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2017

Новости за 01.05.2017

Independent Political Speech, Then and Now

Cato Institute 

The playing field for independent speech has improved, but there are challenges still for small groups that want to influence elections. Michael G. Adams and Neil Reiff are campaign finance attorneys in Washington.

Arsenal Fan’s Forum Meeting Minutes and Surveys

Arsenal Scotland Supporters Club 

Arsenal Scotland members may be interested to see for yourselves the level of questions and answers raised at the quarterly Forum Meetings. Please see below the minutes of the December 2016 and April 2017 meetings together with submitted surveys and statements raised by AISA (Arsenal Independant Supporters’ Association) and AST (Arsenal Supporters’ Trust) . These […]

Degradation and ESR Failures in MnO2 Chip Tantalum Capacitors

Sti.nasa.gov 

Abstract: Equivalent series resistance (ESR) of chip tantalum capacitors determines the rate of energy delivery and power dissipation thus affecting temperature and reliability of the parts. Employment of advanced capacitors with reduced ESR decreases power losses and improves efficiency in power systems. Stability of ESR is essential for correct operations of power units and might cause malfunctioning and failures when ESR becomes too high or too low. Several cases with ESR values in CWR29 capacitors... Читать дальше...



Innovative Manufacturing of Launch Vehicle Structures - Integrally Stiffened Cylinder Process

Sti.nasa.gov 

Abstract: Reducing launch costs is essential to ensuring the success of NASA's visions for planetary exploration and earth science, economical support of the International Space Station, and competitiveness of the U.S. commercial launch industry. Reducing launch vehicle manufacturing cost supports NASA's budget and technology development priorities.

High-Contrast Imaging of Epsilon Eridani with Ground-Based Instruments

Sti.nasa.gov 

Abstract: Epsilon Eridani is one of the nearest solar-type stars. Its proximity and relatively young age allow high-contrast imaging observations to achieve sensitivities to planets at narrow separations down to an inner radius of approximately 5 AU. Previous observational studies of the system report a dust disk with asymmetric morphology as well as a giant planet with large orbital eccentricity, which may require another massive companion to induce the peculiar morphology and to enhance the large... Читать дальше...

The Geometry of the Infrared and X-Ray Obscurer in a Dusty Hyperluminous Quasar

Sti.nasa.gov 

Abstract: We study the geometry of the active galactic nucleus (AGN) obscurer in IRAS 09104+4109, an IR-luminous, radio-intermediate FR-I source at z = 0.442, using infrared data from Spitzer and Herschel, X-ray data from NuSTAR, Swift, Suzaku, and Chandra, and an optical spectrum from Palomar. The infrared data imply a total rest-frame 1-1000 micron luminosity of 5.5 × 10(exp 46) ergs/s and require both an AGN torus and a starburst model. The AGN torus has an anisotropy-corrected IR luminosity of... Читать дальше...

The TESS Science Processing Operations Center

Sti.nasa.gov 

Abstract: The Transiting Exoplanet Survey Satellite (TESS) will conduct a search for Earth's closest cousins starting in early 2018 and is expected to discover approximately 1,000 small planets with R(sub p) less than 4 (solar radius) and measure the masses of at least 50 of these small worlds. The Science Processing Operations Center (SPOC) is being developed at NASA Ames Research Center based on the Kepler science pipeline and will generate calibrated pixels and light curves on the NASA Advanced... Читать дальше...

On the Evolution of the Inner Disk Radius with Flux in the Neutron Star Low-mass X-Ray Binary Serpens X-1

Sti.nasa.gov 

Abstract: We analyze the latest Suzaku observation of the bright neutron star (NS) low-mass X-ray binary Serpens X-1 taken in 2013 October and 2014 April. The observation was taken using the burst mode and only suffered mild pile-up effects. A broad iron line is clearly detected in the X-ray spectrum. We test different models and find that the iron line is asymmetric and best interpreted by relativistic reflection. The relativistically broadened iron line is generally believed to originate from the... Читать дальше...

Apocenter Glow in Eccentric Debris Disks: Implications for Fomalhaut and Epsilon Eridani

Sti.nasa.gov 

Abstract: Debris disks often take the form of eccentric rings with azimuthal asymmetries in surface brightness. Such disks are often described as showing pericenter glow, an enhancement of the disk brightness in regions nearest the central star. At long wavelengths, however, the disk apocenters should appear brighter than their pericenters: in the long-wavelength limit, we find that the apocenter pericenter flux ratio scales as 1 + e for disk eccentricity e. We produce new models of this apocenter... Читать дальше...

GIA releases synthetics detector for diamond jewellery

Jewellermagazine.com 

The Gemological Institute of America (GIA) has introduced a testing device that is capable of separating natural diamonds from suspected synthetics regardless of whether the stone is loose or set in jewellery.

