Interferometry And Synthesis In Radio Astronomy

  title={Interferometry And Synthesis In Radio Astronomy},
  author={Stephanie Thalberg},
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Introduction to the Techniques of Interferometry and Lunar Occultation in Radio Astronomy
Radio telescopes allow a 24 × 7 observation time window of those regions of the space which appear dark in the visible region. But, the major problem with a single radio telescope is its poor
Statistical inference in radio astronomy
This thesis unifies several studies, which all are dedicated to the subject of statistical data analysis in radio astronomy and radio astrophysics. Radio astronomy, like astronomy as a whole, has
Low-dimensional data embedding for scalable astronomical imaging in the SKA telescope era
Fast and robust dimensionality reduction methods that embed data to very low sizes while preserving information present in the original data are proposed in the context of compressed sensing theory and related signal recovery techniques and are shown to have quality comparable to those obtained from full data without any reduction.
Planetary Radio Interferometry and Doppler Experiment (PRIDE) for radio occultation studies : A Venus Express test case
The thesis that you are about to read deals with the implementation of a technique to study atmospheres of planets or moons in the Solar System. We use radio telescopes on Earth to track spacecraft
Radio astronomy image reconstruction in the Big Data era
It is shown that PURIFY’s methods provide higher dynamic range than traditional image reconstruction methods, providing a more accurate and detailed sky model for real observations, and sets the stage for state-of-the-art image Reconstruction methods to be distributed and applied to next generation interferometric telescopes.
Frequency smearing in full 3D interferometry
Radio astronomy below 30 MHz has never been properly performed because the ionosphere inhibits this on Earth. In order to properly map the sky at these frequencies, the only financially feasible
Sparse Image Reconstruction for the SPIDER Optical Interferometric Telescope
Algorithms from radio interferometric imaging and sparse image reconstruction are described and their application to the SPIDER concept telescope is demonstrated through simulated observation and reconstruction of the optical sky.
Far-infrared intensity interferometry for high angular resolution imaging
  • H. Matsuo
  • Physics
    Astronomical Telescopes + Instrumentation
  • 2020
High angular resolution astronomical observation in far-infrared better than one milli-arcsecond will open a new field of astronomy, such as imaging inner region of protoplanetary disk and broad line
The Measurement of Polarization in Radio Astronomy
The measurement and calibration process for polarization observations is described and how instrumental polarization can affect a measurement is illustrated to draw attention to the confusion generated by various polarization conventions.
IRASSI: InfraRed astronomy satellite swarm interferometry — Mission concept and description
A current focus of modern astronomy is the characterization of the physical properties and of the chemical processes which can lead to prebiotic conditions in Earth-like planets. In order to identify