Astronomical survey

From Wikipedia, the free encyclopedia

Astronomical surveys generally involve imaging or mapping of regions of the sky using Telescopes. In the past, surveys have been usually restricted to one band of wavelengths of electromagnetic radiation (e.g. light or radio) or to measurements of the flux of one type of particle (e.g. cosmic rays), and they were generally performed as part of the production of an astronomical catalogue for a specific type of astronomical object (like, for example, all the stars brighter than a certain apparent magnitude). Over the last ten years, taking advantage of technological improvements in the construction of telescopes, and following a general expansion in our understanding of astrophysics at all levels, it has become commonplace to conduct surveys that join together many different observations of a given region in the sky, obtained with different telescopes at different wavelengths. This so called multi-wavelength approach is now the new standard for surveys, at least in the fields of Extragalactic astronomy and Observational cosmology.


Contents

[edit] List of sky surveys

  • Radio
  • Planned
    • Pan-STARRS - a proposed 4-telescope large-field survey system to look for transient and variable sources
    • Large Synaptic Survey Telescope - a proposed very large telescope designed to repeatedly survey the whole sky that is visible from its location


[edit] Surveys of the Magellanic Clouds

[edit] Multi-wavelength surveys

Both these surveys are joining together observations obtained from space with the Hubble Space Telescope, the Spitzer Space Telescope, the Chandra X-ray Observatory and the XMM-Newton satellite, with a large set of observations obtained with ground-based telescopes

[edit] Further information

Wikimedia Commons has media related to:
Languages