Graph explorer

Sky Surveys

Sky surveys represent a fundamental data basis for astronomy. We use them to map in a systematic way the universe and its constituents, and to discover new types of objects or phenomena. We review the subject, with an emphasis on the wide-field imaging surveys, placing them in a broader scientific and historical context. Surveys are the largest data generators in astronomy, propelled by the advances in information and computation technology, and have transformed the ways in which astronomy is done. We describe the variety and the general properties of surveys, the ways in which they may be quantified and compared, and offer some figures of merit that can be used to compare their scientific discovery potential. Surveys enable a very wide range of science; that is perhaps their key unifying characteristic. As new domains of the observable parameter space open up thanks to the advances in technology, surveys are often the initial step in their exploration. Science can be done with the survey data alone or a combination of different surveys, or with a targeted follow-up of potentially interesting selected sources. Surveys can be used to generate large, statistical samples of objects th

8 nodes7 linksoverview mapSky Surveys
8 nodes7 links
Sky Surveys8 visible / 8 total nodes / 17 links
Co-authorshipCo-authorshipCo-authorshipCo-authorshipCo-authorshipCo-authorshipCo-authorshipCo-authorshipCo-authorshipCo-authorshipAuthorshipAuthorshipAuthorshipAuthorshipTopic signalTopic signalAuthorshipWSky Surveyspreprint / 2012AS. G. DjorgovskiResearcherAA. A. MahabalResearcherAA. J. DrakeResearcherAM. J. GrahamResearcherTastro-ph.IM4506 worksTphysics.data-an1229 worksAC. DonalekResearcher
PaperSignal 107 links

Sky Surveys

preprint / 2012

Open