Parkes observations for project P1066 semester 2020APRS_04
We propose 36 hrs of Parkes observations to continue our successful Deeper, Wider, Faster (DWF) program to detect fast transients and fast radio burst (FRB) counterparts and help resolve their nature. DWF coordinates over 60 observatories worldwide at all wavelengths, from radio to gamma-ray to dete...
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Online Access: | https://dx.doi.org/10.25919/xkrg-9p32 https://data.csiro.au/collections/collection/CIcsiro:47530v1/DItrue |
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ftdatacite:10.25919/xkrg-9p32 2023-05-15T18:22:33+02:00 Parkes observations for project P1066 semester 2020APRS_04 Gupta, Vivek Price, Danny Flynn, Chris Cooke, Jeff Webb, Sara Andreoni, Igor Gajjar, Vishal Siemion, Andrew Zhang, Jielai 2020 https://dx.doi.org/10.25919/xkrg-9p32 https://data.csiro.au/collections/collection/CIcsiro:47530v1/DItrue unknown CSIRO dataset Dataset 2020 ftdatacite https://doi.org/10.25919/xkrg-9p32 2021-11-05T12:55:41Z We propose 36 hrs of Parkes observations to continue our successful Deeper, Wider, Faster (DWF) program to detect fast transients and fast radio burst (FRB) counterparts and help resolve their nature. DWF coordinates over 60 observatories worldwide at all wavelengths, from radio to gamma-ray to detect and follow-up FRBs and other elusive fast (millisecond-to-hours duration) transients. Crucially, we coordinate simultaneous deep, fast-cadenced, wide-field observations at all wavelengths to observe the same field at the same time as Parkes, enabling multi-wavelength detection before, during, and after the radio detection. Little to no multi-wavelength observations to any significant depth have been done on these timescales, leaving this parameter space underexplored. DWF coordinates major facilities such as South Pole Telescope (mm/sub-mm), GROND (infrared), CTIO Dark Energy Camera (optical), Astrosat (UV/X-ray), HXMT (X-ray), HESS (gamma-ray), and Pierre Auger (high-energy). We perform realtime data processing and transient identification at all wavelengths that enables triggering our deep, rapid-response (within minutes) follow up programs for deep spectroscopy and imaging using the world's largest telescopes (e.g., Keck, VLT, Gemini, SALT, ATCA). Dataset South pole DataCite Metadata Store (German National Library of Science and Technology) South Pole Hess ENVELOPE(-65.133,-65.133,-67.200,-67.200) Gemini ENVELOPE(-62.500,-62.500,-66.133,-66.133) |
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DataCite Metadata Store (German National Library of Science and Technology) |
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We propose 36 hrs of Parkes observations to continue our successful Deeper, Wider, Faster (DWF) program to detect fast transients and fast radio burst (FRB) counterparts and help resolve their nature. DWF coordinates over 60 observatories worldwide at all wavelengths, from radio to gamma-ray to detect and follow-up FRBs and other elusive fast (millisecond-to-hours duration) transients. Crucially, we coordinate simultaneous deep, fast-cadenced, wide-field observations at all wavelengths to observe the same field at the same time as Parkes, enabling multi-wavelength detection before, during, and after the radio detection. Little to no multi-wavelength observations to any significant depth have been done on these timescales, leaving this parameter space underexplored. DWF coordinates major facilities such as South Pole Telescope (mm/sub-mm), GROND (infrared), CTIO Dark Energy Camera (optical), Astrosat (UV/X-ray), HXMT (X-ray), HESS (gamma-ray), and Pierre Auger (high-energy). We perform realtime data processing and transient identification at all wavelengths that enables triggering our deep, rapid-response (within minutes) follow up programs for deep spectroscopy and imaging using the world's largest telescopes (e.g., Keck, VLT, Gemini, SALT, ATCA). |
format |
Dataset |
author |
Gupta, Vivek Price, Danny Flynn, Chris Cooke, Jeff Webb, Sara Andreoni, Igor Gajjar, Vishal Siemion, Andrew Zhang, Jielai |
spellingShingle |
Gupta, Vivek Price, Danny Flynn, Chris Cooke, Jeff Webb, Sara Andreoni, Igor Gajjar, Vishal Siemion, Andrew Zhang, Jielai Parkes observations for project P1066 semester 2020APRS_04 |
author_facet |
Gupta, Vivek Price, Danny Flynn, Chris Cooke, Jeff Webb, Sara Andreoni, Igor Gajjar, Vishal Siemion, Andrew Zhang, Jielai |
author_sort |
Gupta, Vivek |
title |
Parkes observations for project P1066 semester 2020APRS_04 |
title_short |
Parkes observations for project P1066 semester 2020APRS_04 |
title_full |
Parkes observations for project P1066 semester 2020APRS_04 |
title_fullStr |
Parkes observations for project P1066 semester 2020APRS_04 |
title_full_unstemmed |
Parkes observations for project P1066 semester 2020APRS_04 |
title_sort |
parkes observations for project p1066 semester 2020aprs_04 |
publisher |
CSIRO |
publishDate |
2020 |
url |
https://dx.doi.org/10.25919/xkrg-9p32 https://data.csiro.au/collections/collection/CIcsiro:47530v1/DItrue |
long_lat |
ENVELOPE(-65.133,-65.133,-67.200,-67.200) ENVELOPE(-62.500,-62.500,-66.133,-66.133) |
geographic |
South Pole Hess Gemini |
geographic_facet |
South Pole Hess Gemini |
genre |
South pole |
genre_facet |
South pole |
op_doi |
https://doi.org/10.25919/xkrg-9p32 |
_version_ |
1766201964481216512 |