2,236 research outputs found
Paper Session I-C - The Role of the University in Commercial Launch Activities
Success of the U.S. in the international space arena depends largely on our ability to reduce the cost-to-orbit of payloads. To reduce costs, significant effort must be expended to upgrade commercial launch vehicles, processing facilities and operational procedures.
The universities have much to contribute to such an effort. This paper discusses the positive role that universities can play in helping industry and government be more successful in commercial space. Activities include needs assessments* problem definition, research, test and evaluation, business assistance, and education. Emphasis is placed on establishing a permanent capability to continuously advance launch systems technology, and on developing education and research programs that are complementary to each other
Ultraviolet-Bright, High-Redshift ULIRGS
We present Spitzer Space Telescope observations of the z=2.38 lya-emitter
over-density associated with galaxy cluster J2143-4423, the largest known
structure (110 Mpc) above z=2. We imaged 22 of the 37 known lya-emitters within
the filament-like structure, using the MIPS 24um band. We detected 6 of the
lya-emitters, including 3 of the 4 clouds of extended (>50 kpc) lyman alpha
emission, also known as Lya Blobs. Conversion from rest-wavelength 7um to total
far-infrared luminosity using locally derived correlations suggests all the
detected sources are in the class of ULIRGs, with some reaching Hyper-LIRG
energies. Lya blobs frequently show evidence for interaction, either in HST
imaging, or the proximity of multiple MIPS sources within the Lya cloud. This
connection suggests that interaction or even mergers may be related to the
production of Lya blobs. A connection to mergers does not in itself help
explain the origin of the Lya blobs, as most of the suggested mechanisms for
creating Lya blobs (starbursts, AGN, cooling flows) could also be associated
with galaxy interactions.Comment: 12 pages, 3 figures, accepted by ApJ Letter
Abolishing user fees for children and pregnant women trebled uptake of malaria-related interventions in Kangaba, Mali.
Malaria is the most common cause of morbidity and mortality in children under 5 in Mali. Health centres provide primary care, including malaria treatment, under a system of cost recovery. In 2005, MĂ©decins sans Frontieres (MSF) started supporting health centres in Kangaba with the provision of rapid malaria diagnostic tests and artemisinin-based combination therapy. Initially MSF subsidized malaria tests and drugs to reduce the overall cost for patients. In a second phase, MSF abolished fees for all children under 5 irrespective of their illness and for pregnant women with fever. This second phase was associated with a trebling of both primary health care utilization and malaria treatment coverage for these groups. MSF's experience in Mali suggests that removing user fees for vulnerable groups significantly improves utilization and coverage of essential health services, including for malaria interventions. This effect is far more marked than simply subsidizing or providing malaria drugs and diagnostic tests free of charge. Following the free care strategy, utilization of services increased significantly and under-5 mortality was reduced. Fee removal also allowed for more efficient use of existing resources, reducing average cost per patient treated. These results are particularly relevant for the context of Mali and other countries with ambitious malaria treatment coverage objectives, in accordance with the United Nations Millennium Development Goals. This article questions the effectiveness of the current national policy, and the effectiveness of reducing the cost of drugs only (i.e. partial subsidies) or providing malaria tests and drugs free for under-5s, without abolishing other related fees. National and international budgets, in particular those that target health systems strengthening, could be used to complement existing subsidies and be directed towards effective abolition of user fees. This would contribute to increasing the impact of interventions on population health and, in turn, the effectiveness of aid
PAH Emission Within Lyman Alpha Blobs
We present Spitzer observations of Lya Blobs (LAB) at z=2.38-3.09. The
mid-infrared ratios (4.5/8um and 8/24um) indicate that ~60% of LAB infrared
counterparts are cool, consistent with their infrared output being dominated by
star formation and not active galactic nuclei (AGN). The rest have a
substantial hot dust component that one would expect from an AGN or an extreme
starburst. Comparing the mid-infrared to submillimeter fluxes (~850um or rest
frame far infrared) also indicates a large percentage (~2/3) of the LAB
counterparts have total bolometric energy output dominated by star formation,
although the number of sources with sub-mm detections or meaningful upper
limits remains small (~10). We obtained Infrared Spectrograph (IRS) spectra of
6 infrared-bright sources associated with LABs. Four of these sources have
measurable polycyclic aromatic hydrocarbon (PAH) emission features, indicative
of significant star formation, while the remaining two show a featureless
continuum, indicative of infrared energy output completely dominated by an AGN.
