My primary research interests are high temporal resolution astrophysics, time-domain sky surveys, astronomical data processing pipelines and transient detection algorithms. I am currently working on the development of automated data analysis pipelines for various time domain sky surveys, and participating in the development of transient detection and characterization infrastructure for upcoming Vera C. Rubin Legacy Survey of Space and Time
(LSST).
As the precise measurements of faint object fluxes require a thorough understanding of detectors used, I am also interested in the characterization of astronomical detectors of various types, from normal and electron-multiplying CCDs to CMOSes and various photon-counting instruments, and my current activities include the establishment of astronomical detector characterization laboratory at Institute of Physics, CAS, and laboratory testing of various cameras for astronomical applications.
I am also supporting the operation and data archive of FRAM telescopes of the Institute of Physics, installed in Chile, Argentina and on La Palma (Spain) and used for both atmospheric characterization of the sites of Pierre Auger and CTA observatories, and for performing various astrophysical tasks.
I work at the Institute of Physics of the Czech Academy of Sciences.
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