3,328 research outputs found
Properties of galaxy dark matter halos from weak lensing
We present the results of a study of weak lensing by galaxies based on 45.5
deg of band imaging data from the Red-Sequence Cluster Survey (RCS).
We present the first weak lensing detection of the flattening of galaxy dark
matter halos. We use a simple model in which the ellipticity of the halo is
times the observed ellipticity of the lens. We find a best fit value of
, suggesting that the dark matter halos are somewhat
rounder than the light distribution. The fact that we detect a significant
flattening implies that the halos are well aligned with the light distribution.
Given the average ellipticity of the lenses, this implies a halo ellipticity of
, in fair agreement with results from
numerical simulations of CDM. This result provides strong support for the
existence of dark matter, as an isotropic lensing signal is excluded with 99.5%
confidence. We also study the average mass profile around the lenses, using a
maximum likelihood analysis. We consider two models for the halo mass profile:
a truncated isothermal sphere (TIS) and an NFW profile. We adopt
observationally motivated scaling relations between the lens luminosity and the
velocity dispersion and the extent of the halo. The best fit NFW model yields a
mass and a scale
radius kpc. This value for the scale radius is
in excellent agreement with predictions from numerical simulations for a halo
of this mass.Comment: Significantly revised version, accepted for publication in ApJ 11
pages, 6 figure
Robustness of Cosmological Simulations I: Large Scale Structure
The gravitationally-driven evolution of cold dark matter dominates the
formation of structure in the Universe over a wide range of length scales.
While the longest scales can be treated by perturbation theory, a fully
quantitative understanding of nonlinear effects requires the application of
large-scale particle simulation methods. Additionally, precision predictions
for next-generation observations, such as weak gravitational lensing, can only
be obtained from numerical simulations. In this paper, we compare results from
several N-body codes using test problems and a diverse set of diagnostics,
focusing on a medium resolution regime appropriate for studying many
observationally relevant aspects of structure formation. Our conclusions are
that -- despite the use of different algorithms and error-control methodologies
-- overall, the codes yield consistent results. The agreement over a wide range
of scales for the cosmological tests is test-dependent. In the best cases, it
is at the 5% level or better, however, for other cases it can be significantly
larger than 10%. These include the halo mass function at low masses and the
mass power spectrum at small scales. While there exist explanations for most of
the discrepancies, our results point to the need for significant improvement in
N-body errors and their understanding to match the precision of near-future
observations. The simulation results, including halo catalogs, and initial
conditions used, are publicly available.Comment: 32 pages, 53 figures, data from the simulations is available at
http://t8web.lanl.gov/people/heitmann/arxiv, accepted for publication in
ApJS, several minor revisions, reference added, main conclusions unchange
Electrical Control of 2D Magnetism in Bilayer CrI3
The challenge of controlling magnetism using electric fields raises
fundamental questions and addresses technological needs such as low-dissipation
magnetic memory. The recently reported two-dimensional (2D) magnets provide a
new system for studying this problem owing to their unique magnetic properties.
