Parkes observations for project P1066 semester 2020APRS_03
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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| Language: | unknown |
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Commonwealth Scientific and Industrial Research Organisation
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| Online Access: | https://doi.org/10.25919/hk7c-3235 https://researchdata.edu.au/parkes-observations-project-semester-2020aprs03/1670229 https://data.csiro.au/collection/csiro:47529 http://hdl.handle.net/102.100.100/386855?index=1 |
| Summary: | 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. \r\n\r\nDWF 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). |
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