointing limit for the Shane telescope is +75.0 degrees. However, due to cable length restrictions, attempting to observe that far north requires extreme caution to ensure no cables are damaged. Advance approval is required to observe north of the nominal northern Declination limit. Approval may be granted on a source-by-source basis by the Directorship or their designated proxy (e.g. Support Astronomers or Head of Telescope Operations).

South Pointing Limit: -35.0 degrees (as of May 2018).


The following (pre-2010) image should only be used for approximate guidance. Find the declination of your target (green lines) and read the zenith distance (Y-axis) for a given hour angle (X-axis). Note that several obstructions (horizontal red lines) are encountered before reaching the software limits (80 degrees zenith distance or 5h 40m hour angle). Each of these obstructions - lower shutter, windscreen, and elevator - requires about 5 minutes to be moved out of the way.

The inoperative windscreen was completely removed in early 2010, so it no longer can cause any obstruction of the telescope aperture.


Support Astronomers
Last modified: Fri September 20 00:00:00 PDT 2024