Spectro-Timing Study of GX 339-4 in a Hard Intermediate State

Sti.nasa.gov 

Abstract: We present an analysis of Nuclear Spectroscopic Telescope Array observations of a hard intermediate state of the transient black hole GX 339-4 taken in 2015 January. With the source softening significantly over the course of the 1.3 day long observation we split the data into 21 sub-sets and find that the spectrum of all of them can be well described by a power-law continuum with an additional relativistically blurred reflection component. The photon index increases from approx. 1.69 to... Читать дальше...

Extremes of the Jet-Accretion Power Relation of Blazars, as Explored by Nustar

Sti.nasa.gov 

Abstract: Hard X-ray observations are crucial to study the non-thermal jet emission from high-redshift, powerful blazars. We observed two bright z > 2 flat-spectrum radio quasars (FSRQs) in hard X-rays to explore the details of their relativistic jets and their possible variability. S50014+81 (at z = 3.366) and B0222+185 (at z = 2.690) have been observed twice by the Nuclear Spectroscopic Telescope Array (NuSTAR) simultaneously with Swift X-ray Telescope, showing different variability behaviors. Читать дальше...

Cryo-Vacuum Testing of the JWST Integrated Science Instrument Module

Sti.nasa.gov 

Abstract: In late 2015 early 2016, a major cryo-vacuum test was carried out for the Integrated Science Instrument Module (ISIM) of the James Webb Space Telescope. This test comprised the final cryo-certification and calibration test of the ISIM before its delivery for integration with the rest of the JWST observatory. Over the roughly 100-day period of the round-the-clock test program, the full complement of ISIM flight instruments, structure, harness radiator, and electronics were put through a... Читать дальше...

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Москва

Москву и Санкт-Петербург назвали лучшими городами для подработки


Detection of the Pairwise Kinematic Sunyaev-Zel'dovich Effect with BOSS DR11 and the Atacama Cosmology Telescope

Sti.nasa.gov 

Abstract: We present a new measurement of the kinematic Sunyaev-Zel'dovich effect using data from the Atacama Cosmology Telescope (ACT) and the Baryon Oscillation Spectroscopic Survey (BOSS). Using 600 square degrees of overlapping sky area, we evaluate the mean pairwise baryon momentum associated with the positions of 50,000 bright galaxies in the BOSS DR11 Large Scale Structure catalog. A non-zero signal arises from the large-scale motions of halos containing the sample galaxies. The data fits... Читать дальше...

Development and Testing of Harpoon-Based Approaches for Collecting Comet Samples (Video Supplement)

Sti.nasa.gov 

Abstract: This video supplement contains a set of videos created during the approximately 10-year-long course of developing and testing the Goddard Space Flight Center (GSFC) harpoon-based approach for collecting comet samples. The purpose of the videos is to illustrate various design concepts used in this method of acquiring samples of comet material, the testing used to verify the concepts, and the evolution of designs and testing. To play the videos this PDF needs to be opened in the freeware... Читать дальше...

Development and Testing of Harpoon-Based Approaches for Collecting Comet Samples

Sti.nasa.gov 

Abstract: Comets, having bright tails visible to the unassisted human eye, are considered to have been known about since pre-historic times. In fact 3,000-year old written records of comet sightings have been identified. In comparison, asteroids, being so dim that telescopes are required for observation, were not discovered until 1801. Yet, despite their later discovery, a space mission returned the first samples of an asteroid in 2010 and two more asteroid sample return missions have already been... Читать дальше...

Suprem SB 135 Squash Racquets

Courtside Sports 

Suprem SB 135 Squash Racquets (Adult Squash Racquets)

The Tecnifibre Suprem SB 135 squash racquet is the heaviest of the Suprem series of frames and offers lots of power with its' large sweetspot. Considered to be an all-around frame, touch players will...

Your Price: CDN$199.95

Availability: In Stock

Suprem SB 130 Squash Racquets

Courtside Sports 

Suprem SB 130 Squash Racquets (Adult Squash Racquets)

The Tecnifibre Suprem SB 130 squash racquet offers advanced players great power and has a very forgiving sweetspot due to the large headsize. Features:SB Storm Bridge - Exclusive new yoke provides l...

Your Price: CDN$199.95

Availability: In Stock

Identification of the Hard X-Ray Source Dominating the E > 25 keV Emission of the Nearby Galaxy M31

Sti.nasa.gov 

Abstract: We report the identification of a bright hard X-ray source dominating the M31 bulge above 25 keV from a simultaneous NuSTAR-Swift observation. We find that this source is the counterpart to Swift J0042.6+4112, which was previously detected in the Swift BAT All-Sky Hard X-Ray Survey. This Swift BAT source had been suggested to be the combined emission from a number of point sources; our new observations have identified a single X-ray source from 0.5 to 50 keV as the counterpart for the first... Читать дальше...


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