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Cosmology from cosmic shear with Dark Energy Survey Science Verification data
- Source :
- Abbott, T, Abdalla, F B, Allam, S, Amara, A, Annis, J, Armstrong, R, Bacon, D, Banerji, M, Bauer, A H, Baxter, E, Becker, M R, Benoit-Lévy, A, Bernstein, R A, Bernstein, G M, Bertin, E, Blazek, J, Bonnett, C, Bridle, S L, Brooks, D, Bruderer, C, Buckley-Geer, E, Burke, D L, Busha, M T, Capozzi, D, Rosell, A C, Kind, M C, Carretero, J, Castander, F J, Chang, C, Clampitt, J, Crocce, M, Cunha, C E, D'Andrea, C B, Costa, L N D, Das, R, DePoy, D L, Desai, S, Diehl, H T, Dietrich, J P, Dodelson, S, Doel, P, Drlica-Wagner, A, Efstathiou, G, Eifler, T F, Erickson, B, Estrada, J, Evrard, A E, Neto, A F, Nichol, R C, Thomas, D & Dark Energy Survey Collaboration 2016, ' Cosmology from cosmic shear with Dark Energy Survey Science Verification Data ', Physical Review D, vol. 94, no. 2, 022001 . https://doi.org/10.1103/PhysRevD.94.022001, Abbott, T, Abdalla, F B, Allam, S, Amara, A, Annis, J, Armstrong, R, Bacon, D, Banerji, M, Bauer, A H, Baxter, E, Becker, M R, Benoit-Lévy, A, Bernstein, R A, Bernstein, G M, Bertin, E, Blazek, J, Bonnett, C, Bridle, S L, Brooks, D, Bruderer, C, Buckley-Geer, E, Burke, D L, Busha, M T, Capozzi, D, Carnero Rosell, A, Carrasco Kind, M, Carretero, J, Castander, F J, Chang, C, Clampitt, J, Crocce, M, Cunha, C E, D'Andrea, C B, da Costa, L N, Das, R, DePoy, D L, Desai, S, Diehl, H T, Dietrich, J P, Dodelson, S, Doel, P, Drlica-Wagner, A, Efstathiou, G, Eifler, T F, Erickson, B, Estrada, J, Evrard, A E, Fausti Neto, A, Fernandez, E, Finley, D A, Flaugher, B, Fosalba, P, Friedrich, O, Frieman, J, Gangkofner, C, Garcia-Bellido, J, Gaztanaga, E, Gerdes, D W, Gruen, D, Gruendl, R A, Gutierrez, G, Hartley, W, Hirsch, M, Honscheid, K, Huff, E M, Jain, B, James, D J, Jarvis, M, Kacprzak, T, Kent, S, Kirk, D, Krause, E, Kravtsov, A, Kuehn, K, Kuropatkin, N, Kwan, J, Lahav, O, Leistedt, B, Li, T S, Lima, M, Lin, H, MacCrann, N, March, M, Marshall, J L, Martini, P, McMahon, R G, Melchior, P, Miller, C J, Miquel, R, Mohr, J J, Neilsen, E, Nichol, R C, Nicola, A, Nord, B, Ogando, R, Palmese, A, Peiris, H V, Plazas, A A, Refregier, A, Roe, N, Romer, A K, Roodman, A, Rowe, B, Rykoff, E S, Sabiu, C, Sadeh, I, Sako, M, Samuroff, S, Sanchez, E, Sánchez, C, Seo, H, Sevilla-Noarbe, I, Sheldon, E, Smith, R C, Soares-Santos, M, Sobreira, F, Suchyta, E, Swanson, M E C, Tarle, G, Thaler, J, Thomas, D, Troxel, M A, Vikram, V, Walker, A R, Wechsler, R H, Weller, J, Zhang, Y, Zuntz, J & Dark Energy Survey Collaboration, U 2016, ' Cosmology from cosmic shear with Dark Energy Survey Science Verification data ', Physical Review D, Particles and fields, vol. 94, no. 2, pp. 22001 . https://doi.org/10.1103/PhysRevD.94.022001
- Publication Year :
- 2016
- Publisher :
- American Physical Society (APS), 2016.
-
Abstract
- We present the first constraints on cosmology from the Dark Energy Survey (DES), using weak lensing measurements from the preliminary Science Verification (SV) data. We use 139 square degrees of SV data, which is less than 3% of the full DES survey area. Using cosmic shear 2-point measurements over three redshift bins we find σ8(Ωm/0.3)0.5=0.81±0.06 (68% confidence), after marginalizing over 7 systematics parameters and 3 other cosmological parameters. We examine the robustness of our results to the choice of data vector and systematics assumed, and find them to be stable. About 20% of our error bar comes from marginalizing over shear and photometric redshift calibration uncertainties. The current state-of-the-art cosmic shear measurements from CFHTLenS are mildly discrepant with the cosmological constraints from Planck CMB data; our results are consistent with both data sets. Our uncertainties are ∼30% larger than those from CFHTLenS when we carry out a comparable analysis of the two data sets, which we attribute largely to the lower number density of our shear catalogue. We investigate constraints on dark energy and find that, with this small fraction of the full survey, the DES SV constraints make negligible impact on the Planck constraints. The moderate disagreement between the CFHTLenS and Planck values of σ8(Ωm/0.3)0.5 is present regardless of the value of ω.
- Subjects :
- Cosmology and Gravitation
PARAMETER CONSTRAINTS
Dark matter
Cosmic microwave background
WEAK-LENSING TOMOGRAPHY
Astrophysics::Cosmology and Extragalactic Astrophysics
Astrophysics
Astronomy & Astrophysics
GALAXY ELLIPTICITIES
01 natural sciences
Cosmology
Physics, Particles & Fields
symbols.namesake
PRECISION COSMOLOGY
MATTER POWER SPECTRUM
LARGE-SCALE STRUCTURE
0103 physical sciences
Planck
010303 astronomy & astrophysics
STFC
Weak gravitational lensing
QB
Photometric redshift
Physics
Science & Technology
010308 nuclear & particles physics
RCUK
Astronomy
INTRINSIC ALIGNMENTS
Redshift
Physical Sciences
astro-ph.CO
Dark energy
symbols
COVARIANCE-MATRIX
BARYON ACOUSTIC-OSCILLATIONS
HUBBLE CONSTANT
Subjects
Details
- ISSN :
- 24700029, 24700010, and 15507998
- Volume :
- 94
- Database :
- OpenAIRE
- Journal :
- Physical Review D
- Accession number :
- edsair.doi.dedup.....9eaca70b66ac0ff2ea4dc3f49d8fb321
- Full Text :
- https://doi.org/10.1103/physrevd.94.022001