NASA High Resolution Microwave Survey

Target entity: NASA High Resolution Microwave Survey
Context triple: [Project Phoenix, relatedTo, NASA High Resolution Microwave Survey]

• A. WISE 3-band cryogenic survey
  The WISE 3-band cryogenic survey was a phase of NASA’s Wide-field Infrared Survey Explorer mission that mapped the sky in three infrared bands while the spacecraft’s cryogen was still available, providing key data for later all-sky infrared catalogs.
• B. Multi-frequency Scanning Microwave Radiometer
  The Multi-frequency Scanning Microwave Radiometer is a satellite-borne instrument designed to measure ocean and atmospheric parameters such as sea surface temperature, wind speed, and water vapor using multiple microwave frequency channels.
• C. Arecibo L-band Feed Array survey
  The Arecibo L-band Feed Array survey is a major radio astronomy project that used the Arecibo telescope’s multi-beam receiver to map neutral hydrogen and study the large-scale structure and dynamics of galaxies.
• D. Legacy Archive for Microwave Background Data Analysis
  The Legacy Archive for Microwave Background Data Analysis is a NASA astrophysics data repository dedicated to preserving and providing access to observations and analysis tools related to the cosmic microwave background.
• E. Differential Microwave Radiometers
  Differential Microwave Radiometers are highly sensitive instruments designed to measure tiny temperature fluctuations in the cosmic microwave background radiation across the sky.
• F. None of above. chosen
• G. Unsure - the case is ambiguous/there is not enough information to decide.

Target entity: NASA High Resolution Microwave Survey
Target entity description: The NASA High Resolution Microwave Survey was a space agency program designed to systematically scan the sky at microwave frequencies in search of potential extraterrestrial radio signals.

• A. WISE 3-band cryogenic survey
  The WISE 3-band cryogenic survey was a phase of NASA’s Wide-field Infrared Survey Explorer mission that mapped the sky in three infrared bands while the spacecraft’s cryogen was still available, providing key data for later all-sky infrared catalogs.
• B. Multi-frequency Scanning Microwave Radiometer
  The Multi-frequency Scanning Microwave Radiometer is a satellite-borne instrument designed to measure ocean and atmospheric parameters such as sea surface temperature, wind speed, and water vapor using multiple microwave frequency channels.
• C. Arecibo L-band Feed Array survey
  The Arecibo L-band Feed Array survey is a major radio astronomy project that used the Arecibo telescope’s multi-beam receiver to map neutral hydrogen and study the large-scale structure and dynamics of galaxies.
• D. Legacy Archive for Microwave Background Data Analysis
  The Legacy Archive for Microwave Background Data Analysis is a NASA astrophysics data repository dedicated to preserving and providing access to observations and analysis tools related to the cosmic microwave background.
• E. Differential Microwave Radiometers
  Differential Microwave Radiometers are highly sensitive instruments designed to measure tiny temperature fluctuations in the cosmic microwave background radiation across the sky.
• F. None of above. chosen