Showing 101 - 120 results of 291 for search '"redshift survey"', query time: 0.32s Refine Results
  1. 101

    A measurement of the cosmological mass density from clustering in the 2dF Galaxy Redshift Survey. by Peacock, J, Cole, S, Norberg, P, Baugh, C, Bland-Hawthorn, J, Bridges, T, Cannon, R, Colless, M, Collins, C, Couch, W, Dalton, G, Deeley, K, De Propris, R, Driver, S, Efstathiou, G, Ellis, R, Frenk, C, Glazebrook, K, Jackson, C, Lahav, O, Lewis, I, Lumsden, S, Maddox, S, Percival, W, Peterson, B

    Published 2001
    “…Here we report a precise measurement of this clustering, using the redshifts of more than 141,000 galaxies from the two-degree-field (2dF) galaxy redshift survey. We determine the parameter beta = Omega0.6/b = 0.43 +/- 0.07, where Omega is the total mass-density parameter of the Universe and b is a measure of the 'bias' of the luminous galaxies in the survey. …”
    Journal article
  2. 102

    The 2dF galaxy redshift survey: Constraints on cosmic star formation history from the cosmic spectrum by Baldry, I, Glazebrook, K, Baugh, C, Bland-Hawthorn, J, Bridges, T, Cannon, R, Cole, S, Colless, M, Collins, C, Couch, W, Dalton, G, De Propris, R, Driver, S, Efstathiou, G, Ellis, R, Frenk, C, Hawkins, E, Jackson, C, Lahav, O, Lewis, I, Lumsden, S, Maddox, S, Madgwick, D, Norberg, P, Peacock, J

    Published 2002
    “…We present the first results on the history of star formation in the universe based on the "cosmic spectrum," in particular the volume-averaged, luminosity-weighted, stellar absorption-line spectrum of present-day galaxies from the 2dF Galaxy Redshift Survey. This method is novel in that, unlike previous studies, it is not an estimator based on total luminosity density. …”
    Journal article
  3. 103
  4. 104

    The 2dF QSO Redshift Survey - XIV. Structure and evolution from the two-point correlation function by Croom, S, Boyle, B, Shanks, T, Smith, R, Miller, L, Outram, P, Loaring, N, Hoyle, F, Angela, J

    Published 2004
    “…We present a clustering analysis of QSOs using over 20000 objects from the final catalogue of the 2dF QSO Redshift Survey (2QZ), measuring the z-space correlation function, xi(s). …”
    Journal article
  5. 105
  6. 106
  7. 107

    The 2dF Galaxy Redshift Survey: the nature of the relative bias between galaxies of different spectral type by Conway, E, Maddox, S, Wild, V, Peacock, J, Hawkins, E, Norberg, P, Madgwick, D, Baldry, I, Baugh, C, Hawthorn, J, Bridges, T, Cannon, R, Cole, S, Colless, M, Collins, C, Couch, W, Dalton, G, De Propris, R, Driver, S, Efstathiou, G, Ellis, R, Frenk, C, Glazebrook, K, Jackson, C, Jones, B

    Published 2005
    “…We present an analysis of the relative bias between early- and late-type galaxies in the Two-degree Field Galaxy Redshift Survey (2dFGRS) - as defined by the η parameter of Madgwick et al., which quantifies the spectral type of galaxies in the survey. …”
    Journal article
  8. 108
  9. 109

    The 2dF QSO Redshift Survey - XIII. A Measurement of Lambda from the QSO Power Spectrum by Outram, P, Shanks, T, Boyle, B, Croom, S, Hoyle, F, Loaring, N, Miller, L, Smith, R

    Published 2003
    “…We report on measurements of the cosmological constant, Lambda, and the redshift space distortion parameter beta=Omega_m^0.6/b, based on an analysis of the QSO power spectrum parallel and perpendicular to the observer's line of sight, from the final catalogue of the 2dF QSO Redshift Survey. We derive a joint Lambda - beta constraint from the geometric and redshift-space distortions in the power spectrum. …”
    Journal article
  10. 110
  11. 111
  12. 112

    The 2dF Galaxy Redshift Survey: The population of nearby radio galaxies at the 1-mJy level by Magliocchetti, M, Maddox, S, Jackson, C, Bland-Hawthorn, J, Bridges, T, Cannon, R, Cole, S, Colless, M, Collins, C, Couch, W, Dalton, G, De Propris, R, Driver, S, Efstathiou, G, Ellis, R, Frenk, C, Glazebrook, K, Lahav, O, Lewis, I, Lumsden, S, Peacock, J, Peterson, B, Sutherland, W, Taylor, K

