Baryon oscillations and dark-energy constraints from imaging surveys
Open accessAbstract
Baryonic oscillations in the galaxy power spectrum have been studied as a way of probing dark-energy models. While most studies have focused on spectroscopic surveys at high redshift, large multicolour imaging surveys have already been planned for the near future. In view of this, we study the prospects for measuring baryonic oscillations from angular statistics of galaxies binned using photometric redshifts. We use the galaxy bispectrum in addition to the power spectrum; this allows us to measure and marginalize over possibly complex galaxy bias mechanisms to get robust cosmological constraints. In our parameter estimation, we allow for a weakly non-linear biasing scheme that may evolve with redshift by two bias parameters in each of 10 redshift bins. We find that a multicolour imaging survey that probes redshifts beyond one can give interesting constraints on dark-energy parameters. In addition, the shape of the primordial power spectrum can be measured to better accuracy than with the cosmic microwave background (CMB) alone. We explore the impact of survey depth, area and calibration errors in the photometric redshifts on dark-energy constraints.
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Higher-order shear and galaxy statistics and shear peak counts can improve dark energy constraints and provide self-calibration of various systematics.
“Higher-order shear and galaxy statistics and shear peak counts can improve dark energy constraints and provide self-calibration of various systematics ( Takada & Jain 2004; Dolney et al. 2006; Huterer et al. 2006; Petri et al. 2016 ) .”
From LSST: From Science Drivers to Reference Design and Anticipated Data Products (2019) · cites this paper as Dolney et al. 2006
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“The idea of using the bispectrum in addition to the power spectrum on large scales to constrain both the amplitude of the mass power spectrum and bias has been suggested and implemented (Fry 1999; Frieman & Gaztanaga 1999; Feldman et al. 2001; Verde et al. 2002).”
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BackgroundCBR anisotropy and the running of the scalar spectral index
Kosowsky, A. B., & Turner, M. S. (1995) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.52.r1739 · Cited by 277 · cited 1× · see citing works
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InfluentialScranton, R., Johnston, D., Dodelson, S., Frieman, J. A., Connolly, A. J., Eisenstein, D. J., Gunn, J. E., Hui, L., Jain, B., Kent, S., et al. (2002) · The Astrophysical Journal · doi:10.1086/342786 · Cited by 272 · see citing works
Self-citationBaryonic signatures in large-scale structure
Meiksin, A. A., White, M. J., & Peacock, J. A. (1999) · Monthly Notices of the Royal Astronomical Society · doi:10.1046/j.1365-8711.1999.02369.x · Cited by 252 · see citing works
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Cosmological Parameters from Eigenmode Analysis of Sloan Digital Sky Survey Galaxy Redshifts
Pope, A., Matsubara, T., Szalay, A. S., Blanton, M. R., Eisenstein, D. J., Gray, J., Jain, B., Bahcall, N. A., Brinkmann, J., Budavári, T., et al. (2004) · The Astrophysical Journal · doi:10.1086/383533 · Cited by 242 · cited 1× · see citing works
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MethodSelf-citationDragan Huterer, A. (2002) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.65.063001 · Cited by 237 · cited 1× · see citing works
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MethodInfluentialDark synergy: Gravitational lensing and the CMB
Hu, W. (2001) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.65.023003 · Cited by 226 · see citing works
Hu, W., & Haiman, Z. (2003) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.68.063004 · Cited by 226 · cited 1× · see citing works
“To measure baryon oscillations, many authors have considered galaxy surveys over different redshift ranges (Eisenstein 2003; Blake & Glazebrook 2003; Linder 2003; Hu & Haiman 2003; Seo & Eisenstein 2003; Matsubara & Szalay 2003).”
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Ma, C.-P., Caldwell, R. R., Bode, P. W., & Wang, L. (1999) · The Astrophysical Journal · doi:10.1086/312183 · Cited by 180 · see citing works
Baryon oscillations as a cosmological probe
Linder, E. V. (2003) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.68.083504 · Cited by 146 · cited 4× · see citing works
“To measure baryon oscillations, many authors have considered galaxy surveys over different redshift ranges (Eisenstein 2003; Blake & Glazebrook 2003; Linder 2003; Hu & Haiman 2003; Seo & Eisenstein 2003; Matsubara & Szalay 2003).”
