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Radio Surveys
Published online by Cambridge University Press: 25 May 2016
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Radio surveys have an important role in astronomy, one that has changed with technology and scientific requirements. Most objects studied by radio astronomers today are the unexpected discoveries of early surveys. The survey “discovery” phase began with Jansky's detection of Galactic radio emission and Reber's 160 MHz maps showing that this emission is non-thermal. Surveys made just after World War II revealed strong discrete sources which were later identified with supernova remnants, radio galaxies, and quasars. Pulsars were discovered during a sky survey for scintillating sources. BL Lac objects were recognized in early high-frequency surveys. The first gravitationally lensed quasar appeared in the extensive Jodrell Bank 960 MHz survey, and the first measurement of gravitational radiation came from the binary pulsar serendipidously found in a pulsar survey.
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- Part 1. General Sky Survey Reviews
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- Copyright
- Copyright © Kluwer 1998
References
Becker, R.H., White, R.L., and Helfand, D.J. (1995) The FIRST Survey: Faint Images of the Radio Sky at Twenty Centimeters, Astrophys. J., 450, 559. http://sundog.stsci.edu.CrossRefGoogle Scholar
Blain, A.W., and Longair, M.S. (1996) Observing Strategies for Blank-field Surveys in the Submillimeter Waveband, Mon. Not. R. astron. Soc., 279, 847.CrossRefGoogle Scholar
Condon, J.J. (1989) The 1.4 GHz Luminosity Function and Its Evolution, Astrophys. J., 338, 13.CrossRefGoogle Scholar
Condon, J.J., Anderson, E., and Broderick, J.J. (1995) Radio Identifications of Extra-galactic IRAS Sources, Astron. J., 109, 2318.CrossRefGoogle Scholar
Condon, J.J., Cotton, W.D., Greisen, E.W., Yin, Q.F., Perley, R.A., Taylor, G.B., and Broderick, J.J. (1996) NRAO VLA Sky Survey, http://www.cv.nrao.edu/~jcondon/nvss.html.Google Scholar
Condon, J.J., Frayer, D.T., and Broderick, J.J. (1991) UGC Galaxies Stronger Than 25 mJy at 4.85 GHz, Astron. J., 101, 362.CrossRefGoogle Scholar
de Bruyn, G., Miley, G., Tang, Y., Bremer, M., Brouw, W., Rengelink, R., Bremer, M., and Röttgering, H. (1994) The WENSS Project, Astron NFRA, August, 4-8 and
http://www.strw.leidenuniv.nl/wenss/.Google Scholar
Gregory, P.C., Scott, W.K., Douglas, K., and Condon, J.J. (1996) The GB6 Catalog of Radio Sources, Astrophys. J. Supp., 103, 427. http://www.cv.nrao.edu/~jcondon/gb6ftp.html.CrossRefGoogle Scholar
Gregory, P.C., and Taylor, A.R. (1986) Radio Patrol of the Northern Milky Way, Astron. J., 92, 371.CrossRefGoogle Scholar
Large, M.I., Campbell-Wilson, D., Cram, L.E., Davison, R.G., and Robertson, J.G. (1994) Increasing the Field Size of the Molonglo Observatory Synthesis Telescope, Proc. ASA, 11, 44.Google Scholar
Moshir, M., et al. (1992) Explanatory Supplement to the IRAS Faint Source Survey, Version 2 JPL D-10015 8/92, Jet Propulsion Laboratory, Pasadena.Google Scholar
Normadeau, M., Taylor, A.R., and Dewdney, P.E. (1996) The DRAO Galactic Plane Survey Pilot Project, http://www.ras.ucalgary.ca/pilot_project.html.Google Scholar
Stavely-Smith, L., et al. (1996) The Parkes 21 cm Multibeam Project, http://wwwatnf.atnf.csiro.au/Research/multibeam/multibeam.html.Google Scholar
Wright, A.E., Griffith, M.R., Hunt, A.J., Troup, E., Burke, B.F., and Ekers, R.D. (1996) The Parkes-MIT-NRAO Surveys, Astrophys. J. Supp., 103, 145. http://wwwpks.atnf.csiro.au/databases/surveys/pmn/pmn.html.CrossRefGoogle Scholar
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