Here we describe our ongoing efforts to develop high-performance and sensitive instrumentation for use in the search for extra-terrestrial intelligence (SETI). These efforts include our recently deployed Search for Extraterrestrial Emissions from Nearby Developed Intelligent Populations Spectrometer (SERENDIP V.v) and two instruments currently under development; the Heterogeneous Radio SETI Spectrometer (HRSS) for SETI observations in the radio spectrum and the Optical SETI Fast Photometer (OSFP) for SETI observations in the optical band. We will discuss the basic SERENDIP V.v instrument design and initial analysis methodology, along with instrument architectures and observation strategies for OSFP and HRSS. In addition, we will demonstrate...
The SETI Project is a new kind of approach in the search for extraterrestrial intelligence. Instead ...
We present overall specifications and science goals for a new optical and near-infrared (350 - 1650 ...
We present overall specifications and science goals for a new optical and near-infrared (350 - 1650 ...
Here we describe our ongoing efforts to develop high-performance and sensitive instrumentation for u...
Here we describe our ongoing efforts to develop high-performance and sensitive instrumentation for u...
Over the past 30 years, interest in extraterrestrial intelligence has progressed from philosophical ...
We present developments in the search for engineered radio emissions from advanced extraterrestrial ...
We summarize radio and optical SETI programs based at the University of California, Berkeley. The SE...
The rationale for SETI is based on three arguments. First, there may be a plurality of inhabited wor...
We summarize radio and optical SETI programs based at the University of California, Berkeley. The o...
The SETI (Search for Extraterrestrial Intelligence) Project's primary thrust is to search the microw...
Our group is currently developing two new instruments to conduct commensal searches for extraterrest...
© 2016. The American Astronomical Society. All rights reserved. A spectral line image cube generated...
NASA's Search for Extraterrestrial Intelligence (SETI) project utilizes two complementary search str...
We present plans for an all-sky search for pulsed optical SETI beacons at Agassiz station in Harvard...
The SETI Project is a new kind of approach in the search for extraterrestrial intelligence. Instead ...
We present overall specifications and science goals for a new optical and near-infrared (350 - 1650 ...
We present overall specifications and science goals for a new optical and near-infrared (350 - 1650 ...
Here we describe our ongoing efforts to develop high-performance and sensitive instrumentation for u...
Here we describe our ongoing efforts to develop high-performance and sensitive instrumentation for u...
Over the past 30 years, interest in extraterrestrial intelligence has progressed from philosophical ...
We present developments in the search for engineered radio emissions from advanced extraterrestrial ...
We summarize radio and optical SETI programs based at the University of California, Berkeley. The SE...
The rationale for SETI is based on three arguments. First, there may be a plurality of inhabited wor...
We summarize radio and optical SETI programs based at the University of California, Berkeley. The o...
The SETI (Search for Extraterrestrial Intelligence) Project's primary thrust is to search the microw...
Our group is currently developing two new instruments to conduct commensal searches for extraterrest...
© 2016. The American Astronomical Society. All rights reserved. A spectral line image cube generated...
NASA's Search for Extraterrestrial Intelligence (SETI) project utilizes two complementary search str...
We present plans for an all-sky search for pulsed optical SETI beacons at Agassiz station in Harvard...
The SETI Project is a new kind of approach in the search for extraterrestrial intelligence. Instead ...
We present overall specifications and science goals for a new optical and near-infrared (350 - 1650 ...
We present overall specifications and science goals for a new optical and near-infrared (350 - 1650 ...