181
by Luis Fernando Martinez Pantoja
Published 2019
... of M Ω (with low degree of accuracy) and tens of pF with a considerable consumption of silicon area...
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182
by HECTOR IVAN GOMEZ ORTIZ
Published 2011
... with GBW=575 MHz and a power consumption of 1.25 mW. Simulation results shows that the amplifier has a DC...
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183
by JOANNES BOSCO HERNANDEZ AGUILA
Published 2015
... of diagnostic diagrams to a selected sample of 40 stars of M 67 and found that, under the assumption of solar...
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185
by MILAGROS ZEBALLOS REBAZA
Published 2013
... of sources with S1.1mm > 4 mJy falls within the 95% confidence interval of the density of sources in a...
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186
by RICARDO JIMENEZ ZAVALA
Published 2013
... bajo costo. En este trabajo se han fabricado y caracterizado micro-bolómetros con área de 50x50 μm2. Se...
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188
... imply star formation rates ranging from <200 to ∼1300 Mꙩ yr⁻¹. In addition, we find that for the radio...
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189
by David Hughes
Published 2011
...m. The Spitzer mid-infrared (MIR) spectrum of IRS1 shows prominent emission features from Mg-rich...
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190
by Emanuele Bertone
Published 2012
...) and optical (Lick) narrowband indices. The total bolometric magnitude of NGC 6791 is M ᵇ°ˡ₆₇₉₁= −6.29, with a...
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191
by Manolis Plionis
Published 2012
... band sources (at a median ¯z ≃ 1), which translates into a host dark matter halo mass of ∼ 10¹³ h⁻¹Mꙩ...
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192
... for Imaging and low Resolution Integrated Spectroscopy (OSIRIS) at the 10.4-m Gran Telescopio Canarias (GTC...
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194
...We have undertaken a deep (σ ∼ 1.1 mJy) 1.1-mm survey of the z = 0.54 cluster MS0451.6−0305 using...
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195
by SALVADOR FLORES GUTIERREZ
Published 2008
...-CNNs las cuales consisten en un arreglo rectangular de M × N celdas. Debido a que no siempre es...
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196
...-infrared, 24 μm, and the radio, 1.4GHz. We find that all of our submm-bright NIR-selected galaxies satisfy...
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197
by GORDANA JOVANOVIC DOLECEK
Published 2007
... polynomials such as the order of tangencies m and l. Our analysis indicates that utilizing this approach...
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199
...-scale restructuring of the surrounding ISM. As an extreme example, we infer from the observations of M82...
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