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Title: A framework for collaborative review of candidate events in high data rate streams: The V-FASTR experiment as a case study

Abstract

“Fast radio transients” are defined here as bright millisecond pulses of radio-frequency energy. These short-duration pulses can be produced by known objects such as pulsars or potentially by more exotic objects such as evaporating black holes. The identification and verification of such an event would be of great scientific value. This is one major goal of the Very Long Baseline Array (VLBA) Fast Transient Experiment (V-FASTR), a software-based detection system installed at the VLBA. V-FASTR uses a “commensal” (piggy-back) approach, analyzing all array data continually during routine VLBA observations and identifying candidate fast transient events. Raw data can be stored from a buffer memory, which enables a comprehensive off-line analysis. This is invaluable for validating the astrophysical origin of any detection. Candidates discovered by the automatic system must be reviewed each day by analysts to identify any promising signals that warrant a more in-depth investigation. To support the timely analysis of fast transient detection candidates by V-FASTR scientists, we have developed a metadata-driven, collaborative candidate review framework. The framework consists of a software pipeline for metadata processing composed of both open source software components and project-specific code written expressly to extract and catalog metadata from the incoming V-FASTR data products,more » and a web-based data portal that facilitates browsing and inspection of the available metadata for candidate events extracted from the VLBA radio data.« less

Authors:
; ; ; ; ; ; ;  [1]
  1. Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109 (United States)
Publication Date:
OSTI Identifier:
22342164
Resource Type:
Journal Article
Resource Relation:
Journal Name: Astronomical Journal (New York, N.Y. Online); Journal Volume: 149; Journal Issue: 1; Other Information: Country of input: International Atomic Energy Agency (IAEA)
Country of Publication:
United States
Language:
English
Subject:
79 ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; ASTROPHYSICS; BLACK HOLES; CATALOGS; DATA ANALYSIS; DETECTION; INSPECTION; PULSARS; PULSES; RADIOWAVE RADIATION; STREAMS; TRANSIENTS; VERIFICATION

Citation Formats

Hart, Andrew F., Cinquini, Luca, Khudikyan, Shakeh E., Thompson, David R., Mattmann, Chris A., Wagstaff, Kiri, Lazio, Joseph, and Jones, Dayton, E-mail: andrew.f.hart@jpl.nasa.gov. A framework for collaborative review of candidate events in high data rate streams: The V-FASTR experiment as a case study. United States: N. p., 2015. Web. doi:10.1088/0004-6256/149/1/23.
Hart, Andrew F., Cinquini, Luca, Khudikyan, Shakeh E., Thompson, David R., Mattmann, Chris A., Wagstaff, Kiri, Lazio, Joseph, & Jones, Dayton, E-mail: andrew.f.hart@jpl.nasa.gov. A framework for collaborative review of candidate events in high data rate streams: The V-FASTR experiment as a case study. United States. doi:10.1088/0004-6256/149/1/23.
Hart, Andrew F., Cinquini, Luca, Khudikyan, Shakeh E., Thompson, David R., Mattmann, Chris A., Wagstaff, Kiri, Lazio, Joseph, and Jones, Dayton, E-mail: andrew.f.hart@jpl.nasa.gov. Thu . "A framework for collaborative review of candidate events in high data rate streams: The V-FASTR experiment as a case study". United States. doi:10.1088/0004-6256/149/1/23.
@article{osti_22342164,
title = {A framework for collaborative review of candidate events in high data rate streams: The V-FASTR experiment as a case study},
author = {Hart, Andrew F. and Cinquini, Luca and Khudikyan, Shakeh E. and Thompson, David R. and Mattmann, Chris A. and Wagstaff, Kiri and Lazio, Joseph and Jones, Dayton, E-mail: andrew.f.hart@jpl.nasa.gov},
abstractNote = {“Fast radio transients” are defined here as bright millisecond pulses of radio-frequency energy. These short-duration pulses can be produced by known objects such as pulsars or potentially by more exotic objects such as evaporating black holes. The identification and verification of such an event would be of great scientific value. This is one major goal of the Very Long Baseline Array (VLBA) Fast Transient Experiment (V-FASTR), a software-based detection system installed at the VLBA. V-FASTR uses a “commensal” (piggy-back) approach, analyzing all array data continually during routine VLBA observations and identifying candidate fast transient events. Raw data can be stored from a buffer memory, which enables a comprehensive off-line analysis. This is invaluable for validating the astrophysical origin of any detection. Candidates discovered by the automatic system must be reviewed each day by analysts to identify any promising signals that warrant a more in-depth investigation. To support the timely analysis of fast transient detection candidates by V-FASTR scientists, we have developed a metadata-driven, collaborative candidate review framework. The framework consists of a software pipeline for metadata processing composed of both open source software components and project-specific code written expressly to extract and catalog metadata from the incoming V-FASTR data products, and a web-based data portal that facilitates browsing and inspection of the available metadata for candidate events extracted from the VLBA radio data.},
doi = {10.1088/0004-6256/149/1/23},
journal = {Astronomical Journal (New York, N.Y. Online)},
number = 1,
volume = 149,
place = {United States},
year = {Thu Jan 01 00:00:00 EST 2015},
month = {Thu Jan 01 00:00:00 EST 2015}
}