Two of the counterparts with PAHs are mixed sources, with PAH line-to-continuum
ratios and PAH equivalent widths indicative of large energy contributions from
both star formation and AGN. Most of the LAB infrared counterparts have large
stellar masses, around 10^11 Mo. There is a weak trend of mass upper limit with
the Lya luminosity of the host blob, particularly after the most likely AGN
contaminants are removed. The range in likely energy sources for the LABs found
in this and previous studies suggests that there is no single source of power
that is producing all the known LABs.Comment: 34 pages, 5 figures, accepted by Ap
Polycyclic Aromatic Hydrocarbon Emission within Lyα Blobs
We present Spitzer observations of Lyα blobs (LABs) at z = 2.38-3.09. The mid-infrared ratios (4.5 μm/8 μm and 8 μm/24 μm) indicate that ~60% of LAB infrared counterparts are cool, consistent with their infrared output being dominated by star formation and not active galactic nuclei (AGNs). The rest have a substantial hot dust component that one would expect from an AGN or an extreme starburst. Comparing the mid-infrared to submillimeter fluxes (~850 μm or rest-frame far-infrared) also indicates that a large percentage (~2/3) of the LAB counterparts have total bolometric energy output dominated by star formation, although the number of sources with submillimeter detections or meaningful upper limits remains small (~10). We obtained Infrared Spectrograph (IRS) spectra of six infrared-bright sources associated with LABs. Four of these sources have measurable polycyclic aromatic hydrocarbon (PAH) emission features, indicative of significant star formation, while the remaining two show a featureless continuum, indicative of infrared energy output completely dominated by an AGN. Two of the counterparts with PAHs are mixed sources, with PAH line-to-continuum ratios and PAH equivalent widths indicative of large energy contributions from both star formation and AGN. Most of the LAB infrared counterparts have large stellar masses, around 10^(11) M_⊙. There is a weak trend of mass upper limit with the Lyα luminosity of the host blob, particularly after the most likely AGN contaminants are removed. The range in likely energy sources for the LABs found in this and previous studies suggests that there is no single source of power that is producing all the known LABs
Evaluation of peripheral compression and auditory nerve fiber intensity coding using auditory steady-state responses
Implementing tradable permits for sulfur oxides emissions : a case study in the South Coast Air Basin
Tradable emissions permits have important theoretical advantages over source-specific technical standards as a means for controlling pollution. Nonetheless, difficulties can arise in trying to implement an efficient, competitive market in emissions permits. Simple workable versions of the market concept may fail to achieve the competitive equilibrium, or to take account of important complexities in the relationship between the pattern of emissions and the geographical distribution of pollution. Existing regulatory law may severely limit the range of market opportunities that states can adopt.
This report examines the feasibility of tradable permits for controlling particulate sulfates in the Los Angeles airshed. Although the empirical part of the paper deals with a specific case, the methods developed have general applicability. Moreover, the particular market design that is proposed -- an auction process that involves no net revenue collection by the state -- has attractive features as a general model
Visualization and analysis of the structure of high Reynolds number hydrogen-air premixed flames
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/77272/1/AIAA-1990-161-778.pd
Using auditory steady-state responses to evaluate auditory nerve integrity in normal-hearing and mild hearing-impaired listeners
Cooperativity and Frustration in Protein-Mediated Parallel Actin Bundles
We examine the mechanism of bundling of cytoskeletal actin filaments by two
representative bundling proteins, fascin and espin. Small-angle X-ray studies
show that increased binding from linkers drives a systematic \textit{overtwist}
of actin filaments from their native state, which occurs in a linker-dependent
fashion. Fascin bundles actin into a continuous spectrum of intermediate twist
states, while espin only allows for untwisted actin filaments and
fully-overtwisted bundles. Based on a coarse-grained, statistical model of
protein binding, we show that the interplay between binding geometry and the
intrinsic \textit{flexibility} of linkers mediates cooperative binding in the
bundle. We attribute the respective continuous/discontinous bundling mechanisms
of fascin/espin to differences in the stiffness of linker bonds themselves.Comment: 5 pages, 3 figures, figure file has been corrected in v
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