BackgroundMethodInfluentialGravity, bias, and the galaxy three-point correlation function
Fry, J. N. (1994) · Physical Review Letters · doi:10.1103/physrevlett.73.215 · Cited by 145 · see citing works
Budavari, T., Connolly, A. J., Szalay, A. S., Szapudi, I., Csabai, I., Scranton, R., Bahcall, N. A., Brinkmann, J., Eisenstein, D. J., Frieman, J. A., et al. (2003) · The Astrophysical Journal · doi:10.1086/377168 · Cited by 135 · cited 1× · see citing works
“This is an area of ongoing study (e.g. Connolly et al. 2002; Budavari et al. 2003; Mobasher et al. 2004).”
BackgroundFeldman, H. A., Frieman, J. A., Fry, J. N., & Scoccimarro, R. (2001) · Physical Review Letters · doi:10.1103/physrevlett.86.1434 · Cited by 128 · cited 1× · see citing works
“The idea of using the bispectrum in addition to the power spectrum on large scales to constrain both the amplitude of the mass power spectrum and bias has been suggested and implemented (Fry 1999; Frieman & Gaztanaga 1999; Feldman et al. 2001; Verde et al. 2002).”
MethodPhotometric Redshifts for Galaxies in the GOODS Southern Field
Mobasher, B., Idzi, R., Bentez, N., Cimatti, A., Cristiani, S., Daddi, E., Dahlen, T., Dickinson, M., Erben, T., Ferguson, H. C., et al. (2004) · The Astrophysical Journal · doi:10.1086/378186 · Cited by 114 · cited 1× · see citing works
“This is an area of ongoing study (e.g. Connolly et al. 2002; Budavari et al. 2003; Mobasher et al. 2004).”
BackgroundThe Angular Correlation Function of Galaxies from Early Sloan Digital Sky Survey Data
Connolly, A. J., Scranton, R., Johnston, D., Dodelson, S., Eisenstein, D. J., Frieman, J. A., Gunn, J. E., Hui, L., Jain, B., Kent, S., et al. (2002) · The Astrophysical Journal · doi:10.1086/342787 · Cited by 113 · cited 1× · see citing works
“This is an area of ongoing study (e.g. Connolly et al. 2002; Budavari et al. 2003; Mobasher et al. 2004).”
BackgroundSelf-citationPHOTOMETRIC REDSHIFTS FOR GALAXIES IN THE GOODS SOUTHERN FIELDPreprint
Mobasher, B., Idzi, R., Benítez, N., Cimatti, A., Cristiani, S., Daddi, E., Dahlén, T., Dickinson, M., Erben, T., Ferguson, H. C., et al. (2003) · Cited by 75 · see citing works
Measuring Angular Diameter Distances through Halo Clustering
Cooray, A. R., Hu, W., Dragan Huterer, A., & Joffre, M. (2001) · The Astrophysical Journal · doi:10.1086/323323 · Cited by 74 · cited 1× · see citing works
“We do still have a standard ruler in the no-wiggles case: the peak in the power spectrum corresponding to matter-radiation equality (Cooray et al. 2001).”
BackgroundThe Projected Three-Point Correlation Function: Theory and Observations
Frieman, J. A., & GAZTAÑAGA, E. (1999) · The Astrophysical Journal · doi:10.1086/312195 · Cited by 71 · cited 1× · see citing works
“The idea of using the bispectrum in addition to the power spectrum on large scales to constrain both the amplitude of the mass power spectrum and bias has been suggested and implemented (Fry 1999; Frieman & Gaztanaga 1999; Feldman et al. 2001; Verde et al. 2002).”
