61
by David Hughes
Published 2011
... with the AzTEC camera mounted on the Atacama Submillimeter Telescope Experiment (ASTE) 10 m telescope in Chile...
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62
by OLGA MERCEDES VEGA CASANOVA
Published 2011
... with unusual ratios, e.g. 7.7 μm/11.3 μm ≤ 2.3. Class-3 objects (7.5% of the sample) have emission lines...
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63
..., named M3gl. This algorithm contains three components: a new feature representation containing clockwise...
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64
... ejected by young (t < 20 Myr) and massive (M = 10⁶Mꙩ) coeval stellar cluster with a Salpeter initial mass...
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65
by David Hughes
Published 2010
... field from 100 to 500 μm using both PACS and SPIRE. We fit isothermal modified black bodies...
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66
by Monica Rodriguez
Published 2008
...Multiconfiguration Dirac–Hartree–Fock electric quadrupole (E2) and magnetic dipole (M1) transition...
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67
... the confusion limit of current far-infrared/submillimeter telescopes. Measurements from 100–500 μm bracket...
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68
by GERMAN ANDRES ALVAREZ BOTERO
Published 2009
... was carried out for different transistors with different channel lengths (80nm, 0,25 μm, 0,5 μm, 1 μm) showing...
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69
by ANGEL ENRIQUE SANCHEZ COLIN
Published 2012
... on one side with a thin film (1 μm thick) of silicon-nitride, thus forming a membrane for each cavity...
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70
by Manolis Plionis
Published 2009
... of σ₈, we find stringent simultaneous constraints in the (Ω, w) plane, with Ω= 0.26 ± 0.05, w =−0.93⁺⁰˙¹¹₋₀․₁₉....
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71
by JESUS ALARCON SALAZAR
Published 2017
... with a multilayered structure of nanometric SRO layers (M-LEC). S-LECs and M-LECs showed photo...
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72
... on the Atacama Pathfinder EXperiment (APEX) telescope to measure the continuum emission at 350 μm. Results. CO(1...
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73
... samples using a 975 nm CW laser, focused on a thin (100 – 300 μm) topical layer of copper nitrate (CuNO...
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74
by WILLIAM FRANK WALL
Published 2007
...Far-infrared continuum data from the COBE/DIRBE instrument were combined with Nagoya 4-m ¹³CO J = 1...
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75
by David Hughes
Published 2011
... a catalog of 157 sources with flux densities spanning two orders of magnitude: from 15 mJy to 1500...
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76
by David Hughes
Published 2011
... of these galaxies. We create a deep 1.16mm map (σ ∼ 0.5 mJy) by combining the AzTEC 1.1mm and MAMBO 1.2mm data sets...
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77
by LILIANA HERNANDEZ MARTINEZ
Published 2012
... best fit for the whole sample, we derived a maximum value for the apparent magnitudes of m⋆5007...
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78
by WILLIAM FRANK WALL
Published 2007
... gas. Consequently, far-infrared continuum data from the COBE/DIRBE instrument and Nagoya 4-m ¹³CO J...
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79
...² area which has a uniform sensitivity Of ~1.3 mJy beamˉ¹. 16 sources are detected with S/N ≥ 4.5, where...
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80
... different pumping power that act on the EDF, where we note that from the 60-mW pumping begins to generate...
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