Packet 1: Bonus 3

In the presence of an isotropic, unpolarized, stochastic background of these phenomena, pulsar timing arrays have residuals whose correlation follows the Hellings-Downs curve. For 10 points each:
[10m] What phenomena are causing the orbital decay of the Hulse-Taylor binary pulsar?
ANSWER: gravitational waves [or gravitational radiation; or GWs; accept stochastic gravitational wave background or SGWb; prompt on waves; reject “gravity waves”]
[10h] Pulsar timing arrays typically use this class of pulsars due to their stable periods. Pulsars in this class are formed by a “recycling” mechanism in which they are spun up by accretion from a companion star.
ANSWER: millisecond pulsars [accept MSPs]
[10e] In 1992, the first confirmed detection of these objects studied timing variations in the millisecond pulsar Lich. The Kepler space telescope used the transit method to detect these objects.
ANSWER: exoplanets [or extrasolar planets; accept descriptions of planets outside the solar system; prompt on planets]
<LK, Other Science (Astronomy)> | NAFTA-Packet-1

HeardPPBE %M %H %
2616.92100%50%19%

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Summary

TournamentEditionMatchHeardPPBE %M %H %
2026 NAFTA at Stanford01/17/2026417.50100%50%25%
2026 NAFTA at UBC01/17/2026210.00100%0%0%
2025 NAFTA Online02/14/2026425.00100%75%75%
2026 NAFTA at Vanderbilt02/14/2026313.33100%33%0%
2025 NAFTA at Toronto09/13/2025415.00100%50%0%
2025 NAFTA at Maryland09/27/2025518.00100%40%40%
2025 NAFTA at Harvard10/04/2025313.33100%33%0%
2025 NAFTA at Oxford10/11/2025310.00100%0%0%
2025 NAFTA at Chicago11/08/2025620.00100%67%33%
2025 NAFTA at Columbia11/08/2025520.00100%80%20%
2025 NAFTA at Richmond12/20/2025210.00100%0%0%