Sentences with phrase «mu $»

Data at 100 and 160 $ \ mu $ m were obtained, complemented in some cases with observations at 70 $ \ mu $ m, and at 250, 350 and 500 $ \ mu $ m using SPIRE.

To carry out a wide range of high - spatial resolution observations, it can combine the two AO - corrected 8.4 - m apertures of the LBT in various ways including direct (non-interferometric... ▽ More The Large Binocular Telescope Interferometer (LBTI) is a strategic instrument of the LBT designed for high - sensitivity, high - contrast, and high - resolution infrared (1.5 - 13 $ \ mu $ m) imaging of nearby planetary systems.

Abstract: The Large Binocular Telescope Interferometer uses a near - infrared camera to measure the optical path length variations between the two AO - corrected apertures and provide high - angular resolution observations for all its science channels (1.5 - 13 $ \ mu $ m).

Herschel's high angular resolution ($ \ sim $ 7» FWHM at 100 $ \ mu $ m) provided the capacity for resolving debris belts around nearby stars with radial extents comparable to the solar system (50 to 100 au).

To test for a correlation between magnetic activity and photometric variability, we searched for H$ \ alpha $ emission among eight L3 $ - $ T2 ultra-cool dwarfs with extensive previous photometric monitoring, some of which are known to be variable at 3.6 $ \ mu $ m or 4.5 $ \ mu $ m.

The observing strategy was to integrate as deep as possible at 100 $ \ mu $ m to detect the stellar photosphere.

Some discs display peculiar SEDs with spectral indexes in the 70 - 160 $ \ mu $ m range steeper than the Rayleigh - Jeans one.

Additionally SPICA will provide efficient 30 - 37 $ \ mu $ m broad band mapping, and polarimetric imaging in the 100 - 350 $ \ mu $ m range.

As a result, we find that the interband ratio of PAH 7.7 $ \ mu $ m / PAH 11.3 $ \ mu $ m varies locally near M17SW, but rather independently of the distance from the OB stars in M17, suggesting that the degree of PAH ionization is mainly controlled by local conditions rather than the global UV environments determined by the OB stars in M17.

The spectra show prominent features due to polycyclic aromatic hydrocarbons (PAHs) at wavelengths of 6.2, 7.7, 8.6, 11.3, 12.0, 12.7, 13.5, and 14.2 $ \ mu $ m.

We also find that the interband ratios of the PAH 12.0 $ \ mu $ m, 12.7 $ \ mu $ m, 13.5 $ \ mu $ m, and 14.2 $ \ mu $ m features to the PAH 11.3 $ \ mu $ m feature are high near the M17 center, which suggests structural changes of PAHs through processing due to intense UV radiation, producing abundant edgy irregular PAHs near the M17 center.

(iv) Observations of far - infrared cooling lines such as [OI] 63 $ \ mu $ m from star - forming molecular clouds in our Galaxy will evaluate the importance of shocks to dissipate turbulent energy.

IRDIS was operated in parallel with the integral field spectrograph (IFS) of SPHERE to collect low - resolution ($ R \ sim30 $), near - infrared (0.94 - 1.64 $ \ mu $ m) spectra of the two innermost planets HR8799d and e.

Abstract: We describe a successful effort to produce a laser comb around 1.55 $ \ mu $ m in the astronomical H band using a method based on a line - referenced, electro - optical - modulation frequency comb.

We performed polarimetric imaging of T Cha with IRDIS (1.6 $ \ mu $ m) and ZIMPOL (0.5 - 0.9 $ \ mu $ m), and obtained intensity images from IRDIS dual - band imaging with simultaneous spectro - imaging with IFS (0.9 - 1.3 $ \ mu $ m).

The core wavelength range and the goal contrast of the coronagraphic mode are 3.5 — 27 $ \ mu $ m, and 10 $ ^ -LCB--6 -RCB- $, respectively.

With these new data, we contribute to completing the spectral energy distribution of these bodies in the 1.0 - 2.5 $ \ mu $ m range.

This indicates that the dust particles in the disk surface are mainly $ \ gtrsim0.3 \, \ mu $ m - sized grains.

The issue is NOT Americqns accepting I$ lam it is mu $ lims accepting American values rather than waiting out untill there is enough of them to I$ lamise America..

here are some good mu $ lims implementing sharia... which a significant bunch in Amercia is trying to convince us it is benign and «mostly in line» with out laws per Ground Zero Imam Faisal!!!

Not exact matches

Additionally cosigned by the CEOs of Micron Technologies (mu), Xerox (xrx), Akamai (akam), and Qualcomm (qcom), the council's report aims to address the United States» growing $ 19 trillion debt and rusting digital infrastructure by providing recommendations from private industry to overhaul federal systems.

The University of Missouri (MU) is losing about 1500 students and is facing a huge $ 32 million budget shortfall four months after it attracted national attention as the site of massive race - based campus protests.

Micron Technology, Inc. (NASDAQ: MU) announced last week its fiscal third - quarter results, which showed 92 - percent year - over-year revenue growth to $ 5.57 billion and non-GAAP earnings per share of $ 1.62 compared to $ 0.90 in the year - ago period.

Shares of Micron Technology, Inc. (NASDAQ: MU) were trading lower by 3 percent early Wednesday morning in reaction to the company's new share offering in which it will sell around $ 1 billion in stock.

Pi $ $ off with your MU's kids.

Even the 4th place will not be easy as MU will become much better, LPool Still very strong and MC and $ CHelski are a grade above us with strength.

I also pointed out that this «scratch» MU team had a midfield which cost over $ 100m and a defence which cost almost the same.