    Published 2002
    “…We use redshift determinations and spectral analysis of galaxies in the 2dF Galaxy Redshift Survey to study the properties of local radio sources with S ≥ 1 mJy. 557 objects (hereafter called the spectroscopic sample) drawn from the FIRST survey, corresponding to 2.3 per cent of the total radio sample, are found in the 2dFGRS catalogue within the area 9h48m ≲ RA(2000) ≲ 14h32m and -2o.77 ≲ Dec.(2000) ≲ 2o.25, down to a magnitude limit bJ = 19.45. …”
    Journal article
  13. 113

    The 2dF QSO Redshift Survey - XIV. Structure and evolution from the two-point correlation function by Croom, S, Boyle, B, Shanks, T, Smith, R, Miller, L, Outram, P, Loaring, N, Hoyle, F, da Angela, A

    Published 2005
    “…In this paper we present a clustering analysis of quasi-stellar objects (QSOs) using over 20 000 objects from the final catalogue of the 2dF QSO Redshift Survey (2QZ), measuring the redshift-space two-point correlation function, ξ(s). …”
    Journal article
  14. 114

    The 2dF Galaxy Redshift Survey: the environmental dependence of galaxy star formation rates near clusters by Lewis, I, Balogh, M, De Propris, R, Couch, W, Bower, R, Offer, A, Bland-Hawthorn, J, Baldry, I, Baugh, C, Bridges, T, Cannon, R, Cole, S, Colless, M, Collins, C, Cross, N, Dalton, G, Driver, S, Efstathiou, G, Ellis, R, Frenk, C, Glazebrook, K, Hawkins, E, Jackson, C, Lahav, O, Lumsden, S

    Published 2002
    “…We have measured the equivalent width of the Ha emission line for 11 006 galaxies brighter than Mb, = -19 (ΩΛ = 0.7, Ωm = 0.3, H0 = 70 km s-1 Mpc-1) at 0.05 < z < 0.1 in the 2dF Galaxy Redshift Survey (2dFGRS), in the fields of 17 known galaxy clusters. …”
    Journal article
  15. 115

    The 2dF QSO Redshift Survey - IV. The QSO Power Spectrum from the 10k Catalogue by Hoyle, F, Outram, P, Shanks, T, Croom, S, Loaring, B, Miller, L, Smith, R

    Published 2001
    “…(ABRIDGED) We present a power spectrum analysis of the 10K catalogue from the 2dF QSO Redshift Survey. We compare the redshift-space power spectra of QSOs to those measured for galaxies and Abell clusters at low redshift and find that they show similar shapes in their overlap range, 50-150h^{-1}Mpc, with P_QSO(k)\propto k^{-1.4}. …”
    Journal article
  16. 116
  17. 117

    Testing General Relativity Using Large-scale Structure Photometric Redshift Surveys and the Cosmic Microwave Background Lensing Effect by Shang Li, Jun-Qing Xia

    Published 2025-01-01
    “…Unlike spectroscopic redshift surveys, photometric redshift measurements are subject to significant redshift uncertainties, making it challenging to constrain the redshift distortion parameter β with high precision. …”
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    Article
  18. 118

    Observations of Mg II Absorption near Z Similar to 1 Galaxies Selected from the Deep2 Redshift Survey by Lovegrove, Elizabeth, Simcoe, Robert A.

    Published 2013
    “…The quasar sight lines were selected from the Sloan Digital Sky Survey DR6 QSO catalog based on proximity to galaxies in the DEEP2 redshift survey. In addition to the 10 small impact systems, we examine 40 additional galaxies at 100 kpc < b < 500 kpc serendipitously located in the same fields. …”
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    Article
  19. 119

    Emission line widths and QSO black hole mass estimates from the 2dF QSO Redshift Survey by Corbett, E, Croom, S, Boyle, B, Netzer, H, Miller, L, Outram, P, Shanks, T, Smith, R, Rhook, K

    Published 2003
    “…We have used composite spectra generated from more than 22000 QSOs observed in the course of the 2dF and 6dF QSO Redshift Surveys to investigate the relationship between the velocity width of emission lines and QSO luminosity. …”
    Journal article
  20. 120

    The 2dF Galaxy Redshift Survey: The amplitudes of fluctuations in the 2dFGRS and the CMB, and implications for galaxy biasing by Lahav, O, Bridle, S, Percival, W, Peacock, J, Efstathiou, G, Baugh, C, Bland-Hawthorn, J, Bridges, T, Cannon, R, Cole, S, Colless, M, Collins, C, Couch, W, Dalton, G, De Propris, R, Driver, S, Ellis, R, Frenk, C, Glazebrook, K, Jackson, C, Lewis, I, Lumsden, S, Maddox, S, Madgwick, D, Moody, S

    Published 2002
    “…We compare the amplitudes of fluctuations probed by the 2dF Galaxy Redshift Survey (2dFGRS) and by the latest measurements of the cosmic microwave background (CMB) anisotropies. …”
    Journal article