Exploring the Dynamic Radio Sky: The Search for Slow Transients with the VLA

While synoptic surveys in the optical and at high energies have revealed a rich discovery phase space of slow transients, a similar yield is still awaited in the radio. Majority of the past blind surveys, carried out with radio interferometers, have suffered from a low yield of slow transients, ambi...

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Main Author: Mooley, Kunal Prakash
Format: Others
Published: 2015
Online Access:https://thesis.library.caltech.edu/8800/1/KunalMooley_25Feb2015_Thesis.pdf
Mooley, Kunal Prakash (2015) Exploring the Dynamic Radio Sky: The Search for Slow Transients with the VLA. Dissertation (Ph.D.), California Institute of Technology. doi:10.7907/Z9PC309C. https://resolver.caltech.edu/CaltechTHESIS:03222015-185636984 <https://resolver.caltech.edu/CaltechTHESIS:03222015-185636984>
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spelling ndltd-CALTECH-oai-thesis.library.caltech.edu-88002019-10-05T03:03:30Z Exploring the Dynamic Radio Sky: The Search for Slow Transients with the VLA Mooley, Kunal Prakash While synoptic surveys in the optical and at high energies have revealed a rich discovery phase space of slow transients, a similar yield is still awaited in the radio. Majority of the past blind surveys, carried out with radio interferometers, have suffered from a low yield of slow transients, ambiguous transient classifications, and contamination by false positives. The newly-refurbished Karl G. Jansky Array (Jansky VLA) offers wider bandwidths for accurate RFI excision as well as substantially-improved sensitivity and survey speed compared with the old VLA. The Jansky VLA thus eliminates the pitfalls of interferometric transient search by facilitating sensitive, wide-field, and near-real-time radio surveys and enabling a systematic exploration of the dynamic radio sky. This thesis aims at carrying out blind Jansky VLA surveys for characterizing the radio variable and transient sources at frequencies of a few GHz and on timescales between days and years. Through joint radio and optical surveys, the thesis addresses outstanding questions pertaining to the rates of slow radio transients (e.g. radio supernovae, tidal disruption events, binary neutron star mergers, stellar flares, etc.), the false-positive foreground relevant for the radio and optical counterpart searches of gravitational wave sources, and the beaming factor of gamma-ray bursts. The need for rapid processing of the Jansky VLA data and near-real-time radio transient search has enabled the development of state-of-the-art software infrastructure. This thesis has successfully demonstrated the Jansky VLA as a powerful transient search instrument, and it serves as a pathfinder for the transient surveys planned for the SKA-mid pathfinder facilities, viz. ASKAP, MeerKAT, and WSRT/Apertif. 2015 Thesis NonPeerReviewed application/pdf https://thesis.library.caltech.edu/8800/1/KunalMooley_25Feb2015_Thesis.pdf https://resolver.caltech.edu/CaltechTHESIS:03222015-185636984 Mooley, Kunal Prakash (2015) Exploring the Dynamic Radio Sky: The Search for Slow Transients with the VLA. Dissertation (Ph.D.), California Institute of Technology. doi:10.7907/Z9PC309C. https://resolver.caltech.edu/CaltechTHESIS:03222015-185636984 <https://resolver.caltech.edu/CaltechTHESIS:03222015-185636984> https://thesis.library.caltech.edu/8800/
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description While synoptic surveys in the optical and at high energies have revealed a rich discovery phase space of slow transients, a similar yield is still awaited in the radio. Majority of the past blind surveys, carried out with radio interferometers, have suffered from a low yield of slow transients, ambiguous transient classifications, and contamination by false positives. The newly-refurbished Karl G. Jansky Array (Jansky VLA) offers wider bandwidths for accurate RFI excision as well as substantially-improved sensitivity and survey speed compared with the old VLA. The Jansky VLA thus eliminates the pitfalls of interferometric transient search by facilitating sensitive, wide-field, and near-real-time radio surveys and enabling a systematic exploration of the dynamic radio sky. This thesis aims at carrying out blind Jansky VLA surveys for characterizing the radio variable and transient sources at frequencies of a few GHz and on timescales between days and years. Through joint radio and optical surveys, the thesis addresses outstanding questions pertaining to the rates of slow radio transients (e.g. radio supernovae, tidal disruption events, binary neutron star mergers, stellar flares, etc.), the false-positive foreground relevant for the radio and optical counterpart searches of gravitational wave sources, and the beaming factor of gamma-ray bursts. The need for rapid processing of the Jansky VLA data and near-real-time radio transient search has enabled the development of state-of-the-art software infrastructure. This thesis has successfully demonstrated the Jansky VLA as a powerful transient search instrument, and it serves as a pathfinder for the transient surveys planned for the SKA-mid pathfinder facilities, viz. ASKAP, MeerKAT, and WSRT/Apertif.
author Mooley, Kunal Prakash
spellingShingle Mooley, Kunal Prakash
Exploring the Dynamic Radio Sky: The Search for Slow Transients with the VLA
author_facet Mooley, Kunal Prakash
author_sort Mooley, Kunal Prakash
title Exploring the Dynamic Radio Sky: The Search for Slow Transients with the VLA
title_short Exploring the Dynamic Radio Sky: The Search for Slow Transients with the VLA
title_full Exploring the Dynamic Radio Sky: The Search for Slow Transients with the VLA
title_fullStr Exploring the Dynamic Radio Sky: The Search for Slow Transients with the VLA
title_full_unstemmed Exploring the Dynamic Radio Sky: The Search for Slow Transients with the VLA
title_sort exploring the dynamic radio sky: the search for slow transients with the vla
publishDate 2015
url https://thesis.library.caltech.edu/8800/1/KunalMooley_25Feb2015_Thesis.pdf
Mooley, Kunal Prakash (2015) Exploring the Dynamic Radio Sky: The Search for Slow Transients with the VLA. Dissertation (Ph.D.), California Institute of Technology. doi:10.7907/Z9PC309C. https://resolver.caltech.edu/CaltechTHESIS:03222015-185636984 <https://resolver.caltech.edu/CaltechTHESIS:03222015-185636984>
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