13,444 research outputs found
Protection of Domestic Violence Victims Under the New York City Human Rights Law\u27s Provisions Prohibiting Discrimination on the Basis of Disability
This Article analyzes the need to create a new protected class of domestic violence victims to shield them from discrimination in employment. The Article examines arguments for and against proposed legislation to revise the human rights law governing disability, section 8-107 of the New York City Administration Code. The Article concludes that this legislation is unnecessary because the law already provides sufficient protection to domestic violence victims without requiring that victims disclose their domestic violence status to their employers
Filament Hunting: Integrated HI 21cm Emission From Filaments Inferred by Galaxy Surveys
Large scale filaments, with lengths that can reach tens of Mpc, are the most
prominent features in the cosmic web. These filaments have only been observed
indirectly through the positions of galaxies in large galaxy surveys or through
absorption features in the spectra of high redshift sources. In this study we
propose to go one step further and directly detect intergalactic medium
filaments through their emission in the HI 21cm line. We make use of high
resolution cosmological simulations to estimate the intensity of this emission
in low redshift filaments and use it to make predictions for the direct
detectability of specific filaments previously inferred from galaxy surveys, in
particular the Sloan Digital Sky Survey. Given the expected signal of these
filaments our study shows that HI emission from large filaments can be observed
by current and next generation radio telescopes. We estimate that gas in
filaments of length 15 Mpc with relatively small
inclinations to the line of sight () can be observed in
hours with telescopes such as GMRT or EVLA, potentially providing
large improvements over our knowledge of the astrophysical properties of these
filaments. Due to their large field of view and sufficiently long integration
times, upcoming HI surveys with the Apertif and ASKAP instruments will be able
to detect large filaments independently of their orientation and curvature.
Furthermore, our estimates indicate that a more powerful future radio telescope
like SKA-2 can be used to map most of these filaments, which will allow them to
be used as a strong cosmological probe.Comment: 16 pages, 11 figures, Accepted for publication in MNRA
The exit-time problem for a Markov jump process
The purpose of this paper is to consider the exit-time problem for a
finite-range Markov jump process, i.e, the distance the particle can jump is
bounded independent of its location. Such jump diffusions are expedient models
for anomalous transport exhibiting super-diffusion or nonstandard normal
diffusion. We refer to the associated deterministic equation as a
volume-constrained nonlocal diffusion equation. The volume constraint is the
nonlocal analogue of a boundary condition necessary to demonstrate that the
nonlocal diffusion equation is well-posed and is consistent with the jump
process. A critical aspect of the analysis is a variational formulation and a
recently developed nonlocal vector calculus. This calculus allows us to pose
nonlocal backward and forward Kolmogorov equations, the former equation
granting the various moments of the exit-time distribution.Comment: 15 pages, 7 figure
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An evaluation of the Amblyopia and Strabismus Questionnaire using Rasch analysis
noPURPOSE. To evaluate whether the Amblyopia and Strabismus Questionnaire (A&SQ) is a suitable instrument for the assessment of vision-related quality-of life (VR-QoL) in individuals with strabismus and/or amblyopia.
METHODS. The A&SQ was completed by 102 individuals, all of whom had amblyopia, strabismus, or both. Rasch analysis was used to evaluate the usefulness of individual questionnaire items (i.e., questions); the response-scale performance; how well the items targeted VR-QoL; whether individual items showed response bias, depending on factors such as whether strabismus was present; and dimensionality.
RESULTS. Items relating to concerns about the appearance of the eyes were applicable only to those with strabismus, and many items showed large ceiling effects. The response scale showed disordered responses and underused response options, which improved after the number of response options was reduced from five to three. This change improved the discriminative ability of the questionnaire (person separation index increased from 1.98 to 2.11). Significant bias was found between strabismic and nonstrabismic respondents. Separate Rasch analyses conducted for subjects with and without strabismus indicated that all A&SQ items seemed appropriate for individuals with strabismus (Rasch infit values between 0.60 and 1.40), but several items fitted the model poorly in amblyopes without strabismus. The AS&Q was not found to be unidimensional.
CONCLUSIONS. The findings highlight the limitations of the A&SQ instrument in the assessment of VR-QoL in subjects with strabismus and especially in those with amblyopia alone. The results suggest that separate instruments are needed to quantify VR-QoL in amblyopes with and without strabismus
Tomographic Intensity Mapping versus Galaxy Surveys: Observing the Universe in H-alpha emission with new generation instruments
The H-alpha line emission is an important probe for a number of fundamental
quantities in galaxies, including their number density, star formation rate
(SFR) and overall gas content. A new generation of low-resolution intensity
mapping probes, e.g. SPHEREx and CDIM, will observe galaxies in H-alpha
emission over a large fraction of the sky from the local Universe till a
redshift of z ~ 6 to 10, respectively. This will also be the target line for
observations by the high-resolution Euclid and WFIRST instruments in the z ~
0.7 - 2 redshift range. In this paper, we estimate the intensity and power
spectra of the H-alpha line in the z ~ 0 - 5 redshift range using observed line
luminosity functions (LFs), when possible, and simulations, otherwise. We
estimate the significance of our predictions by accounting for the modelling
uncertainties (e.g. SFR, extinction, etc.) and observational contamination. We
find that Intensity Mapping (IM) surveys can make a statistical detection of
the full H-alpha emission between z ~ 0.8 - 5. Moreover, we find that the
high-frequency resolution and the sensitivity of the planned CDIM surveys allow
for the separation of H-alpha emission from several interloping lines. We
explore ways to use the combination of these line intensities to probe galaxy
properties. As expected, our study indicates that galaxy surveys will only
detect bright galaxies that contribute up to a few percent of the overall
H-alpha intensity. However, these surveys will provide important constraints on
the high end of the H-alpha LF and put strong constraints on the AGN LF.Comment: Submitted to MNRA
Cosmology with intensity mapping techniques using atomic and molecular lines
We present a systematic study of the intensity mapping technique using
updated models for the different emission lines from galaxies and identify
which ones are more promising for cosmological studies of the post reionization
epoch. We consider the emission of , , H,
optical and infrared oxygen lines, nitrogen lines, CII and the CO rotational
lines. We then identify that , , OII, CII and
the lowest rotational CO lines are the best candidates to be used as IM probes.
These lines form a complementary set of probes of the galaxies emission
spectra. We then use reasonable experimental setups from current, planned or
proposed experiments to access the detectability of the power spectrum of each
emission line. Intensity mapping of emission from to 3
will be possible in the near future with HETDEX, while far-infrared lines
require new dedicated experiments. We also show that the proposed SPHEREx
satellite can use OII and IM to study the large-scale
distribution of matter in intermediate redshifts of 1 to 4. We found that
submilimeter experiments with bolometers can have similar performances at
intermediate redshifts using CII and CO(3-2).Comment: 18 pages, 21 figures, 5 tables, published in MNRAS, typos correcte
Modularity from Fluctuations in Random Graphs and Complex Networks
The mechanisms by which modularity emerges in complex networks are not well
understood but recent reports have suggested that modularity may arise from
evolutionary selection. We show that finding the modularity of a network is
analogous to finding the ground-state energy of a spin system. Moreover, we
demonstrate that, due to fluctuations, stochastic network models give rise to
modular networks. Specifically, we show both numerically and analytically that
random graphs and scale-free networks have modularity. We argue that this fact
must be taken into consideration to define statistically-significant modularity
in complex networks.Comment: 4 page
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