Parkes observations for project P1066 semester 2020APRS_02
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://researchdata.edu.au/parkes-observations-project-semester-2020aprs02/1670625 https://doi.org/10.25919/ezqk-3s44 |
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ftands:oai:ands.org.au::1670625 2023-05-15T18:22:43+02:00 Parkes observations for project P1066 semester 2020APRS_02 CSIRO (hasAssociationWith) CSIRO (isManagedBy) Temporal: From 2020-04-01 to 2020-09-30 https://researchdata.edu.au/parkes-observations-project-semester-2020aprs02/1670625 https://doi.org/10.25919/ezqk-3s44 unknown Commonwealth Scientific and Industrial Research Organisation https://researchdata.edu.au/parkes-observations-project-semester-2020aprs02/1670625 102.100.100/386856 doi:10.25919/ezqk-3s44 https://data.csiro.au/dap/ transients pulsar BPSR P1066_2020APRS Astronomical and Space Sciences not elsewhere classified PHYSICAL SCIENCES ASTRONOMICAL AND SPACE SCIENCES dataset ftands https://doi.org/10.25919/ezqk-3s44 2022-12-19T23:57:00Z 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 Research Data Australia (Australian National Data Service - ANDS) South Pole Hess ENVELOPE(-65.133,-65.133,-67.200,-67.200) Gemini ENVELOPE(-62.500,-62.500,-66.133,-66.133) |
institution |
Open Polar |
collection |
Research Data Australia (Australian National Data Service - ANDS) |
op_collection_id |
ftands |
language |
unknown |
topic |
transients pulsar BPSR P1066_2020APRS Astronomical and Space Sciences not elsewhere classified PHYSICAL SCIENCES ASTRONOMICAL AND SPACE SCIENCES |
spellingShingle |
transients pulsar BPSR P1066_2020APRS Astronomical and Space Sciences not elsewhere classified PHYSICAL SCIENCES ASTRONOMICAL AND SPACE SCIENCES Parkes observations for project P1066 semester 2020APRS_02 |
topic_facet |
transients pulsar BPSR P1066_2020APRS Astronomical and Space Sciences not elsewhere classified PHYSICAL SCIENCES ASTRONOMICAL AND SPACE SCIENCES |
description |
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). |
author2 |
CSIRO (hasAssociationWith) CSIRO (isManagedBy) |
format |
Dataset |
title |
Parkes observations for project P1066 semester 2020APRS_02 |
title_short |
Parkes observations for project P1066 semester 2020APRS_02 |
title_full |
Parkes observations for project P1066 semester 2020APRS_02 |
title_fullStr |
Parkes observations for project P1066 semester 2020APRS_02 |
title_full_unstemmed |
Parkes observations for project P1066 semester 2020APRS_02 |
title_sort |
parkes observations for project p1066 semester 2020aprs_02 |
publisher |
Commonwealth Scientific and Industrial Research Organisation |
url |
https://researchdata.edu.au/parkes-observations-project-semester-2020aprs02/1670625 https://doi.org/10.25919/ezqk-3s44 |
op_coverage |
Temporal: From 2020-04-01 to 2020-09-30 |
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_source |
https://data.csiro.au/dap/ |
op_relation |
https://researchdata.edu.au/parkes-observations-project-semester-2020aprs02/1670625 102.100.100/386856 doi:10.25919/ezqk-3s44 |
op_doi |
https://doi.org/10.25919/ezqk-3s44 |
_version_ |
1766202134809804800 |