Enrique Gaztañaga researcher
Gaztañaga Balbás, Enrique
VIAF ID: 86632958 (Personal)
Permalink: http://viaf.org/viaf/86632958
Preferred Forms
- 100 0 _ ‡a Enrique Gaztañaga ‡c researcher
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- 100 1 0 ‡a Gaztañaga Balbás, Enrique
- 100 1 _ ‡a Gaztañaga Balbás, Enrique
4xx's: Alternate Name Forms (2)
Works
Title | Sources |
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Cosmologia i formació d'estructures Cosmology and structures formation | |
Cosmological perturbation theory and the spherical collapse model | |
Cosmology with galaxy surveys : how galaxies trace mass at large scales | |
Cross-correlating spectroscopic and photometric galaxy surveys | |
The Formation of large scale structures in the universe : new hints from the power spectrum and the three-point correlation function | |
GALAXIES IN X-RAY SELECTED CLUSTERS AND GROUPS IN DARK ENERGY SURVEY DATA. I. STELLAR MASS GROWTH OF BRIGHT CENTRAL GALAXIES SINCEz∼ 1.2 | |
Higher resolution photometric redshifts for cosmological surveys | |
Large-Scale Clustering from Non-Gaussian Texture Models | |
Large scale structure and dark energy | |
Large‐Scale Structures in the Early Sloan Digital Sky Survey: Comparison of the North and South Galactic Strips | |
The local bias model in the large-scale halo distribution | |
Mapping and simulating systematics due to spatially varying observing conditions in DES science verification data | |
Measurement of the gravitational potential evolution from the cross-correlation betweenWMAPand the APM Galaxy Survey | |
The MICE grand challenge lightcone simulation – I. Dark matter clustering | |
Modelos estadísticos de la estructura a gran escala del universo | |
Models of the strongly lensed quasar DES J0408−5354 | |
More out of less: an excess integrated Sachs–Wolfe signal from supervoids mapped out by the Dark Energy Survey | |
N-point correlation functions in the CfA and SSRS redshift distribution of galaxies | |
Nearest Neighbor: The Low-mass Milky Way Satellite Tucana III | |
New light on dark cosmos | |
A new method to measure galaxy bias by combining the density and weak lensing fields | |
nIFTy cosmology: the clustering consistency of galaxy formation models | |
No galaxy left behind: accurate measurements with the faintest objects in the Dark Energy Survey | |
Non-local bias contribution to third-order galaxy correlations | |
Nonlinear Gravitational Growth Inside and Outside the Standard Cosmology | |
Observation of two new L4 Neptune trojans in the dark energy survey supernova fields | |
On the APM power spectrum and the CMB anisotropy: evidence for a phase transition during inflation? | |
On the Evolution of Cosmological Type IA Supernovae and the Gravitational Constant | |
On the Interpretation of Clustering from the Angular APM Galaxy Survey | |
On the probability distribution for the cosmological constant | |
The onion universe: all sky lightcone simulations in spherical shells | |
Optical–SZE scaling relations for DES optically selected clusters within the SPT-SZ Survey | |
Optimising the measurement of relativistic distortions in large-scale structure | |
Overview of the DESI Legacy Imaging Surveys | |
OzDES multifibre spectroscopy for the Dark Energy Survey: first-year operation and results | |
Paint it black weak lensing analysis of an all-sky simulation | |
The PAU camera at the WHT | |
PAUCam filter interchange system | |
Photo-z quality cuts and their effect on the measured galaxy clustering | |
Photometric redshifts and clustering of emission line galaxies selected jointly by DES and eBOSS | |
Populating cosmological simulations with galaxies using the HOD model | |
Precise photometric redshifts with a narrow-band filter set: the PAU survey at the William Herschel Telescope | |
A prescription for galaxy biasing evolution as a nuisance parameter | |
Probing the statistics of primordial fluctuations and their evolution | |
Processing and compression of noise-dominated data: application to the cosmic microwave background data on board the Planck satellite | |
Reconstruction of cosmological density and velocity fields in the Lagrangian Zel'dovich approximation | |
Recovering 3D clustering information with angular correlations | |
redMaGiC: selecting luminous red galaxies from the DES Science Verification data | |
Redshift inference from the combination of galaxy colours and clustering in a hierarchical Bayesian model – Application to realistic <i>N</i>-body simulations | |
Redshift-space distortions from the cross-correlation of photometric populations | |
The Scale Dependence of Mass Assembly in Galaxies | |
The SCUBA Half-Degree Extragalactic Survey -- I. Survey motivation, design and data processing | |
SDSS-IV eBOSS emission-line galaxy pilot survey | |
SEARCH FOR GAMMA-RAY EMISSION FROM DES DWARF SPHEROIDAL GALAXY CANDIDATES WITHFERMI-LAT DATA | |
Search for RR Lyrae stars in DES ultrafaint systems: Grus I, Kim 2, Phoenix II, and Grus II | |
Searching for an Early Epoch of Star Formation with MM/Sub-MM Blank Field Surveys | |
Simulating the Universe with MICE: the abundance of massive clusters | |
The Space Density of Galaxy Peaks and the Linear Matter Power Spectrum | |
Star/galaxy separation at faint magnitudes: application to a simulated Dark Energy Survey | |
Statistical analysis of galaxy surveys — II. The three-point galaxy correlation function measured from the 2dFGRS | |
Statistical analysis of galaxy surveys - IV. An objective way to quantify the impact of superstructures on galaxy clustering statistics | |
Statistical distribution of number-density fluctuations of galaxies | |
Status of the Dark Energy Survey Camera (DECam) project | |
Stellar kinematics and metallicities in the ultra-faint dwarf galaxy Reticulum II | |
Subhaloes gone Notts: the clustering properties of subhaloes | |
Supplement: "Localization and broadband follow-up of the gravitational-wave transient GW150914" (2016, ApJL, 826, L13) | |
Testing Ansatze for quasi-non-linear clustering: the linear APM power spectrum | |
Testing deprojection algorithms on mock angular catalogues: evidence for a break in the power spectrum | |
Testing the lognormality of the galaxy and weak lensing convergence distributions from Dark Energy Survey maps | |
Tracing the sound horizon scale with photometric redshift surveys | |
Void probability as a function of the void's shape and scale-invariant models | |
What determines large scale galaxy clustering: halo mass or local density? | |
Wide-field lensing mass maps from Dark Energy Survey science verification data: Methodology and detailed analysis |