[PDF] Top 20 Cosmological constraints from multiple probes in the Dark Energy Survey
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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
Dark energy survey year 1 results: the photometric data set for cosmology
... describe the creation, content, and validation of the Dark Energy Survey (DES) internal year-one cosmology data set, Y1A1 GOLD, in support of upcoming cosmological ... See full document
36
Quasar accretion disk sizes from continuum reverberation mapping from the dark energy survey
... for the DES quasars that had yielded tentative r, i, and /or z lag measurements relative to the g ...restrict the DRW damping timescale to fall between 100 and 300 days for this ...good ... See full document
14
Testing the lognormality of the galaxy and weak lensing convergence distributions from Dark Energy Survey maps
... for the DES Projects has been provided by the US De- partment of Energy, the US National Science Foundation, the Min- istry of Science and Education of Spain, the Science and ... See full document
19
Candidate massive galaxies at z similar to 4 in the Dark Energy Survey
... within the locus predicted for z ∼ 4 massive ...by the model selection ...constrain the models is the addition, to the optical DES bands g, r, i, z, and Y, of near-IR J, H, K s data ... See full document
23
Cosmic voids and void lensing in the Dark Energy Survey science verification data
... standard cosmological parameters, voids have been used to investigate alternative dark matter sce- narios like warm dark matter (Yang et ...or the effects of neutrinos on void lensing (Massara ... See full document
15
DES Y1 results: validating cosmological parameter estimation using simulated dark energy surveys
... galaxy survey simulations designed to resemble the Dark Energy Survey Year 1 (DES Y1) data to validate and inform cosmological parameter ...real survey data, they provide ... See full document
23
The morphology and structure of stellar populations in the Fornax dwarf spheroidal galaxy from Dark Energy Survey Data
... of the CMD is dominated by a composite subgiant branch and MSTO feature, as a result of multiple overlapping stellar populations covering a large range in ...magnitudes. The CMD of BP is ... See full document
15
First cosmology results using SNe Ia from the Dark Energy Survey: analysis, systematic uncertainties, and validation
... present the analysis underpinning the measurement of cosmological parameters from 207 spectroscopically classi fied SNe Ia from the first 3 years of the Dark ... See full document
30
Rapidly evolving transients in the dark energy survey
... Over the last decade a new interesting class of transient with rapid photometric evolution has been ...brightness in 10 d and exponential decline in 30 d after the peak in rest frame, ... See full document
25
The evolution of active galactic nuclei in clusters of galaxies from the Dark Energy Survey
... Galaxies in clusters are known to evolve at different rates than galaxies in the ...example, in the local Universe the bulk of galaxies in clusters exhibit little or no ... See full document
10
Estruturas em larga escala e o Dark Energy Survey
... appear in this interpretation, (a) whether the model postulated is a correct physical description of the Universe evolution and (b) given a model, whether the theoretical predictions are ... See full document
175
First cosmology results using Type Ia supernovae from the Dark Energy Survey: effects of chromatic corrections to supernova photometry on measurements of cosmological parameters
... improve the absolute calibration, PS1 measured the full transmission function including instrument (telescope + CCD) and ...measured the instrumental transmission using in-dome monochromator ... See full document
17
Constraining H0 in general dark energy models from Sunyaev-Zeldovich/X-ray technique and complementary probes
... on the extragalactic distance ladder, being fully independent of any local calibrator [ 9 , 10 ]; ii) it is a cross-checking for local direct estimates; and iii) it is free from Hubble bubbles, since ... See full document
21
Expected constraints on dark energy parameters with euclid
... agree. In the picture envisaged so far, one can imagine a set of observers, all at rest with respect to the matter distribution in their immediate ...Therefore, the time t measured by ... See full document
105
Galaxy-galaxy lensing in the Dark Energy Survey science verification data
... establish the feasibility of measuring galaxy–galaxy lensing with DES, test our measurement pipelines, and make an estimate of the halo properties for a selected galaxy ...sample. The detailed tests ... See full document
16
On the relative bias of void tracers in the Dark Energy Survey
... on the cosmological principle, voids represent a population of statistically isotropic spheres distributed at different redshifts, allowing us to probe the expansion history of the Universe by ... See full document
18
A search for kilonovae in the Dark Energy Survey
... (GW) from binary black hole mergers (Abbott et ...). The decay of these r-process elements results in isotropic thermal emission and is called a “kilonova” ...as cosmological distance ... See full document
16
Dark energy survey year 1 results: galaxy-galaxy lensing
... all cosmological parameters, the measurements of galaxy clustering and galaxy-galaxy lensing can provide independent measurements of the galaxy bias of a given lens ...population. The DES Y1 ... See full document
28
Dark Energy Survey year 1 results: constraints on extended cosmological models from galaxy clustering and weak lensing
... Cruz, the University of Cambridge, Centro de Investigaciones Energ´eticas, Medioambientales y Tecnológicas-Madrid, the University of Chicago, University College London, the DES-Brazil Consortium, ... See full document
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