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ARCONS: a Highly Multiplexed Superconducting UV-to-Near-IR Camera

O'Brien, Kieran and Mazin, Ben and McHugh, Sean and Meeker, Seth and Bumble, Bruce (2012) ARCONS: a Highly Multiplexed Superconducting UV-to-Near-IR Camera. In: New Horizons in Time Domain Astronomy. IAU Symposium Proceedings Series. Vol.7. No.S285. Cambridge University Press , Cambridge, pp. 385-388. ISBN 9781107019850. https://resolver.caltech.edu/CaltechAUTHORS:20160311-130908112

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Abstract

ARCONS, the Array Camera for Optical to Near-infrared Spectrophotometry, was recently commissioned at the coudé focus of the 200-inch Hale Telescope at the Palomar Observatory. At the heart of this unique instrument is a 1024-pixel Microwave Kinetic Inductance Detector (MKID), exploiting the Kinetic Inductance effect to measure the energy of the incoming photon to better than several percent. The ground-breaking instrument is lens-coupled with a pixel scale of 0''.23/pixel, each pixel recording the arrival time (< 2 μ sec) and energy of a photon (~10%) in the optical to near-IR (0.4-1.1 microns) range. The scientific objectives of the instrument include the rapid follow-up and classification of transient phenomena.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1017/S1743921312001159DOIArticle
http://arxiv.org/abs/1201.5904arXivDiscussion Paper
Additional Information:© 2012 International Astronomical Union. We would like to thank the management and staff of Palomar Observatory for their hard work and support during the commissioning of ARCONS. Material in this paper is based upon work supported by the National Aeronautics and Space Administration under Grant NNX09AD54G, issued through the Science Mission Directorate, Jet Propulsion Lab’s Research & Technology Development Program, and a grant from the W.M. Keck Institute for Space Studies. Part of the research was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration.
Group:Keck Institute for Space Studies
Funders:
Funding AgencyGrant Number
NASANNX09AD54G
JPL Research and Technology Development FundUNSPECIFIED
Keck Institute for Space Studies (KISS)UNSPECIFIED
NASA/JPL/CaltechUNSPECIFIED
Subject Keywords:instrumentation : detectors, instrumentation : spectrographs , pulsars : individual (Crab)
Series Name:IAU Symposium Proceedings Series
Issue or Number:S285
DOI:10.1017/S1743921312001159
Record Number:CaltechAUTHORS:20160311-130908112
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20160311-130908112
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:65303
Collection:CaltechAUTHORS
Deposited By: Colette Connor
Deposited On:11 Mar 2016 23:25
Last Modified:10 Nov 2021 23:43

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