For instance, bilayer chromium triiodide (CrI3) behaves as a layered
antiferromagnet with a magnetic field-driven metamagnetic transition. Here, we
demonstrate electrostatic gate control of magnetism in CrI3 bilayers, probed by
magneto-optical Kerr effect (MOKE) microscopy. At fixed magnetic fields near
the metamagnetic transition, we realize voltage-controlled switching between
antiferromagnetic and ferromagnetic states. At zero magnetic field, we
demonstrate a time-reversal pair of layered antiferromagnetic states which
exhibit spin-layer locking, leading to a remarkable linear dependence of their
MOKE signals on gate voltage with opposite slopes. Our results pave the way for
exploring new magnetoelectric phenomena and van der Waals spintronics based on
2D materials.Comment: To appear in Nature Nanotechnolog
NCS-1 associates with adenosine A2A receptors and modulates receptor function
Modulation of G protein-coupled receptor (GPCR) signaling by local changes in intracellular calcium concentration is an established function of Calmodulin (CaM) which is known to interact with many GPCRs. Less is known about the functional role of the closely related neuronal EF-hand Ca2+-sensor proteins that frequently associate with CaM targets with different functional outcome. In the present study we aimed to investigate if a target of CaMâthe A2A adenosine receptor is able to associate with two other neuronal calcium binding proteins (nCaBPs), namely NCS-1 and caldendrin. Using bioluminescence resonance energy transfer (BRET) and co-immunoprecipitation experiments we show the existence of A2AâNCS-1 complexes in living cells whereas caldendrin did not associate with A2A receptors under the conditions tested. Interestingly, NCS-1 binding modulated downstream A2A receptor intracellular signaling in a Ca2+-dependent manner. Taken together this study provides further evidence that neuronal Ca2+-sensor proteins play an important role in modulation of GPCR signaling
The PAndAS Field of Streams: stellar structures in the Milky Way halo toward Andromeda and Triangulum
We reveal the highly structured nature of the Milky Way stellar halo within
the footprint of the PAndAS photometric survey from blue main sequence and main
sequence turn-off stars. We map no fewer than five stellar structures within a
heliocentric range of ~5 to 30 kpc. Some of these are known (the Monoceros
Ring, the Pisces/Triangulum globular cluster stream), but we also uncover three
well-defined stellar structures that could be, at least partly, responsible for
the so-called Triangulum/Andromeda and Triangulum/Andromeda 2 features. In
particular, we trace a new faint stellar stream located at a heliocentric
distance of ~17 kpc. With a surface brightness of \Sigma_V ~ 32-32.5
mag/arcsec^2, it follows an orbit that is almost parallel to the Galactic plane
north of M31 and has so far eluded surveys of the Milky Way halo as these tend
to steer away from regions dominated by the Galactic disk. Investigating our
follow-up spectroscopic observations of PAndAS, we serendipitously uncover a
radial velocity signature from stars that have colors and magnitudes compatible
with the stream. From the velocity of eight likely member stars, we show that
this stellar structure is dynamically cold, with an unresolved velocity
dispersion that is lower than 7.1 km/s at the 90-percent confidence level.
Along with the width of the stream (300-650 pc), its dynamics points to a
dwarf-galaxy-accretion origin. The numerous stellar structures we can map in
the Milky Way stellar halo between 5 and 30 kpc and their varying morphology is
a testament to the complex nature of the stellar halo at these intermediate
distances.Comment: 11 pages, 8 figures, accepted for publication in the ApJ, Figure 3 is
the money plo
Neuronal calcium and cAMP cross-talk mediated by cannabinoid CB1 receptor and EF-hand calcium sensor interactions.
Endocannabinoids are important players in neural development and function. They act via receptors, whose activation inhibits cAMP production. The aim of the paper was to look for calcium- and cAMP-signaling cross-talk mediated by cannabinoid CB1 receptors (CB1R) and to assess the relevance of EF-hand CaM-like calcium sensors in this regard. Using a heterologous expression system, we demonstrated that CB1R interacts with calneuron-1 and NCS1 but not with caldendrin. Furthermore, interaction motives were identified in both calcium binding proteins and the receptor, and we showed that the first two sensors competed for binding to the receptor in a Ca2+-dependent manner. Assays in neuronal primary cultures showed that, CB1R-NCS1 complexes predominate at basal Ca2+ levels, whereas in the presence of ionomycin, a calcium ionophore, CB1R-calneuron-1 complexes were more abundant. Signaling assays following forskolin-induced intracellular cAMP levels showed in mouse striatal neurons that binding of CB1R to NCS1 is required for CB1R-mediated signaling, while the binding of CB1R to calneuron-1 completely blocked Gi-mediated signaling in response to a selective receptor agonist, arachidonyl-2-chloroethylamide. Calcium levels and interaction with calcium sensors may even lead to apparent Gs coupling after CB1R agonist challenge