MethodMeasuring Angular Diameter Distances through Halo Clustering
Cooray, A. R., Hu, W., Dragan Huterer, A., & Joffre, M. (2001) · CERN Document Server (European Organization for Nuclear Research) · Cited by 47 · see citing works
The Projected Three-point Correlation Function: Theory and Observations
Frieman, J. A., & Gaztañaga, E. (1999) · CERN Document Server (European Organization for Nuclear Research) · Cited by 45 · see citing works
Cosmological Parameters from Eigenmode Analysis of Sloan Digital Sky Survey Galaxy Redshifts
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Apparent Clustering of Intermediate-Redshift Galaxies as a Probe of Dark Energy
Matsubara, T., & Szalay, A. S. (2003) · Physical Review Letters · doi:10.1103/physrevlett.90.021302 · Cited by 30 · cited 1× · see citing works
“To measure baryon oscillations, many authors have considered galaxy surveys over different redshift ranges (Eisenstein 2003; Blake & Glazebrook 2003; Linder 2003; Hu & Haiman 2003; Seo & Eisenstein 2003; Matsubara & Szalay 2003).”
Background
Flagged first, then by citations
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Cited by
Sorted by citations
LSST: From Science Drivers to Reference Design and Anticipated Data Products
Ivezić, Ž., Kahn, S. M., Tyson, J. A., Abel, B., Acosta, E., Allsman, R., Alonso, D., AlSayyad, Y., Anderson, S. F., Andrew, J., et al. (2019) · The Astrophysical Journal · doi:10.3847/1538-4357/ab042c · Cited by 4,357 · see citing works
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On the Robustness of the Acoustic Scale in the Low‐Redshift Clustering of Matter
Eisenstein, D. J., Seo, H., & White, M. J. (2007) · The Astrophysical Journal · doi:10.1086/518755 · Cited by 460 · see citing works
The clustering of luminous red galaxies in the Sloan Digital Sky Survey imaging data
Padmanabhan, N., Schlegel, D. J., Seljak, U., Makarov, A., Bahcall, N. A., Blanton, M. R., Brinkmann, J. V., Eisenstein, D. J., Finkbeiner, D. P., Gunn, J. E., et al. (2007) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2007.11593.x · Cited by 360 · see citing works
Improved Forecasts for the Baryon Acoustic Oscillations and Cosmological Distance Scale
Seo, H., & Eisenstein, D. (2007) · The Astrophysical Journal · doi:10.1086/519549 · Cited by 278 · see citing works
“…using the BAO from future galaxy redshift surveys (Eisenstein 2003; Blake&Glazebrook 2003; Linder 2003; Hu &Haiman 2003; Seo & Eisenstein 2003; Cooray 2004; Matsubara 2004; Amendola et al. 2005; Blake & Bridle 2005; Glazebrook & Blake 2005; Dolney et al. 2006; Zhan & Knox 2006; Blake et al. 2006).”
MethodMatsubara, T. (2008) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.78.083519 · Cited by 255 · see citing works
Measuring DA and H at z=0.35 from the SDSS DR7 LRGs using baryon acoustic oscillations
Xu, X., Cuesta, A. J., Padmanabhan, N., Eisenstein, D. J., & McBride, C. K. (2013) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stt379 · Cited by 214 · see citing works
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“…considered before as promising probes of cosmology themselves, including galaxy clustering from photometric redshift surveys (Blake & Bridle 2005; Dolney et al. 2006; Zhan 2006; Blake et al. 2007; Padmanabhan et al. 2007) galaxygalaxy lensing (e.g. Schneider & Rix 1997; Guzik & Seljak 2001,…”
BackgroundImproved forecasts for the baryon acoustic oscillations and cosmological distance scale
Seo, H. J., & Eisenstein, D. J. (2007) · CERN Document Server (European Organization for Nuclear Research) · Cited by 184 · see citing works
Clustering of dark matter tracers: Renormalizing the bias parameters
McDonald, P. (2006) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.74.103512 · Cited by 175 · see citing works
McDonald, P., & Eisenstein, D. J. (2007) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.76.063009 · Cited by 161 · see citing works
Motion of the acoustic peak in the correlation function
