Panoramic Optical and Near-Infrared SETI Instrument: Overall Specifications and Science Program
Panoramic optical and near-infrared SETI instrument: overall specifications and science program Shelley A. Wrighta,b, Paul Horowitzc,J´erˆomeMairea,DanWerthimerd, Franklin Antonioe, Michael Aronsonf,MarenCosensa,b,FrankD.Drakeg, Andrew W. Howardh, Geo↵rey W. Marcyd,RickRa↵antii, Andrew P. V. Siemiond,g,j,k,RemingtonP.S.Stonel,RichardR. Tre↵ersm, Avinash Uttamchandanic,SamChaim-Weismannd, a Center for Astrophysics & Space Sciences, University of California San Diego, USA; b Department of Physics, University of California San Diego, USA; c Department of Physics, Harvard University, USA; d Department of Astronomy, University of California Berkeley, CA, USA; e Qualcomm Research Center, 5775 Morehouse Dr, San Diego, CA, USA; f Electronic Packaging Man, Encinitas, CA, USA g SETI Institute, Mountain View, USA; h Astronomy Department, California Institute of Technology, USA; i Techne Instruments, Berkeley, CA, USA; j Radboud University, Nijmegen , Netherlands; kInstitute of Space Sciences and Astronomy, University of Malta; l University of California Observatories, Lick Observatory, USA; m Starman Systems, Alamo, USA; n Space Sciences Laboratory, University of California Berkeley, CA, USA ABSTRACT We present overall specifications and science goals for a new optical and near-infrared (350 - 1650 nm) instru- ment designed to greatly enlarge the current Search for Extraterrestrial Intelligence (SETI) phase space. The Pulsed All-sky Near-infrared Optical SETI (PANOSETI) observatory will be a dedicated SETI facility that aims to increase sky area searched, wavelengths covered, number of stellar systems observed, and duration of time monitored. This observatory will o↵er an “all-observable-sky” optical and wide-field near-infrared pulsed tech- nosignature and astrophysical transient search that is capable of surveying the entire northern hemisphere.
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