A parametric physical model for the intracluster medium and its use in joint SZ/X-ray analyses of galaxy clusters
We present a parameterized model of the intra-cluster medium that is suitable
for jointly analysing pointed observations of the Sunyaev-Zel'dovich (SZ)
effect and X-ray emission in galaxy clusters. The model is based on assumptions
of hydrostatic equilibrium, the Navarro, Frenk and White (NFW) model for the
dark matter, and a softened power law profile for the gas entropy. We test this
entropy-based model against high and low signal-to-noise mock observations of a
relaxed and recently-merged cluster from N-body/hydrodynamic simulations, using
Bayesian hyper-parameters to optimise the relative statistical weighting of the
mock SZ and X-ray data. We find that it accurately reproduces both the global
values of the cluster temperature, total mass and gas mass fraction (fgas), as
well as the radial dependencies of these quantities outside of the core (r >
kpc). For reference we also provide a comparison with results from the single
isothermal beta model. We confirm previous results that the single isothermal
beta model can result in significant biases in derived cluster properties.Comment: Published in MNRAS. 20 pages. 9 figure
PAndAS' cubs: discovery of two new dwarf galaxies in the surroundings of the Andromeda and Triangulum galaxies
We present the discovery of two new dwarf galaxies, Andromeda XXI and
Andromeda XXII, located in the surroundings of the Andromeda and Triangulum
galaxies (M31 and M33). These discoveries stem from the first year data of the
Pan-Andromeda Archaeological Survey (PAndAS), a photometric survey of the
M31/M33 group conducted with the Megaprime/MegaCam wide-field camera mounted on
the Canada-France-Hawaii Telescope. Both satellites appear as spatial
overdensities of stars which, when plotted in a color-magnitude diagram, follow
metal-poor, [Fe/H]=-1.8, red giant branches at the distance of M31/M33.
Andromeda XXI is a moderately bright dwarf galaxy (M_V=-9.9+/-0.6), albeit with
low surface brightness, emphasizing again that many relatively luminous M31
satellites still remain to be discovered. It is also a large satellite, with a
half-light radius close to 1 kpc, making it the fourth largest Local Group
dwarf spheroidal galaxy after the recently discovered Andromeda XIX, Andromeda
II and Sagittarius around the Milky Way, and supports the trend that M31
satellites are larger than their Milky Way counterparts. Andromeda XXII is much
fainter (M_V=-6.5+/-0.8) and lies a lot closer in projection to M33 than it
does to M31 (42 vs. 224 kpc), suggesting that it could be the first Triangulum
satellite to be discovered. Although this is a very exciting possibility in the
context of a past interaction of M33 with M31 and the fate of its satellite
system, a confirmation will have to await a good distance estimate to confirm
its physical proximity to M33. Along with the dwarf galaxies found in previous
surveys of the M31 surroundings, these two new satellites bring the number of
dwarf spheroidal galaxies in this region to 20.Comment: 10 pages, 6 figures, accepted for publication in ApJ; v2: minor
typographical correction
Barred Galaxies at z > 0.7: NICMOS HDFN Observations
Previous optical studies found an unexpected deficit of bars at z > 0.7. To
investigate the effects of bandshifting, we have studied the fraction of barred
spirals in the NICMOS Deep Field North. At z > 0.7 we find at least four barred
spirals, doubling the number previously detected. The number of barred galaxies
is small because these (and previous) data lack adequate spatial resolution. A
typical 5 kpc bar at z > 0.7 is only marginally detectable for WFPC2 at
0.8microns; the NICMOS data have even lower resolution and can only find the
largest bars. The average size of the four bars seen at z > 0.7 is 12 kpc. The
fraction of such large bars (4/95) is higher than that seen in nearby spirals
(1/44); all known selection effects suggest that the observed fraction is a
lower limit. However, important caveats such as small numbers and difficulties
in defining comparable samples at high and low redshifts should be noted. We
conclude that there is no significant evidence for a decrease in the fraction
of barred spirals beyond z ~ 0.7.Comment: Accepted for publication in ApJ Letters, 4 pages in emulate-apj
style, includes 3 figure
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