Primitive C-complex asteroids, primarily located in the main asteroid belt, are commonly associated with carbonaceous chondrites (CCs) due to their low...
Compositional Characterization of Cliff-Type Trans-Neptunian Objects
Introduction: Trans-Neptunian Objects (TNOs) harbor materials from the early solar nebula (e.g., Gladman et al. 2008; Tegler et al. 2016). Observations from the...
Compositional Characterization of the Polana-Eulalia Complex with JWST
Determining the distribution of water throughout the main asteroid belt can inform us about the formation and evolution of the early Solar System. A powerful...
Compositional study of asteroids in the Erigone collisional family using visible spectroscopy at the 10.4m GTC
Asteroid families are formed by the fragments produced by the disruption of a common parent body (Bendjoya & Zappalà 2002). Primitive asteroids in the solar...
Compressed sensing for next generation instruments
This document discusses the possibility of using compressed sensing techniques for measuring 2D spectro-polarimetric information using only one etalon and a...
Computed color indices and spectral shapes for individual stars are routinely compared with observations for essentially all spectral types, but absolute fluxes...