[PDF] Top 20 Galaxy-galaxy lensing in the Dark Energy Survey science verification data
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Galaxy-galaxy lensing in the Dark Energy Survey science verification data
... between the two methods. The null tests and the- ory uncertainties are described in Section ...is the size split test with the NGMIX catalogue, which showed sig- nificant ... See full document
16
Dark Energy Survey year 1 results: constraints on extended cosmological models from galaxy clustering and weak lensing
... synthetic data In order to verify that our results are robust to modeling assumptions and approximations, we compare the inferred values of the extension parameters ( Ω k ; N eff ; …) obtained ... See full document
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Mass variance from archival X-ray properties of dark energy survey year-1 galaxy clusters
... DES data management system is supported by the Na- tional Science Foundation under grant numbers AST-1138766 and ...AST-1536171. The DES participants from Spanish institutions are partially ... See full document
15
Dark Energy Survey year 1 results: measurement of the galaxy angular power spectrum
... for the DES Projects has been provided by the ...of Energy, the U.S. National Science Foundation, the Ministry of Science and Education of Spain, the Science ... See full document
15
Dark Energy Survey year 1 results: tomographic cross-correlations between Dark Energy Survey galaxies and CMB lensing from South Pole Telescope plus Planck
... by the Kavli Institute for Cosmological Physics at the University of Chicago through Grant ...by the Fermi Research Alliance, LLC under Contract ...with the United States Department of ... See full document
19
Dark Energy Survey year 1 results: galaxy sample for BAO measurement
... BAO in the angular distribution of galaxies, a determination of the photometric redshift as precise as possible brings several ...tomography in the mapping of the BAO evolution ... See full document
17
The DES bright arcs survey: hundreds of candidate strongly lensed galaxy systems from the Dark Energy Survey science verification and year 1 observations
... —mostly in the form of fainter systems, we stopped creating new ...if the system was thought to not be a SL candidate, 1 point if it might be, and 2 points if the system was expected to be an ... See full document
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Cosmological constraints from multiple probes in the Dark Energy Survey
... for the DES Projects has been provided by the DOE and NSF (USA), MEC/MICINN/MINECO (Spain), STFC (UK), HEFCE (United Kingdom), NCSA (UIUC), KICP ...and the Collaborating Institutions in ... See full document
9
Estruturas em larga escala e o Dark Energy Survey
... In the same context, future cosmic shear surveys will play a major role in ...cosmology. The sensitivity of weak lensing observations will be high enough to allow for precision ... See full document
175
Dark energy survey year 1 results: validation of weak lensing cluster member contamination estimates from P(z) decomposition
... with the targeted clusters also enter the catalogue if they satisfy those ...as in Schrabback et al. 2018 ) since they are at the lens redshift and carry no lensing ...However in ... See full document
15
OzDES multifibre spectroscopy for the Dark Energy Survey: 3-yr results and first data release
... In the modern era of large surveys, this observing strategy is being supplemented by ones that incorporate dynamic target selec- ...tion. In these surveys, target selection is done shortly before ... See full document
17
Cosmic voids and void lensing in the Dark Energy Survey science verification data
... identified in spectroscopic galaxy surveys, where 3D information about the large-scale structure of the Universe is ...photometric data is being produced, its potential for void studies ... See full document
15
Dark Energy Survey year 1 results: methodology and projections for joint analysis of galaxy clustering, galaxy lensing, and CMB lensing two-point functions
... of Energy Grant No. DE-SC0007901. The Reichardt and Bianchini acknowledge support from the Australian Research Council ’s Future Fellowships scheme (Grant ...by the Sloan Foundation, Grant ... See full document
23
Dark Energy Survey year 1 results: joint analysis of galaxy clustering, galaxy lensing, and CMB lensing two-point functions
... of galaxy and CMB lensing, we effectively get to measure the lensing effects of LSS ...between the lensing measurements performed with these two sources of light would likely be ... See full document
22
Environmental dependence of the galaxy stellar mass function in the Dark Energy Survey science verification data
... that the RMSE of the standard deviation for the 100 catalogues is ...than the typical width of the photo-z ...between the statistics of the samples and the PDFs can ... See full document
21
Weak-lensing mass calibration of redMaPPer galaxy clusters in Dark Energy Survey Science Verification data
... In a blinded analysis, we split the sample of more than 8000 redMaPPer clusters into 15 subsets, spanning ranges in the richness parameter 5 ≤ λ ≤ 180 and redshift 0.2 ≤ z ≤ 0.8, and fit[r] ... See full document
23
Testing the lognormality of the galaxy and weak lensing convergence distributions from Dark Energy Survey maps
... on the galaxy density contrast and weak lensing convergence maps with HEALPIX pixelization of resolution N side = 4096, which corresponds to an average pixel size of ...construct the PDF, we ... See full document
19
Dark Energy Survey year 1 results: cross-correlation between Dark Energy Survey Y1 galaxy weak lensing and South Pole Telescope plus Planck CMB weak lensing
... from the Natural Sciences and Engineering Research Council of Canada, Canadian Institute for Advanced Research, Canada Research Chairs program, and support from the Kavli ...by the U.S. Department of ... See full document
17
Longslit spectroscopy of the starburst galaxy HRG 02401
... lines. The term “starburst” was originally coined by Weedman et al. [1] to in- dicate qualitatively that a galaxy is undergoing a period of intense star ...On the other hand, for the ... See full document
6
Studying AGN galaxy hosts in the framework of Gaia mission
... test the recuperation of the parameters, it was used the same process described in the previ- ous section, but now with two completely independent components for which we have different ... See full document
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