Seljak, Uroš
Seljak, Uroš 1966-
Uroš Seljak physicist
VIAF ID: 546145858153223022413 ( Personal )
Permalink: http://viaf.org/viaf/546145858153223022413
Preferred Forms
- 100 1 _ ‡a Seljak, Uroš ‡d 1966-
- 100 1 _ ‡a Seljak, Uroš
- 100 1 _ ‡a Seljak, Uroš ‡d 1966-
- 100 0 _ ‡a Uroš Seljak ‡c physicist
4xx's: Alternate Name Forms (10)
Works
Title | Sources |
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[Beta] polarization of the cosmic microwave background as a tracer of strings | |
Cosmological constraints from the cosmic microwave background and Lyman-alpha forest revisited | |
Cosmological model predictions for weak lensing: linear and nonlinear regimes | |
Cosmological parameter constraints from galaxy-galaxy lensing and galaxy clustering with the SDSS DR7 | |
Cosmological parameters from recent cosmological datasets including Lyman-alpha forest data | |
Density profiles of galaxy groups and clusters from SDSS galaxy-galaxy weak lensing | |
Detectability of tensor modes in the presence of foregrounds | |
Determination of the relative branching rations for p[bar]p [to] [pi][sup]+ [pi][sup]- and p[bar]p [to] K[sup]+K[sup]- | |
Ellipticity of dark matter haloes with galaxy-galaxy weak lensing | |
Exact likelihood evaluations and foreground marginalization in low resolution WMAP data | |
Galaxy-dark matter correlations applied to galaxy-galaxy lensing: predictions from the semi-analytic galaxy formation models | |
Galaxy-galaxy lensing: dissipationless simulations versus the halo model | |
Galaxy-galaxy lensing estimators and their covariance properties | |
Global Expansion in an Inhomogeneous Universe | |
Gravitational lensing as a contaminant of the gravity wave signal in the CMB | |
Halo concentration and the dark matter power spectrum | |
Initial performance of CPLEAR | |
Integral solution for the microwave background anisotropies in nonflat universes | |
Intrinsic alignment-lensing interference as a contaminant of cosmic shear | |
"Kaj je razlog, da v vesolju sploh kaj je" : prof. dr. Uroš Seljak | |
Kramljanje o kozmologiji | |
Large-scale bias and stochasticity of haloes and dark matter | |
Lensing-induced cluster signatures in the cosmic microwave background | |
The LHC Olympics 2020 : a community challenge for anomaly detection in high energy physics | |
Light propagation in a weekly perturbed expanding universe : [dissertation] | |
Limits on High (De)Magnification Supernova Events from Power Spectrum Constraints | |
Limits on the density of compact objects from high redshift supernovae | |
The linear theory power spectrum from the Ly[alpha] forest in the Sloan Digital Sky Survey | |
Mapping the universe from weak lensing analysis | |
Maximum-likelihood analysis of the COBE angular correlation function | |
Measurement of baryon acoustic oscillations in the Lyman-alpha forest fluctuations in BOSS data release 9 | |
Measurement of the reaction [pi][sup]+ p [to] [pi][sup]+ [pi][sup]+ n near threshold | |
Od skrivnosti vesolja do žalostne statistike koronavirusa : Uroš Seljak, slovenski profesor na univerzi Berkley, je obdelal podatke smrtnosti za 1600 krajev v Italiji | |
On estimating the QSO transmission power spectrum | |
Pairwise velocities in the halo model: luminosity and scale dependence | |
Physical effects on the Ly[alpha] forest flux power spectrum : damping wings, ionizing radiation fluctuations and galactic winds | |
Power spectra in global defect theories of cosmic structure formation | |
Predstavljamo naše naravoslovne raziskovalce : Uroš Seljak - Packardov nagrajenec | |
Primorski fizik v svetu : dr. Uroš Seljak je postal raziskovalec Harvardske univerze | |
Prospects for ACT : simulations, power spectrum, and non-Gaussian analysis | |
Recent results of PS195 CPLEAR( tests of CP violation with K0 anti-K0 AT LEAR | |
Reconstructing projected matter density power spectrum from cosmic microwave background | |
Redshift-space bias and ß from the halo model | |
Rees-Sciama effect in a cold dark matter universe | |
Scalar, vector, and tensor contributions to CMB anisotropies from cosmic defects | |
SDSS DR4 | |
SDSS galaxy bias from halo mass-bias relation and its cosmological implications | |
The SDSS-IV Extended Baryon Oscillation Spectroscopic Survey overview and early data | |
Sekundarni pojavi v prasevanju : diplomsko delo | |
Shear and ellipticity in gravitational lenses | |
Shear calibration biases in weak-lensing surveys | |
Signatures of relativistic neutrinos in CMB anisotropy and matter clustering | |
Sloan Digital Sky Survey imaging of low Galactic latitude fields : technical summary and data release | |
Status of the CP LEAR experiment and first results : presented at Workshop on Testing CPT and Studying CP Violation at a [phi]- Factory, Ucla 1990 | |
Študij reakcije [pi][zgoraj]+ [v] [pi][zgoraj]+[pi][zgoraj]0p : diplomsko delo | |
Študij temne energije z gravitacijskim lečjem : diplomsko delo | |
The Sunyaev-Zel'dovich angular power spectrum as a probe of cosmological parameters | |
Sunyaev-Zeldovich effect from hydrodynamical simulations | |
Systematic errors in weak lensing : applicetion to SDSS galaxy-galagy weak lensing | |
Tentative detection of galaxy spin correlations in the Tully catalog | |
Testing the theoretical models using potent reconstructed density field | |
Tvorba resonanc pri procesu p[p s črto] [v] K[zgoraj]+K[zgoraj]-[pi][zgoraj]+[pi][zgoraj]- : magistrsko delo | |
Universal gas density and temperature profile | |
Upanje je, da bomo dobili popolnejšo sliko sestave in nastanka vesolja : prof. dr. Uroš Seljak, dobitnik Packardove nagrade | |
Virial masses of galactic haloes from galaxy-galaxy lensing: theoretical modelling and application to Sloan Digital Sky Survey data | |
Weak lensing and CMB : parameter forecasts including a running spectral index | |
Weak lensing by large-scale structure | |
Weak lensing reconstruction and power spectrum estimation: minimum variance methods |