1,046 research outputs found
Immigrati e diritti sociali
Il saggio analizza in chiave critica i problemi pi\uf9 attuali della protezione socia\uacle degli immigrati. Dopo avere ricostruito il quadro normativo attualmente vigente, l\u2019A. esamina le pronunce giurisprudenziali pi\uf9 significative in materia di parit\ue0 di trattamento e divieto di discriminazione, valutandone l\u2019impatto con riferimento ai diversi status di immigrato. L\u2019ultima parte \ue8 dedicata alla questione della condizionalit\ue0 delle prestazioni di assistenza sociale a causa dei vincoli di bilancio imposti agli Stati dalla nuova governance europea.The paper proposes a critical view of the most actual problems concerning social protection of migrant people. On the one hand, it presents the in force legal framework; on the other hand, it examines the most relevant judgements on both equality and non discrimination principles, to compare them with the several immigrant's status. Eventually, due to EU budget limits laid down by Commission, it deal with the main question of relationship between condi\uactionality of social protections and budget balance.
Visualization, Exploration and Data Analysis of Complex Astrophysical Data
In this paper we show how advanced visualization tools can help the
researcher in investigating and extracting information from data. The focus is
on VisIVO, a novel open source graphics application, which blends high
performance multidimensional visualization techniques and up-to-date
technologies to cooperate with other applications and to access remote,
distributed data archives. VisIVO supports the standards defined by the
International Virtual Observatory Alliance in order to make it interoperable
with VO data repositories. The paper describes the basic technical details and
features of the software and it dedicates a large section to show how VisIVO
can be used in several scientific cases.Comment: 32 pages, 15 figures, accepted by PAS
Automated reliability assessment for spectroscopic redshift measurements
We present a new approach to automate the spectroscopic redshift reliability
assessment based on machine learning (ML) and characteristics of the redshift
probability density function (PDF).
We propose to rephrase the spectroscopic redshift estimation into a Bayesian
framework, in order to incorporate all sources of information and uncertainties
related to the redshift estimation process, and produce a redshift posterior
PDF that will be the starting-point for ML algorithms to provide an automated
assessment of a redshift reliability.
As a use case, public data from the VIMOS VLT Deep Survey is exploited to
present and test this new methodology. We first tried to reproduce the existing
reliability flags using supervised classification to describe different types
of redshift PDFs, but due to the subjective definition of these flags, soon
opted for a new homogeneous partitioning of the data into distinct clusters via
unsupervised classification. After assessing the accuracy of the new clusters
via resubstitution and test predictions, unlabelled data from preliminary mock
simulations for the Euclid space mission are projected into this mapping to
predict their redshift reliability labels.Comment: Submitted on 02 June 2017 (v1). Revised on 08 September 2017 (v2).
Latest version 28 September 2017 (this version v3
The VIMOS Ultra Deep Survey. Luminosity and stellar mass dependence of galaxy clustering at z~3
We present the study of the dependence of galaxy clustering on luminosity and
stellar mass in the redshift range 2z3.5 using 3236 galaxies with robust
spectroscopic redshifts from the VIMOS Ultra Deep Survey (VUDS). We measure the
two-point real-space correlation function for four volume-limited
stellar mass and four luminosity, M absolute magnitude selected,
sub-samples. We find that the scale dependent clustering amplitude
significantly increases with increasing luminosity and stellar mass indicating
a strong galaxy clustering dependence on these properties. This corresponds to
a strong relative bias between these two sub-samples of b/b=0.43.
Fitting a 5-parameter HOD model we find that the most luminous and massive
galaxies occupy the most massive dark matter haloes with
M = 10 h M. Similar to the
trends observed at lower redshift, the minimum halo mass M depends on
the luminosity and stellar mass of galaxies and grows from M
=10 hM to M=10 hM
from the faintest to the brightest among our galaxy sample, respectively. We
find the difference between these halo masses to be much more pronounced than
is observed for local galaxies of similar properties. Moreover, at z~3, we
observe that the masses at which a halo hosts, on average, one satellite and
one central galaxy is M4M over all luminosity ranges,
significantly lower than observed at z~0 indicating that the halo satellite
occupation increases with redshift. The luminosity and stellar mass dependence
is also reflected in the measurements of the large scale galaxy bias, which we
model as b(L)=1.92+25.36(L/L). We conclude our study
with measurements of the stellar-to-halo mass ratio (SHMR).Comment: 20 pages, 11 figures, A&A in press, v2. revised discussion in sec.
5.5, changed Fig. 4 and Fig. 11, added reference
Spectroscopic surveys:a different approach to data reduction
We present VIPGI, an automatized human supervised reduction environment,
developed within the VIRMOS project to handle VIMOS guaranteed time data. VIPGI
is now offered to the international community to be used on site in Milano and
Marseille. Born to handle the highly multiplexed MOS VIMOS data, it has been
extended to accomodate also IFU data. The widespread and extensive use of VIPGI
has suggested the idea of an integrated environment allowing users not only to
reduce, but also to organize data in logical structures, to insert results in a
database, and use any user defined plugin for data reduction, analysis and
inspection. See http://cosmos.mi.iasf.cnr.it/pandoraComment: Astronomical Data Analysis III conference proceedin
Observing the high redshift universe using the VIMOS-IFU
We describe the advantages of using Integral Field Spectroscopy to observe
deep fields of galaxy. The VIMOS Integral Field Unit is particularly suitable
for this kind of studies thanks to its large field-of-view (~ 1 arcmin^2).
After a short description of the VIMOS-IFU data reduction, we detail the main
scientific issues which can be addressed using observations of the Hubble Deep
Field South with a combination of Integral Field Spectroscopy and broad band
optical and Near-Infrared imaging.Comment: 4 pages, accepted for publishing in AN (ref. proc. of Euro3D Science
workshop, IoA Cambridge, May 2003
- …