The mean B - field strength, estimated using the Chandrasekhar - Fermi method, is 91 $ \ pm $ 8 -LCB- \ mu -RCB- G. B - field pressure dominates over turbulent and thermal pressures.

Because heavy - flavor production is dominated by gluon - gluon interactions at $ \ sqrt -LCB- s -RCB- = 200 $ GeV, these measurements offer a unique opportunity... ▽ More The cross section and transverse single - spin asymmetries of $ \ mu ^ -LCB-- -RCB- $ and $ \ mu ^ -LCB- + -RCB- $ from open heavy - flavor decays in polarized $ p $ + $ p $ collisions at $ \ sqrt -LCB- s -RCB- = 200 $ GeV were measured by the PHENIX experiment during 2012 at the Relativistic Heavy Ion Collider.

Isuzu Motors India has launched the MU - X SUV in India at a starting price of $ 23.99 lakh (ex-showroom, Delhi) for the 4x2 variant and $ 25.99 lakh (ex-showroom, Delhi) for the 4x4 variant.

The Isuzu MU - X is likely to be launched in India with a price tag north of the $ 25 lakh mark.

2016 Isuzu MU - X LS - T pricing and specifications: Price: $ 54,000 (plus on - road costs) Engine: 3.0 - litre four - cylinder turbo - diesel Output: 130kW / 380Nm Transmission: Five - speed automatic Fuel: 8.3 L / 100 km (ADR Combined) CO2: 219g / km (ADR Combined) Safety Rating: Five - star ANCAP

The base Diesel version of the Isuzu MU - X costs $ 29.07 Lakh, whereas the Diesel top - end costs $ 31.37 Lakh.

The latest, Thai - built MU - X LS - Terrain is more expensive but still competitively priced at $ 54,490 (plus on - road costs) with metallic paint a $ 450 option.

2017 Isuzu MU - X LS - T pricing and specifications: Price: $ 54,800 (plus on - road costs) Engine: 3.0 - litre four - cylinder turbo - diesel Output: 130kW / 430Nm Transmission: Six - speed automatic Fuel: 8.1 L / 100 km (ADR Combined) CO2: 214g / km (ADR Combined) Safety Rating: Five - star ANCAP

Compared here are the Ford Everest ($ 54,990), Holden Trailblazer ($ 52,490), Isuzu MU - X ($ 54,800), Mitsubishi Pajero Sport ($ 53,000) and Toyota Fortuner ($ 54,990).

2017 Isuzu MU - X LS - T pricing and specification Price: $ 56,100 (plus on - road costs) Engine: 3.0 - litre four - cylinder turbo - diesel Output: 130kW / 430Nm Transmission: Six - speed automatic Fuel: 7.9 L / 100 km (ADR Combined) CO2: 209g / km (ADR Combined) Safety Rating: Five - star ANCAP

A rear - drive Terra would give Nissan Australia a direct entry - level, sub - $ 50K rival for the Everest and MU - X 4x2s.

2017 Isuzu UTE MU - X 4 × 4 pricing: LS - M seven - seat SUV — $ 47,000 (man) / $ 49,100 (auto) LS - U seven - seat SUV — $ 49,000 (man) / $ 51,100 (auto) LS - T seven - seat SUV — $ 54,800 (auto)

If MU remains above $ 40 by the October expiration, then the Oct 40 calls will be exercised and the traders will now own MU stock.

Yesterday opened trend retracement positions on $ JAZZ and $ MU.

RMBS commanded a market valuation of roughly $ 2B before MU won the lawsuit.

SFO - PVG Fares are already declining — coach is down to just $ 1100 round trip compared to about $ 2,200 prior to MU's arrival.

* $: Recent Works, Elms Lesters Painting Room, London C9, MU Art Foundation, Eindhoven 2001 Tokyo First, Parco Gallery, Tokyo 1999 Colette, Paris Group exhibitions 2016 Holding: Selections from MCASD's Collection, Museum of Contemporary Art San Diego, La Jolla, California Greek Gotham, Dio Horia Gallery, Mykonos A Material Legacy: The Nancy A. Nasher and David J. Haemisegger Collection of Contemporary Art, Nasher Museum of Art at Duke Universituy, Durham, North Carolina 2015 Mutated Reality, Gary Tatintsian Gallery, Moscow A Shared Space: KAWS, Karl Wirsum, Tomoo Gokita, Newcomb Art Museum at Woldenburg Art Center, Tulane University, Nueva Orleans, Louisiana Paulin, Paulin, Paulin, Galerie Emmanuel Perrotin, Paris Respect, CAC Málaga - Centro de Arte Contemporáneo de Málaga Along the Way, At This Time, Better Knowing - ArtZuid 2015.

This program is supported by an $ 8.8 million award from the U.S. Department of Justice, Office of Justice Programs, Office for Victims of Crime, Award Number 2017 - MU - MU - K131, and private funding.

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MU - MIMO, band steering on 5 GHz and Alexa integration are all included for $ 200.

Netgear's $ 200 Nighthawk R7000P AC2300 router is made for gaming and streaming, thanks to its beamforming technology and MU - MIMO to stream to multiple devices simultaneously.

If $ 500 is too steep, you'll get 802.11 ad connectivity and better MU - MIMO performance with the $ 350 TP - Link Talon AD7200, but you'll have to do with fewer I / O ports, and there's no 160 MHz Wi - Fi.

Independent licensed clinicians are eligible for a $ 2,000 sign - on bonus of $ 1,000 paid first day of employment and $ 1,000 paid at the end of the six month probationary period If a position requires that an employee be mu