Parkes observations for project P1066 semester 2021APRS_25

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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Format: Dataset
Language:unknown
Published: Commonwealth Scientific and Industrial Research Organisation
Subjects:
Online Access:https://doi.org/10.25919/x2wy-yr47
https://researchdata.edu.au/parkes-observations-project-semester-2021aprs25/1769913
https://data.csiro.au/collection/csiro:52472
http://hdl.handle.net/102.100.100/429801?index=1
id ftands:oai:ands.org.au::1769913
record_format openpolar
spelling ftands:oai:ands.org.au::1769913 2024-09-09T20:09:07+00:00 Parkes observations for project P1066 semester 2021APRS_25 Temporal: From 2021-04-01 to 2021-09-30 https://doi.org/10.25919/x2wy-yr47 https://researchdata.edu.au/parkes-observations-project-semester-2021aprs25/1769913 https://data.csiro.au/collection/csiro:52472 http://hdl.handle.net/102.100.100/429801?index=1 unknown Commonwealth Scientific and Industrial Research Organisation https://researchdata.edu.au/parkes-observations-project-semester-2021aprs25/1769913 https://data.csiro.au/collection/csiro:52472 http://hdl.handle.net/102.100.100/429801?index=1 https://doi.org/10.25919/x2wy-yr47 Commonwealth Scientific and Industrial Research Organisation transients Astronomical sciences not elsewhere classified Astronomical sciences PHYSICAL SCIENCES dataset ftands https://doi.org/10.25919/x2wy-yr47 2024-08-13T00:21:48Z 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 sciences not elsewhere classified
Astronomical sciences
PHYSICAL SCIENCES
spellingShingle transients
Astronomical sciences not elsewhere classified
Astronomical sciences
PHYSICAL SCIENCES
Parkes observations for project P1066 semester 2021APRS_25
topic_facet transients
Astronomical sciences not elsewhere classified
Astronomical sciences
PHYSICAL 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).
format Dataset
title Parkes observations for project P1066 semester 2021APRS_25
title_short Parkes observations for project P1066 semester 2021APRS_25
title_full Parkes observations for project P1066 semester 2021APRS_25
title_fullStr Parkes observations for project P1066 semester 2021APRS_25
title_full_unstemmed Parkes observations for project P1066 semester 2021APRS_25
title_sort parkes observations for project p1066 semester 2021aprs_25
publisher Commonwealth Scientific and Industrial Research Organisation
url https://doi.org/10.25919/x2wy-yr47
https://researchdata.edu.au/parkes-observations-project-semester-2021aprs25/1769913
https://data.csiro.au/collection/csiro:52472
http://hdl.handle.net/102.100.100/429801?index=1
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 Commonwealth Scientific and Industrial Research Organisation
op_relation https://researchdata.edu.au/parkes-observations-project-semester-2021aprs25/1769913
https://data.csiro.au/collection/csiro:52472
http://hdl.handle.net/102.100.100/429801?index=1
https://doi.org/10.25919/x2wy-yr47
op_doi https://doi.org/10.25919/x2wy-yr47
_version_ 1809943243662557184