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121por 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...”
Publicado 2010
Ligazón do recurso
info:eu-repo/semantics/article -
122“... with 1 GHz bandwidth. The TIA shows 9 pA / p Hz input-referred spectral noise and only 6.9 mW power...”
Ligazón do recurso
info:eu-repo/semantics/article -
123por 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...”
Publicado 2018
Ligazón do recurso
info:eu-repo/semantics/masterThesis -
124por Carla Berrospe Rodríguez“... to generate fast microjets (velocities up to 100 m/s), with the aim of study its penetration depth in low...”
Publicado 2017
Ligazón do recurso
info:eu-repo/semantics/doctoralThesis -
125por IVAN HERNANDEZ ROMANO“.../SWCNT film (thickness 200 μm) and SU8-2075 film (thickness 100 μm) were tested. The saturation intensity...”
Publicado 2011
Ligazón do recurso
info:eu-repo/semantics/doctoralThesis -
126por Carlos del Burgo Díaz“... around ~100 μm or shorter. However, six out of 31 excess sources studied in the Herschl ͣ Open Time Key...”
Publicado 2013
Ligazón do recurso
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127por 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...”
Publicado 2011
Ligazón do recurso
info:eu-repo/semantics/article -
128por 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...”
Publicado 2008
Ligazón do recurso
info:eu-repo/semantics/article -
129“... originally targeted at λ = 850 μm with the Submillimetre Common-User Bolometer Array (SCUBA) in the SCUBA...”
Ligazón do recurso
info:eu-repo/semantics/article -
130“.... Typical CMOS (Complementary Metal-Oxide Semiconductor) N-well 0.35 μm Austria Micro Systems process...”
Ligazón do recurso
info:eu-repo/semantics/article -
131por MARCELINO ANGUIANO MORALES, MARCELA MARIBEL MENDEZ OTERO, MARCELO DAVID ITURBE CASTILLO, SABINO CHAVEZ CERDALigazón do recurso
Publicado 2007
info:eu-repo/semantics/article -
132por Manolis Plionis“... halo mass is ∼ 10¹³ h⁻¹ Mꙩ and ≿5 × 10¹³ h⁻¹ Mꙩ, respectively....”
Publicado 2008
Ligazón do recurso
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133por GORDANA JOVANOVIC DOLECEK“... are the decimation factors, M1 and M2, numbers of cascaded CIC filters L and K, and parameter b of the compensator....”
Publicado 2010
Ligazón do recurso
info:eu-repo/semantics/article -
134por Marcial Becerril“... of 150 mK, using a novel closed-cycle cooling system. This camera belongs to the new generation...”
Publicado 2019
Ligazón do recurso
info:eu-repo/semantics/masterThesis -
135“... of our approach, we test the forecasters on the time series of the M1 and M3 time series competitions...”
Ligazón do recurso
info:eu-repo/semantics/article -
136por Itziar Aretxaga“...We present mid-infrared (MIR) 8–13μm spectroscopy of the nuclear regions of the interacting galaxy...”
Publicado 2013
Ligazón do recurso
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137por 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...”
Publicado 2012
Ligazón do recurso
info:eu-repo/semantics/masterThesis -
138“...We measure the local galaxy far-infrared (FIR) 60 to 100 μm colour–luminosity distribution using...”
Ligazón do recurso
info:eu-repo/semantics/article -
139por David Hughes“... provide estimates of number counts at the three BLAST wavelengths 250, 350, and 500 μm; instead...”
Publicado 2009
Ligazón do recurso
info:eu-repo/semantics/article -
140por David Hughes“...) made resolved maps of seven nearby (<25 Mpc) galaxies at 250, 350, and 500 μm. During its 2005 June...”
Publicado 2009
Ligazón do recurso
info:eu-repo/semantics/article