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The VIMOS Public Extragalactic Redshift Survey (VIPERS). Environmental effects shaping the galaxy stellar mass function
I. Davidzon, O. Cucciati, M. Bolzonella +38
We exploit the first public data release of VIPERS to investigate environmental effects in galaxy evolution between and . The large number of spectroscopic redshift…
The absolute age of the globular cluster M15 using near-infrared adaptive optics images from PISCES/LBT
M. Monelli, V. Testa, G. Bono +26
We present deep near-infrared (NIR) J, Ks photometry of the old, metal-poor Galactic globular cluster M\,15 obtained with images collected with the LUCI1 and PISCES cameras availab…
The VIMOS Public Extragalactic Redshift Survey (VIPERS): Reconstruction of the redshift-space galaxy density field
B. R. Granett, E. Branchini, L. Guzzo +43
Aims. Using the VIMOS Public Extragalactic Redshift Survey (VIPERS) we aim to jointly estimate the key parameters that describe the galaxy density field and its spatial correlation…
A high-dimensional look at VIPERS galaxies
B. R. Granett, U. Abbas, C. Adami +44
We investigate how galaxies in VIPERS (the VIMOS Public Extragalactic Redshift Survey) inhabit the cosmological density field by examining the correlations across the observable pa…
The VIMOS Public Extragalactic Redshift Survey (VIPERS). Hierarchical scaling and biasing
A. Cappi, F. Marulli, J. Bel +47
We investigate the higher-order correlation properties of the VIMOS Public Extragalactic Redshift Survey (VIPERS) to test the hierarchical scaling hypothesis at z~1 and the depende…
The VIMOS Public Extragalactic Redshift Survey (VIPERS): On the correct recovery of the count-in-cell probability distribution function
J. Bel, E. Branchini, C. Di Porto +45
We compare three methods to measure the count-in-cell probability density function of galaxies in a spectroscopic redshift survey. From this comparison we found that when the sampl…
HII regions within a compact high velocity cloud. A nearly star-less dwarf galaxy?
M. Bellazzini, L. Magrini, A. Mucciarelli +9
Within the SECCO survey we identified a candidate stellar counterpart to the Ultra Compact High Velocity Cloud (UCHVC) HVC274.68+74.70-123, that was suggested by Adams et al. (2013…