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://researchdata.edu.au/parkes-observations-project-semester-2020aprs04/1668570 https://doi.org/10.25919/xkrg-9p32 |
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ftands:oai:ands.org.au::1668570 2023-05-15T18:22:43+02:00 Parkes observations for project P1066 semester 2020APRS_04 CSIRO (hasAssociationWith) CSIRO (isManagedBy) Vivek Gupta (hasPrincipalInvestigator) Temporal: From 2020-04-01 to 2020-09-30 https://researchdata.edu.au/parkes-observations-project-semester-2020aprs04/1668570 https://doi.org/10.25919/xkrg-9p32 unknown Commonwealth Scientific and Industrial Research Organisation https://researchdata.edu.au/parkes-observations-project-semester-2020aprs04/1668570 102.100.100/386857 doi:10.25919/xkrg-9p32 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/xkrg-9p32 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) Gemini ENVELOPE(-62.500,-62.500,-66.133,-66.133) Hess ENVELOPE(-65.133,-65.133,-67.200,-67.200) South Pole |
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_04 |
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) Vivek Gupta (hasPrincipalInvestigator) |
format |
Dataset |
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 |
Commonwealth Scientific and Industrial Research Organisation |
url |
https://researchdata.edu.au/parkes-observations-project-semester-2020aprs04/1668570 https://doi.org/10.25919/xkrg-9p32 |
op_coverage |
Temporal: From 2020-04-01 to 2020-09-30 |
long_lat |
ENVELOPE(-62.500,-62.500,-66.133,-66.133) ENVELOPE(-65.133,-65.133,-67.200,-67.200) |
geographic |
Gemini Hess South Pole |
geographic_facet |
Gemini Hess South Pole |
genre |
South pole |
genre_facet |
South pole |
op_source |
https://data.csiro.au/dap/ |
op_relation |
https://researchdata.edu.au/parkes-observations-project-semester-2020aprs04/1668570 102.100.100/386857 doi:10.25919/xkrg-9p32 |
op_doi |
https://doi.org/10.25919/xkrg-9p32 |
_version_ |
1766202134063218688 |