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121per VICTOR RODOLFO GONZALEZ DIAZ, MIGUEL ANGEL GARCIA ANDRADE, GUILLERMO ESPINOSA FLORES VERDAD“...-magnitude reduction is used to demonstrate that an M -bit MASH architecture dithered by a simple M -bit...”
Publicat 2010
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122“... 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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123per OSCAR JAVIER VELANDIA CABALLERO“...) with a thickness of 8 ± 2nm. This structure gets an Isc of 43 ± 2mA and a Voc of 0.44 ± 0.02 V...”
Publicat 2018
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124per Carla Berrospe Rodríguez“... to generate fast microjets (velocities up to 100 m/s), with the aim of study its penetration depth in low...”
Publicat 2017
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125per IVAN HERNANDEZ ROMANO“.../SWCNT film (thickness 200 μm) and SU8-2075 film (thickness 100 μm) were tested. The saturation intensity...”
Publicat 2011
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126per Carlos del Burgo Díaz“... around ~100 μm or shorter. However, six out of 31 excess sources studied in the Herschl ͣ Open Time Key...”
Publicat 2013
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127per Esperanza Carrasco Licea“... in the first 2 km above the 1.5 m and the 2.1 m telescopes decrease by 15.8% and 13.6%, respectively...”
Publicat 2011
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128per VAHRAM CHAVUSHYAN, LUIS CARRASCO BAZUA, JONATHAN FRANCISCO LEON TAVARES, JOSE RAMON VALDES PARRA“... the 6-m and the 1-m SAO’s telescopes (Russia), the GHAO’s 2.1-m telescope (Cananea, México), and the OAN...”
Publicat 2008
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129“... originally targeted at λ = 850 μm with the Submillimetre Common-User Bolometer Array (SCUBA) in the SCUBA...”
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130“.... Typical CMOS (Complementary Metal-Oxide Semiconductor) N-well 0.35 μm Austria Micro Systems process...”
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131per MARCELINO ANGUIANO MORALES, MARCELA MARIBEL MENDEZ OTERO, MARCELO DAVID ITURBE CASTILLO, SABINO CHAVEZ CERDAObtenir text complet
Publicat 2007
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132per Manolis Plionis“... halo mass is ∼ 10¹³ h⁻¹ Mꙩ and ≿5 × 10¹³ h⁻¹ Mꙩ, respectively....”
Publicat 2008
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133per GORDANA JOVANOVIC DOLECEK“... are the decimation factors, M1 and M2, numbers of cascaded CIC filters L and K, and parameter b of the compensator....”
Publicat 2010
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134per Marcial Becerril“... of 150 mK, using a novel closed-cycle cooling system. This camera belongs to the new generation...”
Publicat 2019
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135“... of our approach, we test the forecasters on the time series of the M1 and M3 time series competitions...”
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136per Itziar Aretxaga“...We present mid-infrared (MIR) 8–13μm spectroscopy of the nuclear regions of the interacting galaxy...”
Publicat 2013
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137per JHOAN ALBERTO SALINAS DELGADO“... at an offset frequency of 1 MHz, and a power consumption of 80 mW is achieved. For the whole system, designed...”
Publicat 2012
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138“...We measure the local galaxy far-infrared (FIR) 60 to 100 μm colour–luminosity distribution using...”
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139per David Hughes“... provide estimates of number counts at the three BLAST wavelengths 250, 350, and 500 μm; instead...”
Publicat 2009
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140per David Hughes“...) made resolved maps of seven nearby (<25 Mpc) galaxies at 250, 350, and 500 μm. During its 2005 June...”
Publicat 2009
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