161
by PAULINA MARIANA MAYA HERNANDEZ
Published 2012
... integrados de amplificador lockin con tecnología CMOS de 0.18m y voltaje de alimentación única de 1.8V...
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Format: info:eu-repo/semantics/masterThesis
162
... high-resolution simulations of the SZE produced by massive galaxy clusters (M > 1014 M_) at different...
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163
by DELIA MARIA HURTADO CASTAÑEDA
Published 2009
... emission in 0.8 α 1.75µm range. Quantitative results of transport properties in semiconductor silicon...
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164
by CARLOS ALVAREZ MACIAS
Published 2007
... estructuras grabadas. Se lograron velocidades de grabado isotrópico mayores a 13 μm/min, óptimas para...
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165
... de la cámara CCD ANDOR iXon Ultra 888 en el telescopio de 2.11 m del OAGH, que consistió en la...
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166
... = 0.2 and W/L = 10 μm/2 μm has been characterized. Sensing capabilities from 90 μT to 27 μ...
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167
... 100 mT (mili-Tesla) static B field a variation of the 6% (1.5 nA/27 nA) of the gate current...
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168
... 4.9x10⁶ and 4.3x10⁷Mꙩ and between 1.8 and 8.7x10⁶Mꙩ for the individual star clusters. Stellar and gas...
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169
...-wavelength camera AzTEC on the 10-m Atacama Submillimeter Telescope Experiment (ASTE), have revealed...
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170
... performed in a vacuum chamber with pressure P=10 mTorr. In general the S(f) measured on our devices...
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171
...-mm-FIR colours of 120 robustly detected 850μm sources in the Lockman Hole East (LH) and Subaru XMM...
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172
by Manolis Plionis
Published 2007
...We use group-sized haloes, with masses in the range 1013 < M < 2 × 1014 h−1Mʘ, identified with a...
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173
by Luisa Cardona
Published 2019
... for dust extinction with observations at 24 μm and the SFR🇮🇷 is derived from the submillimeter...
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174
...-shifted component for E0 ≈ 50 kV/μm. Regarding P-EMF, we found that anomalous diffusion suppress...
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175
by DIEGO ANDRES BLANCO MORA
Published 2013
... resistencia (TCR) alto entre 5% y 68% y una resistencia eléctrica entre 2MΏ y 2MΏ, a temperatura ambiente....
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176
by Itziar Aretxaga, David Hughes
Published 2011
... survey. ID 141 was observed using the IRAM 30 m telescope and Plateau de Bure interferometer (PdBI...
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177
... peaks is spatially anti-correlated with that of the 100μm emission and the ¹²CO emission.We detected...
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178
by Itziar Aretxaga, David Hughes
Published 2012
... formation rates of 10²⁻³ Mꙩ yr⁻¹ . Lower limits for the dust masses (∼a few 10⁸ Mꙩ) and spatial extents (∼1...
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180
by David Hughes
Published 2010
...-ATLAS alone statistically detects the quasars in its survey área at > 5σ at 250, 350 and 500 μm. From...
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