Astronomical instrumentation can be broadly defined. For the purposes of the Astronova Fellowship and this host institution application, when we refer to "astronomical instrumentation" in this application, this is what we mean:
- The scientific questions to be answered by data from the instrument, once completed (and, if relevant, installed with the other parts in the system), must be related to astronomy/astrophysics, cosmology, or planetary science.
- Instruments must be focused on directing/collecting, detecting, or characterizing photons from astrophysical sources, i.e., electromagnetic radiation from radio waves to gamma rays. Examples of such instruments may include optics, detectors, imagers, spectrometers/spectrographs, astrophotonics, etc. Instruments can be ground-based, airborne, or space-based, including suborbital missions.
- Projects can be at any stage except fully complete and operational by external users. This includes stages such as design, development, fabrication, calibration, testing, and commissioning.
- Instrument-related projects that can potentially be seen as adjacent such as readout software or data pipeline development are allowed, as long as there is a clear link to a specific astronomical instrument.
Projects with the following characteristics are out of scope:
- Instruments most relevant to heliophysics;
- Multimessenger instrument projects such as those focused on gravitational waves, neutrinos, or cosmic rays;
- Laboratory searches for dark matter candidate particles;
- Projects focused on performing observations with an instrument that is already fully operational by external users;
- Elements focused on the optimal functioning of the overall system and more related to engineering (e.g., starshades, navigation control, etc.)