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Cited article:

How to distinguish a nearly flat Universe from a flat Universe using the orientation independence of a comoving standard ruler

B. F. Roukema

A&A, 369 3 (2001) 729-735

Published online: 2001-04-15

DOI: https://doi.org/10.1051/0004-6361:20010174

This article has been cited by the following article(s):

Using the large scale quasar clustering to constrain flat quintessential universes

A. Zandivarez and H. J. Martínez
Astronomy & Astrophysics 498 (2) 347 (2009)
DOI: 10.1051/0004-6361/200811360
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Constraints on $(\Omega_\mathsf{m},\Omega_\Lambda)$ using distributions of inclination angles for high redshift filaments

M. Weidinger, P. Møller, J. P. U. Fynbo, B. Thomsen and M. P. Egholm
Astronomy & Astrophysics 391 (1) 13 (2002)
DOI: 10.1051/0004-6361:20020792
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