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201by David Hughes, ITZIAR ARETXAGA MENDEZ, DANIEL FERRUSCA RODRIGUEZ, IDALIA HERNANDEZ CURIEL, ALFREDO AGUSTIN MONTAÑA BARBANO“...-wavelength camera AzTEC on the 10-m Atacama Submillimeter Telescope Experiment (ASTE), have revealed...”
Published 2008
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202by GERARD FRANZ SANTILLAN QUIÑONEZ, VICTOR HUGO CHAMPAC VILELA, ROBERTO STACK MURPHY ARTEAGA“... = 0.2 and W/L = 10 μm/2 μm has been characterized. Sensing capabilities from 90 μT to 27 μ...”
Published 2010
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203by EDMUNDO ANTONIO GUTIERREZ DOMINGUEZ, JOEL MOLINA REYES, PEDRO JAVIER GARCIA RAMIREZ“... 100 mT (mili-Tesla) static B field a variation of the 6% (1.5 nA/27 nA) of the gate current...”
Published 2010
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204by Carlos Alberto Guerrero Peña, Fernando Fabian Rosales-Ortega, GUSTAVO AMILCAR ESCOBEDO LOPEZ, Javier Martínez, Luis Felix“... de la cámara CCD ANDOR iXon Ultra 888 en el telescopio de 2.11 m del OAGH, que consistió en la...”
Published 2019
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205by DELIA MARIA HURTADO CASTAÑEDA“... emission in 0.8 α 1.75µm range. Quantitative results of transport properties in semiconductor silicon...”
Published 2009
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206by CARLOS ALVAREZ MACIAS“... estructuras grabadas. Se lograron velocidades de grabado isotrópico mayores a 13 μm/min, óptimas para...”
Published 2007
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207by Luisa Cardona“... for dust extinction with observations at 24 μm and the SFR🇮🇷 is derived from the submillimeter...”
Published 2019
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208by VIRGINIA MONSERRAT CAMACHO PERNAS“...-shifted component for E0 ≈ 50 kV/μm. Regarding P-EMF, we found that anomalous diffusion suppress...”
Published 2009
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209by Jos´é Manuel Pérez Corte“... obtained when manufacturing the device are encouraging, because speeds of 30 m / s and jet lengths...”
Published 2019
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210by DIEGO ANDRES BLANCO MORA“... resistencia (TCR) alto entre 5% y 68% y una resistencia eléctrica entre 2MΏ y 2MΏ, a temperatura ambiente....”
Published 2013
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212by David Hughes“...-ATLAS alone statistically detects the quasars in its survey área at > 5σ at 250, 350 and 500 μm. From...”
Published 2010
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213“... survey. ID 141 was observed using the IRAM 30 m telescope and Plateau de Bure interferometer (PdBI...”
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214“... peaks is spatially anti-correlated with that of the 100μm emission and the ¹²CO emission.We detected...”
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215“... 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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216“... submillimeter galaxies (SMGs; F1mm> 5.5 mJy) in the COSMOS field, initially detected with MAMBO and AzTEC...”
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220“...-m telescope at the Guillermo Haro observatory in Cananea, Sonora, México. © 2007 Wiley Periodicals...”
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