Smith, R. C., Scoccimarro, R., & Sheth, R. K. (2008) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.77.043525 · Cited by 152 · see citing works
Nonlinear Structure Formation and the Acoustic Scale
Seo, H., Siegel, E. R., Eisenstein, D. J., & White, M. J. (2008) · The Astrophysical Journal · doi:10.1086/589921 · Cited by 150 · see citing works
Desjacques, V., Crocce, M., Scoccimarro, R., & Sheth, R. K. (2010) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.82.103529 · Cited by 143 · see citing works
Xu, X., Padmanabhan, N., Eisenstein, D. J., Mehta, K., & Cuesta, A. J. (2012) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2012.21573.x · Cited by 139 · see citing works
Differentiating dark energy and modified gravity with galaxy redshift surveys
Wang, Y. (2008) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2008/05/021 · Cited by 134 · see citing works
Dark matter clustering: A simple renormalization group approach
McDonald, P. (2007) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.75.043514 · Cited by 130 · see citing works
Joachimi, B., & Bridle, S. (2010) · Springer Link (Chiba Institute of Technology) · doi:10.1051/0004-6361/200913657/pdf · Cited by 123 · see citing works
ACOUSTIC SCALE FROM THE ANGULAR POWER SPECTRA OF SDSS-III DR8 PHOTOMETRIC LUMINOUS GALAXIES
Seo, H., Ho, S., White, M. J., Cuesta, A. J., Ross, A. J., Saito, S., Reid, B., Padmanabhan, N., Percival, W. J., de Putter, R., et al. (2012) · The Astrophysical Journal · doi:10.1088/0004-637x/761/1/13 · Cited by 117 · see citing works
“…in 1+z is at least required to recover H(z) (Seo & Eisenstein 2003). surveys (Seo & Eisenstein 2003; Amendola et al. 2005; Blake & Bridle 2005; Dolney et al. 2006; Zhan & Knox 2006) and this prospect has motivated current and future imaging BAO surveys such as the Dark Energy Survey26 (DES;…”
BackgroundBaryon acoustic signature in the clustering of density maxima
Desjacques, V. (2008) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.78.103503 · Cited by 97 · see citing works
What is the best way to measure baryonic acoustic oscillations?
Sánchez, A. G., Baugh, C. M., & Angulo, R. E. (2008) · Max Planck Digital Library · Cited by 93 · see citing works
Cosmic tomographies: baryon acoustic oscillations and weak lensing
Zhan, H. (2006) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2006/08/008 · Cited by 60 · see citing works
Sato, M., & Matsubara, T. (2011) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.84.043501 · Cited by 54 · see citing works
Órdenes-Briceño, Y., Eigenthaler, P., Taylor, M. A., Puzia, T. H., Álamo-Martínez, K., Ribbeck, K. X., Muñoz, R. P., Zhang, H., Grebel, E. K., Ángel, S., et al. (2018) · The Astrophysical Journal · doi:10.3847/1538-4357/aaba70 · Cited by 51 · see citing works
“…a random distribution without a restriction to Gaussianity (e.g., Connolly et al. 2002; Sato et al. 2009) and is typically used to constrain cosmological parameters and structure formation models (e.g., Bernardeau et al. 2002; Cooray & Sheth 2002; Tegmark et al. 2002, 2004; Dolney et al. 2006).”
BackgroundZhan, H., & Knox, L. (2006) · The Astrophysical Journal · doi:10.1086/503622 · Cited by 50 · see citing works
“Several papers have studied the prospects for measuring BAOs from photometric surveys (SE03; Dolney et al. 2006; Blake & Bridle 2005; Glazebrook & Blake 2005; Linder 2005).”
BackgroundWhat is the best way to measure baryonic acoustic oscillations?
Sánchez, A. G., Baugh, C. M., & Angulo, R. E. (2008) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2008.13769.x · Cited by 49 · see citing works
The Nonlinear Matter Power Spectrum
Ma, Z. (2007) · The Astrophysical Journal · doi:10.1086/519440 · Cited by 45 · see citing works
“…history of the universe and cosmological distances (Eisenstein et al. 1998; Cooray et al. 2001; Blake & Glazebrook 2003; Hu & Haiman 2003; Seo & Eisenstein 2003; Linder 2003, 2005;Matsubara et al. 2004; Amendola et al. 2005; Blake & Bridle 2005; Glazebrook & Blake 2005; Dolney et al. 2006).”
