Submillimetre Common-User Bolometer Array

Target entity: Submillimetre Common-User Bolometer Array
Context triple: [SCUBA, fullName, Submillimetre Common-User Bolometer Array]

• A. Submillimeter Array
  The Submillimeter Array is a radio interferometer of eight 6-meter telescopes that observes the universe at submillimeter wavelengths, enabling high-resolution studies of cold gas, dust, and star-forming regions in space.
• B. Heterodyne Instrument for the Far Infrared
  The Heterodyne Instrument for the Far Infrared (HIFI) is a high-resolution spectrometer aboard the Herschel Space Observatory designed to study the chemical composition and physical conditions of interstellar gas and dust in the far-infrared and submillimeter range.
• C. Caltech Submillimeter Observatory
  The Caltech Submillimeter Observatory was a pioneering radio telescope facility specializing in submillimeter-wavelength astronomy, contributing significantly to the study of cold dust, gas, and star formation in the universe.
• D. SPT-SZ camera
  The SPT-SZ camera is a millimeter-wave imaging instrument designed to survey the cosmic microwave background and detect galaxy clusters via the Sunyaev–Zel’dovich effect.
• E. Cooled Mid-Infrared Camera and Spectrometer
  The Cooled Mid-Infrared Camera and Spectrometer (COMICS) is an astronomical instrument designed for high-sensitivity imaging and spectroscopy in the mid-infrared wavelength range, typically used on large ground-based telescopes to study dust, gas, and thermal emission in various celestial objects.
• F. None of above. chosen
• G. Unsure - the case is ambiguous/there is not enough information to decide.

Target entity: Submillimetre Common-User Bolometer Array
Target entity description: Submillimetre Common-User Bolometer Array is a highly sensitive submillimetre-wavelength camera used on the James Clerk Maxwell Telescope to observe cold dust and gas in the universe.

• A. Submillimeter Array
  The Submillimeter Array is a radio interferometer of eight 6-meter telescopes that observes the universe at submillimeter wavelengths, enabling high-resolution studies of cold gas, dust, and star-forming regions in space.
• B. Heterodyne Instrument for the Far Infrared
  The Heterodyne Instrument for the Far Infrared (HIFI) is a high-resolution spectrometer aboard the Herschel Space Observatory designed to study the chemical composition and physical conditions of interstellar gas and dust in the far-infrared and submillimeter range.
• C. Caltech Submillimeter Observatory
  The Caltech Submillimeter Observatory was a pioneering radio telescope facility specializing in submillimeter-wavelength astronomy, contributing significantly to the study of cold dust, gas, and star formation in the universe.
• D. SPT-SZ camera
  The SPT-SZ camera is a millimeter-wave imaging instrument designed to survey the cosmic microwave background and detect galaxy clusters via the Sunyaev–Zel’dovich effect.
• E. Cooled Mid-Infrared Camera and Spectrometer
  The Cooled Mid-Infrared Camera and Spectrometer (COMICS) is an astronomical instrument designed for high-sensitivity imaging and spectroscopy in the mid-infrared wavelength range, typically used on large ground-based telescopes to study dust, gas, and thermal emission in various celestial objects.
• F. None of above. chosen