121
by David Hughes
Published 2011
“..., 350, and 500 μm, combined with rich data sets for this well-studied region. Our primary goal...”Published 2011
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122
by MARIO MORENO MORENO, ANDREY KOSAREV, ALFONSO TORRES JACOME, ROBERO CARLOS AMBROSIO LAZARO
Published 2007
“... in the array have a ìbridge typeî
configuration. In this case, a SiNx supporting film is suspended 2.5 μm from...”Published 2007
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123
by MIGUEL ANGEL BELLO JIMENEZ, EVGENY KUZIN, BALDEMAR IBARRA ESCAMILLA, ARIEL FLORES ROSAS
Published 2009
“... breakup effect. The bunch of solitons was generated in a 500-m fiber pumped by 25-ps pulses...”Published 2009
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124
by Tovmassian Hrant
Published 2010
“...By observations with the 1.5m telescope at San Pedro Martir (OAN, UNAM, Mexico) the BVR magnitudes...”Published 2010
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125
by IVANIO PUERARI
Published 2007
“...Ks-band images of 20 barred galaxies show an increase in the peak amplitude of the normalized m = 2...”Published 2007
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126
by SALVADOR ALCANTARA INIESTA, BLANCA SUSANA SOTO CRUZ, Wilfrido Calleja Arriaga, GABRIEL ROMERO PAREDES RUBIO, MARGARITA GALINDO MENTLE
Published 2010
“... to obtain a sensor with dimensions of 100X20X15μm from silicon semiconductor technology and bulk...”Published 2010
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127
by JOSE LUIS AVILES URBIOLA
Published 2010
“... to retrieve
high vertical resolution profiles (down to 8 m) with no precedent among the
optical profilers...”Published 2010
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128
by David Hughes
Published 2009
“... is accurate to 9.5%, 8.7%, and 9.2% at the 250, 350, and 500 μm bands, respectively. The errors are highly...”Published 2009
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129
by MIGUEL ANGEL BELLO JIMENEZ, EVGENY KUZIN, BALDEMAR IBARRA ESCAMILLA, ARIEL FLORES ROSAS
Published 2010
“... breakup effect. The bunch of solitons was generated in a 500-m fiber pumped by 25-ps pulses...”Published 2010
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130
by GABRIELA MOLAR VELAZQUEZ, FRANCISCO JAVIER RENERO CARRILLO, WILFRIDO CALLEJA ARRIAGA
Published 2010
“.... The optical parameters, which physical dimensions are between 50 and 500 μm, are obtained within...”Published 2010
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131
by David Hughes
Published 2012
“.... We used multi-wavelength continuum data: three BLAST bands at 250, 350, and 500 μm and one IRAS...”Published 2012
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132
by ELIZABETH GALINDO LINARES
Published 2007
“...
carriers in the Si layers is modulated at a level of 1019=cm3, the wavelength
of light being xed at 1:54m...”Published 2007
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133
by EDGAR CASTILLO DOMINGUEZ
Published 2011
“... main mirrors of
LMT installed. Detections for M1, M42, Saturn and Moon were obtained....”Published 2011
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134
by JUAN PABLO PADILLA MARTINEZ
Published 2009
“... signal of the bead trapped. The obtained results for the stiffness
are around of 2.66 and 3.73 pN/μm...”Published 2009
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135
“... 17.4mW de una fuente de 3.3V.
Las altas prestaciones se logran al realizar un diseño completamente...”
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136
“... from 500 µA to 35 mA, generates a magnetic flux density at a rate of 100 µT/mA. When these magnetic...”
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137
by Vahram Chavushyan
Published 2012
“.... The observations were done with the 2.1-m telescope of the Observatorio Astronómico Nacional at San Pedro Mártir...”Published 2012
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138
by CELSO VELASQUEZ ORDOÑEZ, JOSE JAVIER SANCHEZ MONDRAGON, DANIEL ALBERTO MAY ARRIOJA
Published 2009
“... of samples. In particular, a positive nonlinear refractive index of 5.0115x10 ⁻¹⁰m²/W was obtained for a...”Published 2009
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139
by GORDANA JOVANOVIC DOLECEK
Published 2009
“...This paper presents the multiplierless CIC compensation filter based on the 2M-order filter...”Published 2009
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140
by BERTHA ALICIA PORRAS JUAREZ
Published 2007
“... of the “Cores to Disks” Legacy Science project. Photometry from 3.6-70 μm indicates at least 20 candidate low...”Published 2007
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