101
by NOEMI JASMIN SALAZAR HERMENEGILDO
Published 2015
“... spatial and temporal resolution. A modified laser speckle imaging (mLSI) enables
computation of blood flow...”Published 2015
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102
“... originally targeted at λ = 850 μm with the Submillimetre Common-User Bolometer Array (SCUBA) in the SCUBA...”
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103
by VAHRAM CHAVUSHYAN, LUIS CARRASCO BAZUA, JONATHAN FRANCISCO LEON TAVARES, JOSE RAMON VALDES PARRA
Published 2008
“... the 6-m and the 1-m SAO’s telescopes (Russia), the GHAO’s 2.1-m telescope (Cananea, México), and the OAN...”Published 2008
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104
by IVAN HERNANDEZ ROMANO
Published 2011
“.../SWCNT film (thickness 200 μm) and SU8-2075 film (thickness 100 μm) were tested. The saturation intensity...”Published 2011
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105
by Carla Berrospe Rodríguez
Published 2017
“... to generate fast microjets (velocities up to 100 m/s), with the
aim of study its penetration depth in low...”Published 2017
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106
“... with 1 GHz bandwidth. The TIA shows 9 pA / p Hz input-referred spectral noise and only 6.9 mW power...”
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107
“... Complementario Metal-Oxido), de 0.6 μm. El diseño incluye el blindaje alrededor del arreglo de microelectrodos y...”
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108
by OSCAR MAURICIO GELVEZ LIZARAZO
Published 2015
“... la presión en la cámara de proceso (450 a 900 mTorr), además la rugosidad RMS (0.7- 5.1 nm) puede ser...”Published 2015
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109
by JHOAN ALBERTO SALINAS DELGADO
Published 2012
“... at an offset frequency of 1
MHz, and a power consumption of 80 mW is achieved. For the whole system, designed...”Published 2012
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110
by David Hughes
Published 2011
“...We present observations at 250, 350 and 500 μm of the nearby galaxy cluster Abell 3112 (z = 0.075...”Published 2011
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111
by Abdu Orduña Díaz, Edgar Castillo Domínguez, ALFONSO TORRES JACOME, FRANCISCO JAVIER DE LA HIDALGA WADE, CARLOS GERARDO TREVIÑO PALACIOS
Published 2011
“... deposition (PECVD) technique at low frequency on a 0.45 μm thick silicon nitride membrane sustained by a...”Published 2011
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112
“...We measure the local galaxy far-infrared (FIR) 60 to 100 μm colour–luminosity distribution using...”
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113
by David Hughes
Published 2009
“... provide estimates of number counts at the three BLAST wavelengths 250, 350, and 500 μm; instead...”Published 2009
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114
by David Hughes
Published 2009
“...) made resolved maps of seven nearby (<25 Mpc) galaxies at 250, 350, and 500 μm. During its 2005 June...”Published 2009
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115
by David Hughes
Published 2008
“...We present the first results from a new 250, 350, and 500μm Galactic Plane survey taken...”Published 2008
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116
by Jonathan Santiago Fernández
Published 2018
“...% conversion efficiency. The simulations and layout were made using an ON Semiconductorᴿ 0.5μm standard CMOS...”Published 2018
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117
by MARTHA CORAL GALINDO DOMINGUEZ
Published 2008
“...% for subtypes M2, M3, and M5. With these results we outperformed the average classification accuracy obtained...”Published 2008
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118
by GORDANA JOVANOVIC DOLECEK
Published 2010
“... are the decimation factors, M1 and M2, numbers of cascaded CIC filters L and K, and parameter b of the compensator....”Published 2010
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119
by Manolis Plionis
Published 2008
“... halo mass is ∼ 10¹³ h⁻¹ Mꙩ and ≿5 × 10¹³ h⁻¹ Mꙩ, respectively....”Published 2008
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120
by MARCELINO ANGUIANO MORALES, MARCELA MARIBEL MENDEZ OTERO, MARCELO DAVID ITURBE CASTILLO, SABINO CHAVEZ CERDA
Published 2007
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