1,082 research outputs found
No well-defined remnant Fermi surface in Sr2CuO2Cl2
In angle-resolved photoelectron spectra of the antiferromagnetic insulators
Ca2CuO2Cl2 and Sr2CuO2Cl2 a sharp drop of the spectral intensity of the
lowest-lying band is observed along a line in k space equivalent to the Fermi
surface of the optimally doped high-temperature superconductors. This was
interpreted as a signature of the existence of a remnant Fermi surface in the
insulating phase of the high-temperature superconductors. In this paper it is
shown that the drop of the spectral intensity is not related to the spectral
function but is a consequence of the electron-photon matrix elementComment: 4 pages, 3 figure
Galactic contamination in the QMAP experiment
We quantify the level of foreground contamination in the QMAP Cosmic
Microwave Background (CMB) data with two objectives: (a) measuring the level to
which the QMAP power spectrum measurements need to be corrected for foregrounds
and (b) using this data set to further refine current foreground models. We
cross-correlate the QMAP data with a variety of foreground templates. The 30
GHz Ka-band data is found to be significantly correlated with the Haslam 408
MHz and Reich and Reich 1420 MHz synchrotron maps, but not with the Diffuse
Infrared Background Experiment (DIRBE) 240, 140 and 100 micron maps or the
Wisconsin H-Alpha Mapper (WHAM) survey. The 40 GHz Q-band has no significant
template correlations. We discuss the constraints that this places on
synchrotron, free-free and dust emission. We also reanalyze the
foreground-cleaned Ka-band data and find that the two band power measurements
are lowered by 2.3% and 1.3%, respectively.Comment: 4 ApJL pages, including 4 figs. Color figures and data at
http://www.hep.upenn.edu/~angelica/foreground.html#qmap or from
[email protected]
An Optical Emission Line Survey of Large Planetary Nebulae
Accurate emission line fluxes from planetary nebulae (PNe) provide important
constraints on the nature of the final phases of stellar evolution. Large,
evolved PNe may trace the latest stages of PN evolution, where material from
the AGB wind is returned to the interstellar medium. However, the low surface
brightness and spatially extended emission of large PNe have made accurate
measurements of line fluxes difficult with traditional long-slit spectroscopic
techniques. Furthermore, distinguishing these nebulae from HII regions,
supernova remnants, or interstellar gas ionized by a hot, evolved stellar core
can be challenging. Here, we report on an ongoing survey of large Galactic PNe
(r > 5') with the Wisconsin H-Alpha Mapper (WHAM), a Fabry-Perot spectrograph
designed to detect faint diffuse optical emission lines with high sensitivity
and spectral resolution. Our sample includes newly revealed H-alpha
enhancements from the AAO/UKST and WHAM H-alpha surveys of Parker et al. and
Haffner et al. We present accurate emission line fluxes of H-alpha, [NII], and
[OIII], and compare our data to other measurements. We use the emission line
ratios and kinematics of the ionized gas to assess, or in some cases reassess,
the identification of some nebulae.Comment: 2 pages, 1 figure, to be published in IAU Symp. 234: `Planetary
Nebulae in Our Galaxy and Beyond', eds. M.J. Barlow, R.H. Mende
Measurement of a Magnetic Field in a Leading Arm High Velocity Cloud
Using a recent catalogue of extragalactic Faraday rotation derived from the
NRAO VLA Sky Survey we have found an agreement between Faraday rotation
structure and the HI emission structure of a High Velocity Cloud (HVC)
associated with the Leading Arm of the Magellanic System. We suggest that this
morphological agreement is indicative of Faraday rotation through the HVC.
Under this assumption we have used 48 rotation measures through the HVC,
together with estimates of the electron column density from H-\alpha\
measurements and QSO absorption lines to estimate a strength for the
line-of-sight component of the coherent magnetic field in the HVC of >
6 {\rm \mu G}B_{r}/B_{||} < 0.8$, which suggests that the random field does not dominate
over the coherent field as it does in the Magellanic Clouds from which this HVC
likely originates.Comment: 17 pages, 3 figure
miRNAs are essential for survival and differentiation of newborn neurons but not for expansion of neural progenitors during early neurogenesis in the mouse embryonic neocortex
Neurogenesis during the development of the mammalian cerebral cortex involves a switch of neural stem and progenitor cells from proliferation to differentiation. To explore the possible role of microRNAs (miRNAs) in this process, we conditionally ablated Dicer in the developing mouse neocortex using Emx1-Cre, which is specifically expressed in the dorsal telencephalon as early as embryonic day (E) 9.5. Dicer ablation in neuroepithelial cells, which are the primary neural stem and progenitor cells, and in the neurons derived from them, was evident from E10.5 onwards, as ascertained by the depletion of the normally abundant miRNAs miR-9 and miR-124. Dicer ablation resulted in massive hypotrophy of the postnatal cortex and death of the mice shortly after weaning. Analysis of the cytoarchitecture of the Dicer-ablated cortex revealed a marked reduction in radial thickness starting at E13.5, and defective cortical layering postnatally. Whereas the former was due to neuronal apoptosis starting at E12.5, which was the earliest detectable phenotype, the latter reflected dramatic impairment of neuronal differentiation. Remarkably, the primary target cells of Dicer ablation, the neuroepithelial cells, and the neurogenic progenitors derived from them, were unaffected by miRNA depletion with regard to cell cycle progression, cell division, differentiation and viability during the early stage of neurogenesis, and only underwent apoptosis starting at E14.5. Our results support the emerging concept that progenitors are less dependent on miRNAs than their differentiated progeny, and raise interesting perspectives as to the expansion of somatic stem cells
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