Looking down the light cone: Can deep redshift surveys alone measure the power spectrum?

Monthly Notices of the Royal Astronomical Society

Volumn 299, Issue 4, 1998, Pages 977-984

  De Laix, Andrew A ^a   Starkman, Glenn D ^b  

^a WOLFRAM RESEARCH INC   (United States)

^b CASE WESTERN RESERVE UNIVERSITY   (United States)

Author keywords

Cosmology: observations; Large scale structure of Universe; Surveys

Indexed keywords

COSMOLOGY; HARMONIC ANALYSIS; HARMONIC FUNCTIONS; RED SHIFT; SURVEYS;

ALL-SKY; CONE EFFECTS; COSMOLOGICAL PARAMETERS; COSMOLOGY OBSERVATIONS; HARMONIC MODES; LARGE SCALE STRUCTURE OF UNIVERSE; POWER-SPECTRA; RED SHIFT; SPHERICAL HARMONICS; WINDOW FUNCTIONS;

POWER SPECTRUM;

EID: 0000181449     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.1998.01833.x     Document Type: Review

References (8)

1. Fry J., 1996, ApJ, 461, L5
2. Gunn J. E., Weinberg D. H., 1995, in Maddox S. J., Aragón-Salamanca A., eds, World Scientific, Singapore
3. Heavens A. F., Taylor A. N., 1995, MNRAS, 275, 483
4. Nakamura T. T., Matsubara T., Suto Y., 1998, ApJ, 494, 13
5. Peebles P. J. E., 1980, The Large Scale Structure of the Universe. Princeton Univ. Press, Princeton
6. Strauss M. A., 1997, in Turok N., ed., Critical Dialogs in Cosmology. World Scientific, Singapore
7. Taylor K., Gray P. M., 1994, in Crawford D. L., Craine E. R., eds, Instrumentation in Astronomy VIII. Proc. SPIE 2198, 136
8. Tegmark M., 1995, ApJ, 455, 429