Determination of rotation periods of M stars with photometric techniques
This work is part of the project CARMENES (Calar Alto search for high-Resolution M dwarfs With Exoearths With Near-infrared and optical Echelle spectrographs)...
Determination of SPI coded mask transmission matrix
The goal of this paper is to present the Transmission Matrix of the SPI Mask STM/QM Model. The experimental set-up used to determine INTEGRAL Spectrometer (SPI)...
Determination of the near-UV absorption in the spectra of primitive asteroids
C-complex asteroids are dark, low-albedo objects, mainly containing carbon components. Their spectra are usually featureless, especially in the visible-near...
Determination of Time Dependence in the Temperature Structure of Ionized Interstellar Gas
It is well known that the temperature structure of ionized interstellar gas departs considerably from homogeneity. This is detected in the form of ``temperature...
Determining Magnesium and Silicon Abundances from CARMENES Spectra
The study of chemical abundances of stars that host planets is critical to our current un- derstanding of the structure, formation, evolution of rocky planets...
Determining the Local Black Hole Mass Function from the Pitch Angles of Nearby Spiral Galaxies
We present pitch angle measurements of a nearly complete sample of nearby spiral galaxies. Using these results along with the relationship between supermassive...