ICONN — THE INFRARED COHERENCING NEAREST NEIGHBOR TRACKER

Author:

JURGENSON C. A.1,SANTORO F. G.2,MCCRACKEN T. M.3,YOUNG J. S.4,SENETA E.4,BUSCHER D. F.4,CREECH-EAKMAN M.3,HANIFF C.4

Affiliation:

1. Department of Astronomy, Yale University, J.W. Gibbs Laboratory, 260 Whitney Avenue, New Haven, CT 06511, USA

2. GMTO Corporation, 251 South Lake Avenue, Suite 300, Pasadena, CA 91101, USA

3. Magdalena Ridge Observatory, New Mexico Institute of Mining and Technology, 801 Leroy Place, Socorro, New Mexico 87801, USA

4. Cavendish Laboratory, Astrophysics Group, University of Cambridge, JJ Thomson Avenue, Cambridge CB3 OHE, UK

Abstract

ICONN is a dedicated fringe tracker for the Magdalena Ridge Observatory Interferometer (MROI) that employs a baseline bootstrapping combination scheme utilizing the interferometer's "Y"-shaped telescope array. The ICONN optomechanics are designed in a modular fashion to combine light from two to ten telescopes while tracking on the nearest neighbor baselines. The software tasked with operating ICONN is designed to interface with the larger MROI software supervisory system. Commands are distributed to high level processes within ICONN, which in turn pass them down internally to lower level threads. The design of ICONN is now complete and laboratory testing has commenced. This paper details the optomechanical and software design of ICONN.

Publisher

World Scientific Pub Co Pte Lt

Subject

Astronomy and Astrophysics,Instrumentation

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