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I am seeing lots (1000's to 10,000s) of transients being created in the database which slows the site a lot.
I am concerned that this may be because I am hitting the API regularly, but when I firs…
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Looming on the horizon, and one of the most significant facilities for this decade, is the Rubin Observatory. It is expected to detect ~10 million transients per night and Australia leads a transient …
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In the last decade, both ASKAP and MWA have proven themselves world-leading instruments for transient discovery, due to their wide fields of view, and technical search capabilities. This has been led …
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At ATNF we are researching a new radio aperture-array telescope concept called CASATTTA (Coherent all-sky all-the-time array).
In it's final form (64k elements) it has the sensitivity of Parkes / …
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CTA is the next major step in TeV gamma-ray astronomy. For the first time, CTA will offer sub-arcminute resolution in gamma-ray astronomy and a wide energy coverage (~20 GeV to 300 TeV) overlapping th…
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Incorporating the STEREO/Waves dataset (radio spectra) into Helioviewer would be advantageous as it would enable users to merge solar wind transients with their radio signatures. The calibrated L3 STE…
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Many of the questions that this working group is interested in are underpinned by transient surveys, searching for variability in a given messenger/wavelength on a given timescale. Whether that is sea…
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### Prerequisites
- [X] I have carried out troubleshooting steps and I believe I have found a bug.
- [X] I have searched for similar bugs in both open and closed issues and cannot find a duplicate…
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A significant fraction of what we know about nature and the Universe has been discovered or informed by transients. This question addresses the large amount of work done, and that will be done in the …
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This issue is to gauge interest in an Australian-led 8m-class discovery optical imager with fast spectroscopic follow up for the transient community to be operational near the start of this Decadal Pl…