BackgroundLensing corrections to features in the angular two-point correlation function and power spectrum
Loverde, M., Hui, L., & GAZTAÑAGA, E. (2008) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.77.023512 · Cited by 42 · see citing works
USING A PHENOMENOLOGICAL MODEL TO TEST THE COINCIDENCE PROBLEM OF DARK ENERGY
Chen, Y., Zhu, Z., Alcaniz, J. S., & Gong, Y. (2010) · The Astrophysical Journal · doi:10.1088/0004-637x/711/1/439 · Cited by 41 · see citing works
“…of BAO peak can be used as a “standard cosmological ruler” to constrain the cosmological parameters (Blake & Glazebrook 2003; Seo & Eisenstein 2003; Dolney et al. 2006), which was first successfully found by detecting of a peak in the correlation function of about 50,000 luminous red galaxies…”
Background3D spherical analysis of baryon acoustic oscillations
Rassat, A., & Refregier, A. R. (2012) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201118638 · Cited by 39 · see citing works
“Until now, BAOs have been studied in Cartesian space, either in Fourier space (Seo & Eisenstein 2003, 2007), or in real space (Eisenstein et al. 2005; Xu et al. 2010; Slosar et al. 2009), and in 2D spherical harmonic space on thin spherical shells (Dolney et al. 2006).”
BackgroundMethodCosmic tomographies: baryon acoustic oscillations and weak lensingPreprint
Zhan, H. (2006) · Cited by 42 · see citing works
CALIBRATION OF GRB LUMINOSITY RELATIONS WITH COSMOGRAPHY
GAO, H., Liang, N., & Zhu, Z. (2012) · International Journal of Modern Physics D · doi:10.1142/s0218271812500162 · Cited by 34 · see citing works
Chaves-Montero, J., Angulo, R. E., & Hernández-Monteagudo, C. (2018) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/sty924 · Cited by 34 · see citing works
Zhan, H., & Knox, L. (2005) · CERN Document Server (European Organization for Nuclear Research) · Cited by 33 · see citing works
Optimizing future imaging survey of galaxies to confront dark energy and modified gravity models
Yamamoto, K., Parkinson, D., Hamana, T., Nichol, R. C., & Suto, Y. (2007) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.76.023504 · Cited by 27 · see citing works
Lanusse, F., Rassat, A., & Starck, J. (2015) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201424456 · Cited by 25 · see citing works
“…and planned future surveys, and the analysis can be performed in various spaces, for example, Fourier space (Seo & Eisenstein 2003, 2007), configuration space (Eisenstein et al. 2005; Xu et al. 2010; Slosar et al. 2009), and spherical harmonic space (e.g., Dolney et al. 2006; Kirk et al. 2012).”
BackgroundTidal alignments as a contaminant of the galaxy bispectrum
Krause, E., & Hirata, C. M. (2010) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2010.17638.x · Cited by 25 · see citing works
“This enables one remove the effects of galaxy biasing and measure the cosmological growth of structure from the galaxy distribution (Fry 1994; Verde et al. 1998; Scoccimarro et al. 1999; Verde et al. 2000), and thus constrai dark energy (e.g. Dolney et al. 2006).”
MethodPratten, G., & Munshi, D. (2013) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stt1854 · Cited by 22 · see citing works
“…(Seo & Eisenstein 2003, 2007), real-space analysis (Eisenstein et al. 2005; Slosar et al. 2009; Xu et al. 2010; Juszkiewicz, Hellwing & van de Weygaert 2013), in 2D spherical harmonics defined on thin spherical shells (Dolney et al. 2006), but also in the sFB expansion (Rassat & Refregier 2012).”
BackgroundMock galaxy redshift catalogues from simulations: implications for Pan-STARRS1
Cai, Y.-C., Angulo, R. E., Baugh, C. M., Cole, S., Frenk, C. S., & Jenkins, A. (2009) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2009.14402.x · Cited by 21 · see citing works
“Several authors have investigated the implications of c© 0000 RAS, MNRAS 000, 000–000 photometric redshift errors on the clustering measurements in general and on the BAO in particular (Seo & Eisenstein 2003; Amendola et al. 2005; Dolney et al. 2006; Blake & Bridle 2005).”
