G. Clementini
Papers
1
Total Citations
75
H-Index
1
About
G. Clementini is a leading figure in stellar astrophysics, renowned for her transformative work on RR Lyrae variables as precise distance indicators and tracers of stellar populations. Her research centers on the calibration of the cosmic distance ladder, the structure of the Milky Way and its satellites, and the pulsation properties of variable stars. A cornerstone of her impact is the landmark paper "Standard Galactic Field RR Lyrae. I. Optical to Mid-infrared Phased Photometry" (2017, 75 citations), which compiled multi-wavelength light curves for 55 field RR Lyrae variables over up to 30 years, providing an essential reference for calibrating period-luminosity relations from optical to mid-infrared bands. This work, alongside her contributions to the VISTA Variables in the Via Lactea (VVV) survey and Gaia mission data validation, has significantly refined our understanding of Galactic structure and the absolute magnitude of RR Lyrae stars. Her efforts have been instrumental in establishing robust, extinction-free distance measurements, cementing her legacy as a key architect of modern stellar population and distance scale studies.
Research Focus
Key Achievements
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