213 research outputs found
Aggressive immunosuppressive treatment of Susac's syndrome in an adolescent: using treatment of dermatomyositis as a model
We describe aggressive immunosuppressive treatment of an adolescent with Susac's syndrome (SS), a disease of the microvasculature in the brain, retina, and inner ear. Because the immunopathogenesis of SS appears to have much in common with that of juvenile dermatomyositis (JDM), the patient was treated with an approach that has been effective for severe JDM. The patient's outcome provides evidence for the importance of prompt, aggressive, and sustained immunosuppressive treatment of encephalopathic SS
The CFHTLS Strong Lensing Legacy Survey: I. Survey overview and T0002 release sample
AIMS: We present data from the CFHTLS Strong Lensing Legacy Survey (SL2S).
Due to the unsurpassed combined depth, area and image quality of the
Canada-France-Hawaii Legacy Survey it is becoming possible to uncover a large,
statistically well-defined sample of strong gravitational lenses which spans
the dark halo mass spectrum predicted by the concordance model from galaxy to
cluster haloes. METHODS: We describe the development of several automated
procedures to find strong lenses of various mass regimes in CFHTLS images.
RESULTS: The preliminary sample of about 40 strong lensing candidates
discovered in the CFHTLS T0002 release, covering an effective field of view of
28 deg is presented. These strong lensing systems were discovered using an
automated search and consist mainly of gravitational arc systems with splitting
angles between 2 and 15 arcsec. This sample shows for the first time that it is
possible to uncover a large population of strong lenses from galaxy groups with
typical halo masses of about . We discuss the future
evolution of the SL2S project and its main scientific aims for the next 3
years, in particular our observational strategy to extract the hundreds of
gravitational rings also present in these fields.Comment: 11 pages, 5 figures, A&A in pres
Хірургічне лікування нирковоклітинного раку з внутрішньовенозним розповсюдженням та імплантацією тромбу в стінку нижньої порожнистої вени
This work presents the results of surgical treatment of renal cell carcinoma with internally venous dissemination and implantation of thrombus intra vena cava inferior tissue. In 3 cases was performed a prosthesis of vena cava inferior byGoreTexor PTFE prothesis (2 – above the renal veins, 1 – below the renal veins). Histologically confirmed an invasion of tumor thrombus by renal cell carcinoma intra vena cava inferior tissue is an evidence to resection of tissue or an area of vena cava inferior which repairs via prosthesis.У роботі представлено результати хірургічного лікування нирковоклітинного раку з внутрішньовенозним розповсюдженням та імплантацією тромбу в стінку нижньої порожнистої вени. У 3 випадках виконано протезування нижньої порожнистої вени протезами Gore Tex чи ПТФЕ (2 – вище ниркових вен, 1 – нижче ниркових вен). Гістологічно підтверджена інвазія пухлинного тромбу при нирковоклітинному раку в стінку нижньої порожнистої вени є показанням до резекції стінки чи ділянки нижньої порожнистої вени, яка відновлюється за допомогою протезування
Gauging the dark matter fraction in a S0 galaxy at z=0.47 through gravitational lensing from deep HST/ACS imaging
We analyze a new gravitational lens, OAC-GL J1223-1239, serendipitously found
in a deep I-band image of the Hubble Space Telescope (HST) Advanced Camera for
Surveys (ACS). The lens is a L_*, edge-on S0 galaxy at z=0.4656. The
gravitational arc has a radius of 0.42 arcsec. We have determined the total
mass and the dark matter (DM) fraction within the Einstein radius as a function
of the lensed source redshift, which is presently unknown. For z ~ 1.3, which
is in the middle of the redshift range plausible for the source according to
