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 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...
Determining the population of Cataclysmic Variables in the Globular Cluster NGC2808
Close binaries, and in particular cataclysmic variables (CVs), play a vital role in the dynamical evolution of globular clusters. It is, therefore, important to...