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][6][7] and voids are prominent features in the survey.
^"The Las Campanas Redshift Survey". qold.astro.utoronto.ca. Archived from the original on 2012-06-30. Retrieved 2016-12-26.
^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. S2CID 18220980.
^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.
^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. S2CID 14486062.
^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. S2CID 10427122.{{cite journal}}: CS1 maint: multiple names: authors list (link)
^Bharadwaj, Somnath; Bhavsar, Suketu; Sheth, Jatush V. (2004). "The Size of the Longest Filaments in the Universe". The Astrophysical Journal. 606 (1): 25–31. arXiv:astro-ph/0311342. Bibcode:2004ApJ...606...25B. doi:10.1086/382140. ISSN 0004-637X. S2CID 10473973.
^Bharadwaj, Somnath; Pandey, Biswajit (2004). "Using the filaments in the LCRS to test the LambdaCDM model". The Astrophysical Journal. 615 (1): 1–6. arXiv:astro-ph/0405059. doi:10.1086/424476. ISSN 0004-637X.
and 14 Related for: Las Campanas Redshift Survey information
The LasCampanasRedshiftSurvey 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...
billion light years (redshift ~ 0.2). It was the world's largest redshiftsurvey between 1998 (overtaking LasCampanasRedshiftSurvey) and 2003 (overtaken...
and WMAP, and to galaxy redshiftsurveys such as the LasCampanasRedshiftSurvey, the 2dF Survey and the Sloan Digital Sky Survey. With Daniel Eisenstein...
The Sloan Digital Sky Survey or SDSS is a major multi-spectral imaging and spectroscopic redshiftsurvey using a dedicated 2.5-m wide-angle optical telescope...
Shectman and others he participated in the LasCampanasRedshiftSurvey, a pioneering 35,000 galaxy survey using fiber optics and plug plates. Kirshner...
Evolution Survey is a medium-band imaging survey that aims to establish an observational benchmark of galaxy properties at redshift z > 1. The survey uses...
observatories, including Kitt Peak in Arizona, Palomar in California, LasCampanas and Cerro Tololo in Chile, Sutherland in South Africa, and the Special...
discovery. The photometry was obtained on the 1 m Swope Telescope at the LasCampanas Observatory. Observations were acquired twice per night in order to look...
diameter (3.3 ft) Swope Telescope operating in the near infrared at LasCampanas Observatory, Chile. They were also the first to announce it, naming their...
Data obtained in optical light with the Magellan I and II telescopes in LasCampanas, Chile, also provides intriguing information about this object, which...
observations in late 2015, using both of the Magellan instruments at LasCampanas, Chile. These observations included more detailed spectral data and also...
and its optical counterpart SSS17a was detected 11 hours later at the LasCampanas Observatory. Further optical observations e.g. by the Hubble Space Telescope...
2017cbv was discovered on 10 March 2017 by the Swope 1-m telescope at LasCampanas Observatory, and was classified as a very young Ia supernova. It increased...
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