Question

Answer the following about the Square Kilometer Array, or SKA (“S-K-A”), an ambitious international project to build a radio telescope, for 10 points each.
[10m] The SKA will use this spectral feature to study the cosmic dark ages and the epoch of reionization. This spectral feature is created by a transition between hyperfine levels of the 1s (“one-S”) ground state.
ANSWER: 21-centimeter line [or 21 cm line; accept neutral hydrogen line or H I line (“H-one line”); prompt on hydrogen line or H line]
[10e] The SKA will use over 100,000 antennae to meet its requirements for sensitivity and this quantity. This quantity measures the angular distance between objects that a telescope can distinguish.
ANSWER: angular resolution [accept resolving power or minimum resolvable angle]
[10h] Like the Very Large Array, SKA will use this interferometric technique, which is based on the Van Cittert–Zernike (“vahn SIT-ert SAIR-nee-kuh”) theorem. This technique uses an array of paired telescopes to simulate a single telescope with higher resolution.
ANSWER: aperture synthesis [or synthesis imaging or aperture synthesis imaging]
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2024 ACF Nationals2024-04-21Y2410.0063%38%0%

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Claremont CollegesArizona State0000
Chicago CVanderbilt0000
Chicago ACornell A010010
IllinoisGeorgia Tech1010020
KentuckyHarvard0000
Johns HopkinsIowa State1010020
MarylandToronto A0000
Chicago DMinnesota B100010
NYUMichigan100010
North Carolina BCornell B1010020
NorthwesternBrown010010
PennOttawa0000
IndianaPurdue1010020
FloridaRutgers010010
South CarolinaMcGill010010
StanfordMinnesota A010010
TexasColumbia A1010020
DukeToronto B010010
Berkeley BTruman State010010
Yale BVirginia0000
North Carolina AWUSTL A1010020
WUSTL BColumbia B100010
Chicago BWaterloo010010
Yale ABerkeley A010010