BackgroundCharacterizing unknown systematics in large scale structure surveys
Agarwal, N., Ho, S., Myers, A. D., Seo, H., Ross, A. J., Bahcall, N. A., Brinkmann, J. V., Eisenstein, D. J., Muna, D., Palanque‐Delabrouille, N., et al. (2014) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2014/04/007 · Cited by 20 · see citing works
Observational evidence for negative-energy dust in late-times non-standard cosmologies
Mavromatos, N. E., & Mitsou, V. A. (2008) · Astroparticle Physics · doi:10.1016/j.astropartphys.2008.05.002 · Cited by 13 · see citing works
Schäfer, B. M. (2008) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2008.13526.x · Cited by 11 · see citing works
“…signal to noise ratio Σ q (assuming a Gaussian likelihood) for a measurement of the bispectrum τ q γ 3 − q is given by (Hu 2000; Takada & Jain 2003b, 2004; Dolney et al. 2006): with ℓ p ∈ { ℓ 1 ,ℓ 2 ,ℓ 3 } and ℓ ′ p ∈ ℓ ′ 1 ,ℓ ′ 2 ,ℓ ′ 3 . the For convenience, I abbreviated inverse covariance of…”
Detecting baryon acoustic oscillations by 3d weak lensing
Grassi, A., & Schäfer, B. M. (2013) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stt2075 · Cited by 11 · see citing works
Song, Y. (2011) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.83.103009 · Cited by 9 · see citing works
Detection significance of baryon acoustic oscillations peaks in galaxy and quasar clustering
Ansarinejad, B., & Shanks, T. (2018) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/sty1740 · Cited by 4 · see citing works
“…across a wide range of redshifts, making use of the Baryon Acoustic Oscillation (BAO) feature in the clustering of galaxies (e.g. Shanks 1985; Blake & Glazebrook 2003; Linder 2003; Seo & Eisenstein 2003; Matsubara 2004; Glazebrook & Blake 2005; Dolney et al. 2006; Sánchez et al. 2008).”
BackgroundConstraining dark energy using real and mock galaxy surveys
Cai, Y.-C. (2009) · Durham e-Theses (Durham University)
Ivezić, Ž. (2016) · Zenodo (CERN European Organization for Nuclear Research) · doi:10.5281/zenodo.44697
Large Synoptic Survey Telescope Town Hall
Willman, B. (2016) · Zenodo (CERN European Organization for Nuclear Research) · doi:10.5281/zenodo.44768
The Lsst Data Processing Software Stack
Jenness, T. (2016) · American Astronomical Society Meeting Abstracts #227 · doi:10.5281/zenodo.44634
Wang, P. Y. (2010) · doi:10.1002/9783527629350.refs
Comparat, J. (2013) · doi:10.70675/5873d7e6za48az4788zb32cz18be99041874
“The physics at scales smaller than the radius of curvature of the Universe are well described by Eulerian hydrodynamics and Newtonian mechanics.”
BackgroundMethodInfluential
- Authors
- Dolney, D., Jain, B., & Takada, M.
- Affiliations
- University of Pennsylvania (US)
- Tohoku University (JP)
- Venue
- Monthly Notices of the Royal Astronomical Society
- Publisher
- Oxford University Press (OUP)
- Published
- 2006-03-01
- Volume
- 366
- Issue
- 3
- Pages
- 884-898
- ISSN
- 0035-8711 (ISSN-L)
- 1365-2966
- OpenAlex
- W2167693391
- Cited by
- 52
- References
- 45
- Citations by year
- 2019: 1 · 2018: 3 · 2016: 3 · 2015: 1 · 2014: 1 · 2013: 5 · 2012: 4
- FWCI
- 4.79
- Type
- journal article
- Language
- en
- Open access
- green
- arxiv.org
- Locations
- Monthly Notices of the Royal Astronomical Society (publishedVersion)
- arXiv (Cornell University) (submittedVersion)
- CERN Document Server (European Organization for Nuclear Research) (submittedVersion)
- arXiv (Cornell University)
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Galaxies: Formation, Evolution, Phenomena
- Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Dark Matter and Cosmic Phenomena
- Keywords
- baryon acoustic oscillations, dark energy, galaxy bispectrum, galaxy power spectrum, photometric redshifts, galaxy bias, primordial power spectrum, cosmological parameter estimation
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