Research Areas - (3) Wide-Field Survey Telescope Precision Photometric Calibration (Rubin Observatory / LSST)

Full path: Astronomy / Astrophysics > Astronomical Instrumentation > Optical / IR Astronomical Instrumentation > Wide-Field Survey Telescope Precision Photometric Calibration (Rubin Observatory / LSST)

Department(s)/lab(s): Physics & Astronomy | Munnerlyn Astronomical Instrumentation Laboratory @ TAMU
Summary:

DePoy heads the Munnerlyn Astronomical Instrumentation Lab, building high-throughput spectrographs and precision photometric-calibration systems (DECam/DECal for the Dark Energy Survey, VIRUS for HETDEX, GMACS for the Giant Magellan Telescope). A strong astronomy pivot where detector/spectrograph sensitivity is the enabling technology.

Department(s)/lab(s): Physics, Astronomy | Stubbs Group @ Harvard
Summary:

Stubbs was the inaugural project scientist for the Vera C. Rubin Observatory/LSST and works on precision photometric calibration (e.g. tunable collimated beam projectors) for its 3200-megapixel wide-field survey camera, alongside dark-matter/dark-energy searches and tests of gravitation. Included as a borderline, not-preferred astronomy-instrumentation case: the camera/calibration technology is complex and cutting-edge but is CCD-based rather than a quantum sensor per se.