Parkes observations for project P1066 semester 2021APRS_31
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 80 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-2021aprs31/1790718 https://doi.org/10.25919/tc2c-by63 |
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ftands:oai:ands.org.au::1790718 2023-05-15T18:22:43+02:00 Parkes observations for project P1066 semester 2021APRS_31 CSIRO (hasAssociationWith) CSIRO (isManagedBy) Vivek Gupta (hasPrincipalInvestigator) Temporal: From 2021-04-01 to 2021-09-30 https://researchdata.edu.au/parkes-observations-project-semester-2021aprs31/1790718 https://doi.org/10.25919/tc2c-by63 unknown Commonwealth Scientific and Industrial Research Organisation https://researchdata.edu.au/parkes-observations-project-semester-2021aprs31/1790718 102.100.100/430578 doi:10.25919/tc2c-by63 https://data.csiro.au/dap/ transients Astronomical and Space Sciences not elsewhere classified PHYSICAL SCIENCES ASTRONOMICAL AND SPACE SCIENCES dataset ftands https://doi.org/10.25919/tc2c-by63 2022-12-20T00:04:52Z 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 80 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 to observe with Parkes, 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 Astronomical and Space Sciences not elsewhere classified PHYSICAL SCIENCES ASTRONOMICAL AND SPACE SCIENCES |
spellingShingle |
transients Astronomical and Space Sciences not elsewhere classified PHYSICAL SCIENCES ASTRONOMICAL AND SPACE SCIENCES Parkes observations for project P1066 semester 2021APRS_31 |
topic_facet |
transients 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 80 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 to observe with Parkes, 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 2021APRS_31 |
title_short |
Parkes observations for project P1066 semester 2021APRS_31 |
title_full |
Parkes observations for project P1066 semester 2021APRS_31 |
title_fullStr |
Parkes observations for project P1066 semester 2021APRS_31 |
title_full_unstemmed |
Parkes observations for project P1066 semester 2021APRS_31 |
title_sort |
parkes observations for project p1066 semester 2021aprs_31 |
publisher |
Commonwealth Scientific and Industrial Research Organisation |
url |
https://researchdata.edu.au/parkes-observations-project-semester-2021aprs31/1790718 https://doi.org/10.25919/tc2c-by63 |
op_coverage |
Temporal: From 2021-04-01 to 2021-09-30 |
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-2021aprs31/1790718 102.100.100/430578 doi:10.25919/tc2c-by63 |
op_doi |
https://doi.org/10.25919/tc2c-by63 |
_version_ |
1766202141134815232 |