Paper:	Simulating the Performance of Large Format Sub-mm Focal-plane Arrays
Volume:	278, NAIC-NRAO School on Single-dish Radio Astronomy: Techniques and Applications
Page:	515
Authors:	Chapin, Edward; Hughes, David H.
Abstract:	A robust measurement of the clustering amplitude of the sub-mm population of starburst galaxies requires large-area surveys (>> 1 deg2). Since even the largest-format arrays subtend only 10 arcmin2 on the sky then scan-mapping is a necessary observing mode. Providing realistic representations of the extragalactic sky and atmosphere, as the input to a detailed simulator of the telescope and instrument performance, allows important decisions to be made about the design of large-area fully-sampled surveys and observing strategies. Our simulations include detector noise, time-constants and array geometry, telescope pointing errors, scan speeds and scanning angles, sky noise and sky rotation.

Astronomical Society of the Pacific
Conference Series

© Copyright 1988 - 2024 - Astronomical Society of the Pacific
No part of the material protected by this copyright may be reproduced or used in any form other than for personal use without written permission from the ASP.

Page generated in 0.048 seconds