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Events in this spectral region are characterized by a quantity called the dispersion measure, which had a remarkably high value of 375 for an event named after Duncan Lorimer. In 2006, ARCADE detected noise in this spectral region that was sixfold higher than expected for still-unknown reasons, which has been dubbed a “space roar.” The CHIME telescope has predominantly been used to detect mysterious, extragalactic events in this region lasting milliseconds; those are ■END■
| 2024 ARCADIA at Waterloo | 2024-11-09 | Y | 1 | 100% | 100% | 0% | 70.00 |
| 2024 ARCADIA at Illinois | 2024-11-09 | Y | 1 | 100% | 0% | 0% | 73.00 |
| 2024 ARCADIA at UC Berkeley | 2024-12-06 | Y | 2 | 100% | 50% | 50% | 89.00 |
| 2024 ARCADIA at GT | 2024-12-06 | Y | 4 | 100% | 0% | 50% | 133.50 |
| 2024 ARCADIA at Warwick | 2024-12-06 | Y | 5 | 100% | 0% | 60% | 109.00 |
| Player | Team | Opponent | Buzz Position | Value |
|---|---|---|---|---|
| Swapnil Garg | Berkeley A | Stanford | 45 | 15 |
| Robert Crawley | Warwick A | LSE B | 69 | -5 |
| Liam Kusalik | Waterloo Aspidistra | Waterloo Basic | 70 | 15 |
| Suhit Damani | Innovation Academy B | Lambert | 70 | -5 |
| John Marvin | Chicago A | Illinois Orange | 73 | 10 |
| Shahar Schwartz | Berkeley Past | Berkeley B | 74 | -5 |
| Kevin Flanagan | Bristol | Southampton | 77 | 10 |
| Rachel Bentham | Cambridge B | Imperial A | 78 | -5 |
| Paphon Susikakosol | Imperial A | Cambridge B | 78 | 10 |
| Albert Nyang | LSE A | Warwick B | 81 | -5 |
| Quentin Mot | Georgia Tech B | Georgia Tech C | 89 | -5 |
| Brendan Bethlehem | Cambridge A | Imperial B | 122 | 10 |
| Darren Kellis | Milton | Georgia Tech D | 132 | 10 |
| Anuttam Ramji | Berkeley B | Berkeley Past | 133 | 10 |
| Louis Harney | Georgia Tech C | Georgia Tech B | 134 | 10 |
| Michael Vadakumpaddan | Innovation Academy C | Mississippi State | 134 | 10 |
| Pranav Srambikkal | Lambert | Innovation Academy B | 134 | 10 |
| Adsayan Ganesh | Warwick B | LSE A | 134 | 10 |
| David Worley | LSE B | Warwick A | 134 | 10 |