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61“... the Astronomical Thermal Emission Camera (AzTEC). Comparing with existing 850 μm Submillimetre Common-User...”
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62著者: OLGA MERCEDES VEGA CASANOVA“...We make use of Spitzer imaging between 4 and 16 μm and near-infrared data at 2.2 μm to investigate...”
出版事項 2010
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63著者: David Hughes“...We present high-resolution interferometric imaging of LH 850.02, the brightest 850- and 1200-μm...”
出版事項 2008
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64“...We show that the stellar photored magnitude, m₁₀, of the 10th by brightness galaxy in an Abell...”
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65著者: JUAN NOE SUAREZ PEREA“... with star formation is due to supernovae behaving as cosmic-ray accelerators. To model this emission from M...”
出版事項 2010
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66“... and Infrared Array Camera, and Large APEX Bolometer Camera 870 μm data. Five of the sources (10 per cent) have...”
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67“... and Infrared Array Camera, and Large APEX Bolometer Camera 870 μm data. Five of the sources (10 per cent) have...”
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68著者: Gabriel Mellado Villaseñor“... utilizados para generar un campo Bessel vectorial (VBB, vector Bessel beam) de orden m. Este campo se...”
出版事項 2018
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69著者: JESUS LEONARDO LOPEZ HERNANDEZ“... on spiral galaxies M33 and M101. For M33 the central zone was observed together with the external region IC...”
出版事項 2013
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70著者: José Javier Sánchez Mondragón“... index of the liquid is higher than that of the ferrule, a liquid MMF with a diameter of 125 μm is formed...”
出版事項 2013
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71“..., yield upper limits to the dynamical masses for the individual star clusters between 1.8 and 7.1 × 10⁶M...”
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72“..., yield upper limits to the dynamical masses for the individual star clusters between 1.8 and 7.1 × 10⁶M...”
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73著者: LUIS ABRAHAM SANCHEZ GASPARIANO“... in CadenceVirtuoso v5.0.0. of the complete power amplification stage with the UMC 0.18μm Mixed Mode and RF CMOS...”
出版事項 2011
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74“... circuitos integrados CMOS pozo N Austria Micro Systems (AMS) 0.35 μm y Berkeley 0.13 μm. En base a...”
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75著者: Maxim Kuznetsov“...M dwarf stars are the dominant stellar component of the Galaxy, and therefore they contain...”
出版事項 2019
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76著者: Carlos del Burgo Díaz“... Herschel/PACS to observe a sample of nearby FGK stars. Data at 100 and 160 μm were obtained, complemented...”
出版事項 2013
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77著者: David Hughes“... with the AzTEC camera mounted on the Atacama Submillimeter Telescope Experiment (ASTE) 10 m telescope in Chile...”
出版事項 2011
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78著者: David Hughes“... field from 100 to 500 μm using both PACS and SPIRE. We fit isothermal modified black bodies...”
出版事項 2010
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79著者: ROBERTO GIOVANNI TERLEVICH AFONSO“... ejected by young (t < 20 Myr) and massive (M = 10⁶Mꙩ) coeval stellar cluster with a Salpeter initial mass...”
出版事項 2012
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80著者: MIGUEL ANGEL MEDINA PEREZ, MILTON GARCÍA BORROTO, ANDRES EDUARDO GUTIERREZ RODRIGUEZ, Leopoldo Altamirano Robles“..., named M3gl. This algorithm contains three components: a new feature representation containing clockwise...”
出版事項 2012
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info:eu-repo/semantics/article