White dwarf masses can be determined in several ways. Here we compare masses obtained from Balmer line spectroscopy with those derived from trigonometric...
Comparisons between Observed and Computed Visible and Near-UV Spectra of Vega
By using the Synspec program with different LTE and NLTE atmospheric models of Alpha Lyrae (Vega, spectral type A0V), we obtain different emitted fluxes. Taking...
Complemetary Observations for the CoRoT Exoplanet Program
We review the needs of the CoRoT /exoplanet program in terms of complementary observations. Such observations are indeed an essential element of the science of...
The extraction of resonance parameters from meson photo-reaction data is a challenging effort, that would greatly benefit from the availability of several...
Completing Gemini-South Optical Imaging of ALMA Lensed SMGs Discovered by Herschel
We propose to complete our program of optical imaging of a sample of candidate strong-lensing galaxies discovered in the Herschel Multi-tiered Extragalactic...
Completing the puzzle: AOLI full-commissioning fresh results and AIV innovations
The Adaptive Optics Lucky Imager (AOLI) is a new instrument designed to combine adaptive optics (AO) and lucky imaging (LI) techniques to deliver high spatial...
Complex poles and oscillatory screened potential in QED plasmas
We discuss the mechanism for the oscillatory behavior of the static interparticle potential in a degenerate electron plasma. This behavior, observed in metallic...
Complexity of chaotic fields and standard model parameters
In order to understand the parameters of the standard model of electroweak and strong interactions (coupling constants, masses, mixing angles) one needs to...