41
by Itziar Aretxaga, David Hughes
Published 2011
...We report on the detection of an extremely bright (∼37 mJy at 1100 μm and ∼91 mJy at 880 μm...
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42
by David Hughes
Published 2010
...We present results from Submillimeter Array (SMA) 860 μm subarcsecond astrometry...
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43
...² region with near uniform coverage to a depth of 0.96–1.16mJy beamˉ¹. Our robust catalogue contains 28...
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44
by OMAR LOPEZ CRUZ
Published 2007
... > -21, with a weaker dependence on radius than the red LFs. The dispersion of M* was determined...
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45
... y cuenta con un volumen de medición de 4.5m x 6m horizontal por 4.2m vertical. El instrumento...
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46
by Itziar Aretxaga, David Hughes
Published 2011
...) have flux densities >100 mJy at 500 μm, but are not visible in existing optical imaging. We fit light...
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47
...We present the 250, 350, and 500 μm detection of bright submillimeter emission in the direction...
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48
... at 100μm in the rest frame⁹. At 1 ≤ z ≤ 4, the peak is redshifted to wavelengths between 200 and 500 μm...
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49
by IVANIO PUERARI
Published 2009
... of wavenumbers with a gradual steepening from 3.6 or 4.5μm to 8.0 μm, in the order of an increasing contribution...
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50
by OLGA MERCEDES VEGA CASANOVA
Published 2010
...We make use of Spitzer imaging between 4 and 16 μm and near-infrared data at 2.2 μm to investigate...
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51
... the Astronomical Thermal Emission Camera (AzTEC). Comparing with existing 850 μm Submillimetre Common-User...
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52
by David Hughes
Published 2008
...We present high-resolution interferometric imaging of LH 850.02, the brightest 850- and 1200-μm...
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53
by Itziar Aretxaga, David Hughes
Published 2012
... and Infrared Array Camera, and Large APEX Bolometer Camera 870 μm data. Five of the sources (10 per cent) have...
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54
by JUAN NOE SUAREZ PEREA
Published 2010
... with star formation is due to supernovae behaving as cosmic-ray accelerators. To model this emission from M...
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55
by JESUS LEONARDO LOPEZ HERNANDEZ
Published 2013
... on spiral galaxies M33 and M101. For M33 the central zone was observed together with the external region IC...
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56
by Tovmassian Hrant, Monica Rodriguez
Published 2008
...We show that the stellar photored magnitude, m₁₀, of the 10th by brightness galaxy in an Abell...
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57
... circuitos integrados CMOS pozo N Austria Micro Systems (AMS) 0.35 μm y Berkeley 0.13 μm. En base a...
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58
... in CadenceVirtuoso v5.0.0. of the complete power amplification stage with the UMC 0.18μm Mixed Mode and RF CMOS...
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59
..., yield upper limits to the dynamical masses for the individual star clusters between 1.8 and 7.1 × 10⁶M...
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60
..., yield upper limits to the dynamical masses for the individual star clusters between 1.8 and 7.1 × 10⁶M...
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