some external constraints, we find the central velocity dispersion to be ~180
km/s. With this value, close to that obtained by means of the Faber-Jackson
relation at the lens redshift, we compute a 30% DM fraction within the Einstein
radius (given the uncertainty in the source redshift, the allowed range for the
DM fraction is 25-35 % in our lensing model). When compared with the galaxies
in the local Universe, the lensing galaxy, OAC-GL J1223-1239 seems to fall in
the transition regime between massive DM dominated galaxies and lower-mass, DM
deficient systems.Comment: 18 pages, 5 figures; accepted for publication in Ap
The Structure & Dynamics of Massive Early-type Galaxies: On Homology, Isothermality and Isotropy inside one Effective Radius
Based on 58 SLACS strong-lens early-type galaxies with direct total-mass and
stellar-velocity dispersion measurements, we find that inside one effective
radius massive elliptical galaxies with M_eff >= 3x10^10 M_sun are
well-approximated by a power-law ellipsoid with an average logaritmic density
slope of = -dlog(rho_tot)/dlog(r)=2.085^{+0.025}_{-0.018} (random
error on mean) for isotropic orbits with beta_r=0, +-0.1 (syst.) and
sigma_gamma' <= 0.20^{+0.04}_{-0.02} intrinsic scatter (all errors indicate the
68 percent CL). We find no correlation of gamma'_LD with galaxy mass (M_eff),
rescaled radius (i.e. R_einst/R_eff) or redshift, despite intrinsic differences
in density-slope between galaxies. Based on scaling relations, the average
logarithmic density slope can be derived in an alternative manner, fully
independent from dynamics, yielding =1.959 +- 0.077. Agreement
between the two values is reached for =0.45 +- 0.25, consistent with
mild radial anisotropy. This agreement supports the robustness of our results,
despite the increase in mass-to-light ratio with total galaxy mass: M_eff ~
L_{V,eff}^(1.363+-0.056). We conclude that massive early-type galaxies are
structurally close-to homologous with close-to isothermal total density
profiles (<=10 percent intrinsic scatter) and have at most some mild radial
anisotropy. Our results provide new observational limits on galaxy formation
and evolution scenarios, covering four Gyr look-back time.Comment: Accepted for publication by ApJL; 4 pages, 2 figure
A new gravitational lens from the MUSCLES survey: ULAS J082016.1+081216
We present observations of a new double-image gravitational lens system, ULAS
J082016.1+081216, of image separation 2.3" and high (~6) flux ratio. The system
is selected from the Sloan Digital Sky Survey spectroscopic quasar list using
new high-quality images from the UKIRT Deep Sky Survey (UKIDSS). The lensed
quasar has a source redshift of 2.024, and we identify the lens galaxy as a
faint red object of redshift 0.803+/-0.001. Three other objects from the UKIDSS
survey, selected in the same way, were found not to be lens systems. Together
with the earlier lens found using this method, the SDSS-UKIDSS lenses have the
potential to significantly increase the number of quasar lenses found in SDSS,
to extend the survey to higher flux ratios and lower separations, and to give
greater completeness which is important for statistical purposes.Comment: Accepted by MNRAS. 6 pages, 5 figure
The redshift distribution of gravitational lenses revisited: Constraints on galaxy mass evolution
The redshifts of lens galaxies in known gravitational lens systems probe the
volume distribution of lensing mass. Following earlier work by Kochanek, we
re-derive the lens redshift probability distribution, allowing for mass and
number density evolution of the lensing galaxies, and apply this test to a much
enlarged sample of lens systems. From a literature survey of all known lenses,
we have selected an unbiased sample of 15 lenses with complete redshift
information. For a flat Universe and no lens evolution, we can only put an
upper limit on the cosmological constant of Omega_lambda<0.89 at the 95% CL.
