Pointing Origins

Pointing origins (POs) are calibrated positions within the focal plane of the instrument. Each instrument has at least one, and often several, POs. One might be the center of the science detector, another might be the center of the slit, and a third might be the center of the guider.

The pointing origins are defined in millimeters in the rotator frame, with (0,0) being the rotation axis. Instruments without a rotator use some arbitrary definition of (0,0).

The angle of the coordinate system is usually defined by having "up" on the guider camera be the elevation axis when the rotator is set to physical position angle 0. With the zero-point and the rotation of the system defined, all other relationships between pointing origins are known.

KSD40 is a technical document that describes in detail the definition of POs and the relationships between various coordinate systems. It also contains instrument-specific details about POs.

Last modified: 04/24/2018 20:04
Send questions or comments to:

The information on this page is the property of the W. M. Keck Observatory. The contents of this page or any part thereof shall not be copied or otherwise reproduced or transferred to other documents or used or disclosed to others for any purpose other than observing support at the W. M. Keck Observatory and the subsequent analysis and publication of scientific data obtained from observations conducted at the W. M. Keck Observatory. All rights reserved. © W. M. Keck Observatory.