164 citations · 380 across the 10 of their papers we have counts for
10 papers
The best fit for the observed galaxy Counts-in-Cell distribution function
Ll. Hurtado-Gil, V. J. Martínez, P. Arnalte-Mur +3
The Sloan Digital Sky Survey (SDSS) is the first dense redshift survey encompassing a volume large enough to find the best analytic probability density function that fits the galax…
The ALHAMBRA survey: evolution of galaxy spectral segregation
Ll. Hurtado-Gil, P. Arnalte-Mur, V. J. Martínez +28
We study the clustering of galaxies as a function of spectral type and redshift in the range using data from the Advanced Large Homogeneous Area Medium Band Redshi…
Joint constraints on galaxy bias and through the N-pdf of the galaxy number density
Pablo Arnalte-Mur, Patricio Vielva, Vicent J. Martínez +3
We present a full description of the N-probability density function of the galaxy number density fluctuations. This N-pdf is given in terms, on the one hand, of the cold dark matte…
Wavelet analysis of baryon acoustic structures in the galaxy distribution
P. Arnalte-Mur, A. Labatie, N. Clerc +5
Baryon Acoustic Oscillations (BAO) are a feature imprinted in the density field by acoustic waves travelling in the plasma of the early universe. Their fixed scale can be used as a…
Reliability of the detection of the Baryon Acoustic Peak
Vicent J. Martinez, Pablo Arnalte-Mur, Enn Saar +5
The correlation function of the distribution of matter in the universe shows, at large scales, baryon acoustic oscillations, which were imprinted prior to recombination. This featu…
Measuring Baryon Acoustic Oscillations along the line of sight with photometric redshifs: the PAU survey
N. Benitez, E. Gaztanaga, R. Miquel +24
Baryon Acoustic Oscillations (BAO) provide a standard ruler of known physical length, making it a promising probe of the nature of dark energy. The detection of BAO requires measur…