Omega_lambda~0.7 and no evolution is consistent with the data. Allowing for
evolution in an Omega_m=0.3, Omega_lambda=0.7 cosmology, we find that the
best-fit evolution in sigma* (i.e., the characteristic velocity dispersion in a
Schechter-like function) of early-type galaxies, in the redshift range z~0 to
1, is d[log sigma*(z)]/dz=-0.10+/-0.06. This is consistent with no evolution
and implies that, at 95% CL, sigma* of early-type galaxies at z~1 was at least
63% of its current value. Alternatively, if there is no mass evolution, a
present-day value of sigma*>175 km/s for elliptical galaxies is required (95%
CL).Comment: 15 pages, MNRAS, in pres
Semi-empirical catalog of early-type galaxy-halo systems: dark matter density profiles, halo contraction and dark matter annihilation strength
With SDSS galaxy data and halo data from up-to-date N-body simulations we
construct a semi-empirical catalog (SEC) of early-type systems by making a
self-consistent bivariate statistical match of stellar mass (M_star) and
velocity dispersion (sigma) with halo virial mass (M_vir). We then assign
stellar mass profile and velocity dispersion profile parameters to each system
in the SEC using their observed correlations with M_star and sigma.
Simultaneously, we solve for dark matter density profile of each halo using the
spherical Jeans equation. The resulting dark matter density profiles deviate in
general from the dissipationless profile of NFW or Einasto and their mean inner
density slope and concentration vary systematically with M_vir. Statistical
tests of the distribution of profiles at fixed M_vir rule out the null
hypothesis that it follows the distribution predicted by N-body simulations for
M_vir ~< 10^{13.5-14.5} M_solar. These dark matter profiles imply that dark
matter density is, on average, enhanced significantly in the inner region of
halos with M_vir ~< 10^{13.5-14.5} M_solar supporting halo contraction. The
main characteristics of halo contraction are: (1) the mean dark matter density
within the effective radius has increased by a factor varying systematically up
to ~ 3-4 at M_vir = 10^{12} M_solar, and (2) the inner density slope has a mean
of ~ 1.3 with rho(r) ~ r^{-alpha} and a halo-to-halo rms scatter of
rms(alpha) ~ 0.4-0.5 for 10^{12} M_solar ~< M_vir ~< 10^{13-14} M_solar steeper
than the NFW profile (alpha=1). Based on our results we predict that halos of
nearby elliptical and lenticular galaxies can, in principle, be promising
targets for gamma-ray emission from dark matter annihilation.Comment: 43 pages, 20 figures, JCAP, revised and accepted versio
The mass distribution of a moderate redshift galaxy group and brightest group galaxy from gravitational lensing and kinematics
The gravitational lens system CLASS B2108+213 has two radio-loud lensed
images separated by 4.56 arcsec. The relatively large image separation implies
that the lensing is caused by a group of galaxies. In this paper, new optical
imaging and spectroscopic data for the lensing galaxies of B2108+213 and the
surrounding field galaxies are presented. These data are used to investigate
the mass and composition of the lensing structure. The redshift and stellar
velocity dispersion of the main lensing galaxy (G1) are found to be z = 0.3648
+/- 0.0002 and sigma_v = 325 +/- 25 km/s, respectively. The optical spectrum of
the lensed quasar shows no obvious emission or absorption features and is
consistent with a BL Lac type radio source. However, the tentative detection of
the G-band and Mg-b absorption lines, and a break in the spectrum of the host
galaxy of the lensed quasar gives a likely source redshift of z = 0.67.
Spectroscopy of the field around B2108+213 finds 51 galaxies at a similar
redshift to G1, thus confirming that there is a much larger structure at z ~
0.365 associated with this system. The width of the group velocity distribution
is 694 +/- 93 km/s, but is non-Gaussian, implying that the structure is not yet
viralized. The main lensing galaxy is also the brightest group member and has a
surface brightness profile consistent with a typical cD galaxy. A lensing and
dynamics analysis of the mass distribution, which also includes the newly found
group members, finds that the logarithmic slope of the mass density profile is
on average isothermal inside the Einstein radius, but steeper at the location
of the Einstein radius. This apparent change in slope can be accounted for if
an external convergence gradient, representing the underlying parent halo of
the galaxy group, is included in the mass model.Comment: 18 pages, 14 figures, 5 tables, accepted for publication in MNRA
Neurocognition with maraviroc compared with tenofovir in HIV
To determine whether maraviroc (MVC) has unique neurocognitive benefits in the context of initial antiretroviral therapy (ART)
- …