Las Campanas Redshift Survey

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The Las Campanas Redshift Survey is considered the first attempt to map a large area of the universe out to a redshift of z = 0.2. It was begun in 1991 using the Las Campanas telescope in Chile to catalog 26418 separate galaxies.[1] It is considered one of the first surveys to document the so-called "end of greatness" where the Cosmological Principle of isotropy could be seen. Superclusters[2][3][4][5] and voids are prominent features in the survey.

References[edit]

  1. ^ Las Campanas Redshift Survey web page
  2. ^ Shandarin, Sergei F.;Yess, Capp (1998). "Detection of Network Structure in the Las Campanas Redshift Survey". The Astrophysical Journal 505 (1): 12–17. arXiv:astro-ph/9705155. Bibcode:1998ApJ...505...12S. doi:10.1086/306135. 
  3. ^ Bharadwaj, S.;Gupta, A. K.; Seshadri, T. R. (1999). "Nature of clustering in the Las Campanas redshift survey". Astronomy and Astrophysics 351: 405–412. arXiv:astro-ph/9903252. Bibcode:1999A&A...351..405B. 
  4. ^ Einasto, J.; Einasto, M.; Hütsi, G.; Saar, E.; Tucker, D. L.; Tago, E.; Müller, V.; Heinämäki, P.; Allam, S. S (2003). "Clusters and Superclusters in the Las Campanas Redshift Survey". Astronomy and Astrophysics 410 (2): 425–443. arXiv:astro-ph/0304546. Bibcode:2003A&A...410..425E. doi:10.1051/0004-6361:20031105. 
  5. ^ Bharadwaj, S., Sahni, V., Sathyaprakash, B.S., Shandarin, Sergei F., Yess, Capp (2000). "Evidence for Filamentarity in the Las Campanas Redshift Survey". The Astrophysical Journal 528 (1): 21–29. arXiv:astro-ph/9904406. Bibcode:2000ApJ...528...21B. doi:10.1086/308163.