790 research outputs found
Diagnosis and treatment of paraneoplastic neurological disorders
In about two thirds of cases, patients with paraneoplastic neurological disorders present to the neurologist without a known tumor. Due to the ongoing immune response, this tumor tends to stay biologically relatively benign, and therefore difficult to diagnose. In patients with a known tumor, the neurological symptoms often precede a tumor recurrence. In both scenarios, anti-neuronal antibodies are an invaluable diagnostic help to the clinician, and may be supplemented by other diagnostic tests such as MRI, CSF, and electrophysiology. Tumor therapy remains the mainstay of therapeutic options, although early immune therapy must be started in parallel. It is hoped that the recent fundamental advances in understanding the autoimmune pathology of these disorders, especially the role of cytotoxic T cells, will eventually lead to more effective treatment options
Push it to the limit: Local Group constraints on high-redshift stellar mass functions for Mstar > 10^5 Msun
We constrain the evolution of the galaxy stellar mass function from 2 < z < 5
for galaxies with stellar masses as low as 10^5 Msun by combining star
formation histories of Milky Way satellite galaxies derived from deep Hubble
Space Telescope observations with merger trees from the ELVIS suite of N-body
simulations. This approach extends our understanding more than two orders of
magnitude lower in stellar mass than is currently possible by direct imaging.
We find the faint end slopes of the mass functions to be alpha=
-1.42(+0.07/-0.05) at z = 2 and alpha = -1.57^(+0.06/-0.06) at z = 5, and show
the slope only weakly evolves from z = 5 to z = 0. Our findings are in stark
contrast to a number of direct detection studies that suggest slopes as steep
as alpha = -1.9 at these epochs. Such a steep slope would result in an order of
magnitude too many luminous Milky Way satellites in a mass regime that is
observationally complete (Mstar > 2*10^5 Msun at z = 0). The most recent
studies from ZFOURGE and CANDELS also suggest flatter faint end slopes that are
consistent with our results, but with a lower degree of precision. This work
illustrates the strong connections between low and high-z observations when
viewed through the lens of LCDM numerical simulations
Gold catalyzed multicomponent reactions beyond A3 coupling
The preparation of complex architectures has inspired the search for new methods and new processes in organic synthesis. Multicomponent reactions have become an interesting approach to achieve such molecular diversity and complexity. This review intends to illustrate important gold-catalyzed examples for the past ten years leading to interesting skeletons involved in biologically active compounds
Adsorption geometry and electronic structure of iron phthalocyanine on Ag surfaces: A LEED and photoelectron momentum mapping study
We present a comprehensive study of the adsorption behavior of iron
phthalocyanine on the low-index crystal faces of silver. By combining
measurements of the reciprocal space by means of photoelectron momentum mapping
and low energy electron diffraction, the real space adsorption geometries are
reconstructed. At monolayer coverage ordered superstructures exist on all
studied surfaces containing one molecule in the unit cell in case of Ag(100)
and Ag(111), and two molecules per unit cell for Ag(110). The azimuthal tilt
angle of the molecules against the high symmetry directions of the substrate is
derived from the photoelectron momentum maps. A comparative analysis of the
momentum patterns on the substrates with different symmetry indicates that both
constituents of the twofold degenerate FePc lowest unoccupied molecular orbital
are occupied by charge transfer from the substrate at the interface
TimeMachine: Timeline Generation for Knowledge-Base Entities
We present a method called TIMEMACHINE to generate a timeline of events and
relations for entities in a knowledge base. For example for an actor, such a
timeline should show the most important professional and personal milestones
and relationships such as works, awards, collaborations, and family
relationships. We develop three orthogonal timeline quality criteria that an
ideal timeline should satisfy: (1) it shows events that are relevant to the
entity; (2) it shows events that are temporally diverse, so they distribute
along the time axis, avoiding visual crowding and allowing for easy user
interaction, such as zooming in and out; and (3) it shows events that are
content diverse, so they contain many different types of events (e.g., for an
actor, it should show movies and marriages and awards, not just movies). We
present an algorithm to generate such timelines for a given time period and
screen size, based on submodular optimization and web-co-occurrence statistics
with provable performance guarantees. A series of user studies using Mechanical
Turk shows that all three quality criteria are crucial to produce quality
timelines and that our algorithm significantly outperforms various baseline and
state-of-the-art methods.Comment: To appear at ACM SIGKDD KDD'15. 12pp, 7 fig. With appendix. Demo and
other info available at http://cs.stanford.edu/~althoff/timemachine
A Predicted Correlation Between Age Gradient and Star Formation History in FIRE Dwarf Galaxies
We explore the radial variation of star formation histories in dwarf galaxies
simulated with Feedback In Realistic Environments (FIRE) physics. The sample
contains 9 low-mass field dwarfs with M_ star = 10^5 - 10^7 M_sun from previous
FIRE results, and a new suite of 17 higher mass field dwarfs with M_star = 10^7
- 10^9 M_sun introduced here. We find that age gradients are common in our
dwarfs, with older stars dominant at large radii. The strength of the gradient
correlates with overall galaxy age such that earlier star formation produces a
more pronounced gradient. The relation between formation time and strength of
the gradient is driven by both mergers and star-formation feedback. Mergers can
both steepen and flatten the age gradient depending on the timing of the merger
and star formation history of the merging galaxy. In galaxies without
significant mergers, early feedback pushes stars to the outskirts at early
times. Interestingly, among galaxies without mergers, those with large dark
matter cores have flatter age gradients because these galaxies have more
late-time feedback. If real galaxies have age gradients as we predict, stellar
population studies that rely on sampling a limited fraction of a galaxy can
give a biased view of its global star formation history. We show that central
fields can be biased young by a few Gyrs while outer fields are biased old.
Fields positioned near the 2D half-light radius will provide the least biased
measure of a dwarf galaxy's global star formation history.Comment: 13 pages, 8 figures. Submitted to MNRAS, comments welcom
El hormigón armado en Cataluña (1898-1929): cuatro empresas y su relación con la arquitectura
Between 1898 and 1929 various business initiatives that introduced reinforced concrete in its architecture developed in Catalonia. This article studies the following four companies: AnĂłnima Claudio Duran - Construcciones Monier, Marial Hermanos - Sociedad Colectiva, Construcciones y Pavimentos, S. A. and Material y Obras, S. A. Only thorough knowledge of the production complexities that studies these companies, their technicians and works in all its complexity will allow us to assess how reinforced concrete transformed the construction sector, with new companies of a different productive scale. However, the depressed economic cycle of 1929-1952 weighed down any initiative and artificially lengthened what was left of traditional “Catalan construction”.Entre 1898 y 1929 se desarrollaron en Cataluña variadas iniciativas empresariales que introdujeron el hormigĂłn armado en la arquitectura. En el artĂculo se estudian las empresas AnĂłnima Claudio Duran - Construcciones Monier, Marial Hermanos - Sociedad Colectiva, Construcciones y Pavimentos, S. A., y Material y Obras, S. A. Se propone una aproximaciĂłn al entramado productivo que estudie las empresas, sus tĂ©cnicos y sus obras en toda su complejidad con la intenciĂłn de valorar cĂłmo el hormigĂłn armado transformĂł el sector de la construcciĂłn, con nuevas empresas de otra escala productiva. Sin embargo, el ciclo econĂłmico depresivo 1929-1952 lastrĂł estas iniciativas y alargĂł artificialmente los restos de la tradicional «construcciĂłn catalana»
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